{"title":"Planetary \u0026 Solar Cameras","description":null,"products":[{"product_id":"celestron-neximage-5-solar-system-imager-5mp","title":"Celestron NexImage 5 Solar System Imager (5MP)","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e5.0 Megapixel color CMOS sensor\u003c\/li\u003e\n\u003cli\u003e2.2 micron square pixels for high-resolution sampling\u003c\/li\u003e\n\u003cli\u003eFrame rates from 0.71 up to 52.37 FPS\u003c\/li\u003e\n\u003cli\u003eStandard 1.25\" barrel and C-thread mounting\u003c\/li\u003e\n\u003cli\u003ePowered via a single USB 2.0 cable\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eCelestron NexImage 5 Solar System Imager (5MP)\u003c\/h2\u003e\n\u003cp\u003eThe Celestron NexImage 5 Solar System Imager pairs a 5.0 MP color CMOS sensor with a native resolution of 2592 x 1944 pixels to capture high-resolution images of the Moon, Sun, and planets. Its 2.2 micron square pixels and 12-bit A\/D conversion are ideal for resolving fine details, while frame rates of up to 52.37 FPS allow you to freeze moments of perfect atmospheric seeing for the sharpest possible results.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e5.0 Megapixels and 2.2µm Pixels for High-Resolution Planetary Detail\u003c\/h3\u003e\n\u003cp\u003eAt the heart of the NexImage 5 is a 5.0 MP onsemi MT9P031 CMOS sensor that provides enough resolution to capture the entire disk of Jupiter or Saturn with room to spare. The small 2.2µm pixels are an excellent match for the long focal lengths of Schmidt-Cassegrain and Maksutov-Cassegrain telescopes, ensuring you can sample fine atmospheric details like Jupiter's cloud bands or the Cassini Division in Saturn's rings without needing an aggressive Barlow lens.\u003c\/p\u003e\n\u003cp\u003eThe sensor's physical size of 5.7mm x 4.28mm is optimized for planetary work, keeping file sizes manageable and centering the target on the chip. While this makes it unsuitable for wide-field deep-sky imaging, it is precisely what's needed for high-magnification views of bright solar system objects.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eUp to 52.37 FPS for Freezing Atmospheric Seeing\u003c\/h3\u003e\n\u003cp\u003eThe key to sharp planetary imaging is \"lucky imaging\"—capturing hundreds or thousands of frames in a short video to catch fleeting moments of atmospheric stability. The NexImage 5 excels at this, delivering frame rates from 0.71 to 5.99 FPS at full 2592 x 1944 resolution, and up to 52.37 FPS when using hardware sub-framing to focus on a smaller region of interest.\u003c\/p\u003e\n\u003cp\u003eYou simply record a short video of your target, and the included software (compatible with iCap and DirectShow) helps you analyze the video file, discard the frames blurred by turbulence, and stack only the sharpest ones. This process averages out atmospheric distortion and electronic noise, revealing a bright, clear, and detailed final image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eUSB 2.0 Power and 1.25\" Mounting for Universal Compatibility\u003c\/h3\u003e\n\u003cp\u003eDesigned for simplicity, the NexImage 5 is powered entirely by its 5-foot USB 2.0 cable, eliminating the need for an external power supply in the field. Its extremely light weight of just 2.0 oz (57 g) ensures it won't create balancing issues, even on smaller telescope mounts. The camera body features a standard 1.25\" nosepiece for direct connection to any telescope focuser or diagonal.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eDual Back Focus:\u003c\/strong\u003e The camera offers two back focus distances. With the 1.25\" nosepiece attached, the distance is 13.1mm. By removing the nosepiece, you can access the C-threads for a shorter 10.6mm back focus, useful for custom accessory configurations.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eIntegrated IR-Cut Filter:\u003c\/strong\u003e The optical window has a built-in IR-Cut filter to ensure accurate color balance and sharpness by blocking unfocused infrared light.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat software do I need to use the Celestron NexImage 5?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Celestron NexImage 5 includes a software CD with everything you need to get started on a Windows PC, including drivers and capture software like \u003cstrong\u003eiCap\u003c\/strong\u003e. It is also compatible with other popular freeware like SharpCap and AutoStakkert! for capture and processing. The camera uses a standard \u003cstrong\u003eDirectShow\u003c\/strong\u003e driver for broad compatibility.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the Celestron NexImage 5 a good camera for deep-sky objects?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eNo, the NexImage 5 is not recommended for deep-sky imaging. Its small sensor is designed to frame planets, not large nebulae or galaxies. Furthermore, as an uncooled camera, long exposures (from 0.0001 to \u003cstrong\u003e30 seconds\u003c\/strong\u003e) will exhibit significant thermal noise, which would obscure faint deep-sky details.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the Celestron NexImage 5 work with a Mac?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe included software is Windows-only. While the Celestron NexImage 5 is not officially supported on macOS, some Mac users have found success using third-party software that supports standard USB webcams and planetary cameras, though functionality may be limited.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow will the Celestron NexImage 5 perform on Jupiter with an 8\" SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThis is an excellent combination. An 8\" f\/10 SCT provides the ideal focal length to match with the NexImage 5's \u003cstrong\u003e2.2µm pixels\u003c\/strong\u003e for high-resolution views of Jupiter. This setup will allow you to clearly resolve the main equatorial belts, the Great Red Spot, and shadow transits of the Galilean moons, especially when using the camera's high frame rate to counteract atmospheric turbulence.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Celestron NexImage 5 to image the entire full Moon?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThis depends on your telescope's focal length. With a short focal length refractor, you may be able to fit the entire lunar disk in the \u003cstrong\u003e2592 x 1944\u003c\/strong\u003e frame. However, with a longer focal length instrument like an SCT or Maksutov, you will need to capture multiple videos and stitch them together into a mosaic to show the entire Moon.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the benefit of the Celestron NexImage 5's 12-bit A\/D conversion?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e12-bit\u003c\/strong\u003e Analog-to-Digital converter allows the NexImage 5 to capture 4,096 different levels of brightness. This provides much smoother tonal gradations across planetary surfaces and the lunar terminator compared to older 8-bit cameras, which are limited to just 256 levels. The result is more detail in subtle features and a more realistic final image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eColor onsemi MT9P031 CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e5.0 MP (2592 x 1944)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.2µm square\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003e5.7mm x 4.28mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eA\/D Conversion\u003c\/td\u003e\n\u003ctd\u003e12 bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rate\u003c\/td\u003e\n\u003ctd\u003e0.71 to 5.99 FPS (at 2592x1944)\u003cbr\u003e6.23 to 52.37 FPS (at 640x480)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e0.0001 to 30 seconds\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSub-Framing\u003c\/td\u003e\n\u003ctd\u003eHardware Selectable\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMounting\u003c\/td\u003e\n\u003ctd\u003e1.25\" barrel and C-thread\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e13.1mm (with nosepiece), 10.6mm (without nosepiece)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOptical Window\u003c\/td\u003e\n\u003ctd\u003eIR Cutoff Filter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePower\u003c\/td\u003e\n\u003ctd\u003eUSB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eUSB Cable\u003c\/td\u003e\n\u003ctd\u003e5' long\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSoftware Compatibility\u003c\/td\u003e\n\u003ctd\u003eiCap, IC Capture, DirectShow\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eHousing\u003c\/td\u003e\n\u003ctd\u003eABS with aluminum connection ring\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e2.0 oz (57 g)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOperating Environment\u003c\/td\u003e\n\u003ctd\u003e-22°F to 158°F (-30°C to 70°C)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRecommended Use\u003c\/td\u003e\n\u003ctd\u003eLunar, solar, and planetary imaging\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eNexImage 5 Camera Body\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eUSB Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eInstruction Manual\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Celestron_NexImage_5_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eCelestron NexImage 5 Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/celestron-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eCelestron 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Celestron","offers":[{"title":"Default Title","offer_id":44967142228253,"sku":"CEL-93711","price":306.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/Celestron-NexImage-5-Solar-System-Imager-5MP-93711-1__79221.1594230227.1280.1280.jpg?v=1684337053"},{"product_id":"qhyccd-qhy5iii290m-mono","title":"QHYCCD QHY5III290M Mono","description":"\u003c!-- more --\u003e\u003ch2\u003eFull HD Back-illuminated, Ultra-low Read Noise CMOS Camera\u003c\/h2\u003e\u003cp\u003eThe QHY5-III series cameras are USB3 super-speed cameras and guiders.  They can be used in a standard 1.25-inch eyepiece holder and have an adjustable location ring for confocality with an eyepiece.  All QHY5III series cameras come in a very small but powerful package!\u003c\/p\u003e\u003cp\u003eThe QHY5III290 uses the SONY STARVIS Exmor R back-illuminated CMOS sensor.  STARVIS means you can see very dim stars in real time video. The QHY5III290 can capture magnitude 9 stars with a 50mm F\/1.4 C-mount lens.  Compared to the IMX236 sensor, for example, the IMX290 has twice sensitivity for visible light and three or more times the sensitivity in near infrared.  The QHY5III290 also has ultra low read noise.  The back-illumination and low read noise make this camera an ideal video astronomy camera.  The small 2.9um pixel size is also ideal for planetary imaging.  The QHY5III290 has a fast USB 3.0 interface and produces 135FPS at full HD output . The camera has 10\/12-bit ADC and it outputs an 8-bit or 12-bit image.  Available in both mono (QHY5III290M) and color (QHY5III290C) versions.\u003c\/p\u003e\u003cdiv data-custom-tab\u003e\n\u003cp data-custom-tab-title\u003eSpecifications\u003c\/p\u003e\n\u003cdiv\u003e\u003ctable border=\"0\" width=\"483\" cellspacing=\"0\" cellpadding=\"0\"\u003e\n\u003ccolgroup\u003e\n\u003ccol width=\"212\"\u003e\n\u003ccol width=\"271\"\u003e\n\u003c\/colgroup\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eModel\u003c\/td\u003e\n\u003ctd width=\"271\"\u003eQHY5III290\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eCMOS Sensor\u003c\/td\u003e\n\u003ctd width=\"271\"\u003eIMX290（BSI)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003ePixel Size\u003c\/td\u003e\n\u003ctd width=\"271\"\u003e2.9um\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003ePixel Array\u003c\/td\u003e\n\u003ctd width=\"271\"\u003e1920*1080\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eEffective Pixels\u003c\/td\u003e\n\u003ctd width=\"271\"\u003e1.2 Megapixels\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eSensor Optical Format\u003c\/td\u003e\n\u003ctd width=\"271\"\u003e1\/2.8-inch\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eFrame Rate@Full Frame\u003c\/td\u003e\n\u003ctd width=\"271\"\u003e135FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd rowspan=\"4\" width=\"212\" height=\"81\"\u003eFrame rate @ROI readout\u003c\/td\u003e\n\u003ctd width=\"271\"\u003e220FPS@\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\u003ctd width=\"271\" height=\"20\"\u003e960*540    \u003c\/td\u003e\u003c\/tr\u003e\n\u003ctr\u003e\u003ctd width=\"271\" height=\"20\"\u003e460FPS@\u003c\/td\u003e\u003c\/tr\u003e\n\u003ctr\u003e\u003ctd width=\"271\" height=\"21\"\u003e480*270\u003c\/td\u003e\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eFul Well Capacity\u003c\/td\u003e\n\u003ctd width=\"271\"\u003e15.7ke-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eReadout Noise\u003c\/td\u003e\n\u003ctd width=\"271\"\u003e0.75e to 3.2e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eA\/D \u003c\/td\u003e\n\u003ctd width=\"271\"\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eShutter Type\u003c\/td\u003e\n\u003ctd width=\"271\"\u003eElectric Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eColor Version\u003c\/td\u003e\n\u003ctd width=\"271\"\u003eQHY5III290C\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eMono Version\u003c\/td\u003e\n\u003ctd width=\"271\"\u003eQHY5III290M\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eComputer Interface\u003c\/td\u003e\n\u003ctd width=\"271\"\u003eUSB3.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eGuide Port\u003c\/td\u003e\n\u003ctd width=\"271\"\u003eStandard 6-pin RJ11 Guide Port\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd width=\"271\"\u003e1.25-inch, CS mount\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"212\" height=\"21\"\u003eWeight\u003c\/td\u003e\n\u003ctd width=\"271\"\u003e87g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\u003c\/div\u003e\n\u003c\/div\u003e","brand":"QHYCCD","offers":[{"title":"Default Title","offer_id":44967211958557,"sku":"QHY-QHY5III290M","price":461.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/QHYCCD-QHY5III290M-Mono-1__87359.1595653763.1280.1280.jpg?v=1684339030"},{"product_id":"qhyccd-qhy5iii174c-color","title":"QHYCCD QHY5III174C Color","description":"\u003c!-- more --\u003e\u003cp\u003eThe QHY5-III series cameras are USB3 super-speed cameras and guiders.  They can be used in a standard 1.25-inch eyepiece holder and have an adjustable location ring for confocality with an eyepiece.  All QHY5III series cameras come in a very small but powerful package!\u003c\/p\u003e\u003cp\u003eThe QHY5III174 is the first in the new QHY5III series CMOS USB 3.0 cameras. The camera is designed to be an excellent planetary, lunar, solar and meteor capture video camera. With a 50mm, F\/1.4 C-mount lens it will record 8th to 9th magnitude stars at 30 frames per second (33 ms exposure).  This high sensitivity with HD resolution will push video astronomy to new heights.  Sony introduced a new global shutter (GS) CMOS imaging technology called PregiusTM that redefines the global shutter imaging category and provides the best of both worlds:  fast frame rates and CCD-like imaging performance.  The technology also offers reduced dark noise, which enables higher gains without compromising image quality, as well as higher quantum efficiency.    The global shutter eliminates pixelization when imaging the moon and planets and moon caused by atmospheric agitation and high frame rates. \u003c\/p\u003e\u003cp\u003eThe unique QHYCCD design retains the 1.25-inch eyepiece design of the QHY5-II series but adds features for better cooling.  This design is more efficient in transfer of heat to the outer case enabling lower noise especially in high ambient temperatures.  The 1.25 inch design also offers the shortest possible backfocus, making the camera ideal for off-axis guiding.  In addition, the QHY5III174 uses a more robust LEMO style connector for the guide port.  These connectors are known for being both rugged and reliable.   The QHY5III174 is available in both mono and color versions. The camera is well suited for solar imaging using short focal length telescopes that will capture a full solar disk within the FOV. \u003c\/p\u003e\u003cdiv data-custom-tab\u003e\n\u003cp data-custom-tab-title\u003eSpecifications\u003c\/p\u003e\n\u003cdiv\u003e\u003ctable border=\"0\" width=\"523\" cellspacing=\"0\" cellpadding=\"0\"\u003e\n\u003ccolgroup\u003e\n\u003ccol width=\"219\"\u003e\n\u003ccol width=\"304\"\u003e\n\u003c\/colgroup\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eModel\u003c\/td\u003e\n\u003ctd width=\"304\"\u003eQHY5III174\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eCMOS Sensor\u003c\/td\u003e\n\u003ctd width=\"304\"\u003eIMX174\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003ePixel Size\u003c\/td\u003e\n\u003ctd width=\"304\"\u003e5.86um\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003ePixel Array\u003c\/td\u003e\n\u003ctd width=\"304\"\u003e1920*1200\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eEffective Pixels\u003c\/td\u003e\n\u003ctd width=\"304\"\u003e2.3 Megapixels\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eSensor Optical Format\u003c\/td\u003e\n\u003ctd width=\"304\"\u003e1\/1.2-inch\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eFrame Rate@Full Frame\u003c\/td\u003e\n\u003ctd width=\"304\"\u003e138FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd rowspan=\"4\" width=\"219\" height=\"81\"\u003eFrame rate @ROI readout\u003c\/td\u003e\n\u003ctd width=\"304\"\u003e262FPS@ 960*600\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\u003ctd width=\"304\" height=\"20\"\u003e490FPS@ 480*300\u003c\/td\u003e\u003c\/tr\u003e\n\u003ctr\u003e\u003ctd width=\"304\" height=\"20\"\u003e\u003c\/td\u003e\u003c\/tr\u003e\n\u003ctr\u003e\u003ctd width=\"304\" height=\"21\"\u003e\u003c\/td\u003e\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eFul Well Capacity\u003c\/td\u003e\n\u003ctd width=\"304\"\u003e32ke-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eReadout Noise\u003c\/td\u003e\n\u003ctd width=\"304\"\u003e1.6e- to 5.3e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eA\/D \u003c\/td\u003e\n\u003ctd width=\"304\"\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eShutter Type\u003c\/td\u003e\n\u003ctd width=\"304\"\u003eElectric Global Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eColor Version\u003c\/td\u003e\n\u003ctd width=\"304\"\u003eQHY5III174C\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eMono Version\u003c\/td\u003e\n\u003ctd width=\"304\"\u003eQHY5III174M\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eComputer Interface\u003c\/td\u003e\n\u003ctd width=\"304\"\u003eUSB3.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eGuide Port\u003c\/td\u003e\n\u003ctd width=\"304\"\u003eStandard 6-pin RJ11 Guide Port\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd width=\"304\"\u003e1.25-inch, CS mount\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"219\" height=\"21\"\u003eWeight\u003c\/td\u003e\n\u003ctd width=\"304\"\u003e89g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\u003c\/div\u003e\n\u003c\/div\u003e","brand":"QHYCCD","offers":[{"title":"Default Title","offer_id":44967211991325,"sku":"QHY-100064","price":839.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/QHYCCD-QHY5III174C-Color-1__27394.1595653764.1280.1280.jpg?v=1684339032"},{"product_id":"qhyccd-qhy5iii174m-mono","title":"QHYCCD QHY5III174M Mono","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e1\/1.2-inch Sony IMX174 monochrome sensor\u003c\/li\u003e\n\u003cli\u003eElectronic Global Shutter eliminates motion artifacts\u003c\/li\u003e\n\u003cli\u003e2.3 Megapixel resolution (1920x1200) with 5.86μm pixels\u003c\/li\u003e\n\u003cli\u003eCaptures up to 138 FPS at full resolution\u003c\/li\u003e\n\u003cli\u003eStandard ST-4 guide port and USB 3.0 interface\u003c\/li\u003e\n\u003cli\u003eLightweight 85g body with a 1.25-inch form factor\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eQHYCCD QHY5III174M Monochrome CMOS Camera\u003c\/h2\u003e\n\u003cp\u003eThe QHYCCD QHY5III174M Mono combines the artifact-free imaging of a global shutter with a large 1\/1.2-inch Sony IMX174 sensor, creating a definitive tool for high-resolution solar, lunar, and planetary imaging. Its 2.3 Megapixel sensor with large 5.86μm pixels captures data at a blistering 138 FPS over USB 3.0, freezing moments of atmospheric stability. With a deep 32ke- full well capacity and read noise as low as 2.2e-, the QHY5III174M pulls fine detail from both bright planetary disks and faint solar prominences.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eGlobal Shutter Imaging: The 1\/1.2-inch Sony IMX174\u003c\/h3\u003e\n\u003cp\u003eThe core of the QHY5III174M is its Sony IMX174 sensor, which features an electronic global shutter. Unlike rolling shutters that can distort fast-moving targets or warp images under turbulent seeing, a global shutter exposes all 2.3 million pixels simultaneously. This completely eliminates motion artifacts, ensuring that planetary features and delicate solar granulation are captured without skew, even at high frame rates.\u003c\/p\u003e\n\u003cp\u003eThe sensor's large 1\/1.2-inch format provides a generous field of view for framing the entire solar or lunar disk with shorter focal length telescopes. The 5.86μm pixels offer a good balance of resolution and sensitivity, making them an excellent match for common f\/7 to f\/10 systems like SCTs and Maksutov-Cassegrains without requiring aggressive barlows.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e138 FPS Planetary and Solar Performance\u003c\/h3\u003e\n\u003cp\u003eTo capture moments of perfect seeing, speed is essential. The QHY5III174M delivers a full-resolution frame rate of 138 FPS at 8-bit, enabled by its high-speed USB 3.0 interface. This allows you to acquire thousands of frames in a short period, maximizing your chances of catching sharp data for stacking and processing.\u003c\/p\u003e\n\u003cp\u003eFor even higher speeds when targeting specific features like Jupiter's Great Red Spot or a solar flare, Region of Interest (ROI) can be used. At a 960x600 resolution, the frame rate increases to 262 FPS, and at 480x300, it reaches an incredible 490 FPS. This extreme speed is critical for lucky imaging, effectively freezing atmospheric distortion to resolve the finest details.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eDual-Role Guiding with an 85g Body\u003c\/h3\u003e\n\u003cp\u003eBeyond planetary imaging, the QHY5III174M is a highly capable guide camera. The large 1\/1.2-inch sensor makes it easy to find suitable guide stars, even in star-poor regions of the sky or when using an off-axis guider. A standard ST-4 port provides a direct connection to your mount for autoguiding corrections.\u003c\/p\u003e\n\u003cp\u003eWeighing only 85g and designed with a 1.25-inch eyepiece form factor, the camera adds minimal weight and complexity to your setup. This is particularly advantageous for off-axis guiding on large SCTs, where minimizing load on the focuser is critical. The camera also includes C and CS-mount threads, allowing for direct attachment of C-mount lenses for wide-field applications like meteor detection.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eQHY5III174M vs. ZWO ASI174MM: A 1\/1.2-inch Sensor Showdown\u003c\/h3\u003e\n\u003cp\u003eBoth the QHY5III174M and ZWO ASI174MM are built around the same excellent Sony IMX174 global shutter sensor and share nearly identical imaging specifications. The decision between them often comes down to physical design and ecosystem preference. The ZWO camera has a large, established user base and broad software compatibility.\u003c\/p\u003e\n\u003cp\u003eThe primary differentiator for the QHY5III174M is its unique 1.25-inch eyepiece-style body. This slim, lightweight (85g) form factor is often easier to insert and balance in off-axis guiders and finder-scopes compared to the wider, puck-shaped body of the ZWO. For imagers prioritizing a compact, low-profile guider or planetary camera, the QHY's physical design is a significant advantage.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy is the QHY5III174M's global shutter important for solar imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eSolar features, like granulation and prominences, change rapidly and are viewed through significant atmospheric turbulence (daytime seeing). A \u003cstrong\u003eglobal shutter\u003c\/strong\u003e exposes the entire 1920x1200 sensor at once, preventing the wave-like distortion (\"jello effect\") that rolling shutters can introduce. This results in sharper, more stable video frames, which is critical for producing high-quality stacked images of the Sun.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the QHY5III174M perform for guiding with a long focal length SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe QHY5III174M is an excellent choice for guiding long focal length telescopes like an 8\" or 11\" SCT. Its large \u003cstrong\u003e1\/1.2-inch sensor\u003c\/strong\u003e provides a wide field of view, making it much easier to find a suitable guide star within the small pick-off prism of an off-axis guider (OAG). Its high sensitivity and 5.86μm pixels are well-suited for detecting faint stars.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the QHY5III174M for deep-sky imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWhile primarily designed for high-frame-rate planetary and solar work, the QHY5III174M can be used for electronically-assisted astronomy (EAA) on brighter deep-sky objects like the Orion Nebula (M42) or the Hercules Cluster (M13). However, as an \u003cstrong\u003euncooled camera\u003c\/strong\u003e, it will exhibit more thermal noise on long exposures compared to dedicated deep-sky cameras. It is best suited for live-stacking many short exposures rather than single long-duration shots.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat's the benefit of the QHY5III174M's large 1\/1.2-inch sensor?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eA large sensor provides a wider True Field of View at a given focal length. For imagers, this means you can:\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eCapture the entire Sun or Moon\u003c\/strong\u003e with telescopes up to around 1000mm focal length.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eCreate large mosaics\u003c\/strong\u003e of the lunar surface or solar disk with fewer panels.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eEasily find guide stars\u003c\/strong\u003e when using the camera with an off-axis guider.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat do the C-mount and CS-mount threads on the QHY5III174M let me do?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe C and CS-mount threads allow you to attach a wide variety of industrial, security, or specialized C-mount lenses directly to the camera without a telescope. This is useful for all-sky imaging, meteor monitoring, or wide-field surveillance. The camera's \u003cstrong\u003e12mm back focus\u003c\/strong\u003e is compatible with standard C-mount lenses.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the difference between the QHY5III174M and the ZWO ASI174MM?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eBoth cameras use the same Sony IMX174 monochrome sensor and offer very similar performance in terms of frame rate, resolution, and noise. The main difference is physical design. The \u003cstrong\u003eQHY5III174M has a slim 1.25\" eyepiece-style body\u003c\/strong\u003e that is lightweight (85g) and easy to fit in tight spaces like an off-axis guider. The ZWO ASI174MM has a wider, round \"puck\" shape. Your choice may depend on which form factor best fits your specific telescope and imaging train.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Sensor\u003c\/td\u003e\n\u003ctd\u003eSony IMX174\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Type\u003c\/td\u003e\n\u003ctd\u003eMonochrome FSI CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003e1\/1.2-inch\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e5.86μm x 5.86μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eEffective Resolution\u003c\/td\u003e\n\u003ctd\u003e1920 x 1200 (2.3 Megapixels)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e32ke-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e2.2e- to 5.5e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit (output as 16-bit and 8-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Global Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate (Full)\u003c\/td\u003e\n\u003ctd\u003e138 FPS @ 8-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate (ROI)\u003c\/td\u003e\n\u003ctd\u003e262 FPS @ 960x600 | 490 FPS @ 480x300\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBuilt-in Buffer\u003c\/td\u003e\n\u003ctd\u003e–\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Time Range\u003c\/td\u003e\n\u003ctd\u003e–\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eComputer Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 Type-B\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4 Compatible\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd\u003e1.25-inch, CS-Mount, C-Mount\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOptical Window\u003c\/td\u003e\n\u003ctd\u003eAR Coated Glass\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e85g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.qhyccd.com\/download\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/qhyccd-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eQHYCCD Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"QHYCCD","offers":[{"title":"Default Title","offer_id":44967212024093,"sku":"QHY-100063","price":881.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/QHYCCD-QHY5III174M-Mono-1__13796.1595653764.1280.1280.jpg?v=1684339033"},{"product_id":"qhyccd-qhy5iii462c-color","title":"QHYCCD QHY5III462C Color","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e2 Megapixel Sony IMX462 BSI CMOS Sensor\u003c\/li\u003e\n\u003cli\u003e2.9µm Pixels in a 1920x1080 Array\u003c\/li\u003e\n\u003cli\u003e135 FPS Maximum Frame Rate at 8-bit\u003c\/li\u003e\n\u003cli\u003e0.5e- Ultra-Low Read Noise\u003c\/li\u003e\n\u003cli\u003eExceptional Near-Infrared (NIR) Sensitivity\u003c\/li\u003e\n\u003cli\u003eIncludes IR-Cut and IR850nm Filters\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eQHYCCD QHY5III462C Color Planetary Camera \u0026amp; Autoguider\u003c\/h2\u003e\n\u003cp\u003eThe QHYCCD QHY5III462C Color camera combines a 2 Megapixel Sony IMX462 BSI sensor with 2.9µm pixels for high-resolution planetary imaging at a native 1920x1080 resolution. It achieves a maximum frame rate of 135 FPS over its USB 3.0 interface, while its Super High Conversion Gain mode drops read noise to an exceptionally low 0.5e-. The sensor's 12-bit ADC and 12ke- full well capacity ensure excellent dynamic range for capturing subtle details on targets like Jupiter and Saturn.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eIMX462 STARVIS Sensor: 1920x1080 Resolution at 135 FPS\u003c\/h3\u003e\n\u003cp\u003eAt the heart of the QHY5III462C is the Sony IMX462 STARVIS sensor, featuring the same 2.9µm pixel size and 1920x1080 resolution that made its predecessor a favorite among planetary imagers. This resolution is perfectly matched for sampling planetary details on most amateur telescopes without requiring a Barlow lens.\u003c\/p\u003e\n\u003cp\u003eThe camera's ability to stream full-resolution frames at 135 FPS over USB 3.0 is critical for \"lucky imaging.\" By capturing thousands of frames in a short period, you can freeze moments of atmospheric stability, allowing software to select only the sharpest data for a final, detailed image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSuper High Conversion Gain: Capturing Detail with 0.5e- Read Noise\u003c\/h3\u003e\n\u003cp\u003eThe IMX462 sensor incorporates Super High Conversion Gain (sHCG) technology, enabling it to achieve an astonishingly low read noise of just 0.5e-. This mode prioritizes ultra-low read noise over maximum full well capacity, a trade-off that is ideal for the high-gain, short-exposure techniques of planetary imaging.\u003c\/p\u003e\n\u003cp\u003eWith such a low noise floor, you can stack hundreds or thousands of frames without noise overwhelming the faint, low-contrast details in planetary cloud bands or lunar rilles. The camera's 12-bit A\/D converter ensures the subtle signal you capture is digitized with sufficient depth to withstand aggressive sharpening during processing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eExceptional NIR Sensitivity: Dominating the 850nm Spectrum\u003c\/h3\u003e\n\u003cp\u003eA key advantage of the QHY5III462C is its profound sensitivity in near-infrared (NIR) light. The IMX462's back-illuminated pixels have a deeper physical structure, allowing longer-wavelength photons to be detected efficiently. The result is a peak quantum efficiency in the NIR that is nearly equal to its peak in the visible spectrum.\u003c\/p\u003e\n\u003cp\u003eThis opens up new avenues for planetary science, particularly for methane band imaging. Using the included IR850nm filter, you can capture high-contrast views of Jupiter's and Saturn's high-altitude clouds and storms. For standard visible-light imaging, an included IR-Cut filter ensures proper color balance.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eCompact Design: 88g Body with USB 3.0 and ST-4\u003c\/h3\u003e\n\u003cp\u003eEngineered for practicality, the QHY5III462C weighs only 88g and fits into any standard 1.25-inch focuser or accessory. It also includes C-mount threads for direct connection to lenses or microscopes. The entire camera is powered through its single USB 3.0 Type-B port, eliminating the need for a separate power cable.\u003c\/p\u003e\n\u003cp\u003eA custom ST-4 guide port allows the camera to double as a highly sensitive autoguider. Its ability to detect faint stars, even in the NIR, makes it a reliable choice for guiding long-exposure deep-sky images.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eQHY5III462C vs. QHY5III290C: The NIR Advantage\u003c\/h3\u003e\n\u003cp\u003eThe QHY5III290C set a high standard for planetary imaging, built around a sensor with the same 2.9µm pixels and 1920x1080 resolution as the 462C. It remains a very capable camera for capturing planets in visible light.\u003c\/p\u003e\n\u003cp\u003eHowever, the QHY5III462C's IMX462 sensor introduces two critical advancements. First, the sHCG mode delivers significantly lower read noise (0.5e-) at the high gain settings used for planetary work. Second, and most decisively, the 462C's radically enhanced NIR sensitivity makes it a superior instrument for scientific imaging, especially in the methane band. For imagers wanting to explore atmospheric details on the gas giants, the QHY5III462C is the definitive choice.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the QHY5III462C's NIR sensitivity help when imaging Jupiter?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eJupiter's atmosphere has a strong absorption band around 880nm due to methane gas. Using the \u003cstrong\u003eQHY5III462C\u003c\/strong\u003e with the included \u003cstrong\u003eIR850nm filter\u003c\/strong\u003e allows you to perform methane band imaging. This technique darkens the main cloud decks and makes high-altitude features, like the Great Red Spot and other storms, appear incredibly bright and detailed. This camera's high sensitivity in this wavelength makes it one of the best tools for this type of scientific imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat frame rates can I expect from the QHY5III462C on Saturn with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWhile the camera's maximum rate is \u003cstrong\u003e135 FPS\u003c\/strong\u003e, you won't achieve that on a dim target like Saturn at f\/10. To get enough signal, your exposure time will be longer, reducing the frame rate. However, you can use a Region of Interest (ROI) to capture only the area around the planet, significantly boosting the frame rate. The ultra-low \u003cstrong\u003e0.5e- read noise\u003c\/strong\u003e is crucial here, as it allows you to use higher gain to compensate for short exposures without introducing excessive noise.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is sHCG (Super High Conversion Gain) on the QHY5III462C?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003esHCG is a special mode built into the Sony IMX462 sensor. When you increase the camera's gain past a certain point, the sensor switches to this mode, which dramatically reduces the read noise down to \u003cstrong\u003e0.5e-\u003c\/strong\u003e. This is ideal for planetary \"lucky imaging,\" where you capture thousands of very short exposures. The low read noise ensures that when you stack these frames, the final image is clean and detailed.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDo I need an external power supply for the QHY5III462C?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eNo. The QHY5III462C is powered and controlled entirely through its single \u003cstrong\u003eUSB 3.0 port\u003c\/strong\u003e. This simplifies cable management at the telescope and reduces the number of items you need to power in the field.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the QHY5III462C for autoguiding?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, absolutely. The camera features a built-in \u003cstrong\u003eST-4 guide port\u003c\/strong\u003e and its high sensitivity makes it an excellent autoguider. Its lightweight \u003cstrong\u003e88g\u003c\/strong\u003e body will not put significant strain on your focuser or off-axis guider. Its strong NIR sensitivity can also help find guide stars that are faint in the visible spectrum.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the purpose of the two filters included with the QHY5III462C?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe QHY5III462C includes two key filters for different imaging goals:\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eIR-Cut Filter:\u003c\/strong\u003e This is for standard RGB color imaging of planets. It blocks infrared light to ensure the colors of targets like Jupiter and Mars are rendered accurately.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eIR850nm Filter:\u003c\/strong\u003e This is a pass filter that blocks visible light and only lets near-infrared light through. It's used specifically to take advantage of the camera's high NIR sensitivity for applications like methane band imaging.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Sensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX462 BSI CMOS, Color, Typical 1\/2.8 inch\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size \/ Resolution\u003c\/td\u003e\n\u003ctd\u003e2.9µm x 2.9µm \/ 1920x1080 (2 Megapixels)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e12ke-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e0.5e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eA\/D Converter\u003c\/td\u003e\n\u003ctd\u003e12-bit (output as 16-bit and 8-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e135 FPS @ 8-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eROI Frame Rates\u003c\/td\u003e\n\u003ctd\u003eTBA\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Time Range\u003c\/td\u003e\n\u003ctd\u003e7µs - 900sec\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eComputer Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 Type-B\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eCustom ST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd\u003e1.25-inch, C-Mount\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOptical Window\u003c\/td\u003e\n\u003ctd\u003eAR Anti-reflection Glass\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eIncluded Filters\u003c\/td\u003e\n\u003ctd\u003eIR850nm Filter, IR-Cut Filter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBuilt-in Image Buffer\u003c\/td\u003e\n\u003ctd\u003e–\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e88g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.qhyccd.com\/download\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/qhyccd-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eQHYCCD Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"QHYCCD","offers":[{"title":"Default Title","offer_id":44967212155165,"sku":"QHY-110078","price":419.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/QHYCCD-QHY5III462C-Color-1__01192.1595653764.1280.1280.jpg?v=1684339039"},{"product_id":"zwo-asi174mm-mono","title":"ZWO ASI174MM Mono","description":"\u003cul class=\"DAV-feature-list\"\u003e\n    \u003cli\u003e\n        IMX174 Sensor\n    \u003c\/li\u003e\n    \u003cli\u003e\n        Pixel Size of 5.86 microns\n    \u003c\/li\u003e\n    \u003cli\u003e\n        QE of 77%\n    \u003c\/li\u003e\n    \u003cli\u003e    \n        USB 3.0\n    \u003c\/li\u003e\n    \u003cli\u003e\n        164 FPS\n    \u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n    \u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n    \u003cli\u003eSpecifications\u003c\/li\u003e\n    \u003cli\u003eDiagrams \u0026amp; Resources\u003c\/li\u003e\n    \u003cli\u003eIn the Box\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n    \u003cli class=\"active\"\u003e\n        \u003cdiv\u003e\n            \u003c!-- Title image text --\u003e\n            \u003cdiv class=\"DAV-bg-light\"\u003e\n                \u003c!-- Main Image --\u003e\n                \u003cdiv class=\"DAV-section-center\"\u003e\n                    \u003ch2\u003eZWO ASI174MM - Overview\u003c\/h2\u003e\n                    \u003cp\u003e\n                        The ZWO ASI174MM is a popular choice among astrophotographers, designed around the Sony Exmor IMX174 2.35MP sensor with advanced Pregius global shutter technology. Whether capturing solar, lunar, planetary, or deep-sky objects, this camera offers exceptional performance and reliability.\n                    \u003c\/p\u003e\n                \u003c\/div\u003e\n            \u003c\/div\u003e\n\n            \u003c!-- Features Grid --\u003e\n            \u003cdiv class=\"DAV-feature-grid\"\u003e\n                \u003cdiv class=\"DAV-feature-box\"\u003e\n                    \u003ch3\u003e\n                        Sony IMX174 CMOS Sensor\n                    \u003c\/h3\u003e\n                    \u003cp\u003e\n                        Features a 1\/1.2” monochrome sensor with 1936 x 1216 resolution and large 5.86µm pixels for enhanced light sensitivity and detail.\n                    \u003c\/p\u003e\n                \u003c\/div\u003e\n\n                \u003cdiv class=\"DAV-feature-box\"\u003e\n                    \u003ch3\u003e\n                        Pregius Global Shutter\n                    \u003c\/h3\u003e\n                    \u003cp\u003e\n                        Ensures distortion-free imaging by scanning all pixels simultaneously, making it perfect for solar and lunar imaging under challenging conditions like wind or atmospheric turbulence.\n                    \u003c\/p\u003e\n                \u003c\/div\u003e\n\n                \u003cdiv class=\"DAV-feature-box\"\u003e\n                    \u003ch3\u003e\n                        Sony Exmor Technology\n                    \u003c\/h3\u003e\n                    \u003cp\u003e\n                        Offers high-speed processing, low noise, and energy efficiency through column-parallel A\/D conversion.\n                    \u003c\/p\u003e\n                \u003c\/div\u003e\n\n                \u003cdiv class=\"DAV-feature-box\"\u003e\n                    \u003ch3\u003e\n                        Region of Interest (ROI) Mode\n                    \u003c\/h3\u003e\n                    \u003cp\u003e\n                        Enables higher frame rates with a fully customizable region of interest within the effective pixel array.\n                    \u003c\/p\u003e\n                \u003c\/div\u003e\n\n                \u003cdiv class=\"DAV-feature-box\"\u003e\n                    \u003ch3\u003e\n                        High-Speed Imaging\n                    \u003c\/h3\u003e\n                    \u003cp\u003e\n                        Achieves up to 164.5 fps at 10-bit ADC and 128.2 fps at 12-bit ADC for sharp, detailed images.\n                    \u003c\/p\u003e\n                \u003c\/div\u003e\n\n                \u003cdiv class=\"DAV-feature-box\"\u003e\n                    \u003ch3\u003e\n                        High Quantum Efficiency (QE)\n                    \u003c\/h3\u003e\n                    \u003cp\u003e\n                        Peak QE value estimated at 77%, providing an excellent signal-to-noise ratio for outstanding image quality.\n                    \u003c\/p\u003e\n                \u003c\/div\u003e\n\n                \u003cdiv class=\"DAV-feature-box\"\u003e\n                    \u003ch3\u003e\n                        USB 3.0 \u0026amp; ST4 Ports\n                    \u003c\/h3\u003e\n                    \u003cp\u003e\n                        USB 3.0 Port: Provides 5Gb bandwidth for fast data transfer, enabling smooth operation even at maximum frame rates and resolution.\n                    \u003c\/p\u003e\n                    \u003cp\u003e\n                        ST4 Port: Connects directly to your mount’s autoguide port for precise guiding during long exposure astrophotography.\n                    \u003c\/p\u003e\n                \u003c\/div\u003e\n\n                \u003cdiv class=\"DAV-feature-box\"\u003e\n                    \u003ch3\u003e\n                        Back Focus Flexibility \n                    \u003c\/h3\u003e\n                    \u003cp\u003e\n                        Remove the T2 11mm ring to achieve a compact back focus of just 6.5mm.\n                    \u003c\/p\u003e\n                \u003c\/div\u003e\n            \u003c\/div\u003e\n\n            \u003cdiv class=\"DAV-section-container\"\u003e\n                \u003cdiv class=\"DAV-section-text\"\u003e\n                    \u003ch3\u003e\n                        Setup Instructions\n                    \u003c\/h3\u003e\n                    \u003col\u003e\n                        \u003cli\u003e\n                            Connect the Camera: Use the USB 3.0 interface for high-speed, stable data transmission.\n                        \u003c\/li\u003e\n                        \u003cli\u003e\n                            Integrate with Mount: Utilize the ST4 port for seamless autoguiding during your imaging sessions.\n                        \u003c\/li\u003e\n                        \u003cli\u003e\n                            Optimize Imaging: Experiment with Region of Interest (ROI) mode to capture faster frame rates for specific celestial targets.\n                        \u003c\/li\u003e\n                        \u003cli\u003e\n                            Adjust Back Focus: For precise setups, remove the T2 ring to accommodate shorter optical paths.\n                        \u003c\/li\u003e\n                    \u003c\/ol\u003e\n                \u003c\/div\u003e\n            \u003c\/div\u003e\n\n            \u003cdiv class=\"DAV-section-container\"\u003e\n                \u003cdiv class=\"DAV-section-text\"\u003e\n                    \u003ch3\u003e\n                        Other information\n                    \u003c\/h3\u003e\n                    \u003cp\u003e\n                        The ZWO ASI174MM stands out due to its advanced global shutter design, eliminating focal plane distortions often seen in moving targets or unstable conditions. This makes it ideal for solar and lunar imaging, where fine details are crucial.                    \n                    \u003c\/p\u003e\n                    \u003cp\u003e\n                        With its high-speed imaging capability, ROI mode, and exceptional quantum efficiency, the ASI174MM ensures clear, sharp captures of faint deep-sky objects and bright planetary surfaces alike. The Pregius global shutter technology and Exmor architecture work together to reduce noise, enhance speed, and minimize power consumption, making this camera a favorite among serious astrophotographers.\n                    \u003c\/p\u003e\n                    \u003cp\u003e\n                        For those seeking high performance, versatility, and precision, the ZWO ASI174MM delivers a seamless astrophotography experience with professional-grade results.\n                    \u003c\/p\u003e\n                \u003c\/div\u003e\n            \u003c\/div\u003e\n        \u003c\/div\u003e\n    \u003c\/li\u003e\n\n\n    \u003cli\u003e\n        \u003ctable class=\"DAV-specifications\"\u003e\n            \u003ctbody\u003e\n                \u003ctr\u003e\n                    \u003ctd\u003e\n                        Sensor\n                    \u003c\/td\u003e\n                    \u003ctd\u003e\n                        CMOS IMX174\n                    \u003c\/td\u003e\n                \u003c\/tr\u003e\n                \u003ctr\u003e\n                    \u003ctd\u003e\n                        Read Noise\n                    \u003c\/td\u003e\n                    \u003ctd\u003e\n                        3.5e\n                    \u003c\/td\u003e\n                \u003c\/tr\u003e\n                \u003ctr\u003e\n                    \u003ctd\u003e\n                        Sensor Size\n                    \u003c\/td\u003e\n                    \u003ctd\u003e\n                        1\/1.2\" (11.3x7.1mm)\n                    \u003c\/td\u003e\n                \u003c\/tr\u003e\n                \u003ctr\u003e\n                    \u003ctd\u003e\n                        Full Well\n                    \u003c\/td\u003e\n                    \u003ctd\u003e\n                        32Ke\n                    \u003c\/td\u003e\n                \u003c\/tr\u003e\n                \u003ctr\u003e\n                    \u003ctd\u003e\n                        Resolution\n                    \u003c\/td\u003e\n                    \u003ctd\u003e\n                        1936x1216\n                    \u003c\/td\u003e\n                \u003c\/tr\u003e\n                \u003ctr\u003e\n                    \u003ctd\u003e\n                        QE\n                    \u003c\/td\u003e   \n                    \u003ctd\u003e\n                        77%\n                    \u003c\/td\u003e\n                \u003c\/tr\u003e\n                \u003ctr\u003e\n                    \u003ctd\u003e\n                        ADC\n                    \u003c\/td\u003e\n                    \u003ctd\u003e\n                        12bit\n                    \u003c\/td\u003e\n                \u003c\/tr\u003e\n                \u003ctr\u003e\n                    \u003ctd\u003e\n                        USB\n                    \u003c\/td\u003e\n                    \u003ctd\u003e\n                        3.0\n                    \u003c\/td\u003e\n                \u003c\/tr\u003e\n                \u003ctr\u003e\n                    \u003ctd\u003e\n                        Pixel Size\n                    \u003c\/td\u003e\n                    \u003ctd\u003e\n                        5.86um\n                    \u003c\/td\u003e\n                \u003c\/tr\u003e\n                \u003ctr\u003e\n                    \u003ctd\u003e\n                        FPS\n                    \u003c\/td\u003e\n                    \u003ctd\u003e\n                        164\n                    \u003c\/td\u003e\n                \u003c\/tr\u003e\n            \u003c\/tbody\u003e\n        \u003c\/table\u003e\n    \u003c\/li\u003e\n\n    \u003cli\u003e\n        \u003ch2\u003eAstrophotography Performance\u003c\/h2\u003e\n        \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_Performance.webp?v=1738097521\" alt=\"ASI174MM - Performance\"\u003e \n        \u003ch2\u003eMechanical Diagram\u003c\/h2\u003e\n        \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_Mechanical_Diagram.webp?v=1738097521\" alt=\"ASI174MM - Mechanical Diagram\"\u003e \n        \u003ch2\u003eHigh QE\u003c\/h2\u003e\n        \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_High_QE.webp?v=1738097521\" alt=\"\"\u003e\n        \u003ch2\u003eUSB\u003c\/h2\u003e\n        \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_USB.webp?v=1738097521\" alt=\"ASI174MM - USB\"\u003e \n        \u003ch2\u003eBack Focus\u003c\/h2\u003e\n        \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_Back_Focus.webp?v=1738097520\" alt=\"ASI174MM - Back Focus\"\u003e \n        \u003ch2\u003eReference Images\u003c\/h2\u003e\n        \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_Ref_1.webp?v=1738097520\" alt=\"ASI174MM - Ref 1\"\u003e \n        \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_Ref_2.webp?v=1738097521\" alt=\"ASI174MM - Ref 2\"\u003e \n        \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_Ref_3.webp?v=1738097520\" alt=\"ASI174MM - Ref 3\"\u003e \n        \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_Ref_4.webp?v=1738097521\" alt=\"ASI174MM - Ref 4\"\u003e \n        \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_Ref_5.webp?v=1738097521\" alt=\"ASI174MM - Ref 5\"\u003e \n        \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_Ref_6.webp?v=1738097521\" alt=\"ASI174MM - Ref 6\"\u003e\n    \u003c\/li\u003e\n\n    \u003cli\u003e\n        \u003cul class=\"DAV-grid\"\u003e\n            \u003cli class=\"DAV-grid-item\"\u003e\n                \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_Camera_Body.png?v=1738097521\" alt=\"ASI174MM - In The Box\" class=\"DAV-img-box\"\u003e\n                \u003cdiv\u003e\n                    \u003cp class=\"DAV-item-title\"\u003e\n                        Camera Body\n                    \u003c\/p\u003e\n                    \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n                \u003c\/div\u003e\n            \u003c\/li\u003e\n            \u003cli class=\"DAV-grid-item\"\u003e\n                \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_ST4.png?v=1738097521\" alt=\"ASI174MM - In The Box\" class=\"DAV-img-box\"\u003e\n                \u003cdiv\u003e\n                    \u003cp class=\"DAV-item-title\"\u003e\n                        ST4 Cable\n                    \u003c\/p\u003e\n                    \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n                \u003c\/div\u003e\n            \u003c\/li\u003e\n            \u003cli class=\"DAV-grid-item\"\u003e\n                \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_USB3.0.png?v=1738097521\" alt=\"ASI174MM - In The Box\" class=\"DAV-img-box\"\u003e\n                \u003cdiv\u003e\n                    \u003cp class=\"DAV-item-title\"\u003e\n                        USB 3.0 Cable (2m)\n                    \u003c\/p\u003e\n                    \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n                \u003c\/div\u003e\n            \u003c\/li\u003e\n            \u003cli class=\"DAV-grid-item\"\u003e\n                \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_Nosepiece.png?v=1738097521\" alt=\"ASI174MM - In The Box\" class=\"DAV-img-box\"\u003e\n                \u003cdiv\u003e\n                    \u003cp class=\"DAV-item-title\"\u003e\n                        1.25\" Nosepiece\n                    \u003c\/p\u003e\n                    \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n                \u003c\/div\u003e\n            \u003c\/li\u003e\n            \u003cli class=\"DAV-grid-item\"\u003e\n                \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_Cover.png?v=1738097520\" alt=\"ASI174MM - In The Box\" class=\"DAV-img-box\"\u003e\n                \u003cdiv\u003e\n                    \u003cp class=\"DAV-item-title\"\u003e\n                        1.25\" Cover\n                    \u003c\/p\u003e\n                    \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n                \u003c\/div\u003e\n            \u003c\/li\u003e\n            \u003cli class=\"DAV-grid-item\"\u003e\n                \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ASI174MM_-_Quick_Guide.png?v=1738097521\" alt=\"ASI174MM - In The Box\" class=\"DAV-img-box\"\u003e\n                \u003cdiv\u003e\n                    \u003cp class=\"DAV-item-title\"\u003e\n                        Quick Guide\n                    \u003c\/p\u003e\n                    \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n                \u003c\/div\u003e\n            \u003c\/li\u003e\n            \u003c!-- Add more items as needed --\u003e\n        \u003c\/ul\u003e\n    \u003c\/li\u003e\n\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":44967398768925,"sku":"ZWO-ASI174MM","price":699.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/ZWO-ASI174MM-Mono-1__46344.1596910049.1280.1280.jpg?v=1684341549"},{"product_id":"qhyccd-qhy5iii485c-color","title":"QHYCCD QHY5III485C Color","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e8.4 Megapixel Sony IMX485 Color BSI Sensor\u003c\/li\u003e\n\u003cli\u003eLarge 1\/1.2-inch Sensor Format\u003c\/li\u003e\n\u003cli\u003e2.9μm Pixel Size\u003c\/li\u003e\n\u003cli\u003e44 FPS at Full 3864x2180 Resolution\u003c\/li\u003e\n\u003cli\u003e128MB DDR II Image Buffer\u003c\/li\u003e\n\u003cli\u003eExtremely Low 0.77e- Read Noise\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eQHYCCD QHY5III485C Color Planetary \u0026amp; Guide Camera\u003c\/h2\u003e\n\u003cp\u003eThe QHYCCD QHY5III485C leverages the large 1\/1.2-inch Sony IMX485 back-illuminated sensor to deliver an expansive field of view for planetary and lunar imaging. Its 8.4 Megapixel resolution and 2.9μm pixels capture fine detail, while the camera's architecture achieves an impressively low read noise of 0.77e-. With a full-frame capture rate of 44 FPS and a 128MB DDR II buffer, the QHY5III485C ensures smooth, drop-free video streams essential for high-resolution lucky imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eThe 8.4MP Sony IMX485 Sensor: High-Resolution Lunar and Planetary Imaging\u003c\/h3\u003e\n\u003cp\u003eAt the heart of the QHY5III485C is Sony's IMX485, a large-format color CMOS sensor with a 3864x2180 pixel array. This 1\/1.2-inch sensor provides a significantly wider field of view than typical planetary cameras, allowing you to capture the entire lunar disc with shorter focal length instruments or fit Jupiter and its Galilean moons in a single frame. The 2.9μm pixels offer excellent resolution for a wide range of telescope focal ratios.\u003c\/p\u003e\n\u003cp\u003eThe sensor's back-illuminated (BSI) design and extremely low read noise, as low as 0.77e-, maximize sensitivity to faint planetary details like subtle Martian albedo features or delicate structures in Jupiter's cloud bands. A full well capacity of 12ke- provides ample dynamic range to prevent bright regions from saturating while capturing faint adjacent details.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e44 FPS Capture with a 128MB DDR Buffer for Flawless Lucky Imaging\u003c\/h3\u003e\n\u003cp\u003eSuccessful planetary imaging depends on freezing moments of atmospheric stability, a technique known as \"lucky imaging,\" which requires high frame rates. The QHY5III485C captures full 8.4-megapixel frames at 44 FPS over its USB 3.0 interface. For smaller targets, Region of Interest (ROI) speeds increase dramatically, reaching up to 190 FPS for a 480-line window.\u003c\/p\u003e\n\u003cp\u003eTo guarantee stable data transfer without dropped frames—a common issue that can ruin an imaging run—QHY includes a 128MB DDR II memory buffer. This onboard buffer ensures a consistent data stream to your computer, even if the system is momentarily busy with other tasks, resulting in smooth and complete video files every time.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eFlexible Connectivity: 12mm Back Focus, C\/CS Mounts, and ST-4 Guiding\u003c\/h3\u003e\n\u003cp\u003eThe QHY5III485C is designed for broad compatibility with your existing equipment. It fits standard 1.25-inch focusers and accessories, and also includes C-mount and CS-mount threads for direct attachment to lenses or specialized optical systems. The fixed 12mm back focal length provides a known, repeatable distance for integrating accessories like filter drawers.\u003c\/p\u003e\n\u003cp\u003eBeyond its primary role as a planetary imager, the camera includes a custom ST-4 guide port. This dual-purpose design allows you to use the QHY5III485C's high sensitivity and low noise as a premium autoguider for long-exposure deep-sky astrophotography, making it a valuable tool for multiple imaging disciplines.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eQHY5III485C vs. ZWO ASI485MC: A Head-to-Head Comparison\u003c\/h3\u003e\n\u003cp\u003eBoth the QHY5III485C and ZWO ASI485MC are built around the excellent Sony IMX485 sensor, offering nearly identical imaging potential in terms of resolution, pixel size, and sensitivity. The decision between them often comes down to specific system requirements and hardware features.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eBack Focus:\u003c\/strong\u003e The ZWO ASI485MC offers dual back focus options of 6.5mm and 17.5mm, providing more flexibility for complex imaging trains. The QHY5III485C has a fixed back focus of 12mm, offering simplicity and repeatability.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eImage Buffer:\u003c\/strong\u003e The QHY5III485C includes a 128MB DDR II buffer. The ZWO ASI485MC typically features a larger 512MB DDR3 buffer, which may offer an advantage on systems with very high USB bus traffic.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eSoftware Ecosystem:\u003c\/strong\u003e Your choice may depend on your preferred capture software. Both cameras are supported by major third-party applications like FireCapture and SharpCap, but each manufacturer also offers its own native software suite.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat makes the QHY5III485C a good choice for planetary imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe QHY5III485C combines a high-resolution \u003cstrong\u003e8.4 Megapixel\u003c\/strong\u003e sensor with a fast \u003cstrong\u003e44 FPS\u003c\/strong\u003e frame rate and a large \u003cstrong\u003e1\/1.2-inch format\u003c\/strong\u003e. This combination allows you to capture incredibly detailed, wide-field views of targets like Jupiter and the Moon, while the high speed is critical for \"lucky imaging\" to overcome atmospheric turbulence.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow will the QHY5III485C's 1\/1.2-inch sensor help when imaging the Moon with an 8\" SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWith a typical 8\" f\/10 SCT, the QHY5III485C's large sensor can capture a much larger portion of the lunar surface in a single frame compared to smaller-chip cameras. This means you can create a full mosaic of the Moon with significantly fewer panels to capture and stitch together, saving you time both at the telescope and during processing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the purpose of the 128MB DDR buffer in the QHY5III485C?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e128MB DDR II buffer\u003c\/strong\u003e is onboard memory that temporarily stores image frames before they are sent to the computer via USB 3.0. This prevents frames from being lost if your computer's USB bus or hard drive is temporarily busy. It ensures a smooth, stable video stream, which is essential for capturing high-quality data without gaps.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the QHY5III485C to guide my telescope for deep-sky imaging of the Andromeda Galaxy (M31)?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. The QHY5III485C is equipped with a custom \u003cstrong\u003eST-4 guide port\u003c\/strong\u003e. Its high sensitivity and low read noise make it an excellent autoguider. You can connect it to your mount via the guide port and use software like PHD2 to achieve precise tracking for long-exposure images of faint targets like M31.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat do the C-mount and CS-mount options on the QHY5III485C allow me to do?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe C and CS-mount threads allow you to connect the QHY5III485C directly to C\/CS-mount lenses, which are common in machine vision and security. This is useful for all-sky imaging, meteor capture, or wide-field video astronomy without a telescope. The \u003cstrong\u003e12mm back focus\u003c\/strong\u003e is designed to be compatible with these standards.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the QHY5III485C suitable for long-exposure deep-sky imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWhile it can take exposures up to 900 seconds, the QHY5III485C is an \u003cstrong\u003euncooled\u003c\/strong\u003e camera. On long exposures, thermal noise will build up and can overwhelm faint signals from nebulae and galaxies. It is primarily designed for high-frame-rate, short-exposure imaging of bright solar system objects.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSony IMX485 Color BSI CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003e1\/1.2 inch\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eEffective Pixels\u003c\/td\u003e\n\u003ctd\u003e8.4 Megapixels (3864 x 2180)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9μm x 2.9μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e12,000e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e0.77e- to 2.4e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit (output as 16-bit and 8-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e128MB DDR II Memory\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate (Full)\u003c\/td\u003e\n\u003ctd\u003e44 FPS @ 8-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eROI Frame Rates\u003c\/td\u003e\n\u003ctd\u003eUp to 190 FPS @ 480 lines\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Time Range\u003c\/td\u003e\n\u003ctd\u003e11μs - 900s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eComputer Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 Type-B\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eCustom ST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd\u003e1.25-inch, CS-Mount, C-Mount\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOptical Window\u003c\/td\u003e\n\u003ctd\u003eIR-Cut Filter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e90g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.qhyccd.com\/download\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/qhyccd-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eQHYCCD Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"QHYCCD","offers":[{"title":"Default Title","offer_id":44967911129373,"sku":"QHY-110085","price":503.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/QHY5III485C-Camera__62438.1624386813.1280.1280.jpg?v=1684346903"},{"product_id":"zwo-asi482mc-color","title":"ZWO ASI482MC Color","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003eSony IMX482 1\/1.2” CMOS Color Sensor\u003c\/li\u003e\n\u003cli\u003e1920x1080 Resolution at up to 82.5 FPS\u003c\/li\u003e\n\u003cli\u003eLarge 5.8µm Pixels for High Sensitivity\u003c\/li\u003e\n\u003cli\u003e51,500e Full Well Capacity\u003c\/li\u003e\n\u003cli\u003eUltra-Low 1.5e Read Noise\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI482MC Color CMOS Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI482MC combines a high-sensitivity 1920x1080 Sony IMX482 sensor with massive 5.8µm pixels to deliver exceptional performance on planetary, lunar, and solar targets. Its remarkable 51,500e full well capacity prevents overexposure on bright subjects like Jupiter's core, while an ultra-low read noise of 1.5e and peak QE of 85% ensure faint details are captured cleanly. This camera captures full-resolution frames at up to 82.5 FPS, giving you the speed needed to freeze moments of steady seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eHigh Sensitivity from 5.8µm Pixels\u003c\/h3\u003e\n\u003cp\u003eThe core strength of the ASI482MC lies in its large 5.8µm pixels. This generous pixel size provides a significant light-gathering advantage over smaller-pixel planetary cameras, resulting in a higher signal-to-noise ratio in shorter exposures. This makes the ASI482MC particularly effective for capturing detail on dimmer planets like Saturn and Mars, and it excels in \"lucky imaging\" of brighter deep-sky objects where short exposures are stacked to overcome atmospheric turbulence.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e51.5k Full Well \u0026amp; 12-bit ADC\u003c\/h3\u003e\n\u003cp\u003eUnlike many planetary cameras that struggle with bright targets, the ASI482MC features an enormous 51,500e full well capacity. This prevents bright regions, such as Jupiter's Galilean moons or lunar highlands, from saturating, preserving detail and color gradation across the entire target. Combined with its 12-bit ADC, the camera renders smooth, artifact-free images with a wide dynamic range, capturing subtle tonal variations in planetary cloud bands and solar granulation.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eHCG Mode:\u003c\/strong\u003e At a gain setting of 80 and above, High Conversion Gain mode automatically activates. This drastically reduces read noise to as low as 1.5e while preserving the camera's wide dynamic range, perfect for low-light imaging.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eHigh Frame Rates:\u003c\/strong\u003e The USB 3.0 interface provides enough bandwidth to run the ASI482MC at 57.5 fps at full 1920x1080 resolution with 12-bit depth, or 82.5 fps using the 10-bit high-speed mode.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eIdeal for EAA and Long Focal Lengths\u003c\/h3\u003e\n\u003cp\u003eThe ASI482MC's high sensitivity and large sensor make it an excellent choice for Electronically Assisted Astronomy (EAA). You can achieve near-real-time views of brighter galaxies and nebulae by live-stacking short exposures. Its 5.8µm pixels are also an ideal match for long focal length telescopes like Schmidt-Cassegrains and Maksutovs, providing an optimal image scale for high-resolution planetary imaging without requiring excessive Barlow magnification.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eConnectivity \u0026amp; Mechanical Design\u003c\/h3\u003e\n\u003cp\u003eThe ASI482MC is built for reliability and ease of use in any imaging setup. The high-speed USB 3.0 port ensures fast data transfer, while the ST4 port allows the camera to double as a high-performance autoguider for a deep-sky imaging rig. The camera body includes a standard 1.25\" nosepiece for direct connection to focusers and accessories, and features an AR-coated window to protect the sensor and maximize light transmission.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the ZWO ASI482MC better for planetary or deep-sky imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ZWO ASI482MC is primarily a high-performance planetary, lunar, and solar camera. Its strengths, high frame rate, large pixels, and massive full well capacity, are optimized for capturing bright, high-magnification targets. However, its exceptional sensitivity also makes it very capable for \"lucky imaging\" of brighter deep-sky objects like globular clusters (M13) and planetary nebulae (M57), as well as for Electronically Assisted Astronomy (EAA).\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the ASI482MC perform on Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ASI482MC is an excellent match for an 8\" f\/10 SCT. The 5.8µm pixels produce a good image scale at the native f\/10 focal length. For optimal planetary imaging, which targets a focal ratio between f\/15 and f\/21 with this pixel size, you would use a 1.5x or 2x Barlow lens. This combination will provide high-resolution views of Jupiter's Great Red Spot and cloud bands, while the camera's high frame rate helps freeze moments of good seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is HCG (High Conversion Gain) mode on the ASI482MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eHCG mode is a feature that automatically activates when you set the camera's gain to 80 or higher. It changes how the sensor converts light into a signal, drastically reducing read noise to as low as 1.5 electrons. This allows you to use high gain settings to capture fainter details without introducing significant noise, all while maintaining a wide dynamic range.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDo I need an IR Cut filter with the ZWO ASI482MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, for the most accurate color balance, an IR Cut filter is recommended. The ASI482MC has high sensitivity into the infrared spectrum. While its protective window is AR-coated, it does not block IR light. An IR Cut filter will ensure that only visible light reaches the sensor, resulting in sharper images and more natural colors, which is especially important for planetary imaging with refractor or SCT telescopes.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the ASI482MC as a guide camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. The ZWO ASI482MC includes a standard ST4 guide port and has the sensitivity needed to be a very effective autoguider. Its large pixels can detect guide stars easily, making it a versatile tool for both planetary imaging and guiding a separate deep-sky astrophotography setup.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does the 51,500e full well capacity mean in practice?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe 51,500e full well capacity means each of the camera's 5.8µm pixels can hold a large amount of charge before becoming saturated (turning pure white). This is a significant advantage when imaging targets with a high dynamic range, like the Moon or Jupiter. It allows you to use longer exposures to capture faint details, like wispy lunar rays, without blowing out the highlights on the brighter surfaces.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/1.2\" Sony IMX482 CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e1920 x 1080 (2.07 MP)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e5.8µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Dimensions\u003c\/td\u003e\n\u003ctd\u003e11.13mm x 6.26mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e12.86mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e82.5 fps (10-bit) \/ 57.5 fps (12-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e51,500e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e1.5e to 12.9e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQuantum Efficiency (Peak)\u003c\/td\u003e\n\u003ctd\u003e85% at 530nm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter\u003c\/td\u003e\n\u003ctd\u003eRolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e6.5mm \/ 17.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eAR Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eASI482MC Camera Body\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e2-meter USB 3.0 Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eST4 Autoguider Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Dust Cap\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e2\" Dust Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eQuick Start Guide\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":44967948812573,"sku":"ZWO-ASI482MC","price":416.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/ZWO-ASI482MC-1__37611.1638989292.1280.1280.jpg?v=1684347230"},{"product_id":"zwo-asi662mc-color","title":"ZWO ASI662MC Color","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e2.1 Megapixel Sony IMX662 BSI Sensor\u003c\/li\u003e\n\u003cli\u003e1920 x 1080 Resolution with 2.9µm Pixels\u003c\/li\u003e\n\u003cli\u003e91% Peak Quantum Efficiency\u003c\/li\u003e\n\u003cli\u003eUltra-Low 0.8e Read Noise\u003c\/li\u003e\n\u003cli\u003e107.6 FPS at Full Resolution\u003c\/li\u003e\n\u003cli\u003eZero Amplifier Glow Circuitry\u003c\/li\u003e\n\u003cli\u003e256MB DDR3 Internal Buffer\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI662MC USB3.0 Color Astronomy Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI662MC combines a 2.1 MP Sony IMX662 back-illuminated sensor with 2.9µm pixels to resolve fine detail on planetary targets. Its exceptional 91% peak quantum efficiency and ultra-low 0.8e read noise capture faint atmospheric features, while the deep 38.2ke full well prevents bright planetary cores from saturating. A 256MB DDR3 buffer sustains a capture rate of 107.6 FPS over USB 3.0, ensuring no dropped frames during critical moments of stable seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony STARVIS 2 Sensor with 91% Peak QE\u003c\/h3\u003e\n\u003cp\u003eAt the core of the ASI662MC is Sony's latest STARVIS 2 sensor technology, which delivers a peak quantum efficiency of 91% and heightened sensitivity in near-infrared wavelengths. This back-illuminated structure maximizes photon collection for a stronger signal. The sensor's 38.2ke full well capacity is a significant advantage for planetary imaging, allowing you to use longer exposures on targets like Jupiter and Saturn without blowing out highlights, retaining color data and detail in the brightest regions.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eZero Amp Glow \u0026amp; 0.8e Read Noise for Cleaner Data\u003c\/h3\u003e\n\u003cp\u003eThe ASI662MC integrates circuitry that completely eliminates amplifier glow, a common source of noise in CMOS sensors. This means your raw video files are free of glow from the start, simplifying your calibration and processing. Combined with a read noise of just 0.8e, the camera preserves faint, low-contrast details like Martian dust storms or subtle banding on Saturn, even with the very short exposures used in lucky imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eASI662MC vs. ASI462MC: A Generational Leap\u003c\/h3\u003e\n\u003cp\u003eWhile the preceding ASI462MC was renowned for its high infrared sensitivity, the ASI662MC marks a major upgrade in core imaging fundamentals. The most critical improvement is in dynamic range, driven by a much deeper full well and lower noise.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eFull Well Capacity:\u003c\/strong\u003e The ASI662MC has a full well of 38.2ke, more than three times deeper than the ASI462MC's 11.2ke. This dramatically reduces the risk of overexposing bright targets and provides smoother tonal gradations.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eAmplifier Glow:\u003c\/strong\u003e The ASI662MC features a true zero-amp-glow design, a significant advantage over the ASI462MC which exhibited some glow that required calibration frames to remove.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eRead Noise:\u003c\/strong\u003e With read noise as low as 0.8e, the ASI662MC captures cleaner data with a better signal-to-noise ratio, making it easier to pull out fine details during processing.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e107.6 FPS Capture with a 256MB DDR3 Buffer\u003c\/h3\u003e\n\u003cp\u003eTo freeze moments of perfect atmospheric seeing, high-speed capture is essential. The ASI662MC streams full-resolution 1920x1080 video at 107.6 frames per second. The onboard 256MB DDR3 memory buffer ensures stable data transfer to your computer over USB 3.0, preventing dropped frames that can compromise your data set. Standard connectivity, including an ST-4 guide port and M42 threads, allows the camera to integrate easily into any imaging train.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the ZWO ASI662MC perform on Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ZWO ASI662MC is an excellent match for an 8\" f\/10 SCT. To achieve the ideal image scale for its 2.9µm pixels, you should target a final focal ratio between f\/15 and f\/21. This is perfectly accomplished by adding a 1.5x or 2x Barlow lens to your f\/10 optical train, which will allow you to resolve fine details like the Great Red Spot and intricate cloud bands.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the ZWO ASI662MC for imaging the Orion Nebula (M42)?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, but with limitations. The ASI662MC's high sensitivity makes it suitable for electronically-assisted astronomy (EAA) or short exposures on bright deep-sky objects like the Orion Nebula (M42) or the Hercules Cluster (M13). However, as an uncooled camera, thermal noise will become apparent on exposures longer than a few seconds. Its small 1\/2.8\" sensor also provides a very narrow field of view, making it better for smaller galaxies and planetary nebulae than large, extended targets.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the main advantage of the ASI662MC over the older ASI462MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe primary advantage is its significantly larger \u003cstrong\u003e38.2ke full well capacity\u003c\/strong\u003e, which is more than three times that of the ASI462MC. This provides greater dynamic range, preventing overexposure on bright planets and moons. A second key benefit is the \u003cstrong\u003ezero amplifier glow circuitry\u003c\/strong\u003e, which produces cleaner raw data that is easier to calibrate.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does 'Zero Amp Glow' on the ASI662MC mean for my workflow?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eZero amp glow means the camera's circuitry prevents the sensor from producing a bright, noisy pattern on the edge of the frame during operation. For planetary imaging with its short exposures, this simplifies your workflow: there is no glow pattern to remove, so calibration is easier and faster, saving you time both at the telescope and during processing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDo I need a USB 3.0 port to use the ZWO ASI662MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWhile the camera is backward-compatible with USB 2.0, a USB 3.0 port is highly recommended to take full advantage of its capabilities. Using USB 3.0 is necessary to achieve the maximum frame rate of 107.6 FPS. On a USB 2.0 connection, frame rates will be significantly lower, which limits your ability to capture enough frames during moments of good seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the ZWO ASI662MC a good choice for a beginner in planetary imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, it's an excellent choice. Its high sensitivity, low read noise, and zero amp glow make it very forgiving for a beginner. You can achieve high-quality results with a simplified workflow, allowing you to focus on capture techniques rather than complex calibration procedures.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/2.8\" Sony IMX662 CMOS (Color)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eIllumination\u003c\/td\u003e\n\u003ctd\u003eBSI (Back-Illuminated)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e1920 x 1080 (2.1 MP)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Dimensions\u003c\/td\u003e\n\u003ctd\u003e5.6mm x 3.1mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e6.45mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQuantum Efficiency (Peak)\u003c\/td\u003e\n\u003ctd\u003e91%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e38.2ke-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e0.8e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAmp Glow Control\u003c\/td\u003e\n\u003ctd\u003eZero Amplifier Glow\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e107.6 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBit Depth\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBuffer\u003c\/td\u003e\n\u003ctd\u003e256MB DDR3\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32µs to 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eROI Support\u003c\/td\u003e\n\u003ctd\u003eYes\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCooling\u003c\/td\u003e\n\u003ctd\u003eUncooled\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eComputer Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Connection\u003c\/td\u003e\n\u003ctd\u003eM42x0.75 Thread, 1.25\" Nosepiece\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Window\u003c\/td\u003e\n\u003ctd\u003eAR Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOperating Temperature\u003c\/td\u003e\n\u003ctd\u003e-5°C to 50°C\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eStorage Temperature\u003c\/td\u003e\n\u003ctd\u003e-10°C to 60°C\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOperating Humidity\u003c\/td\u003e\n\u003ctd\u003e20% to 80%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e0.28 lbs\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOS Compatibility\u003c\/td\u003e\n\u003ctd\u003eWindows, Mac, Linux\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eZWO ASI662MC Camera Body\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eUSB 3.0 Cable (2m)\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eST-4 Autoguider Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eQuick Start Guide\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":44968015954205,"sku":"ZWO-ASI662MC","price":279.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/ZWO-ASI662MC-1__75835.1656258904.1280.1280.jpg?v=1684347901"},{"product_id":"zwo-asi678mc-color","title":"ZWO ASI678MC Color","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e8.29 Megapixel Sony IMX678 Color Sensor\u003c\/li\u003e\n\u003cli\u003e2.0µm pixels for high-resolution planetary imaging\u003c\/li\u003e\n\u003cli\u003e47.5 FPS at full 3840x2160 resolution\u003c\/li\u003e\n\u003cli\u003eZero amp glow for clean, long exposures\u003c\/li\u003e\n\u003cli\u003e256MB DDR3 buffer for stable, high-speed data transfer\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI678MC Color CMOS Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI678MC leverages Sony's latest STARVIS 2 technology to deliver exceptional planetary, lunar, and solar detail. Its 8.29 MP IMX678 sensor, with small 2.0µm pixels, achieves high-resolution captures at a rapid 47.5 FPS, while the 12bit ADC and extremely low 0.6e read noise ensure a high dynamic range. A peak Quantum Efficiency of 83% and zero amp glow circuitry combine to produce clean, high-contrast images, even on faint targets or during longer exposures.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony IMX678 Sensor with 2.0µm Pixels\u003c\/h3\u003e\n\u003cp\u003eAt the core of the ASI678MC is a 1\/1.8\" format Sony IMX678 sensor, which provides a 3840x2160 resolution ideal for capturing fine surface details on Jupiter, Saturn's rings, and lunar craters. The small 2.0µm pixel size is a critical factor for achieving optimal sampling on long focal length telescopes, allowing you to resolve intricate features without excessive use of Barlow lenses. This back-illuminated sensor architecture also provides outstanding sensitivity, especially in the near-infrared, giving you a distinct advantage when imaging planets with methane band or IR-pass filters.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eZero Amp Glow \u0026amp; 47.5 FPS Capture Rate\u003c\/h3\u003e\n\u003cp\u003eA standout feature implemented at the hardware level, the ASI678MC exhibits absolutely zero amplifier glow, regardless of exposure length or gain settings. This guarantees clean calibration and removes a major source of noise from your final images, a significant upgrade over previous generation sensors. The camera sustains a maximum frame rate of 47.5 FPS at its full 8.29 MP resolution, enabled by a high-speed USB 3.0 interface and a 256MB DDR3 buffer that prevents dropped frames during critical moments of steady seeing.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eNo Amp Glow:\u003c\/strong\u003e Cleaner dark frames and less post-processing complexity, even with higher gain settings.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003e256MB DDR3 Buffer:\u003c\/strong\u003e Ensures stable, high-speed data transmission to your computer, eliminating frame drops during capture sessions.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eHigh Conversion Gain (HCG) Mode:\u003c\/strong\u003e Automatically activates at gain 182 to reduce read noise to about 1.0e, preserving dynamic range at high gain.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eZWO ASI678MC vs. ASI585MC\u003c\/h3\u003e\n\u003cp\u003eWhile both cameras share the same 4K resolution, the ASI678MC and ASI585MC are optimized for different primary use cases. The choice depends on your telescope and primary imaging targets.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eASI585MC Advantage:\u003c\/strong\u003e The ASI585MC has a larger sensor and bigger 2.9µm pixels, giving it a significantly larger field of view and a deeper full well capacity (40ke vs 11.27ke). This makes it more versatile for capturing not just planets, but also brighter deep-sky objects like the Orion Nebula (M42).\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eASI678MC Advantage:\u003c\/strong\u003e The ASI678MC's smaller sensor and 2.0µm pixels provide a more magnified image scale, which is ideal for framing planets without needing aggressive barlowing. This makes it a more specialized and efficient tool for high-resolution planetary, lunar, and solar imaging.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eConnectivity and Build\u003c\/h3\u003e\n\u003cp\u003eThe ASI678MC is housed in a compact, lightweight body weighing only 126g. It features a standard M42x0.75 female thread for connection to your telescope, with a 1.25\" nosepiece included for use with standard focusers. The camera provides both a high-speed USB 3.0 port for data transfer and an ST-4 guide port, allowing it to double as a highly sensitive autoguider when not being used for primary imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the ZWO ASI678MC good for deep-sky objects?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWhile the ZWO ASI678MC can capture brighter deep-sky objects like the Orion Nebula (M42) or the Hercules Cluster (M13), its primary design is for high-frame-rate planetary, lunar, and solar imaging. Its small pixels and sensor size are optimized for high magnification. For a more versatile camera better suited for a wider range of DSOs, consider the ZWO ASI585MC with its larger sensor and deeper full well capacity.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat focal ratio is best for the ASI678MC's 2.0µm pixels?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor optimal planetary imaging, a good target focal ratio is 5 to 7 times the pixel size. For the ASI678MC's 2.0µm pixels, this means an ideal focal ratio is between f\/10 and f\/14. If you have an f\/5 Newtonian, a 2x or 2.5x Barlow lens would place you in the ideal range. For an f\/10 SCT, you can often image directly without a Barlow, or use a 1.5x Barlow in very good seeing conditions.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the ASI678MC require dark frames?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThanks to its hardware-level \u003cstrong\u003ezero amp glow\u003c\/strong\u003e design, the need for dark frames is significantly reduced, especially for short-exposure planetary imaging. However, for longer exposures on brighter deep-sky objects, taking dark frames is still a best practice to remove warm pixels and minimize dark current noise for the cleanest possible image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the difference between the ZWO ASI678MC and the older ASI178MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ZWO ASI678MC is a direct upgrade to the ASI178MC. The key improvements are:\n\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eZero Amp Glow:\u003c\/strong\u003e The ASI678MC has no amp glow, a significant improvement over the ASI178MC.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eLower Read Noise:\u003c\/strong\u003e It features a lower minimum read noise (0.6e vs. 1.4e), resulting in cleaner images at high gain.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eSTARVIS 2 Technology:\u003c\/strong\u003e The newer sensor has enhanced sensitivity, particularly in near-infrared light.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the ZWO ASI678MC as a guide camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. The ZWO ASI678MC is equipped with an ST-4 guide port and its high sensitivity makes it an excellent autoguiding camera. Its small pixels can detect minute star movements, leading to very precise guiding corrections.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat do I need to use the ASI678MC for solar imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eTo safely image the Sun with the ZWO ASI678MC, you MUST use a certified, full-aperture solar filter over the front of your telescope. Never point your telescope at the Sun without a proper filter, as it will cause immediate and permanent damage to the camera sensor and your eyes.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/1.8” CMOS Sony IMX678\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e8.29 MP (3840 x 2160)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.0µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Depth\u003c\/td\u003e\n\u003ctd\u003e11.27ke\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e47.5 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32µs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e0.6e - 2.7e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQuantum Efficiency (Peak)\u003c\/td\u003e\n\u003ctd\u003e≈83%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e256MB DDR3 Memory\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eAR Coated (D21-1)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDimensions\u003c\/td\u003e\n\u003ctd\u003e62mm Diameter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e126g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOperating Temperature\u003c\/td\u003e\n\u003ctd\u003e-5°C to 50°C\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eASI678MC Camera Body\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Dust Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e2m USB 3.0 Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eST4 Guide Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eQuick Start Guide\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":44968019296541,"sku":"ZWO-ASI678MC","price":419.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/ZWO-ASI678MC-1__89087.1656259708.1280.1280.jpg?v=1684347935"},{"product_id":"zwo-asi585mc-color","title":"ZWO ASI585MC Color","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e8.29 Megapixel 4K Resolution (3840 x 2160)\u003c\/li\u003e\n\u003cli\u003e2.9µm Square Pixels\u003c\/li\u003e\n\u003cli\u003e91% Peak Quantum Efficiency\u003c\/li\u003e\n\u003cli\u003e46.9 FPS at Full Resolution\u003c\/li\u003e\n\u003cli\u003eZero Amplifier Glow Circuitry\u003c\/li\u003e\n\u003cli\u003e256MB DDR3 Internal Buffer\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI585MC USB 3.0 Color CMOS Astronomy Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI585MC captures full 4K planetary video using its 8.29 MP Sony IMX585 sensor, with 2.9µm pixels resolving fine detail on Jupiter's cloud bands and Saturn's rings. A peak Quantum Efficiency of 91% and exceptionally low 0.7e read noise pull faint signals out of the background, while the 256MB DDR3 buffer sustains a full-resolution frame rate of 46.9 FPS over USB 3.0 without dropping frames.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e4K Planetary Imaging at 46.9 FPS\u003c\/h3\u003e\n\u003cp\u003eThe ASI585MC's native 3840 x 2160 resolution is ideal for capturing the entire disk of Jupiter or the Moon in a single frame, eliminating the need for mosaics. The high 46.9 FPS frame rate allows you to collect thousands of frames in minutes, letting software stack the sharpest data from moments of steady seeing. This high-speed capture is stabilized by the onboard 256MB DDR3 memory buffer, preventing data loss during transfer to your computer.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e91% QE and 40ke Full Well for Deep-Sky Imaging\u003c\/h3\u003e\n\u003cp\u003eWith a peak QE of 91% and a deep 40ke full well capacity, the back-illuminated IMX585 sensor gathers photons with extreme efficiency and offers significant dynamic range. This combination is critical for \"lucky imaging\" of brighter deep-sky objects like the Orion Nebula (M42) or the Hercules Cluster (M13). You can use short exposures to freeze atmospheric turbulence while still capturing both faint nebulosity and the bright stellar cores without saturation.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eASI585MC vs. ASI485MC: Key Upgrades\u003c\/h3\u003e\n\u003cp\u003eThe ASI585MC is a direct successor to the popular ASI485MC, incorporating two critical improvements for astrophotography. While the ASI485MC has a limited full well depth and exhibits amp glow on longer exposures, the ASI585MC addresses both limitations directly.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eFull Well Capacity (40ke):\u003c\/strong\u003e The ASI585MC's full well is over three times deeper than the ASI485MC's. This provides substantially greater dynamic range, preventing bright stars from saturating in deep-sky images and capturing more subtle color variations on planets.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eZero Amp Glow:\u003c\/strong\u003e ZWO integrated a hardware-level circuit that completely eliminates amplifier glow, a common source of noise in uncooled cameras during long exposures. This makes dark frame calibration simpler and far more effective.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eZero Amp Glow on an Uncooled Sensor\u003c\/h3\u003e\n\u003cp\u003eAmplifier glow is a faint infrared light source on the sensor itself that can contaminate long exposures. The ASI585MC's Zero Amp Glow circuit prevents this entirely, regardless of exposure length or gain setting. As an uncooled camera, it is still subject to thermal noise on multi-minute exposures of faint targets. However, the absence of amp glow means your dark frames only need to subtract this predictable thermal signal, resulting in cleaner, easier-to-process images.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eFlexible Connectivity with 6.5mm \/ 17.5mm Back Focus\u003c\/h3\u003e\n\u003cp\u003eThe ASI585MC provides two native back focus distances to accommodate different imaging trains. The standard 17.5mm distance is used when placing accessories like a filter wheel or off-axis guider in front of the camera. For setups without these accessories, a 6.5mm distance allows for a more direct connection, which can be critical when working with certain focal reducers or lens adapters.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eTelescope Interface:\u003c\/strong\u003e M42x0.75 female threads.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eIncluded Adapters:\u003c\/strong\u003e A 1.25\" nosepiece allows direct insertion into standard focusers.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eData and Guiding:\u003c\/strong\u003e A USB 3.0 port handles high-speed image transfer, while a dedicated ST-4 port connects to your mount for autoguiding.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat makes the ZWO ASI585MC a strong choice for planetary imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ASI585MC combines three key specifications for high-resolution planetary work: \u003cstrong\u003e4K resolution (3840x2160)\u003c\/strong\u003e to capture the entire planetary disk, small \u003cstrong\u003e2.9µm pixels\u003c\/strong\u003e to resolve fine detail at the correct focal ratio, and a high frame rate of \u003cstrong\u003e46.9 FPS\u003c\/strong\u003e to gather thousands of frames quickly, maximizing your chances of capturing moments of perfect seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the ASI585MC perform on Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThis is an excellent pairing. For the ASI585MC's 2.9µm pixels, the ideal focal ratio for planetary imaging is between f\/14.5 and f\/20. With an f\/10 SCT, using a 1.5x or 2x Barlow lens will place your system in this optimal range, allowing the camera's small pixels to resolve the finest details in Jupiter's cloud bands that your telescope and local seeing conditions can deliver.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the ZWO ASI585MC for deep-sky astrophotography?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, the ASI585MC is very capable for Electronically-Assisted Astronomy (EAA) and \"lucky imaging\" of brighter deep-sky objects. Its high sensitivity and zero amp glow make it a great choice for capturing targets like the Orion Nebula (M42), the Hercules Cluster (M13), or the Ring Nebula (M57) using stacks of short exposures. As an uncooled camera, it is less suited for very long exposures (5+ minutes) on faint nebulae where a cooled camera would be necessary to control thermal noise.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the main advantage of the ASI585MC over the older ASI485MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe two biggest advantages are its \u003cstrong\u003e40ke full well capacity\u003c\/strong\u003e (more than 3x deeper than the ASI485MC) for greater dynamic range, and its \u003cstrong\u003eZero Amp Glow\u003c\/strong\u003e circuit. The lack of amp glow makes dark frame calibration much easier and more effective, especially for deep-sky lucky imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the ASI585MC's 'Zero Amp Glow' mean I don't need dark frames?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eNo, you still need to take dark frames. The Zero Amp Glow feature eliminates the sensor's own light pollution, but it does not eliminate thermal noise (dark current) that accumulates during an exposure. Dark frames are still essential for calibrating out this thermal signal, but they work much better because they don't also have to subtract a complex, temperature-sensitive glow pattern.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat do the 6.5mm and 17.5mm back focus options on the ASI585MC let me do?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThese two options provide flexibility for building your imaging train.\n\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003e17.5mm:\u003c\/strong\u003e This is the standard back focus for use with accessories like a filter wheel or off-axis guider that require a specific amount of spacing.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003e6.5mm:\u003c\/strong\u003e This shorter distance is useful for direct connections to focal reducers, correctors, or camera lenses that require the sensor to be closer to the optics.\u003c\/li\u003e\n\u003c\/ul\u003e\nYou select the appropriate distance based on which components are in your optical path.\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/1.2\" Sony IMX585 BSI CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e3840 x 2160 (8.29 MP)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Dimensions\u003c\/td\u003e\n\u003ctd\u003e11.2mm x 6.3mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e12.84mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePeak Quantum Efficiency (QE)\u003c\/td\u003e\n\u003ctd\u003e91%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e40ke\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e0.7e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e46.9 FPS (at full resolution)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBit Depth\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32µs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAmp Glow Control\u003c\/td\u003e\n\u003ctd\u003eZero Amplifier Glow\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e256MB DDR3\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eROI Support\u003c\/td\u003e\n\u003ctd\u003eYes\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e6.5mm \/ 17.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Window\u003c\/td\u003e\n\u003ctd\u003eAR Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Connection\u003c\/td\u003e\n\u003ctd\u003eM42x0.75 Female Thread\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Type\u003c\/td\u003e\n\u003ctd\u003eUncooled, Color\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e0.28 lbs\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWorking Temperature\u003c\/td\u003e\n\u003ctd\u003e-5℃ to 50℃\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eStorage Temperature\u003c\/td\u003e\n\u003ctd\u003e-10℃ to 60℃\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWorking Relative Humidity\u003c\/td\u003e\n\u003ctd\u003e20% to 80%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOS Compatibility\u003c\/td\u003e\n\u003ctd\u003eWindows 7\/8\/10 (32 \u0026amp; 64-bit), Linux, Mac\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eZWO ASI585MC Camera Body\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e2\" Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eUSB 3.0 Cable (2m)\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eST-4 Autoguider Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eQuick Start Guide\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":44968023720221,"sku":"ZWO-ASI585MC","price":559.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/ZWO-ASI585MC-1__30702.1656260030.1280.1280.jpg?v=1684347976"},{"product_id":"qhyccd-qhy5iii585c-color","title":"QHYCCD QHY5III585C Color","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e8.4 Megapixel Sony IMX585 BSI Color Sensor\u003c\/li\u003e\n\u003cli\u003eLarge 1\/1.2-inch sensor format with 2.9µm pixels\u003c\/li\u003e\n\u003cli\u003e512MB DDR3 image buffer for stable, high-speed capture\u003c\/li\u003e\n\u003cli\u003eUp to 41.5 FPS at full 3856x2180 resolution\u003c\/li\u003e\n\u003cli\u003eExtremely low 0.77e- read noise and 52ke- full well capacity\u003c\/li\u003e\n\u003cli\u003eStandard ST-4 guide port for autoguiding\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eQHYCCD QHY5III585C Color Planetary \u0026amp; Guide Camera\u003c\/h2\u003e\n\u003cp\u003eThe QHYCCD QHY5III585C combines Sony's 8.4 Megapixel IMX585 STARVIS II sensor with a substantial 512MB DDR3 buffer to deliver stable, high-speed planetary imaging. Its 2.9µm pixels and large 1\/1.2-inch format capture expansive, high-resolution views, while the 52ke- full well capacity and 0.77e- read noise ensure high dynamic range on challenging targets like Jupiter. Capable of 41.5 FPS at full resolution, this camera is engineered for lucky imaging without dropped frames, giving you the clean data needed to resolve fine atmospheric details.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony IMX585 Sensor: 8.4 MP and High NIR Sensitivity\u003c\/h3\u003e\n\u003cp\u003eAt the core of the QHY5III585C is the Sony IMX585, a back-illuminated sensor with a 3856x2180 pixel array. This sensor's STARVIS II architecture features deeper pixel wells, which significantly boosts its sensitivity to red and near-infrared (NIR) wavelengths. This makes the camera exceptionally effective for methane band imaging of gas giants or for cutting through atmospheric haze with the included IR850nm filter, revealing surface details on Mars that are invisible in the visual spectrum.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e512MB DDR3 Buffer: 41.5 FPS Full-Frame Capture\u003c\/h3\u003e\n\u003cp\u003eTo prevent data loss during high-speed video capture, the QHY5III585C incorporates a 512MB DDR3 image buffer. This buffer ensures a stable data stream to your computer, eliminating dropped frames that can ruin an imaging run. You can reliably capture at the full 41.5 FPS at 8-bit, or push frame rates up to 199 FPS using a 640-line Region of Interest (ROI), freezing moments of perfect seeing to capture the sharpest possible planetary detail.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e52ke- Full Well and 0.77e- Read Noise for HDR\u003c\/h3\u003e\n\u003cp\u003eThe QHY5III585C achieves an impressive dynamic range through its combination of a deep 52ke- full well capacity and exceptionally low read noise, as low as 0.77e-. This allows you to capture the bright surface of Jupiter and its faint, low-contrast cloud bands in the same exposure without clipping highlights or losing detail in the noise floor. The 12-bit A\/D converter provides the bit depth needed to stretch the data and reveal subtle color variations in post-processing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eDual Back Focus (8mm\/17mm) and ST-4 Guiding\u003c\/h3\u003e\n\u003cp\u003eDesigned for flexibility, the QHY5III585C offers two native back focus distances: 8mm without its adapter and 17mm with the adapter installed. This simplifies integration with various accessories like filter wheels, off-axis guiders, and atmospheric dispersion correctors. The camera includes a standard ST-4 guide port and a lightweight 90g body, making it a highly capable autoguider for deep-sky imaging when not being used for planetary work.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eQHY5III585C vs. ZWO ASI585MC: The 512MB Buffer Advantage\u003c\/h3\u003e\n\u003cp\u003eWhile both the QHY5III585C and ZWO ASI585MC use the same excellent Sony IMX585 sensor, the primary hardware difference lies in the onboard memory buffer. The QHY5III585C's larger buffer is a critical advantage for maintaining stable, high-speed data transfer, especially on systems with slower USB controllers or when running other demanding applications.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eQHY5III585C Buffer:\u003c\/strong\u003e 512MB DDR3 ensures consistent frame rates without drops, crucial for long video captures.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eZWO ASI585MC Buffer:\u003c\/strong\u003e 256MB DDR3, while effective, offers less protection against data transfer bottlenecks under heavy system load.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eGuiding:\u003c\/strong\u003e The QHY5III585C includes a dedicated ST-4 guide port, allowing it to function as a standalone autoguider without requiring a separate ASIAIR or computer-based pulse guiding connection.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the QHY5III585C's 512MB buffer help with planetary imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e512MB DDR3 buffer\u003c\/strong\u003e acts as a temporary storage for image frames before they are sent to the computer via USB 3.0. This prevents data loss (dropped frames) if the computer's hard drive or processor is temporarily busy. For planetary \"lucky imaging,\" a consistent, high frame rate is essential, and this large buffer ensures every moment of good seeing is captured reliably.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the QHY5III585C for imaging Jupiter's methane bands?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, absolutely. The Sony IMX585 sensor has excellent sensitivity in the near-infrared (NIR) spectrum. When paired with the included \u003cstrong\u003eIR850nm filter\u003c\/strong\u003e, the QHY5III585C is highly effective for imaging in the 889nm methane absorption band, which reveals high-altitude structures in Jupiter's and Saturn's atmospheres.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat back focus should I use with the QHY5III585C on my 8\" f\/10 SCT with a filter wheel?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor an f\/10 SCT, you will typically need the \u003cstrong\u003e17mm back focus\u003c\/strong\u003e configuration, which is achieved by keeping the included adapter on the camera. This provides more space to accommodate accessories like a filter wheel or an atmospheric dispersion corrector (ADC) in the optical train while still reaching focus.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the main advantage of the Sony IMX585 sensor in the QHY5III585C?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe primary advantage is its combination of high resolution (\u003cstrong\u003e8.4 Megapixels\u003c\/strong\u003e), high sensitivity from its back-illuminated structure, and very low read noise (as low as \u003cstrong\u003e0.77e-\u003c\/strong\u003e). This makes it a versatile sensor capable of capturing detailed, low-noise images of planets, the Moon, and even brighter deep-sky objects with short exposures.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan the QHY5III585C be used as a primary guide camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. With its high sensitivity, low noise, and built-in \u003cstrong\u003eST-4 guide port\u003c\/strong\u003e, the QHY5III585C is an excellent high-end guide camera. Its large 1\/1.2-inch sensor makes finding a suitable guide star easy, even when using an off-axis guider with a long focal length telescope.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the QHY5III585C require an external power supply?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eNo, the QHY5III585C is powered entirely through its \u003cstrong\u003eUSB 3.0 Type-C connection\u003c\/strong\u003e. It does not require a separate 12V power supply, which simplifies cable management at the telescope.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSony IMX585 BSI CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Type\u003c\/td\u003e\n\u003ctd\u003eColor\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003e1\/1.2-inch (11.1mm x 6.3mm)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e3856 x 2180 (8.4 Megapixels)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9µm x 2.9µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e52,000e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e0.77e- to 8e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eA\/D Converter\u003c\/td\u003e\n\u003ctd\u003e12-bit (output as 16-bit and 8-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e512MB DDR3 Memory\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate (Full)\u003c\/td\u003e\n\u003ctd\u003e41.5 FPS @ 8-bit, 23.5 FPS @ 16-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rate (ROI)\u003c\/td\u003e\n\u003ctd\u003eUp to 199 FPS @ 8-bit\/16-bit (640 lines)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Time Range\u003c\/td\u003e\n\u003ctd\u003e11µs to 900s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eComputer Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 Type-C\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd\u003e1.25\" Nosepiece, C-Mount, CS-Mount\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOptical Window\u003c\/td\u003e\n\u003ctd\u003eIR-Cut Filter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eIncluded Filters\u003c\/td\u003e\n\u003ctd\u003eIR850nm Filter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e17mm (with adapter), 8mm (without adapter)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e90g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.qhyccd.com\/download\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/qhyccd-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eQHYCCD Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"QHYCCD","offers":[{"title":"Default Title","offer_id":44968076181789,"sku":"QHY-110133","price":559.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/QHY5III200M__81459.1680275521.1280.1280.jpg?v=1684348746"},{"product_id":"qhyccd-qhy5iii200m-mono","title":"QHYCCD QHY5III200M Mono","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e1\/1.8-inch SC2210 BSI Monochrome Sensor\u003c\/li\u003e\n\u003cli\u003e4.0µm x 4.0µm Pixel Size\u003c\/li\u003e\n\u003cli\u003e1920 x 1080 (2 Megapixel) Resolution\u003c\/li\u003e\n\u003cli\u003eUp to 96.5 FPS at Full Resolution (8-bit)\u003c\/li\u003e\n\u003cli\u003eUltra-Low Read Noise of 0.75e-\u003c\/li\u003e\n\u003cli\u003e512MB DDR3 Onboard Image Buffer\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eQHYCCD QHY5III200M Mono Planetary \u0026amp; Guide Camera\u003c\/h2\u003e\n\u003cp\u003eThe QHYCCD QHY5III200M Mono combines a highly sensitive 1\/1.8-inch SC2210 BSI sensor with large 4µm pixels to create a versatile planetary and guide camera. Its 2-megapixel resolution (1920x1080) is matched with an exceptionally low read noise floor of just 0.75e- and a full well capacity of 8ke-, preserving dynamic range on bright targets. A 512MB DDR3 memory buffer ensures stable data transfer at up to 96.5 FPS over its USB 3.0 Type-C interface, eliminating dropped frames during critical moments of steady seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSC2210 BSI Sensor: 4µm Pixels and High NIR Sensitivity\u003c\/h3\u003e\n\u003cp\u003eAt the core of the QHY5III200M is the SC2210 back-illuminated sensor, which offers significant sensitivity advantages, especially in the near-infrared. The 4µm pixels provide a large surface area for light collection, boosting signal-to-noise ratio on faint targets and guide stars. This pixel size is an excellent match for the focal lengths of many off-axis guiders and guide scopes, providing accurate tracking without needing a Barlow or reducer to achieve proper image scale.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eBack-Illuminated Structure (BSI):\u003c\/strong\u003e Maximizes photon capture by placing the sensor's wiring layer behind the photodiodes, increasing quantum efficiency.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eIncluded IR850nm Filter:\u003c\/strong\u003e The camera's high NIR sensitivity can be leveraged for methane band imaging of Jupiter and Saturn, and this filter allows you to isolate that specific wavelength.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eLow Read Noise (0.75e-):\u003c\/strong\u003e The extremely low minimum read noise ensures that faint guide stars are cleanly detected and that planetary detail is not lost in the noise floor during short exposures.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eHigh-Speed Planetary Imaging: 96.5 FPS with a 512MB DDR3 Buffer\u003c\/h3\u003e\n\u003cp\u003eFor planetary imaging, capturing thousands of frames in a short period is key to freezing atmospheric turbulence. The QHY5III200M is built for this task, streaming full-resolution 1920x1080 frames at 96.5 FPS in 8-bit mode or 60 FPS in 16-bit mode for greater bit depth. The integrated 512MB DDR3 buffer is critical, preventing data bottlenecks and lost frames that can occur when a computer's resources are momentarily strained.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eA Dual-Role Guider: 4µm Pixels and 8mm\/17mm Back Focus\u003c\/h3\u003e\n\u003cp\u003eEngineered as both a planetary imager and a dedicated autoguider, the QHY5III200M features the necessary connectivity and form factor for any setup. A standard ST-4 guide port provides direct communication with your mount, while the lightweight 90g body adds minimal load to your focuser. The camera provides two native back focus distances—8mm and 17mm—to accommodate different optical configurations without requiring a large stack of adapters.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003e8mm Back Focus:\u003c\/strong\u003e Ideal for attaching C\/CS-mount lenses directly or for use in setups where minimal back focus is required.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003e17mm Back Focus:\u003c\/strong\u003e Provides the standard spacing needed to insert accessories like a filter wheel or work within the optical path of most off-axis guiders.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003e1.25-inch Format:\u003c\/strong\u003e The camera body slips directly into any standard 1.25-inch focuser or visual back, making it universally compatible.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eQHY5III200M vs. ZWO ASI290MM Mini: Pixel Size and Guiding\u003c\/h3\u003e\n\u003cp\u003eA common alternative for guiding and planetary imaging is the ZWO ASI290MM Mini. While both are excellent cameras, they are optimized for slightly different scenarios.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eZWO ASI290MM Mini Advantage:\u003c\/strong\u003e The ASI290MM uses smaller 2.9µm pixels. This can yield higher resolution on shorter focal length telescopes, resolving finer detail if the seeing conditions permit.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eQHY5III200M Advantage:\u003c\/strong\u003e The larger 4µm pixels of the QHY5III200M are more sensitive and provide a better image scale for guiding on longer focal length instruments (like SCTs with off-axis guiders) without resorting to binning. This can result in detecting more guide stars and achieving a higher signal-to-noise ratio on each one, leading to more stable guiding.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the main advantage of the QHY5III200M's 4µm pixels?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e4µm pixels\u003c\/strong\u003e offer a balance of resolution and sensitivity. They are large enough to capture more photons per pixel, which is excellent for detecting faint guide stars and reducing noise. This size often provides a better image scale for guiding with long focal length telescopes compared to cameras with smaller pixels, which can be prone to oversampling (seeing-limited resolution spread over too many pixels).\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the 512MB DDR3 buffer on the QHY5III200M help with planetary imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e512MB DDR3 buffer\u003c\/strong\u003e acts as a temporary memory cache for image frames before they are sent to the computer. This prevents frame drops, which can happen if your computer's CPU or hard drive is momentarily busy. For planetary \"lucky imaging,\" where you capture thousands of frames at high speed, a stable data stream is essential, and the buffer ensures you don't lose the sharpest data.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow would the QHY5III200M perform as a guider on an 8\" SCT at f\/10 with an off-axis guider?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe QHY5III200M is an excellent choice for this setup. The high sensitivity of its BSI sensor and 4µm pixels will help detect guide stars even in the dimmer, off-axis light path of an SCT. At a focal length of ~2000mm, the 4µm pixels provide a good image scale for precise guiding without being overly affected by seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the QHY5III200M a good choice for imaging Jupiter's cloud bands with a 6-inch Newtonian?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. A 6-inch Newtonian typically has a focal length of around 750mm (f\/5). To get a large enough image of Jupiter, you would typically use a 2.5x or 3x Barlow lens, increasing the effective focal ratio to f\/12.5 or f\/15. The QHY5III200M's high frame rate of \u003cstrong\u003e96.5 FPS\u003c\/strong\u003e and low read noise are ideal for capturing sharp detail on Jupiter's cloud bands in these conditions.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat do the 8mm and 17mm back focus options on the QHY5III200M let me do?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe dual back focus options provide flexibility for connecting different accessories. The \u003cstrong\u003e8mm distance\u003c\/strong\u003e is used when attaching C-mount or CS-mount lenses directly to the camera for wide-field applications. The \u003cstrong\u003e17mm distance\u003c\/strong\u003e provides the necessary spacing to achieve focus when the camera is used with standard 1.25\" accessories like filter wheels or in most off-axis guiders.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the QHY5III200M for near-infrared imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAbsolutely. The camera's SC2210 BSI sensor has high sensitivity in the near-infrared (NIR) spectrum. It even comes with an \u003cstrong\u003eIR850nm filter\u003c\/strong\u003e, making it ready for specialized imaging techniques like capturing Jupiter's methane bands, which can reveal high-altitude atmospheric features not visible in normal light.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Sensor\u003c\/td\u003e\n\u003ctd\u003eSC2210\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Type\u003c\/td\u003e\n\u003ctd\u003eMonochrome, Back-Side Illuminated (BSI)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003e1\/1.8 inch\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e4.0µm x 4.0µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e1920 x 1080 (2 Megapixels)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e8,000e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e0.75e- to 3e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eA\/D Converter\u003c\/td\u003e\n\u003ctd\u003e12-bit (output as 16-bit and 8-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e512MB DDR3 Memory\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate (Full)\u003c\/td\u003e\n\u003ctd\u003e96.5 FPS @ 8-bit | 60 FPS @ 16-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate (ROI)\u003c\/td\u003e\n\u003ctd\u003e187 FPS @ 960 Lines (8-bit) | 209 FPS @ 480 Lines (8-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Time Range\u003c\/td\u003e\n\u003ctd\u003e15µs to 900s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eComputer Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 Type-C\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd\u003e1.25-inch, C-Mount, CS-Mount\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e8mm (without adapter) | 17mm (with adapter)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOptical Window\u003c\/td\u003e\n\u003ctd\u003eAR Anti-Reflection Glass\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eIncluded Filter\u003c\/td\u003e\n\u003ctd\u003eIR850nm Pass Filter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e90g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.qhyccd.com\/download\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/qhyccd-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eQHYCCD Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"QHYCCD","offers":[{"title":"Default Title","offer_id":44968076214557,"sku":"QHY-110132","price":433.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/QHY5III200M__34194.1680275583.1280.1280.jpg?v=1684348748"},{"product_id":"zwo-asi715mc-color","title":"ZWO ASI715MC Color","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e3864x2192 Resolution Sony STARVIS Sensor\u003c\/li\u003e\n\u003cli\u003e1.45µm Pixel Size for High-Resolution Planetary Imaging\u003c\/li\u003e\n\u003cli\u003e45.1 FPS at Full Resolution over USB 3.0\u003c\/li\u003e\n\u003cli\u003ePeak Quantum Efficiency (QE) of 80%\u003c\/li\u003e\n\u003cli\u003eUltra-low 0.72e Read Noise\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI715MC Color Astronomy Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI715MC Color Astronomy Camera leverages a Sony IMX715 sensor to deliver a high-resolution 3864x2192 pixel array for detailed planetary imaging. Its exceptionally small 1.45µm pixels are designed for critical sampling on long focal-length telescopes, while the camera's 80% peak QE and 0.72e read noise capture faint surface details on planets and the Moon. At full resolution, the ASI715MC streams data at 45.1 FPS, ensuring you can capitalize on moments of steady seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e1.45µm Pixels for Critical Sampling\u003c\/h3\u003e\n\u003cp\u003eThe defining feature of the ASI715MC is its 1.45µm pixel size, one of the smallest available in astronomy cameras. This allows you to achieve a high-resolution image scale without aggressive Barlow lenses, perfectly matching the resolving power of Schmidt-Cassegrain and Maksutov-Cassegrain telescopes operating near f\/10. The resulting 3864x2192 effective pixel array resolves fine details like Jupiter's smallest cloud bands, divisions in Saturn's rings, and subtle crater wall textures on the Moon.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eHigh-Speed Imaging with 80% QE and 0.72e Read Noise\u003c\/h3\u003e\n\u003cp\u003eFor planetary work, capturing thousands of frames in a short time (\"lucky imaging\") is essential. The ASI715MC's sensor achieves a peak Quantum Efficiency of 80% and an extremely low read noise of just 0.72e. This combination ensures that faint signals from planetary surfaces are captured cleanly above the noise floor, even during the very short exposures required to freeze atmospheric turbulence. The primary trade-off for such small pixels is a modest full well capacity of 6.0Ke, making this camera ideal for planetary and lunar work rather than long-exposure deep-sky imaging of high-dynamic-range targets.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eASI715MC vs. ASI462MC: A Question of Resolution\u003c\/h3\u003e\n\u003cp\u003eThe ASI715MC is often compared to the popular ZWO ASI462MC. The choice between them depends entirely on your telescope and imaging goals.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eZWO ASI462MC Advantage:\u003c\/strong\u003e The ASI462MC's larger 2.9µm pixels are more forgiving to average seeing conditions and pair well with faster, shorter focal length telescopes. It also has exceptional sensitivity in the near-infrared, which helps cut through atmospheric haze.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eZWO ASI715MC Advantage:\u003c\/strong\u003e With a resolution of 3864x2192 compared to the ASI462MC's 1936x1096, the ASI715MC captures a far more detailed image over the same field of view. If you have a long focal length telescope (f\/10 or slower) and good seeing, the ASI715MC will resolve finer features that the ASI462MC cannot.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e45.1 FPS Data Transfer and Connectivity\u003c\/h3\u003e\n\u003cp\u003eThe camera's performance is supported by modern hardware that prevents data bottlenecks during high-speed capture sessions. A built-in 256MB DDR3 cache acts as a buffer, ensuring stable frame delivery without dropping data.\n\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eUSB 3.0 Port:\u003c\/strong\u003e Delivers the 5Gbps bandwidth required to run the camera at its maximum 45.1 FPS at full resolution in 10-bit high-speed mode.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eST4 Guide Port:\u003c\/strong\u003e Allows the ASI715MC to double as a high-resolution autoguider for a separate imaging rig, connecting directly to any ST4-compatible mount.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eStandard Mounting:\u003c\/strong\u003e Includes a 1.25\" nosepiece and M42x0.75 threads for direct connection to focusers, filter wheels, and other standard accessories.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the ASI715MC perform on Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ZWO ASI715MC is an excellent match for an 8\" f\/10 SCT. The optimal focal ratio for its 1.45µm pixels is between f\/7.25 and f\/10.15. This means at the native f\/10, you are already at the ideal image scale for high-resolution imaging on nights of good seeing, often without needing a Barlow lens. On nights of exceptional seeing, a 1.5x or 2x Barlow can push the resolution even further.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the ASI715MC a good choice for imaging the Andromeda Galaxy (M31)?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eNo, the ZWO ASI715MC is not designed for large deep-sky objects like the Andromeda Galaxy. Its 1\/2.8\" sensor has a diagonal of only 6.43mm, which results in a very narrow field of view. It is built specifically for high-magnification targets like planets, the Moon, the Sun (with a proper solar filter), and for \"lucky imaging\" of small, bright planetary nebulae or globular cluster cores.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDo I need an IR Cut filter with the ZWO ASI715MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. Like most color astronomy cameras, the ZWO ASI715MC's sensor is sensitive to infrared (IR) light. To achieve correct color balance and sharpness, an IR Cut or UV\/IR Cut filter is required. Without one, stars and planetary details will appear slightly bloated and have a reddish\/magenta tint.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy would I choose the ASI715MC over a camera with larger pixels?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYou should choose the ASI715MC if you have a telescope with a long focal length (typically over 1500mm) and you want to capture the finest possible details on the planets. Its small 1.45µm pixels allow you to reach the ideal image scale for high resolution without using strong Barlow lenses, which can dim the image and introduce optical aberrations.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan the ZWO ASI715MC be used for autoguiding?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. The ZWO ASI715MC can be used as a very capable autoguider thanks to its low read noise and built-in ST4 port. Its high resolution can detect very small guide star movements, though its narrow field of view may sometimes make finding a suitable guide star more challenging than with a dedicated, larger-chip guide camera.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat software is compatible with the ZWO ASI715MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ZWO ASI715MC works with most popular astronomy software packages. For planetary capture, imagers commonly use \u003cstrong\u003eFireCapture\u003c\/strong\u003e or \u003cstrong\u003eSharpCap\u003c\/strong\u003e. For autoguiding, it is fully supported by \u003cstrong\u003ePHD2 Guiding\u003c\/strong\u003e. All necessary ASCOM and native drivers are available for free download from the ZWO website.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSKU\u003c\/td\u003e\n\u003ctd\u003eZWO-ASI715MC\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/2.8\" Sony IMX715 Color CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eEffective Pixel Array\u003c\/td\u003e\n\u003ctd\u003e3864 x 2192\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e1.45µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Dimensions\u003c\/td\u003e\n\u003ctd\u003e5.6mm x 3.2mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e6.43mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePeak Quantum Efficiency (QE)\u003c\/td\u003e\n\u003ctd\u003e80%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e6.0Ke\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e0.72e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e45.1 FPS (at full resolution)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBit Depth\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Type\u003c\/td\u003e\n\u003ctd\u003eUncooled Color\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Sensor\u003c\/td\u003e\n\u003ctd\u003eNo\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eASI715MC Color Camera\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eLens Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eUSB 3.0 Cable (2m)\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eST4 Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eZWO ASI Camera Quick Guide\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":47109447090461,"sku":"ZWO-ASI715MC","price":279.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/EN--ASI715MC_09.jpg?v=1700075986"},{"product_id":"zwo-asi462mm-mono","title":"ZWO ASI462MM Mono","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e2.1MP Sony IMX462 Monochrome Sensor\u003c\/li\u003e\n\u003cli\u003eExceptional Near-Infrared (NIR) Sensitivity\u003c\/li\u003e\n\u003cli\u003e136.1 FPS at Full 1936x1096 Resolution\u003c\/li\u003e\n\u003cli\u003eUltra-Low Read Noise as low as 0.47e-\u003c\/li\u003e\n\u003cli\u003e256MB DDR3 Buffer for Stable Data Transfer\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI462MM Mono Planetary \u0026amp; Guiding Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI462MM Mono combines the groundbreaking Sony IMX462 sensor with an ultra-low read noise of 0.47e- to redefine monochrome planetary imaging. Its 2.9µm pixels and 2.1MP resolution capture fine details on Jupiter and Mars, while the staggering 136.1 FPS frame rate freezes moments of perfect seeing. With a peak Quantum Efficiency of approximately 89% and unmatched sensitivity in the near-infrared, this camera excels at cutting through atmospheric turbulence for remarkably sharp lunar, solar, and planetary captures.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eUnrivaled Near-Infrared (NIR) Sensitivity at 800nm+\u003c\/h3\u003e\n\u003cp\u003eThe core strength of the ASI462MM is the Sony IMX462 sensor's extraordinary sensitivity in the near-infrared spectrum. Where other planetary cameras see their response drop off sharply, the ASI462MM maintains high efficiency beyond 800nm. This allows you to leverage methane and other long-pass filters to reveal deep atmospheric features on Jupiter and Saturn that are invisible in the visible spectrum, effectively calming atmospheric seeing for sharper final images.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e136.1 FPS Capture Rate with Zero Amp Glow\u003c\/h3\u003e\n\u003cp\u003eAt a full resolution of 1936x1096, the ASI462MM streams data at up to 136.1 frames per second via its USB 3.0 interface. This high-speed capability is critical for \"lucky imaging,\" allowing you to capture thousands of frames in a short period to overcome atmospheric distortion. The integrated 256MB DDR3 buffer ensures stable, drop-free data transfer, while the sensor architecture eliminates amp glow entirely, even on longer exposures when using the camera for guiding.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eHigh-Speed Mode:\u003c\/strong\u003e Captures full-resolution frames at 136.1 fps with a 10-bit ADC for maximum frame rate.\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eHigh-Dynamic-Range Mode:\u003c\/strong\u003e Utilizes the full 12-bit ADC at 63.9 fps for smoother tonal gradations and a full well capacity of 11.2ke-.\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eUltra-Low Read Noise of 0.47e- for Cleaner Stacks\u003c\/h3\u003e\n\u003cp\u003eThe ASI462MM leverages STARVIS technology and an integrated High Conversion Gain (HCG) mode to achieve a minimum read noise of just 0.47 electrons. This mode automatically activates at a gain setting of 80 and higher, drastically reducing noise without sacrificing the camera's wide dynamic range. The result is a cleaner signal-to-noise ratio, allowing you to pull out faint details from your stacked images with less aggressive noise reduction.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eZWO ASI462MM vs. ASI290MM: A Generational Leap\u003c\/h3\u003e\n\u003cp\u003eThe ASI462MM is the direct successor to the legendary ASI290MM, offering significant improvements in key areas for planetary imagers.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eRead Noise:\u003c\/strong\u003e The ASI462MM's minimum read noise of 0.47e- is substantially lower than the ASI290MM's, leading to cleaner images at high gain.\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eInfrared Sensitivity:\u003c\/strong\u003e While the ASI290MM was a capable IR performer, the ASI462MM's IMX462 sensor provides a dramatic boost in quantum efficiency in the 800-1000nm range, making it the superior choice for methane band imaging.\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eQE Peak:\u003c\/strong\u003e The ASI462MM boasts a higher peak QE of ~89%, ensuring more of the light hitting the sensor is converted into a usable signal.\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cp\u003eFor imagers seeking the ultimate in monochrome planetary performance, particularly for imaging Jupiter and Saturn through atmospheric turbulence, the ASI462MM offers a clear and measurable advantage.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat makes the ASI462MM so good for imaging Jupiter?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ZWO ASI462MM's exceptional sensitivity in the near-infrared (NIR) allows it to excel with filters like a methane band (890nm). This wavelength cuts through the Earth's atmospheric turbulence (\"seeing\"), revealing fine details in Jupiter's cloud bands that are often blurred at visible wavelengths. Its high frame rate of 136.1 FPS is also crucial for capturing moments of atmospheric stability.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the ZWO ASI462MM a good guide camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, the ASI462MM is an excellent autoguiding camera. Its high sensitivity and extremely low 0.47e- read noise allow it to detect faint guide stars easily. The 2.9µm pixel size provides high-resolution guiding for a wide range of guide scope focal lengths, and the standard ST4 port ensures compatibility with virtually any equatorial mount.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the optimal focal ratio for the ASI462MM for planetary imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor ideal planetary imaging that critically samples the image, a focal ratio between f\/14 and f\/20 is recommended with the ASI462MM's 2.9µm pixels. For an f\/10 Schmidt-Cassegrain, this is typically achieved with a 1.5x to 2x Barlow lens, depending on local seeing conditions.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDo I need an IR-cut filter with the ASI462MM?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor LRGB (Luminance, Red, Green, Blue) imaging, you will need an IR-cut filter for the RGB channels to ensure accurate color balance, as the sensor is highly sensitive to infrared light. For luminance or specialized IR imaging (like methane band), you would use a luminance filter (which passes IR) or a specific IR-pass filter, not an IR-cut filter.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the ASI462MM compare to the color ASI462MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ASI462MM (monochrome) is significantly more sensitive than its color counterpart because it does not have a Bayer filter matrix over the sensor. This allows it to capture finer detail (higher resolution) and fainter signals, making it the preferred choice for advanced planetary imagers who use a separate filter wheel to create color images. The color version offers convenience but at the cost of some sensitivity and resolution.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the ASI462MM suffer from amp glow?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eNo. The ZWO ASI462MM's sensor design and circuitry completely eliminate amplifier glow. This means your dark frames will be clean and free of the characteristic glow seen in the corners of older sensors, simplifying your calibration process, especially for longer exposures when guiding.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/2.8” Sony IMX462 CMOS (Monochrome)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e2.1MP (1936 x 1096)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQuantum Efficiency (Peak)\u003c\/td\u003e\n\u003ctd\u003e~89%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e0.47e- to 2.65e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e11.2ke-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e136.1 fps at 1936x1096\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Buffer\u003c\/td\u003e\n\u003ctd\u003e256MB DDR3\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eAR Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eASI462MM Camera Body\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece Adapter\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Dust Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e2 meter USB 3.0 Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e2 meter ST4 Guide Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eQuick Start Guide\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":47901976396061,"sku":"ZWO-ASI462MM","price":416.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/51c34a08f8466e3da0dab0781569a381-2.jpg?v=1711564921"},{"product_id":"zwo-asi585mc-pro-color","title":"ZWO ASI585MC Pro Color","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e8.29 Megapixel 1\/1.2\" Sony IMX585 Color Sensor\u003c\/li\u003e\n\u003cli\u003e2.9µm Pixel Size for High-Resolution Imaging\u003c\/li\u003e\n\u003cli\u003e91% Peak Quantum Efficiency\u003c\/li\u003e\n\u003cli\u003e47 FPS at Full 3840x2160 Resolution\u003c\/li\u003e\n\u003cli\u003e512MB DDR3 Internal Image Buffer\u003c\/li\u003e\n\u003cli\u003eRegulated Two-Stage TEC Cooling\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI585MC Pro USB3 Cooled Color Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI585MC Pro combines a high-resolution 8.29 MP Sony IMX585 sensor with regulated cooling to excel at both planetary and deep-sky astrophotography. Its 2.9µm pixels resolve fine detail on Jupiter's cloud bands, while a peak Quantum Efficiency of 91% and read noise as low as 0.7e capture faint signal from distant nebulae. The camera sustains a full-resolution frame rate of 47 FPS over USB 3.0, with a 512MB DDR3 buffer ensuring no frames are dropped during critical lucky imaging sessions.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e4K Resolution from a 1\/1.2\" Back-Illuminated Sensor\u003c\/h3\u003e\n\u003cp\u003eAt the core of the ASI585MC Pro is a Sony IMX585 back-illuminated CMOS sensor, delivering a native resolution of 3840 x 2160 pixels. The 1\/1.2\" format provides a generous field of view for framing larger targets like the Andromeda Galaxy (M31) or lunar mosaics, while the small 2.9µm pixels are critically sampled for high-resolution planetary work on telescopes with longer focal ratios. Because the sensor is back-illuminated (BSI), wiring and electronics are placed behind the photodiode layer, maximizing the light-gathering area of each pixel and contributing to its high sensitivity.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e91% QE and 40Ke Full Well for High Signal-to-Noise\u003c\/h3\u003e\n\u003cp\u003eCapturing faint deep-sky objects requires exceptional sensitivity, and the ASI585MC Pro's 91% peak QE means it converts the vast majority of incoming photons into usable electronic signal. This efficiency, combined with a read noise floor as low as 0.7e, allows you to pull faint wisps of nebulosity out of the background. The sensor's deep 40Ke full well capacity prevents bright stars in the field from saturating, preserving color and detail in dense star clusters and the cores of bright nebulae.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e47 FPS at Full Resolution with a 512MB DDR3 Buffer\u003c\/h3\u003e\n\u003cp\u003eFor planetary imaging, freezing moments of steady seeing is critical. The ASI585MC Pro streams its full 8.29 MP output at up to 47 frames per second in 10-bit high-speed mode, allowing you to capture thousands of frames in a short period for lucky imaging. To handle this massive data throughput without interruption, the camera features an onboard 512MB DDR3 buffer. This buffer prevents dropped frames that can occur from USB bus contention on the host computer, ensuring your data stream is stable and complete.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eASI585MC Pro vs. ASI585MC: Why Cooling Matters for Deep Sky\u003c\/h3\u003e\n\u003cp\u003eThe uncooled ASI585MC is lighter and more affordable, making it an excellent choice for dedicated planetary imagers. However, for deep-sky astrophotography where exposure times stretch beyond a few seconds, the ASI585MC Pro's regulated two-stage TEC cooling becomes essential.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eThermal Noise Reduction:\u003c\/strong\u003e The Pro's cooling system dramatically reduces thermal noise (dark current) that builds up during long exposures, resulting in cleaner, higher-contrast images of faint nebulae and galaxies. This is the single most important advantage for DSO imaging.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eConsistent Dark Frames:\u003c\/strong\u003e Regulated cooling allows you to maintain a consistent sensor temperature across imaging sessions. This means dark frames taken on one night can be reliably reused on another, simplifying your calibration workflow.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eWeight Trade-off:\u003c\/strong\u003e The cooling hardware adds weight, making the Pro model 1.04 lb compared to the uncooled version's lighter profile. This is a necessary trade-off for the low-noise deep-sky imaging it enables.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat makes the ZWO ASI585MC Pro a good hybrid planetary and deep-sky camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ASI585MC Pro is a strong hybrid because its specifications serve both disciplines. The \u003cstrong\u003e2.9µm pixels\u003c\/strong\u003e and \u003cstrong\u003e47 FPS\u003c\/strong\u003e frame rate are ideal for high-resolution lucky imaging of planets. For deep-sky objects, the \u003cstrong\u003e91% QE\u003c\/strong\u003e, \u003cstrong\u003e0.7e read noise\u003c\/strong\u003e, and regulated TEC cooling allow for the capture of clean, high-sensitivity, long-exposure images.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow should I set up the ASI585MC Pro for imaging Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor planetary imaging, the ideal focal ratio is typically 5 to 7 times the camera's pixel size. With the ASI585MC Pro's 2.9µm pixels, your target focal ratio is between f\/14.5 and f\/20.3. On an f\/10 SCT, using a 1.5x or 2x Barlow lens will place you in this optimal range, allowing you to resolve fine details in Jupiter's cloud bands under good seeing conditions.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan the ASI585MC Pro capture the Orion Nebula (M42) without blowing out the Trapezium stars?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. The camera's \u003cstrong\u003e40Ke full well capacity\u003c\/strong\u003e provides significant dynamic range. To capture both the faint outer nebulosity of M42 and the bright Trapezium core, you would use an HDR (High Dynamic Range) imaging technique. This involves taking a series of short exposures to capture the core without saturation and blending them with longer exposures that reveal the faint outer regions.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy does the ZWO ASI585MC Pro have a 512MB DDR3 buffer?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe 512MB DDR3 buffer acts as a temporary, high-speed memory cache for image data before it's transferred to the computer via USB 3.0. This is crucial at high frame rates like 47 FPS, as it prevents data loss (dropped frames) if the host computer's USB bus is momentarily busy with other tasks. It ensures a stable and reliable data transfer.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDo I need a separate UV\/IR cut filter with the ASI585MC Pro?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. The protective window on the ASI585MC Pro is AR-coated but does not block ultraviolet or infrared light. For correct color balance on broadband targets like galaxies and stars, a separate UV\/IR cut (or Luminance) filter is required to prevent star bloat and ensure focus across the visual spectrum.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIf I only image planets, is the ASI585MC Pro still the right choice over the uncooled ASI585MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor strictly planetary imaging, where exposures are very short, the uncooled ASI585MC is often sufficient and more cost-effective. Thermal noise is not a significant factor in short exposures. The primary reason to choose the ASI585MC Pro is if you plan to do any long-exposure deep-sky imaging, where its cooling system is essential for clean images.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/1.2\" Sony IMX585 BSI CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e8.29 MP (3840 x 2160)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e12.84 mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e47 FPS (at full resolution)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQuantum Efficiency (Peak)\u003c\/td\u003e\n\u003ctd\u003e91%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Depth\u003c\/td\u003e\n\u003ctd\u003e40Ke\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e0.7e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCooling\u003c\/td\u003e\n\u003ctd\u003eCooled, Two-Stage TEC\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e512MB DDR3\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBit Depth\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Window\u003c\/td\u003e\n\u003ctd\u003eAR Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eComputer Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd\u003eM42 x 0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDimensions\u003c\/td\u003e\n\u003ctd\u003e78mm x 73.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e1.04 lb.\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOS Compatibility\u003c\/td\u003e\n\u003ctd\u003eWindows, Linux \u0026amp; Mac OSX\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eASI585MC Pro Cooled Camera\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eCamera Bag\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e2m USB 3.0 Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e0.5m USB 2.0 Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 2\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eM42-1.25\" Filter Adapter (for mounting a 1.25\" filter)\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e11mm M42 Extender (pre-attached to camera)\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Dust Cap\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e2\" Dust Cap\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eM42-M48 16.5mm Extender\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eM42-M42 21mm Extender\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eM48-M42 Adapter\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eSpacers\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 4\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eQuick Guide\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":47959687266589,"sku":"ZWO-ASI585MC-P","price":849.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ZWO-ASI585MC-P-1.jpg?v=1712018460"},{"product_id":"zwo-asi678mm-mono","title":"ZWO ASI678MM Mono","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e8.29 Megapixel Resolution (3840 x 2160)\u003c\/li\u003e\n\u003cli\u003e2.0µm Square Pixels\u003c\/li\u003e\n\u003cli\u003e83% Peak Quantum Efficiency (Monochrome)\u003c\/li\u003e\n\u003cli\u003e0.6e Minimum Read Noise\u003c\/li\u003e\n\u003cli\u003e47.5 Frames Per Second at Full Resolution\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI678MM Monochrome Astronomy Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI678MM Monochrome Astronomy Camera leverages a back-illuminated Sony sensor to deliver 8.29 MP resolution at a rapid 47.5 FPS. Its tiny 2µm pixels resolve fine planetary and solar detail, while the 83% peak QE and an exceptionally low 0.6e minimum read noise capture faint signal during high-speed lucky imaging. A 256MB DDR3 buffer ensures stable data transfer over USB 3.0, preventing frame drops during critical moments of steady seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony IMX678 Sensor with 2µm Pixels\u003c\/h3\u003e\n\u003cp\u003eAt the core of the ASI678MM is a Sony STARVIS 2 CMOS sensor, featuring a 3840 x 2160 pixel array. The 2µm pixel size is an excellent match for short focal length refractors or for imagers using SCTs at their native focal ratio, often eliminating the need for a Barlow lens to reach ideal image sampling. This back-illuminated (BSI) sensor architecture places circuitry behind the photodiode, maximizing the light-gathering area of each pixel for a peak QE of 83%.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eLow Noise Floor of 0.6e at 47.5 FPS\u003c\/h3\u003e\n\u003cp\u003eFor planetary, lunar, and solar imaging, success is defined by capturing thousands of frames to freeze moments of atmospheric stability. The ASI678MM reads out its full 8.29 MP frame at 47.5 FPS with a read noise as low as 0.6 electrons, ensuring that faint, low-contrast details are not lost in the camera's own noise floor. The camera also features Zero Amp Glow circuitry, which produces clean raw frames without the characteristic glow that requires dark frame subtraction, simplifying your processing workflow.\u003c\/p\u003e\n\u003cp\u003eAs an uncooled camera, the ASI678MM is designed for the short exposures typical of solar system imaging. It is not intended for long-exposure deep-sky astrophotography, where thermal noise would accumulate and degrade the image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eASI678MM vs. ASI178MM: A Comparison of 2µm vs. 2.4µm\u003c\/h3\u003e\n\u003cp\u003eWhen choosing a small-pixel monochrome camera, a common decision is between the ASI678MM and the older ASI178MM. While both use back-illuminated Sony sensors, their specifications serve different imaging setups.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eResolution and Sampling:\u003c\/strong\u003e The ASI678MM's smaller 2µm pixels and higher 8.29 MP resolution provide a finer image scale than the ASI178MM's 2.4µm pixels and 6.4 MP sensor. This gives the 678MM an advantage in resolving detail at any given focal length.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eRead Noise:\u003c\/strong\u003e With a minimum read noise of 0.6e, the ASI678MM is significantly quieter than the ASI178MM's 1.4e minimum. This results in a cleaner signal and better visibility of low-contrast features on targets like Jupiter's cloud bands.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eUse Case:\u003c\/strong\u003e The ASI178MM's slightly larger 2.4µm pixels may be a better fit for telescopes with very long focal lengths or for observers in locations with average seeing, as it is less demanding of atmospheric stability. The ASI678MM excels when seeing is good or when used with shorter focal length instruments.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eStable Imaging with a 256MB Buffer\u003c\/h3\u003e\n\u003cp\u003eTo handle the data stream from its 8.29 MP sensor at 47.5 FPS, the ASI678MM includes a 256MB DDR3 memory buffer. This buffer prevents dropped frames that can occur from data transmission issues between the camera and computer, ensuring your video files are complete. The camera connects via a USB 3.0 port for maximum speed and includes a standard ST-4 autoguiding port for deep-sky imagers who wish to use its high sensitivity for guiding purposes.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat Barlow do I need for the ASI678MM with an 8\" f\/10 SCT on Jupiter?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor planetary imaging, the ideal focal ratio is typically 5 to 7 times the camera's pixel size. With the ASI678MM's 2µm pixels, the target focal ratio is between f\/10 and f\/14. An 8\" f\/10 SCT is already perfectly matched to this camera for imaging Jupiter under average seeing conditions, so \u003cstrong\u003eno Barlow is required\u003c\/strong\u003e. In moments of excellent seeing, a 1.5x Barlow could be used to push the focal ratio to f\/15 for slightly more resolution.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the ZWO ASI678MM suitable for long-exposure deep-sky imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eNo, the ASI678MM is an \u003cstrong\u003euncooled\u003c\/strong\u003e camera. While its high sensitivity and low read noise are excellent, it is not designed for multi-minute exposures of faint deep-sky objects like nebulae and galaxies. Thermal noise will build up over long exposures, degrading the image. It is optimized for high-frame-rate \"lucky imaging\" of bright targets like the Moon, Sun, and planets.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the ASI678MM for solar imaging with a dedicated H-alpha telescope?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, the ASI678MM is an excellent choice for high-resolution solar imaging. Its monochrome sensor provides maximum detail and sensitivity for capturing features like surface granulation, filaments, and prominences. The high frame rate of 47.5 FPS is critical for overcoming atmospheric turbulence during daytime imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the ASI678MM compare to the color ASI678MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ASI678MM is the monochrome version of the ASI678MC. The primary differences are:\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eSensitivity \u0026amp; Resolution:\u003c\/strong\u003e The ASI678MM (mono) is inherently more sensitive and captures finer detail because it does not have a Bayer color filter array covering the pixels. Every pixel contributes to the luminance image.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eWorkflow:\u003c\/strong\u003e The ASI678MC (color) provides a color image in a single shot, which is more convenient. The ASI678MM requires shooting through separate Red, Green, and Blue filters and combining them later to create a color image, but this method yields a much higher quality final result.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does the \"Zero Amp Glow\" feature on the ASI678MM do?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAmplifier glow is a common artifact in CMOS sensors where a faint glow appears in the corner of images, especially on longer exposures. The \u003cstrong\u003eZero Amp Glow\u003c\/strong\u003e circuitry in the ASI678MM physically prevents this from occurring. This means you get cleaner raw data without needing to subtract dark frames to remove the glow, simplifying your image processing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDo I need an IR Cut filter with the ZWO ASI678MM?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003e\u003cstrong\u003eYes, for most planetary imaging.\u003c\/strong\u003e As a monochrome camera, the ASI678MM is sensitive to both visible and infrared (IR) light. Different wavelengths focus at slightly different points, which can soften the image. Using an IR Cut filter ensures only visible light reaches the sensor, resulting in a sharper luminance (L) channel for LRGB imaging. Alternatively, an IR Pass filter can be used to capture data specifically in the infrared, which can help stabilize images in poor seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/1.8\" Sony IMX678 BSI CMOS (Monochrome)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e8.29 MP (3840 x 2160)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.0 µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQuantum Efficiency (Peak)\u003c\/td\u003e\n\u003ctd\u003e83%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e0.6e to 3.5e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e47.5 FPS at full resolution\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e256MB DDR3\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBit Depth\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32 µs to 2000 s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAmp Glow Control\u003c\/td\u003e\n\u003ctd\u003eZero Amplifier Glow\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e12.5 mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd\u003eM42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Window\u003c\/td\u003e\n\u003ctd\u003eAR Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCooled \/ Uncooled\u003c\/td\u003e\n\u003ctd\u003eUncooled\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOperating Temperature\u003c\/td\u003e\n\u003ctd\u003e-5°C to 50°C\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e0.3 lb.\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003e7.68mm x 4.32mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOS Compatibility\u003c\/td\u003e\n\u003ctd\u003eWindows 7\/8\/10, Linux, Mac\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eZWO ASI678MM Camera Body\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eT2-1.25\" Adapter\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eUSB 3.0 Cable (2m)\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eST4 Guide Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eUser Manual\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":48343933485341,"sku":"ZWO-ASI678MM","price":489.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ZWO-ASI678MC-1__89087.1656259708.1280.1280.jpg?v=1714576640"},{"product_id":"zwo-asi676mc-color","title":"ZWO ASI676MC Color","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e12.6 Megapixel 3552 x 3552 Square Sensor\u003c\/li\u003e\n\u003cli\u003e2.0µm Pixel Size\u003c\/li\u003e\n\u003cli\u003e83% Peak Quantum Efficiency\u003c\/li\u003e\n\u003cli\u003eZero Amplifier Glow Circuitry\u003c\/li\u003e\n\u003cli\u003e256MB DDR3 Internal Buffer\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI676MC Color Astronomy Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI676MC combines a high-resolution 12.6 MP Sony IMX676 sensor with small 2µm pixels, resolving fine detail on planetary surfaces and small deep-sky targets. Its perfectly square 3552 x 3552 pixel array simplifies mosaic construction, while the 83% peak QE and back-illuminated structure capture faint signal efficiently. With a maximum frame rate of 31.2 FPS at full resolution and a 256MB DDR3 buffer, you can capture sharp frames during moments of steady seeing without dropping data.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSquare 12.6 MP Sensor for Seamless Mosaics\u003c\/h3\u003e\n\u003cp\u003eThe ASI676MC's defining feature is its 1\/1.6\" format, 3552 x 3552 square CMOS sensor. This format eliminates the need for rotating the camera between mosaic panels, streamlining the capture of large targets like the lunar surface or sprawling solar active regions. The 12.6 megapixel resolution gives you the image scale to create vast, high-definition composites without sacrificing detail.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e2µm Pixels \u0026amp; 83% QE for High-Resolution Detail\u003c\/h3\u003e\n\u003cp\u003eWith a pixel size of just 2µm, the ASI676MC is built for high-resolution imaging on long focal length instruments like Schmidt-Cassegrains and Maksutovs. The back-illuminated Sony sensor achieves a peak Quantum Efficiency of 83%, ensuring that a high percentage of incoming photons are converted to signal. This sensitivity is critical for reducing exposure times on planets, which helps freeze atmospheric turbulence.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eZero Amp Glow \u0026amp; 256MB DDR3 Buffer\u003c\/h3\u003e\n\u003cp\u003eZWO engineered the ASI676MC with circuitry that completely eliminates amplifier glow, a common source of noise in CMOS sensors that typically requires dark frame subtraction. This results in cleaner raw data and a more streamlined processing workflow. The onboard 256MB DDR3 buffer ensures stable, high-speed data transfer over USB 3.0, preventing dropped frames during critical planetary video captures.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eZWO ASI676MC vs. ASI178MC\u003c\/h3\u003e\n\u003cp\u003eThe ASI676MC represents a significant evolution from its popular predecessor, the ASI178MC, primarily for planetary and lunar imagers.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eSensor Format:\u003c\/strong\u003e The ASI178MC uses a rectangular 6.4 MP sensor, while the ASI676MC's 12.6 MP square sensor offers double the resolution and is purpose-built for mosaics without camera rotation.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003ePixel Size:\u003c\/strong\u003e The ASI676MC's smaller 2.0µm pixels provide higher resolution sampling compared to the 2.4µm pixels of the ASI178MC, allowing you to resolve finer detail at the same focal length.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eAmp Glow:\u003c\/strong\u003e The ASI178MC can exhibit minor amp glow on longer exposures, a problem completely eliminated by the hardware design of the ASI676MC.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eFull Well \u0026amp; Bit Depth:\u003c\/strong\u003e The ASI178MC has a slight advantage with a deeper full well (15Ke vs 10.55Ke) and 14-bit ADC, giving it more dynamic range for solar or brighter targets. However, for planetary imaging, the ASI676MC's higher resolution and cleaner sensor are often the deciding factors.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eUncooled Design for Planetary and Guiding\u003c\/h3\u003e\n\u003cp\u003eAs an uncooled camera, the ASI676MC is optimized for short-exposure \"lucky imaging\" of the Moon, planets, and Sun (with a proper solar filter). Its lightweight body and ST-4 port also make it a capable, high-resolution autoguider. The lack of a cooling system means thermal noise will become a factor on multi-second exposures, making it less suitable for imaging faint deep-sky objects than a dedicated cooled camera.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the main advantage of the ASI676MC's square sensor?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e3552 x 3552 square sensor\u003c\/strong\u003e is ideal for creating mosaics of large areas like the Moon or Sun. You can capture adjacent panels without rotating the camera, which simplifies both the acquisition process at the telescope and the image stitching process in software.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow will the ASI676MC's 2µm pixels perform on Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAn 8\" f\/10 SCT has a focal length of around 2000mm. With 2µm pixels, this provides good image sampling, but for optimal planetary resolution, you typically want to image between f\/10 and f\/14 (5 to 7 times the pixel size). On typical nights, the native f\/10 focal ratio is already in this range, so \u003cstrong\u003eno Barlow is needed\u003c\/strong\u003e. On nights of excellent seeing, a \u003cstrong\u003e1.5x Barlow lens\u003c\/strong\u003e brings the focal ratio to f\/15, which lets the ASI676MC resolve the finest details in Jupiter's cloud bands.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan the ZWO ASI676MC capture the entire lunar disc in one shot?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWhether the ASI676MC can capture the full Moon depends on your telescope's focal length. On a short refractor with a focal length of 400-500mm, you can easily frame the entire disc. On a longer instrument like an SCT, the 10mm sensor diagonal will only show a portion of the Moon, making it a perfect candidate for creating a high-resolution mosaic.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the ZWO ASI676MC suffer from amp glow?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eNo. The ZWO ASI676MC features a \u003cstrong\u003eZero Amplifier Glow\u003c\/strong\u003e hardware design. The circuitry is engineered to prevent the light leakage that causes amp glow, so you do not need to subtract dark frames to remove it, even on longer exposures for guiding.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the ASI676MC as a guide camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. The ASI676MC is an excellent high-resolution guide camera. It includes a standard \u003cstrong\u003eST-4 guide port\u003c\/strong\u003e to connect directly to your mount. Its high sensitivity and small pixels can detect very faint guide stars and register minute star movements for precise tracking corrections.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy choose the ASI676MC over a camera like the ASI462MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe choice depends on your primary target. The ASI462MC has extreme sensitivity in near-infrared light, making it a specialist for imaging methane bands on Jupiter and Saturn. The \u003cstrong\u003eASI676MC\u003c\/strong\u003e, however, offers a much higher 12.6 MP resolution (vs 2.1 MP) and a square sensor, making it far superior for high-resolution lunar, solar, and general planetary color imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/1.6\" Sony IMX676 BSI CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e12.6 MP (3552 x 3552)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Dimensions\u003c\/td\u003e\n\u003ctd\u003e7.1mm x 7.1mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e10mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQuantum Efficiency (Peak)\u003c\/td\u003e\n\u003ctd\u003e83%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e10.55Ke\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBit Depth\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e31.2 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAmp Glow Control\u003c\/td\u003e\n\u003ctd\u003eZero Amplifier Glow\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e256MB DDR3\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Type\u003c\/td\u003e\n\u003ctd\u003eColor, Uncooled\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eComputer Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd\u003eM42x0.75 Threads, 1.25\" Nosepiece\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Window\u003c\/td\u003e\n\u003ctd\u003eIR-Cut\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSeries\u003c\/td\u003e\n\u003ctd\u003eZWO ASI676\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSKU\u003c\/td\u003e\n\u003ctd\u003eZWO-ASI676MC\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eASI676MC Camera Body\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e2m USB 3.0 Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eST-4 Guide Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eQuick Guide\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":49014001271069,"sku":"ZWO-ASI676MC","price":559.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ZWO-ASI676MC-1.jpg?v=1723061109"},{"product_id":"zwo-asi664mc-color","title":"ZWO ASI664MC Color","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e4.15 Megapixel Sony IMX664 Color CMOS Sensor\u003c\/li\u003e\n\u003cli\u003e2.9µm Pixel Size\u003c\/li\u003e\n\u003cli\u003e91% Peak Quantum Efficiency\u003c\/li\u003e\n\u003cli\u003e95 FPS at Full Resolution\u003c\/li\u003e\n\u003cli\u003e256MB DDR3 Internal Buffer\u003c\/li\u003e\n\u003cli\u003eZero Amplifier Glow\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI664MC Color Astronomy Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI664MC combines a high-resolution 4.15 MP Sony IMX664 sensor with sensitive 2.9µm pixels, making it ideal for detailed planetary, lunar, and solar imaging. Its back-illuminated architecture achieves a peak Quantum Efficiency of 91%, capturing faint signal with minimal noise. A full-resolution frame rate of 95 FPS, supported by a 256MB DDR3 buffer and USB 3.0 interface, ensures you can capture moments of perfect seeing without dropping frames.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony STARVIS 2 Sensor: 91% QE and 2.9µm Pixels\u003c\/h3\u003e\n\u003cp\u003eAt the core of the ASI664MC is Sony's latest STARVIS 2 technology, a back-illuminated (BSI) sensor design that places circuitry behind the photodiode layer. This maximizes light collection, pushing the peak QE to 91% and dramatically improving signal-to-noise ratio. The 2.9µm pixels are an excellent match for short-to-medium focal length refractors and Schmidt-Cassegrains operating with a Barlow lens, resolving fine detail on Jupiter's cloud bands or in lunar rilles.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eZero Amp Glow and 256MB DDR3 Buffer\u003c\/h3\u003e\n\u003cp\u003eThe ASI664MC integrates circuitry that completely eliminates amplifier glow, a common source of noise in CMOS sensors that typically requires calibration frames to remove. This results in cleaner raw data and a more streamlined processing workflow. To handle the massive data stream, a 256MB DDR3 memory buffer ensures stable, high-speed image transfer to your computer over the USB 3.0 connection, preventing data loss even at the maximum frame rate.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e95 FPS at Full 4.15 MP Resolution\u003c\/h3\u003e\n\u003cp\u003eFor planetary imagers, capturing thousands of frames in a short period is critical to overcome atmospheric turbulence. The ASI664MC delivers a sustained 95 frames per second at its full 2704 x 1536 resolution, allowing you to effectively \"freeze\" moments of steady seeing. As an uncooled camera, it excels at this type of short-exposure work; while it can be used for brighter deep-sky objects, thermal noise will become a factor on multi-minute exposures where a cooled camera would be required.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eASI664MC vs. ASI462MC: A Generational Upgrade\u003c\/h3\u003e\n\u003cp\u003eThe ASI664MC serves as a direct successor to the popular ASI462MC, offering significant upgrades for most imaging scenarios.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eASI462MC's Advantage:\u003c\/strong\u003e The ASI462MC maintains a slight edge in extreme near-infrared sensitivity, which can be beneficial for imaging planets like Venus or methane-band imaging of Jupiter and Saturn.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eASI664MC's Advantages:\u003c\/strong\u003e The ASI664MC provides double the resolution (4.15 MP vs. 2.1 MP) and a larger 1\/1.8\" sensor, giving you a wider field of view for lunar mosaics or capturing Jupiter with all its Galilean moons. For general-purpose planetary, lunar, and solar imaging, the higher resolution and larger sensor make the ASI664MC the superior choice.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the optimal focal ratio for the ZWO ASI664MC on planets like Jupiter?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor planetary imaging, the ideal focal ratio is 5 to 7 times the camera's pixel size. With the ASI664MC's \u003cstrong\u003e2.9µm pixels\u003c\/strong\u003e, you should aim for a final focal ratio between f\/14.5 and f\/20.3. If you are using a typical f\/10 Schmidt-Cassegrain telescope, a 1.5x or 2x Barlow lens will place you in this optimal range for resolving the most detail under good seeing conditions.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan the ZWO ASI664MC be used for imaging the Orion Nebula (M42)?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, but with limitations. The ASI664MC is an \u003cstrong\u003euncooled camera\u003c\/strong\u003e, which makes it best suited for short exposures (\"lucky imaging\") of bright targets like planets. While it is sensitive enough to capture bright deep-sky objects like the Orion Nebula (M42) or the Hercules Cluster (M13) with many short exposures, thermal noise will accumulate and degrade image quality on the long, multi-minute exposures needed for fainter targets. For serious deep-sky imaging, a dedicated cooled camera is recommended.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the ZWO ASI664MC's \"Zero Amp Glow\" feature improve images?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAmplifier glow is a faint illumination that appears in the corners of an image, caused by heat from the sensor's readout electronics. On many cameras, this must be removed by subtracting dark frames. The ZWO ASI664MC uses special hardware to prevent this glow from ever being generated, meaning your raw images are cleaner and require less complex calibration during processing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does the 256MB DDR3 buffer in the ZWO ASI664MC do?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e256MB DDR3 buffer\u003c\/strong\u003e acts as a temporary high-speed memory cache for the camera. When imaging at high frame rates like 95 FPS, the data transfer can sometimes be slowed by the computer's processor or hard drive. The buffer stores the images from the sensor, preventing dropped frames and ensuring a smooth, stable data stream to your computer, which is critical for planetary imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the ZWO ASI664MC a good upgrade from the ASI462MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor most users, yes. The ZWO ASI664MC offers double the resolution (\u003cstrong\u003e4.15 MP\u003c\/strong\u003e vs. 2.1 MP), and a larger sensor for a wider field of view. This makes it a more capable and versatile camera for lunar, solar, and general planetary imaging. The only reason to choose the ASI462MC is if you specifically require its slightly higher sensitivity in the near-infrared for specialized imaging, such as methane band.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat software do I need to use the ZWO ASI664MC?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYou will need to download the latest camera drivers from the ZWO website. For image capture, popular free software includes \u003cstrong\u003eSharpCap\u003c\/strong\u003e (Windows) and \u003cstrong\u003eFireCapture\u003c\/strong\u003e (Windows\/Mac\/Linux). You can also control the camera with an ASIAIR device. For processing the captured video files, imagers commonly use AutoStakkert! and RegiStax.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSKU\u003c\/td\u003e\n\u003ctd\u003eZWO-ASI664MC\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/1.8\" Sony IMX664 BSI CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Type\u003c\/td\u003e\n\u003ctd\u003eColor, Uncooled\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eEffective Pixels\u003c\/td\u003e\n\u003ctd\u003e4.15 MP\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Array\u003c\/td\u003e\n\u003ctd\u003e2704 x 1536\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Dimensions\u003c\/td\u003e\n\u003ctd\u003e7.8mm x 4.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e9mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePeak Quantum Efficiency (QE)\u003c\/td\u003e\n\u003ctd\u003e91%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBit Depth\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e95 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e256MB DDR3\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAmp Glow Control\u003c\/td\u003e\n\u003ctd\u003eZero Amplifier Glow\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Window\u003c\/td\u003e\n\u003ctd\u003eAR Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eComputer Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd\u003eM42x0.75 Threads\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Sensor Included?\u003c\/td\u003e\n\u003ctd\u003eNo\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAnti-Dew Heater Included?\u003c\/td\u003e\n\u003ctd\u003eNo\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eHumidity Sensor Included?\u003c\/td\u003e\n\u003ctd\u003eNo\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eASI664MC Camera\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eSensor Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eUSB 3.0 Cable (2m)\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eST4 Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eQuick Guide\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":49346244280605,"sku":"ZWO-ASI664MC","price":419.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ZWO-ASI664MC-Color.jpg?v=1731025631"},{"product_id":"qhyccd-qhy5iii585m-mono","title":"QHYCCD QHY5III585M Mono","description":"\u003c!-- more --\u003e\n\u003cp\u003eIn this latest generation of sensors, the photodiode portion of the pixel well is physically deeper than in previous sensors, allowing photons of longer wavelengths to penetrate deeper into the substrate. This dramatically increases the sensor’s sensitivity to red and near-infrared (NIR) light. The sensor displays almost equal peak sensitivity to NIR light as it does to light in the visible spectrum.\u003c\/p\u003e\n\u003cp\u003eThe IMX585 is a Sony Starvis II processor that enables high sensitivity and high dynamic range (HDR). It also improves sensitivity in the near-infrared range by approximately 1.7 times* compared to the IMX485.\u003c\/p\u003e","brand":"QHYCCD","offers":[{"title":"Default Title","offer_id":49396223475997,"sku":"QHY-110198","price":489.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/QHY5III585M.jpg?v=1732228593"},{"product_id":"qhyccd-qhy5iii568m-mono-1","title":"QHYCCD QHY5III568M Mono","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003eMonochrome Planetary \u0026amp; Guide Camera\u003c\/li\u003e\n\u003cli\u003eHigh-Sensitivity for Short Exposures\u003c\/li\u003e\n\u003cli\u003eCompact 1.25\" Form Factor\u003c\/li\u003e\n\u003cli\u003eIdeal for \"Lucky Imaging\" and Autoguiding\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section-center\"\u003e\n      \u003ch2\u003eQHYCCD QHY5III568M Monochrome CMOS Camera\u003c\/h2\u003e\n      \u003cp\u003eThe QHYCCD QHY5III568M is a dedicated monochrome CMOS camera engineered for two critical astronomical tasks: high-resolution planetary imaging and precision autoguiding. Its design focuses on delivering the sensitivity required to capture fleeting moments of excellent seeing on planets like Jupiter and Saturn, while also serving as a reliable eye for your mount to ensure sharp, round stars during long deep-sky exposures. The monochrome sensor provides maximum detail and sensitivity, making it a workhorse for the serious imager.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eDual-Role Design: A High-Sensitivity Planetary and Guiding Camera\u003c\/h3\u003e\n      \u003cp\u003eThe QHY5III568M is built around a monochrome sensor, which offers a significant sensitivity advantage over color counterparts. For planetary imagers, this means you can use shorter exposures and higher frame rates, increasing your chances of capturing sharp frames through atmospheric turbulence—a technique known as \"lucky imaging.\" The monochrome output allows you to capture luminance data for maximum sharpness or use LRGB filters to create full-color planetary portraits with more detail than a one-shot-color camera can typically resolve.\u003c\/p\u003e\n      \u003cp\u003eAs an autoguider, that same sensitivity allows the camera to detect fainter guide stars, giving you more options for finding a suitable star anywhere in the sky. This is a critical advantage when imaging in star-poor regions or when using an off-axis guider. The camera's compact, lightweight body fits a standard 1.25\" focuser or guider port, adding minimal weight and complexity to your imaging setup.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n\u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat are the main uses for the QHY5III568M camera?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe QHY5III568M is a specialized dual-purpose camera. Its primary functions are \u003cstrong\u003ehigh-frame-rate planetary imaging\u003c\/strong\u003e of objects like Jupiter, Saturn, and Mars, and \u003cstrong\u003ehigh-sensitivity autoguiding\u003c\/strong\u003e for long-exposure deep-sky astrophotography.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhy choose a monochrome camera like the QHY5III568M for planets?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eA monochrome sensor is inherently more sensitive and captures finer detail than a color sensor because every pixel is used to detect light, rather than being filtered for red, green, or blue. For planetary imaging, this allows you to shoot through separate \u003cstrong\u003eL, R, G, and B filters\u003c\/strong\u003e to create a final color image that is significantly sharper and more detailed than what a comparable one-shot-color camera could produce.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the QHY5III568M perform as an autoguider?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eIts high sensitivity makes it an excellent autoguider. It can detect faint guide stars, which is crucial when your target is in a part of the sky with few bright stars. The camera connects to your mount via an ST-4 cable or pulse guiding and works with software like \u003cstrong\u003ePHD2\u003c\/strong\u003e to send tiny corrections to the mount, ensuring your main imaging camera captures sharp, pinpoint stars.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the QHY5III568M for deep-sky photos of nebulae like the Orion Nebula (M42)?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eNo, this camera is not designed for long-exposure deep-sky imaging. While it is excellent for guiding those exposures, its sensor is optimized for the very short exposures (fractions of a second) used in planetary imaging. It lacks the cooling and low-noise architecture needed to take multi-minute exposures of faint deep-sky objects without being overwhelmed by thermal noise.\u003c\/p\u003e\n  \u003c\/div\u003e\n    \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat telescope is a good match for the QHY5III568M to image Saturn's rings?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eTo resolve details like the Cassini Division in Saturn's rings, you need high magnification. The QHY5III568M pairs best with long focal-length telescopes such as a \u003cstrong\u003eSchmidt-Cassegrain (SCT)\u003c\/strong\u003e, \u003cstrong\u003eMaksutov-Cassegrain\u003c\/strong\u003e, or a refractor with a Barlow lens. These systems provide the image scale necessary to make the planet large enough on the sensor for detailed capture.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat software is required to operate the QHY5III568M?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eYou will need to install the QHYCCD drivers for your operating system. For capturing video, popular software choices include \u003cstrong\u003eSharpCap\u003c\/strong\u003e or \u003cstrong\u003eFireCapture\u003c\/strong\u003e. For autoguiding, the standard software is \u003cstrong\u003ePHD2 Guiding\u003c\/strong\u003e. These programs recognize the camera once the drivers are installed.\u003c\/p\u003e\n  \u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003ctable class=\"DAV-specifications\"\u003e\n    \u003ctbody\u003e\n      \n    \u003c\/tbody\u003e\n  \u003c\/table\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cul class=\"DAV-grid\"\u003e\n    \n  \u003c\/ul\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.qhyccd.com\/download\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/qhyccd-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eQHYCCD Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"QHYCCD","offers":[{"title":"Default Title","offer_id":49396226883869,"sku":"QHY-110185","price":558.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/QHY5III568M.jpg?v=1732228747"},{"product_id":"qhyccd-qhy5iii568c-color","title":"QHYCCD QHY5III568C Color","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003eColor CMOS Sensor\u003c\/li\u003e\n\u003cli\u003ePlanetary Imaging Camera\u003c\/li\u003e\n\u003cli\u003eAutoguiding Camera\u003c\/li\u003e\n\u003cli\u003eUSB 3.0 Interface\u003c\/li\u003e\n\u003cli\u003eST-4 Guide Port\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section-center\"\u003e\n      \u003ch2\u003eQHYCCD QHY5III568C Color Planetary and Guide Camera\u003c\/h2\u003e\n      \u003cp\u003eThe QHYCCD QHY5III568C is engineered as a versatile, dual-purpose camera, serving as both a high-frame-rate planetary imager and a sensitive autoguider. Its color sensor simplifies the process of capturing planets, the Moon, and the Sun (with a proper solar filter), delivering vibrant images in a single shot. This same sensitivity makes it a reliable guide camera, capable of tracking faint stars to ensure sharp, pinpoint results during long-exposure deep-sky astrophotography.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eCapturing Solar System Targets in Color\u003c\/h3\u003e\n      \u003cp\u003eThe QHY5III568C is designed for high-resolution imaging of our solar system neighbors. The built-in color sensor array eliminates the need for a filter wheel and monochrome imaging sequences, streamlining your workflow at the telescope. This one-shot-color capability is ideal for capturing fleeting moments of steady seeing, allowing you to record detailed images of Jupiter's cloud bands, Saturn's rings, and Martian surface features with straightforward acquisition and processing.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eA Sensitive Guide Camera for Deep-Sky Imaging\u003c\/h3\u003e\n      \u003cp\u003eBeyond its planetary role, the QHY5III568C functions as a capable autoguider. When connected to your mount's guide port, it can detect and lock onto faint guide stars, issuing precise corrections to counteract tracking errors from your mount's drive system. This is critical for obtaining sharp, round stars in multi-minute exposures of nebulae and galaxies with a separate imaging telescope.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n\u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat makes the QHY5III568C a good choice for planetary imaging?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe \u003cstrong\u003eQHY5III568C\u003c\/strong\u003e is designed for planetary work, which involves capturing thousands of frames in a short time (a technique called \"lucky imaging\"). Its color sensor simplifies this process by capturing full-color data in every frame, eliminating the complexity of using separate red, green, and blue filters.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the QHY5III568C perform as an autoguider for deep-sky objects?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eAs an autoguider, the \u003cstrong\u003eQHY5III568C\u003c\/strong\u003e connects to an off-axis guider or a separate guide scope. It takes short, continuous exposures of a star near your imaging target. Guiding software like PHD2 analyzes the star's position and sends correction commands to the telescope mount via the camera's ST-4 port, ensuring your main camera captures sharp, untrailed images of faint targets like the Orion Nebula (M42).\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eIs the QHY5III568C suitable for imaging Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eYes, this is an excellent combination. An 8\" SCT provides the focal length needed to achieve a large image scale on Jupiter. The \u003cstrong\u003eQHY5III568C\u003c\/strong\u003e would be used with a 2x or 3x Barlow lens to bring out fine details like the Great Red Spot and individual cloud bands. Its ability to capture high-speed video is essential for freezing moments of atmospheric stability.\u003c\/p\u003e\n  \u003c\/div\u003e\n    \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eDo I need any filters to use the QHY5III568C?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eFor most planetary and guiding work, no color filters are needed since the \u003cstrong\u003eQHY5III568C\u003c\/strong\u003e is a color camera. However, an \u003cstrong\u003eIR\/UV Cut filter\u003c\/strong\u003e is highly recommended to sharpen the image and improve color balance, as most telescopes are not designed to focus infrared and ultraviolet light at the same point as visible light. For solar imaging, a certified, full-aperture solar filter must be placed on the front of your telescope.\u003c\/p\u003e\n  \u003c\/div\u003e\n    \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat software is compatible with the QHY5III568C?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe \u003cstrong\u003eQHY5III568C\u003c\/strong\u003e is supported by QHYCCD's own drivers and capture software. It is also compatible with a wide range of third-party astrophotography software via its ASCOM driver. For planetary capture, popular choices include \u003cstrong\u003eFireCapture\u003c\/strong\u003e and \u003cstrong\u003eSharpCap\u003c\/strong\u003e. For autoguiding, it works seamlessly with \u003cstrong\u003ePHD2 Guiding\u003c\/strong\u003e.\u003c\/p\u003e\n  \u003c\/div\u003e\n    \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the QHY5III568C connect to a telescope?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe QHY5III series cameras typically use a 1.25\" nosepiece form factor. This allows the \u003cstrong\u003eQHY5III568C\u003c\/strong\u003e to be inserted directly into any standard 1.25\" focuser or accessory, just like an eyepiece. It connects to a computer via a USB cable for data transfer and power, and has a separate ST-4 port for connecting to a telescope mount's autoguide input.\u003c\/p\u003e\n  \u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003ctable class=\"DAV-specifications\"\u003e\n    \u003ctbody\u003e\n      \n    \u003c\/tbody\u003e\n  \u003c\/table\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cul class=\"DAV-grid\"\u003e\n    \n  \u003c\/ul\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.qhyccd.com\/download\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/qhyccd-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eQHYCCD Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"QHYCCD","offers":[{"title":"Default Title","offer_id":49396230816029,"sku":"QHY-110184","price":558.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/QHY5III568M.jpg?v=1732228747"},{"product_id":"qhyccd-qhy5iii462m-mono","title":"QHYCCD QHY5III462M Mono","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e2.0 Megapixel Sony IMX462 BSI CMOS Sensor\u003c\/li\u003e\n\u003cli\u003e2.9µm pixels and 1920x1080 resolution\u003c\/li\u003e\n\u003cli\u003eExceptional Near-Infrared (NIR) sensitivity\u003c\/li\u003e\n\u003cli\u003eUltra-low 0.5e- read noise with sHCG mode\u003c\/li\u003e\n\u003cli\u003e135 FPS at full resolution via USB 3.0\u003c\/li\u003e\n\u003cli\u003eIncludes IR850nm pass filter\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eQHYCCD QHY5III462M Mono Camera\u003c\/h2\u003e\n\u003cp\u003eThe QHYCCD QHY5III462M Mono camera leverages Sony's 6th generation IMX462 STARVIS sensor to deliver category-defining near-infrared sensitivity and exceptionally low noise for planetary imaging. Its 2.0 Megapixel, 1920x1080 sensor has 2.9µm pixels perfectly suited for short focal ratio telescopes, while the camera's back-illuminated structure and Super High Conversion Gain (sHCG) technology achieve an ultra-low read noise of just 0.5e-. Capable of capturing full-frame video at 135 FPS over USB 3.0, the QHY5III462M is engineered to freeze atmospheric turbulence and reveal fine details on Jupiter, Saturn, and Mars.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003esHCG and 0.5e- Read Noise for Planetary Stacking\u003c\/h3\u003e\n\u003cp\u003eThe QHY5III462M features Sony's Super High Conversion Gain (sHCG) technology, which dramatically reduces read noise to an exceptionally low 0.5e- at high gain settings. This is a critical advantage for planetary \"lucky imaging,\" where hundreds or thousands of short exposures are stacked to overcome atmospheric seeing. With noise this low, the signal from faint planetary details is preserved in each sub-frame, leading to a final stacked image with significantly higher contrast and clarity.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eEnhanced NIR Sensitivity: A Methane Band Advantage at 850nm\u003c\/h3\u003e\n\u003cp\u003eA key innovation in the IMX462 sensor is its profound sensitivity to near-infrared (NIR) light. The sensor's photodiodes are physically deeper, allowing it to capture long-wavelength photons with a peak quantum efficiency around 800nm that rivals its efficiency in the visible spectrum. This makes the QHY5III462M an ideal camera for methane band imaging of Jupiter and Saturn, which centers around 880nm. To leverage this capability, the camera includes an IR850nm pass filter, allowing you to isolate this wavelength for high-contrast views of the gas giants' atmospheric features.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e135 FPS Capture at 1920x1080 Resolution\u003c\/h3\u003e\n\u003cp\u003ePowered by a USB 3.0 interface, the QHY5III462M streams its full 1920x1080 resolution at up to 135 frames per second (at 8-bit). This high frame rate is essential for mitigating the effects of atmospheric turbulence. By capturing a massive volume of frames in a short period, you increase the probability of catching fleeting moments of perfect seeing, which can then be selected and stacked to produce a final image far sharper than any single frame.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eQHY5III462M vs. QHY5III290M: The NIR Successor\u003c\/h3\u003e\n\u003cp\u003eThe QHY5III462M shares the same 2.9µm pixel size and 1920x1080 resolution as the legendary QHY5III290M, but its key advantage lies in its sensor generation. While both cameras offer extremely low read noise, the QHY5III462M's back-illuminated IMX462 sensor provides a dramatic boost in sensitivity in red and near-infrared light. For imagers focused on methane band or other long-wavelength planetary science, the 462M is the clear successor, offering access to data the 290M's sensor cannot efficiently capture.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eCompact 88g Body with ST-4 Guiding and C-Mount\u003c\/h3\u003e\n\u003cp\u003eHoused in the standard 1.25-inch eyepiece-style body, the QHY5III462M weighs a mere 88g, adding minimal weight to your imaging train and making balancing easy. It includes a standard ST-4 guide port for use as a high-sensitivity autoguider on a separate guide scope. The camera also features a C-mount thread, providing a short 12mm back focus distance for use with microscopes, lenses, and other specialized optical systems.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the main advantage of the QHY5III462M's sHCG mode?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003e\u003cstrong\u003eSuper High Conversion Gain (sHCG)\u003c\/strong\u003e is a sensor mode that allows the camera to achieve its lowest read noise of \u003cstrong\u003e0.5e-\u003c\/strong\u003e. For planetary imaging, where you use high gain and very short exposures, this mode ensures that the faint signal from the planet is not lost in the camera's own electronic noise, resulting in cleaner data and sharper final images after stacking.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the QHY5III462M's NIR sensitivity help when imaging Jupiter?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eJupiter's atmosphere has prominent features that are best seen in the methane absorption band around 880nm. The QHY5III462M is extremely sensitive in this near-infrared (NIR) region, far more so than older sensors. Using the included \u003cstrong\u003eIR850nm filter\u003c\/strong\u003e, you can capture high-contrast images that highlight Jupiter's high-altitude clouds and storms, which appear bright against the darker, methane-absorbing belts.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the QHY5III462M a good choice for guiding an 8\" SCT on an equatorial mount?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, absolutely. With its high sensitivity and low read noise, the QHY5III462M is an excellent autoguider. The \u003cstrong\u003e2.9µm pixels\u003c\/strong\u003e provide good sampling resolution for guiding, and its NIR sensitivity helps detect faint guide stars that might be invisible to other guide cameras, ensuring a stable lock for long exposures.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDo I need an external power supply for the QHY5III462M?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eNo. The QHY5III462M is powered entirely through its \u003cstrong\u003eUSB 3.0 Type-B port\u003c\/strong\u003e. This simplifies your cable management at the telescope, as no separate 12V power cable is required for camera operation.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy would I choose the mono QHY5III462M over the color version?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe mono QHY5III462M offers higher ultimate resolution and sensitivity compared to its color counterpart. By shooting through separate Red, Green, and Blue filters, you can capture more detail and have greater control over the final color balance. The mono sensor is also essential for narrowband imaging techniques, such as using the included \u003cstrong\u003eIR850nm filter\u003c\/strong\u003e for methane band work.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does the 12mm back focal length on the QHY5III462M mean?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e12mm back focal length\u003c\/strong\u003e is the distance from the front C-mount threads to the sensor. This short distance is advantageous when using the camera with accessories like filter wheels or off-axis guiders, as it leaves more room in the optical path to reach focus. It is also a standard distance for many C-mount lenses and industrial applications.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Sensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX462, Back-Illuminated (BSI)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003eTypical 1\/2.8 inch\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eEffective Pixels\u003c\/td\u003e\n\u003ctd\u003e2.0 Megapixels (1920 x 1080)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9µm x 2.9µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e0.5e- (sHCG Mode)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e12ke-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e135 FPS @ 8-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit (output as 16-bit and 8-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Time Range\u003c\/td\u003e\n\u003ctd\u003e7µs - 900sec\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eComputer Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 Type-B\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4 Compatible\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd\u003e1.25-inch, C-Mount\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOptical Window\u003c\/td\u003e\n\u003ctd\u003eAR Anti-reflection Glass\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eIncluded Filter\u003c\/td\u003e\n\u003ctd\u003eIR850nm Pass Filter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e88g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eQHY5III462M Camera Body\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eIR 850nm Pass Filter\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.qhyccd.com\/download\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/qhyccd-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eQHYCCD Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"QHYCCD","offers":[{"title":"Default Title","offer_id":49396232454429,"sku":"QHY-110131","price":349.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/products\/QHYCCD-QHY5III462C-Color-1__01192.1595653764.1280.1280.jpg?v=1684339039"},{"product_id":"qhyccd-qhy5iii678m-mono","title":"QHYCCD QHY5III678M Mono","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e8.4 Megapixel Sony IMX678 BSI Sensor\u003c\/li\u003e\n\u003cli\u003e2.0µm Pixel Size\u003c\/li\u003e\n\u003cli\u003e43 FPS at 8-bit Full Resolution\u003c\/li\u003e\n\u003cli\u003e512MB DDR3 Image Buffer\u003c\/li\u003e\n\u003cli\u003eStandard ST-4 Guide Port\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section-center\"\u003e\n      \u003ch2\u003eQHYCCD QHY5III678M Mono Planetary \u0026amp; Guiding Camera\u003c\/h2\u003e\n      \u003cp\u003eThe QHYCCD QHY5III678M combines Sony's 8.4 Megapixel IMX678 back-illuminated sensor with a deep 512MB DDR3 buffer to deliver high-resolution planetary images at up to 43 FPS. Its 2.0µm pixels are ideal for sampling celestial targets with a wide range of telescopes, while its extremely low 0.57e- read noise ensures faint details are captured cleanly. With exceptional sensitivity in the near-infrared spectrum and an included IR850nm filter, this camera is built for advanced techniques like methane band imaging of gas giants.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eSony IMX678 BSI Sensor: 8.4 MP and High Near-Infrared Sensitivity\u003c\/h3\u003e\n      \u003cp\u003eAt the core of the QHY5III678M is an 8.4 MP Sony IMX678 sensor, offering a 3856x2180 resolution for capturing wide lunar landscapes or fine details on Jupiter's cloud bands. The back-illuminated (BSI) architecture and small 2.0µm pixels maximize quantum efficiency for bright, high-contrast images. This sensor exhibits remarkable sensitivity into the near-infrared, a key advantage for cutting through atmospheric turbulence and isolating specific spectral features with the included IR850nm pass filter.\u003c\/p\u003e\n      \u003cul\u003e\n        \u003cli\u003e\n\u003cstrong\u003eLow Read Noise:\u003c\/strong\u003e With a minimum read noise of just 0.57e-, the camera preserves faint signal, critical for low-contrast planetary features and for its secondary role as a sensitive guide camera.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003e12-bit ADC:\u003c\/strong\u003e The 12-bit A\/D converter provides excellent dynamic range, capturing subtle brightness variations from the sunlit limb of a planet to its terminator without clipping highlights or crushing shadows.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003eFull Well Capacity:\u003c\/strong\u003e A 9ke- full well capacity helps prevent pixel saturation on bright targets like Jupiter or Mars, allowing for longer exposures when needed for specific filter bandpasses.\u003c\/li\u003e\n      \u003c\/ul\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n    \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003e43 FPS Planetary Capture with a 512MB DDR3 Buffer\u003c\/h3\u003e\n      \u003cp\u003eFor planetary imaging, capturing a high volume of frames in a short time is essential to \"freeze\" moments of steady seeing. The QHY5III678M streams its full 8.4 MP resolution at 43 FPS in 8-bit mode or 22 FPS in 16-bit mode. To ensure this data stream is stable and free of dropped frames, QHY has equipped the camera with a substantial 512MB DDR3 image buffer—a significant advantage over cameras that rely solely on the speed of the USB bus.\u003c\/p\u003e\n       \u003cul\u003e\n        \u003cli\u003e\n\u003cstrong\u003eHigh ROI Frame Rates:\u003c\/strong\u003e By selecting a Region of Interest (ROI), frame rates increase dramatically, reaching 85 FPS for a 1080-line window, ideal for keeping a planet centered in the frame while maximizing capture speed.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003eUSB 3.0 Type-C Interface:\u003c\/strong\u003e A modern and reliable USB Type-C port provides the high bandwidth necessary for these frame rates, ensuring a stable connection to your acquisition computer.\u003c\/li\u003e\n      \u003c\/ul\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eA 90g Platform with ST-4 and C-Mount Versatility\u003c\/h3\u003e\n      \u003cp\u003eEngineered as both a primary planetary imager and a high-performance autoguider, the QHY5III678M weighs only 90g, minimizing its impact on telescope balance. It includes a standard ST-4 port for direct connection to nearly any equatorial mount. The camera's front interface provides multiple mounting options, including a 1.25-inch nosepiece for standard focusers and both C-mount and CS-mount threads for use with lenses or specialized optical systems.\u003c\/p\u003e\n       \u003cul\u003e\n        \u003cli\u003e\n\u003cstrong\u003eDual Back Focus:\u003c\/strong\u003e The camera presents two native back focus distances, 17mm and 8mm. This flexibility is critical for achieving focus with different accessories like off-axis guiders, filter wheels, or C\/CS-mount lenses which have strict spacing requirements.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003eAR Coated Window:\u003c\/strong\u003e The monochrome version features a high-transmission anti-reflection coated optical window, maximizing light throughput across the visual and near-infrared spectrum.\u003c\/li\u003e\n      \u003c\/ul\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n       \u003ch3\u003eQHY5III678M vs. QHY5III178M: Key Sensor and Buffer Upgrades\u003c\/h3\u003e\n       \u003cp\u003eThe QHY5III678M is a direct successor to the popular QHY5III178M, offering significant improvements in resolution and data handling. While the 178M was a capable performer, the 678M's larger sensor and buffer make it a more powerful tool for modern planetary imaging.\u003c\/p\u003e\n       \u003cul\u003e\n        \u003cli\u003e\n\u003cstrong\u003eResolution:\u003c\/strong\u003e The QHY5III678M provides a major resolution increase to 8.4 MP, up from the 6.1 MP of the 178M. This allows for larger, more detailed captures of the Moon and Sun.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003ePixel Size:\u003c\/strong\u003e The 678M uses smaller 2.0µm pixels compared to the 178M's 2.4µm pixels. This can provide better image sampling (resolution per arcsecond) on telescopes with shorter focal lengths without needing a Barlow lens.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003eImage Buffer:\u003c\/strong\u003e The most critical upgrade is the buffer size. The QHY5III678M features a 512MB DDR3 buffer, four times larger than the 128MB buffer in the 178M, ensuring much more reliable, drop-free video capture at high frame rates.\u003c\/li\u003e\n       \u003c\/ul\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat makes the QHY5III678M a good choice for near-infrared imaging?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe QHY5III678M uses Sony's IMX678 sensor, which has exceptionally high quantum efficiency in the near-infrared (NIR) spectrum, particularly around the 850nm wavelength. This makes it highly effective for techniques like methane band imaging of Jupiter and Saturn, or for using an IR-pass filter to cut through atmospheric turbulence for sharper lunar and planetary detail. The camera includes an \u003cstrong\u003eIR850nm filter\u003c\/strong\u003e to get you started with these techniques immediately.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the purpose of the 512MB DDR3 buffer in the QHY5III678M?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe \u003cstrong\u003e512MB DDR3 buffer\u003c\/strong\u003e acts as a temporary high-speed memory cache for image frames before they are sent to the computer via USB. This is crucial for high-speed planetary imaging because it prevents data loss (dropped frames) if the host computer's USB bus is temporarily busy. A large buffer ensures a smooth, stable video stream, which is essential for lucky imaging software like AutoStakkert!.\u003c\/p\u003e\n  \u003c\/div\u003e\n    \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eCan the QHY5III678M be used for deep-sky imaging?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eWhile the QHY5III678M has very low read noise, it is primarily designed for planetary, lunar, and solar imaging. It is an uncooled camera, so long exposures (typically over 30 seconds) will show significant thermal noise. It is best suited for \"lucky imaging\" of brighter deep-sky objects like planetary nebulae or globular clusters using thousands of very short exposures, but a dedicated, cooled astronomy camera is a better choice for faint galaxies and nebulae.\u003c\/p\u003e\n  \u003c\/div\u003e\n    \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eHow will the QHY5III678M's 2.0µm pixels perform on Jupiter with an 8-inch f\/10 SCT?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eAn 8\" f\/10 SCT has a focal length of roughly 2000mm. With the QHY5III678M's \u003cstrong\u003e2.0µm pixels\u003c\/strong\u003e, this combination yields an image scale of 0.21 arcseconds per pixel. This is an excellent sampling rate for high-resolution planetary imaging, falling well within the ideal range for capturing fine detail on Jupiter under good seeing conditions. You would likely not need a Barlow lens, allowing for a brighter image and faster frame rates.\u003c\/p\u003e\n  \u003c\/div\u003e\n    \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eIs the QHY5III678M a good choice for methane band imaging of Saturn?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eYes, it's an excellent choice. Methane band filters transmit light around 890nm, a wavelength where the IMX678 sensor retains very high sensitivity. Combined with its low read noise (\u003cstrong\u003e0.57e-\u003c\/strong\u003e), the QHY5III678M can capture a strong signal through this dark filter, making it ideal for highlighting the atmospheric features of Saturn and Jupiter that are prominent in this part of the spectrum.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat do the 8mm and 17mm back focus options on the QHY5III678M allow me to do?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe dual back focus options provide flexibility for connecting different accessories. The shorter \u003cstrong\u003e8mm back focus\u003c\/strong\u003e is ideal for C-mount and CS-mount lenses, which require the sensor to be very close to the lens threads. The longer \u003cstrong\u003e17mm back focus\u003c\/strong\u003e is better suited for standard astronomy configurations, providing the correct spacing when using the 1.25\" nosepiece with filter wheels, off-axis guiders, or Barlow lenses.\u003c\/p\u003e\n  \u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003ctable class=\"DAV-specifications\"\u003e\n    \u003ctbody\u003e\n      \u003ctr\u003e\n\u003ctd\u003eImage Sensor\u003c\/td\u003e\n\u003ctd\u003eSony IMX678 BSI CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003e1\/1.8-inch\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eMono\/Color\u003c\/td\u003e\n\u003ctd\u003eMonochrome\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eEffective Pixels\u003c\/td\u003e\n\u003ctd\u003e8.4 Megapixels (3856 x 2180)\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.0µm x 2.0µm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e9,000e-\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e0.57e- to 3.3e-\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eA\/D Converter\u003c\/td\u003e\n\u003ctd\u003e12-bit (output as 16-bit and 8-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e512MB DDR3 Memory\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eMax Frame Rate (Full)\u003c\/td\u003e\n\u003ctd\u003e43 FPS @ 8-bit, 22 FPS @ 16-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eROI Frame Rate (1080 lines)\u003c\/td\u003e\n\u003ctd\u003e85 FPS @ 8-bit, 43.5 FPS @ 16-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eROI Frame Rate (640 lines)\u003c\/td\u003e\n\u003ctd\u003e140 FPS @ 8-bit, 71 FPS @ 16-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eExposure Time Range\u003c\/td\u003e\n\u003ctd\u003e11µs - 900s\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eComputer Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 Type-C\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd\u003e1.25-inch, CS-Mount, C-Mount\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e17mm or 8mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eOptical Window\u003c\/td\u003e\n\u003ctd\u003eAR Anti-reflection Glass\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eIncluded Filter\u003c\/td\u003e\n\u003ctd\u003eIR850nm Pass Filter\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e90g\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003c\/tbody\u003e\n  \u003c\/table\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cul class=\"DAV-grid\"\u003e\n    \u003cli class=\"DAV-grid-item\"\u003e\n      \u003cdiv\u003e\n        \u003cp class=\"DAV-item-title\"\u003eQHY5III678M Camera Body\u003c\/p\u003e\n        \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n      \u003c\/div\u003e\n    \u003c\/li\u003e\n  \u003c\/ul\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.qhyccd.com\/download\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/qhyccd-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eQHYCCD Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"QHYCCD","offers":[{"title":"Default Title","offer_id":49396233568541,"sku":"QHY-110134","price":489.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/QHY5III678M.jpg?v=1732229310"},{"product_id":"zwo-asi585mm-p-mono","title":"ZWO ASI585MM-P Mono","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e8.29 Megapixel (3840x2160) Sony IMX585 Monochrome Sensor\u003c\/li\u003e\n\u003cli\u003eHigh 91% Peak Quantum Efficiency for Maximum Signal\u003c\/li\u003e\n\u003cli\u003e2.9µm Pixels for High-Resolution Planetary and DSO Imaging\u003c\/li\u003e\n\u003cli\u003e512MB DDR3 Buffer Ensures Stable Data Transfer at 47 FPS\u003c\/li\u003e\n\u003cli\u003eTEC Cooling Reduces Thermal Noise for Clean Long Exposures\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI585MM Pro USB3.0 Monochrome Astronomy Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI585MM Pro pairs a 4K resolution, 8.29 MP Sony IMX585 sensor with small 2.9µm pixels to resolve fine detail on planetary targets and compact deep-sky objects. Its back-illuminated architecture achieves a peak Quantum Efficiency of 91%, capturing faint signal that other sensors miss. A 512MB DDR3 buffer sustains a full-resolution frame rate of 47 FPS over USB 3.0, preventing dropped frames during critical lucky imaging sequences.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e4K Resolution from the 8.29 MP Sony IMX585 Sensor\u003c\/h3\u003e\n\u003cp\u003eAt the core of the ASI585MM Pro is a 1\/1.2\" format Sony CMOS sensor with a 3840 x 2160 pixel array. The 2.9µm pixel size is small enough to sample targets critically on short-focal-length refractors while providing the resolution needed for detailed lunar and planetary imaging with larger instruments. As a monochrome camera, it directs all incoming light to each pixel without the light loss inherent to a color filter array, maximizing its sensitivity to faint structures.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e91% Peak QE and Zero Amp Glow for Deep-Sky Imaging\u003c\/h3\u003e\n\u003cp\u003eWith a peak QE of 91%, the ASI585MM Pro converts the vast majority of photons into usable signal, a critical factor for imaging faint nebulae and galaxies. This high sensitivity is complemented by ZWO's zero amplifier glow circuitry, which eliminates a common source of noise and gradients in long-exposure frames. The result is cleaner raw data that requires less aggressive processing to reveal faint details against a dark sky background.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eTEC Cooling and 512MB DDR3 Buffer\u003c\/h3\u003e\n\u003cp\u003eTwo-stage thermoelectric cooling (TEC) actively reduces the sensor's temperature, which is the primary defense against thermal noise during long exposures required for deep-sky astrophotography. For high-speed planetary work, the onboard 512MB DDR3 memory buffer ensures stable, high-speed data transfer to your computer, even at the maximum 47 FPS rate. This combination makes the camera a true hybrid, capable of producing low-noise, single-frame deep-sky images and thousands of high-speed subframes for planetary stacking.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eASI585MM Pro vs. ASI585MC Pro: Monochrome Signal Advantage\u003c\/h3\u003e\n\u003cp\u003eCompared to its one-shot-color sibling, the ASI585MC Pro, the ASI585MM Pro holds a significant advantage in raw sensitivity and resolution. The primary trade-off is workflow complexity, as the monochrome camera requires LRGB or narrowband filters and a filter wheel to produce a color image.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eASI585MM Pro (Mono):\u003c\/strong\u003e Captures the highest possible detail and signal by using every one of its 8.29 million pixels for luminance data. It is the superior choice for narrowband imaging of emission nebulae or for imagers seeking maximum resolution on any target.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eASI585MC Pro (Color):\u003c\/strong\u003e Delivers a full-color image in a single exposure, simplifying the capture process. This convenience comes at the cost of reduced signal per pixel, as the Bayer matrix filters light, lowering the effective quantum efficiency compared to its mono counterpart.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eNative M42 Interface and Connection Flexibility\u003c\/h3\u003e\n\u003cp\u003eThe camera body features a standard M42x0.75 female thread for direct connection to most astronomical accessories. ZWO includes a comprehensive set of adapters and extenders, including M42-M48 and 1.25\" nosepieces, to facilitate correct spacing with filter wheels, off-axis guiders, and focal reducers. The built-in USB 2.0 hub provides two extra ports for managing accessories like a guide camera or electronic focuser, reducing cable clutter from the mount to the computer.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat makes the ZWO ASI585MM Pro a hybrid planetary and deep-sky camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ASI585MM Pro combines features ideal for both disciplines. Its 2.9µm pixels and 47 FPS frame rate are excellent for \"lucky imaging\" the planets, while its TEC cooling, 91% QE, and zero amp glow are essential for clean, long-exposure deep-sky astrophotography.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the ASI585MM Pro perform on Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor planetary imaging, the ideal focal ratio is 5 to 7 times the camera's pixel size. With the ASI585MM Pro's 2.9µm pixels, the target focal ratio is between f\/14.5 and f\/20.3. On an f\/10 SCT, using a 1.5x or 2x Barlow lens will place the system in this optimal range, allowing you to resolve fine details in Jupiter's cloud bands and the Great Red Spot under good seeing conditions.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the ASI585MM Pro a good choice for imaging the Orion Nebula (M42) with a fast refractor?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, it's an excellent match. The camera's high 91% QE is particularly effective at capturing the faint, extended nebulosity of M42. When paired with a fast refractor (f\/4 to f\/6), the 12.85mm sensor diagonal can frame the entire nebula, including the Running Man Nebula, while the 2.9µm pixels provide high-resolution sampling of the Trapezium star cluster at the core.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy is a monochrome camera like the ASI585MM Pro more sensitive than a color camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eA monochrome sensor allows all incoming light to fall on each pixel. A color camera uses a Bayer matrix (a grid of red, green, and blue filters) over the pixels, which blocks roughly two-thirds of the light from reaching any given pixel. By avoiding this light loss, the ASI585MM Pro achieves higher overall sensitivity, especially for narrowband imaging where all light is of a single wavelength.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDo I need an external power supply for the ASI585MM Pro?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. The camera does not run from USB power alone. To operate the camera, including its TEC cooling system, you must connect a separate 12V DC power supply (not included). Without external power, the camera will not operate.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the main trade-off when choosing the ZWO ASI585MM Pro?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe primary trade-off is complexity. To create color images, the ASI585MM Pro requires a filter wheel and a set of LRGB (Luminance, Red, Green, Blue) or narrowband filters. This increases cost, weight, and the number of steps in both image acquisition and processing compared to a one-shot-color camera, but it delivers the highest possible image quality.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSKU\u003c\/td\u003e\n\u003ctd\u003eZWO-ASI585MM-P\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Series\u003c\/td\u003e\n\u003ctd\u003eZWO ASI585\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/1.2\" Sony IMX585 BSI CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Dimensions\u003c\/td\u003e\n\u003ctd\u003e11.2mm x 6.3mm (12.85mm diagonal)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e8.29 MP (3840 x 2160)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9 µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eColor\/Mono\u003c\/td\u003e\n\u003ctd\u003eMonochrome\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCooling\u003c\/td\u003e\n\u003ctd\u003eCooled (TEC)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQuantum Efficiency (Peak)\u003c\/td\u003e\n\u003ctd\u003e91%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e38.7Ke\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBit Depth\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e47 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAmp Glow Control\u003c\/td\u003e\n\u003ctd\u003eZero Amplifier Glow\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e512MB DDR3\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd\u003eM42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eComputer Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuiding Sensor\u003c\/td\u003e\n\u003ctd\u003eNo\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDimensions\u003c\/td\u003e\n\u003ctd\u003e78mm x 73.8mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e1.04 lb.\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOS Compatibility\u003c\/td\u003e\n\u003ctd\u003eWindows, Linux \u0026amp; Mac OSX\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eASI585MM Pro Cooled Camera\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eM48-M42 Adapter\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eUSB 3.0 Cable (2m)\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eUSB 2.0 Cables (0.5m)\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 2\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eM42-M48 16.5mm Extender\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eM42-M42 21mm Extender\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eM42-1.25\" Adapter\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eSpacers\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 4\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e2\" Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eCamera Bag\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eQuick Guide\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":49798846808349,"sku":"ZWO-ASI585MM-P","price":989.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ZWO-ASI585MM-P-1.jpg?v=1742318721"},{"product_id":"zwo-asi585mm-mono","title":"ZWO ASI585MM Mono","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e8.29 Megapixel (3840 x 2160) Monochrome Sensor\u003c\/li\u003e\n\u003cli\u003e2.9µm Pixel Size\u003c\/li\u003e\n\u003cli\u003e91% Peak Quantum Efficiency\u003c\/li\u003e\n\u003cli\u003e46.9 FPS at Full Resolution\u003c\/li\u003e\n\u003cli\u003e256MB DDR3 Buffer\u003c\/li\u003e\n\u003cli\u003eZero Amplifier Glow\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI585MM USB3.0 Monochrome Astronomy Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI585MM Mono combines a high-resolution 8.29 MP Sony IMX585 sensor with sensitive 2.9µm pixels, engineered for high-magnification lunar and planetary imaging. Its back-illuminated architecture achieves a peak Quantum Efficiency of 91%, while the onboard 256MB DDR3 buffer sustains a full-resolution frame rate of 46.9 FPS over USB 3.0 without dropping frames. Zero Amp Glow circuitry ensures the 1\/1.2\" sensor produces exceptionally clean data, which is critical for stacking thousands of short exposures in planetary imaging and Electronically Assisted Astronomy (EAA).\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony IMX585 Sensor: 91% Peak QE from a 1\/1.2\" Monochrome Chip\u003c\/h3\u003e\n\u003cp\u003eAt the core of the ASI585MM is a Sony STARVIS 2 sensor designed for extreme low-light sensitivity. The monochrome design removes the Bayer matrix, allowing every one of the 8.29 million pixels to capture the full luminance signal, resulting in a significant increase in detail and signal-to-noise ratio over a color equivalent. This raw sensitivity, quantified by its 91% peak QE, allows you to capture fainter details with shorter exposures, a key advantage when imaging planets or using narrowband filters for EAA.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e46.9 FPS at 8.29 MP: Sustained Transfer with a 256MB DDR3 Buffer\u003c\/h3\u003e\n\u003cp\u003ePlanetary imaging relies on \"lucky imaging\", capturing thousands of frames to freeze moments of steady atmospheric seeing. The ASI585MM captures full 3840 x 2160 frames at 46.9 FPS, a rate that would overwhelm a direct USB connection. To solve this, a 256MB DDR3 memory buffer ensures stable, drop-free data transmission to your computer, preserving the integrity of your capture session. This high-speed capability, combined with the camera's Zero Amp Glow design, produces clean, stackable video files essential for resolving fine details on Jupiter's cloud bands or in the Cassini Division of Saturn's rings.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eASI585MM vs. ASI585MC: Monochrome Sensitivity vs. One-Shot Color\u003c\/h3\u003e\n\u003cp\u003eThe primary difference between the ASI585MM (Monochrome) and its sibling, the ASI585MC (Color), lies in how they capture light. The color version offers the convenience of capturing a full-color image in a single shot, which is ideal for quick setups. However, the ASI585MM provides superior raw data for the discerning imager.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eHigher Resolution \u0026amp; Sensitivity:\u003c\/strong\u003e Without a color filter array, the ASI585MM uses every pixel for luminance, delivering a sharper, more detailed image and capturing more signal in the same amount of time.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eNarrowband Imaging:\u003c\/strong\u003e The monochrome sensor is the only way to effectively use specialized narrowband filters (H-alpha, OIII, SII) for imaging emission nebulae, a capability the color camera lacks.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eTrade-off:\u003c\/strong\u003e Achieving a color image with the ASI585MM requires a filter wheel and LRGB filters, adding complexity and cost to the imaging train. For maximum detail, the monochrome version is the clear choice; for simplicity, the color version is more direct.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e6.5mm \/ 17.5mm Back Focus and Physical Connections\u003c\/h3\u003e\n\u003cp\u003eThe ASI585MM provides flexible connection options for any optical train. A standard USB 3.0 port provides the 5Gbps bandwidth needed for high-frame-rate captures, while an ST-4 port allows direct connection to a mount for autoguiding. The camera body features native back focus distances of 6.5mm and 17.5mm, accommodating different accessory configurations. The 17.5mm spacing is standard for use with filter wheels and off-axis guiders, while the 6.5mm option is ideal for setups with strict spacing requirements, such as when used with specific focal reducers or camera lenses.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the ZWO ASI585MM best for?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ZWO ASI585MM excels at high-frame-rate imaging of bright targets where short exposures are key. This includes:\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eLunar and Planetary Imaging:\u003c\/strong\u003e Its 2.9µm pixels and high resolution are ideal for capturing fine details on Jupiter, Saturn, and Mars.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eSolar Imaging:\u003c\/strong\u003e With a proper, full-aperture solar filter, it can resolve intricate details in sunspots and surface granulation.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eElectronically Assisted Astronomy (EAA):\u003c\/strong\u003e The camera's 91% QE makes it excellent for live-stacking short exposures of brighter deep-sky objects like globular clusters and planetary nebulae.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cp\u003eAs an \u003cstrong\u003euncooled camera\u003c\/strong\u003e, it is not optimized for traditional long-exposure deep-sky astrophotography, where thermal noise can become a factor in multi-minute exposures.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the ASI585MM perform on Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eIt's an excellent match. For optimal planetary imaging, the ideal focal ratio is typically 5 to 7 times the camera's pixel size. With the ASI585MM's 2.9µm pixels, you should aim for a final focal ratio between f\/14.5 and f\/20.3. On an 8\" f\/10 SCT, using a \u003cstrong\u003e1.5x or 2x Barlow lens\u003c\/strong\u003e will place you squarely in this optimal range, allowing you to achieve critical sampling of Jupiter's atmospheric details under good seeing conditions.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the ZWO ASI585MM for EAA on globular clusters like M13?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAbsolutely. The ZWO ASI585MM is a superb camera for EAA on bright targets like the Hercules Cluster (M13). Its high sensitivity (91% Peak QE) allows you to use very short exposures (2-10 seconds) to capture individual stars without saturation. Live-stacking software can then combine these short subs in real-time to build up a clean, detailed view that resolves the cluster's dense core.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eShould I get the ASI585MM Mono or the ASI585MC Color version?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eChoose the camera that matches your imaging goals.\n\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eZWO ASI585MM (Mono):\u003c\/strong\u003e Choose this for the highest possible resolution, detail, and sensitivity. It is the superior choice for serious planetary imagers and those who want to shoot with narrowband filters. It requires a filter wheel and LRGB filters to create color images.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eZWO ASI585MC (Color):\u003c\/strong\u003e Choose this for simplicity and convenience. You get a full-color image directly from the camera without extra accessories, making it a faster and easier way to start capturing planets.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat do the 6.5mm and 17.5mm back focus options on the ASI585MM let me do?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe dual back focus values provide the flexibility needed for different imaging setups, without requiring you to guess at spacing.\n\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003e17.5mm:\u003c\/strong\u003e This is the standard back focus for most ZWO cameras and is the correct distance to use when adding accessories like a ZWO filter wheel or off-axis guider to your imaging train.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003e6.5mm:\u003c\/strong\u003e This shorter optical path is useful for specific applications where total back focus is limited, such as with some camera lens adapters or focal reducers.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the ZWO ASI585MM compatible with the ASIAIR?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, the ZWO ASI585MM is fully compatible with the entire ASIAIR ecosystem (ASIAIR Plus and ASIAIR Pro). It is recognized natively by the ASIAIR app, allowing for complete camera control, image capture, and guiding without needing a separate laptop.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSKU\u003c\/td\u003e\n\u003ctd\u003eZWO-ASI585MM\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Series\u003c\/td\u003e\n\u003ctd\u003eZWO ASI585\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/1.2\" Sony IMX585 BSI CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eColor\/Mono\u003c\/td\u003e\n\u003ctd\u003eMonochrome\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCooling\u003c\/td\u003e\n\u003ctd\u003eUncooled\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e3840 x 2160 (8.29 MP)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Dimensions\u003c\/td\u003e\n\u003ctd\u003e11.2mm x 6.3mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e12.85mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePeak Quantum Efficiency\u003c\/td\u003e\n\u003ctd\u003e91%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e46.9 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e256MB DDR3\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAmp Glow Control\u003c\/td\u003e\n\u003ctd\u003eZero Amplifier Glow\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e6.5mm \/ 17.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eComputer Interface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd\u003eM42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Window\u003c\/td\u003e\n\u003ctd\u003eAR Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e0.3 lb.\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWorking Temperature\u003c\/td\u003e\n\u003ctd\u003e-5°C to 50°C\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eStorage Temperature\u003c\/td\u003e\n\u003ctd\u003e-10°C to 60°C\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWorking Humidity\u003c\/td\u003e\n\u003ctd\u003e0% to 80%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOS Compatibility\u003c\/td\u003e\n\u003ctd\u003eWindows 7\/8\/10, Linux, Mac\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eZWO ASI585MM Monochrome Camera\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e2\" Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eUSB 3.0 Cable (2m)\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eST4 Guide Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eQuick Start Guide\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":49803393368349,"sku":"ZWO-ASI585MM","price":699.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ZWO-ASI585MM-Main-1.jpg?v=1742412620"},{"product_id":"qhyccd-minicam8-mono-camera","title":"QHYCCD miniCAM8 Mono Camera","description":"\u003c!-- more--\u003e\n\u003cp\u003eAt just over 4 inches in diameter and a few inches thick (IMX585), the new miniCAM8 is a compact, high-resolution, high-performance, cooled imaging system capable of exceptional, high-quality deep space images as well as high-quality, high-resolution planetary images. So often, compactness in astroimaging is achieved at the expense of some other critical feature found in multi-component cooled systems, such as sensor quality or thermoelectric cooling, etc. Such is not the case with the new miniCAM8. Based on Sony’s IMX585 8 MP sensor, the miniCAM8 includes full TE cooling capable of reaching a delta of -45℃ from ambient along with a built-in 8-position filter wheel for complete LRGB and narrowband imaging.\u003c\/p\u003e\n\u003cp\u003eThe combo version comes with LRGB and 7nm Ha, OIII and SII filters!\u003c\/p\u003e","brand":"QHYCCD","offers":[{"title":"miniCAM8 DeepSky Combo","offer_id":49884455010589,"sku":"QHY-120022","price":1142.0,"currency_code":"CAD","in_stock":true},{"title":"miciCAM8 Camera (LRGB+SHO 7nm)","offer_id":49884455043357,"sku":"QHY-110191","price":859.0,"currency_code":"CAD","in_stock":true},{"title":"Deep Sky Combo EVO (LRGB+SHO 3nm)","offer_id":52958039736605,"sku":"QHY-MINICAM8M-EVO","price":1258.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/image_bf57e45d-82aa-4d28-807f-baa4bb376e60.jpg?v=1744483882"},{"product_id":"qhyccd-minicam8-color-camera","title":"QHYCCD miniCAM8 Color Camera","description":"\u003c!-- more--\u003e\n\u003cp\u003eAt just over 4 inches in diameter and a few inches thick (IMX585), the new miniCAM8 is a compact, high-resolution, high-performance, cooled imaging system capable of exceptional, high-quality deep space images as well as high-quality, high-resolution planetary images. So often, compactness in astroimaging is achieved at the expense of some other critical feature found in multi-component cooled systems, such as sensor quality or thermoelectric cooling, etc. Such is not the case with the new miniCAM8. Based on Sony’s IMX585 8 MP sensor, the miniCAM8 includes full TE cooling capable of reaching a delta of -45℃ from ambient along with a built-in 8-position filter wheel for complete LRGB and narrowband imaging.\u003c\/p\u003e\n\u003cp\u003eThe combo version comes with \u003cspan\u003e1x Light Pollution Filter, 1x Heavy Light Pollution Filter, 1x Four-Channel Enhancement Filter and 1x UV\/IR cut filter.\u003c\/span\u003e\u003c\/p\u003e","brand":"QHYCCD","offers":[{"title":"miniCAM8 DeepSky Combo","offer_id":49884462186781,"sku":"QHY-110197","price":999.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/image_bf57e45d-82aa-4d28-807f-baa4bb376e60.jpg?v=1744483882"},{"product_id":"zwo-asi662mm-mono","title":"ZWO ASI662MM Mono","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e2.1 Megapixel Sony IMX662 Monochrome Sensor\u003c\/li\u003e\n\u003cli\u003e2.9µm Pixel Size\u003c\/li\u003e\n\u003cli\u003e91% Peak Quantum Efficiency\u003c\/li\u003e\n\u003cli\u003e107.6 FPS at Full 1920x1080 Resolution\u003c\/li\u003e\n\u003cli\u003eZero Amplifier Glow Circuitry\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI662MM Monochrome Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI662MM combines the Sony IMX662's 91% peak quantum efficiency with an extremely low 0.8e read noise, capturing faint planetary and lunar details with exceptional clarity. Its 2.1 MP sensor with 2.9µm pixels achieves a maximum frame rate of 107.6 FPS over USB 3.0, while the large 38.2ke full well capacity prevents bright features from saturating. A 256MB DDR3 buffer ensures stable, drop-free data transfer during high-speed video capture.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony IMX662 Sensor: 91% QE and 38.2ke Full Well\u003c\/h3\u003e\n\u003cp\u003eThe core of the ASI662MM is its back-illuminated Sony sensor, which achieves a 91% peak QE, making it extraordinarily sensitive to faint light. This monochrome design utilizes every photon hitting its 1920 x 1080 pixel array. The sensor's 38.2ke full well capacity is more than three times larger than previous generations, allowing you to capture extreme brightness variations, from Jupiter's equatorial bands to its dimmer polar regions, in a single exposure without clipping highlights.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eZero Amp Glow \u0026amp; 256MB DDR3 Buffer\u003c\/h3\u003e\n\u003cp\u003eZWO engineered the ASI662MM with a circuit design that produces zero amplifier glow, a common source of noise in uncooled CMOS cameras. This eliminates the need for dark frame subtraction to remove corner glow, simplifying your image processing workflow. To handle the data from its high-speed 107.6 FPS capture rate, a 256MB DDR3 buffer provides a stable, high-speed data cache that prevents dropped frames and ensures consistent transfer to your computer.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eASI662MM vs. ASI462MM: A Generational Leap in Planetary Imaging\u003c\/h3\u003e\n\u003cp\u003eWhile the ASI462MM remains an excellent camera known for its infrared sensitivity, the ASI662MM represents a significant step forward for imaging in the visible spectrum. The primary advantage of the ASI462MM is its response deep into the IR, which can be beneficial for cutting through atmospheric turbulence when imaging planets with a methane filter. However, for standard LRGB planetary work, the ASI662MM's specifications are superior across the board.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eFull Well Capacity:\u003c\/strong\u003e The ASI662MM's 38.2ke full well is dramatically larger than the 11.2ke of the ASI462MM. This gives you far greater dynamic range, preventing the bright cores of planets and lunar features from blowing out while still capturing subtle albedo details.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eRead Noise:\u003c\/strong\u003e At 0.8e, the ASI662MM's read noise is very low (the ASI462MM reaches 0.47e in HCG mode), keeping a clean signal-to-noise ratio, especially during short exposures used in lucky imaging.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eAmp Glow:\u003c\/strong\u003e The ASI662MM has zero amplifier glow, a persistent artifact on the ASI462MM that requires calibration frames to remove.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eUncooled Design for High-Speed Imaging and Guiding\u003c\/h3\u003e\n\u003cp\u003eThe ASI662MM's uncooled design keeps its weight down to just 0.28 lb., making it an ideal choice for planetary imaging where active cooling is unnecessary for short video captures. This high sensitivity and low read noise also make it a capable autoguider. As an uncooled camera, thermal noise will build up on multi-second guide exposures, but for the vast majority of guiding scenarios where exposure times are under 5 seconds, the camera's raw sensitivity delivers sharp, consistent tracking.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eConnectivity: 12.5mm Back Focus and Standard Ports\u003c\/h3\u003e\n\u003cp\u003eThe ASI662MM is built for easy integration into any imaging train. It uses a standard M42 thread for direct connection and includes a 1.25\" nosepiece for use in standard focusers or filter wheels. The native back focus of 12.5mm is a critical distance for correct spacing with various accessories.\n\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eUSB 3.0 Interface:\u003c\/strong\u003e Provides the 5Gb bandwidth necessary to run the camera at its maximum 107.6 FPS frame rate.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eST-4 Guide Port:\u003c\/strong\u003e Allows for direct connection to a telescope mount for autoguiding, bypassing the need for pulse guiding via a computer.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eM42x0.75 Threads:\u003c\/strong\u003e The standard T-thread interface ensures compatibility with a vast ecosystem of adapters, filter wheels, and off-axis guiders.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the ASI662MM perform on Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe ZWO ASI662MM is an excellent match for an 8\" f\/10 SCT for imaging Jupiter. The camera's 2.9µm pixels are best sampled at a focal ratio between f\/14.5 and f\/20.3. Using a 1.5x or 2x Barlow lens with your SCT will place the system squarely in this optimal range, allowing you to resolve fine details like the Great Red Spot and intricate cloud bands.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the ASI662MM for imaging craters along the Moon's terminator with a 4\" refractor?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAbsolutely. The ZWO ASI662MM's high sensitivity and high frame rate are perfect for lunar imaging. The large 38.2ke full well capacity is a major advantage here, as it can handle the extreme contrast between the brightly lit crater rims and the deep shadows on the terminator without saturating the highlights. The 1920x1080 resolution is well-suited to capturing wide mosaics of the lunar surface with a 4\" refractor.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy should I choose the ASI662MM over the older ASI462MM?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor most planetary, lunar, and solar imaging, the ZWO ASI662MM is the superior choice. Its key advantages are a \u003cstrong\u003emuch larger full well capacity (38.2ke vs. 11.2ke)\u003c\/strong\u003e for better dynamic range, \u003cstrong\u003every low read noise (0.8e)\u003c\/strong\u003e, and \u003cstrong\u003ezero amplifier glow\u003c\/strong\u003e. The only scenario where the ASI462MM holds an advantage is for imaging in very specific near-infrared wavelengths, like methane band imaging, due to its exceptional IR sensitivity.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does \"Zero Amp Glow\" on the ASI662MM mean for my workflow?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eZero Amplifier Glow means the camera's internal circuitry does not create a bright gradient or glow at the edge of the sensor, even on longer exposures. For the ZWO ASI662MM, this simplifies your processing significantly because you don't need to shoot and subtract dark frames to remove this specific artifact, resulting in cleaner raw data from the start.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the ASI662MM a good choice for an autoguiding camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, the ZWO ASI662MM is a very capable autoguiding camera due to its high sensitivity and low read noise. It can detect faint guide stars with very short exposures (typically 1-3 seconds). As it is an uncooled camera, you may see thermal noise accumulate on guide exposures longer than 5-10 seconds, but for most guiding applications, its performance is excellent.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat software do I need to use the ZWO ASI662MM?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eTo use the ZWO ASI662MM, you will need to download the latest drivers from the ZWO website. It is compatible with most popular capture software like SharpCap, FireCapture, and N.I.N.A. through its native or ASCOM drivers. ZWO also provides its own free software suite, ASIStudio, which includes tools for planetary capture, deep-sky imaging, and live stacking.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/2.8\" Sony IMX662 BSI CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e1920 x 1080 (2.1 MP)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Dimensions\u003c\/td\u003e\n\u003ctd\u003e5.6mm x 3.1mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e6.45mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQuantum Efficiency (Peak)\u003c\/td\u003e\n\u003ctd\u003e91%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e38.2ke-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e0.8e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e107.6 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAmp Glow Control\u003c\/td\u003e\n\u003ctd\u003eZero Amplifier Glow\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32µs to 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBit Depth\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e256MB DDR3\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eROI Support\u003c\/td\u003e\n\u003ctd\u003eYes\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eInterface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Connection\u003c\/td\u003e\n\u003ctd\u003eM42x0.75 \/ 1.25\" Nosepiece\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Window\u003c\/td\u003e\n\u003ctd\u003eAR\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Type\u003c\/td\u003e\n\u003ctd\u003eUncooled Monochrome\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e0.28 lb\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWorking Temperature\u003c\/td\u003e\n\u003ctd\u003e-5℃ to 50℃\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eStorage Temperature\u003c\/td\u003e\n\u003ctd\u003e-20℃ to 60℃\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWorking Relative Humidity\u003c\/td\u003e\n\u003ctd\u003e20% to 80%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOS Compatibility\u003c\/td\u003e\n\u003ctd\u003eWindows, Mac, Linux\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eZWO ASI662MM Monochrome Camera\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eUSB 3.0 Cable (2m)\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eST4 Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eQuick Start Guide\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":50638694220061,"sku":"ZWO-ASI662MM","price":419.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ZWO-ASI662MM-Mono-1.jpg?v=1763566764"},{"product_id":"zwo-asi676mm-mono-camera","title":"ZWO ASI676MM Mono Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e12.6 MP Square Sensor (3552 x 3552)\u003c\/li\u003e\n\u003cli\u003e2µm Pixel Size\u003c\/li\u003e\n\u003cli\u003e83% Peak Quantum Efficiency\u003c\/li\u003e\n\u003cli\u003e0.56e Ultra-Low Read Noise\u003c\/li\u003e\n\u003cli\u003eZero Amplifier Glow\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eZWO ASI676MM Monochrome Astronomy Camera\u003c\/h2\u003e\n\u003cp\u003eThe ZWO ASI676MM Monochrome Astronomy Camera combines a square 12.6 MP Sony sensor with 2µm pixels to deliver high-resolution planetary, lunar, and all-sky views. Its back-illuminated architecture achieves a peak Quantum Efficiency of 83%, while an exceptionally low 0.56e read noise ensures faint details are captured during high-speed captures running at up to 31.2 FPS. A 256MB DDR3 buffer maintains stable data transfer over USB 3.0, and the sensor's design completely eliminates amplifier glow for perfectly clean calibration frames.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSquare 12.6 MP Sensor for Seamless Imaging\u003c\/h3\u003e\n\u003cp\u003eThe ASI676MM's unique 3552 x 3552 pixel array is a significant advantage for specific imaging tasks. The square format perfectly matches the circular image field of all-sky lenses, maximizing data collection without wasting pixels on empty corners. This geometry also simplifies the creation of large mosaics of the Moon or deep-sky regions, as frames can be stitched together with uniform overlap and no rotation required between panels.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e2µm Pixels \u0026amp; 83% QE for Critical Sampling\u003c\/h3\u003e\n\u003cp\u003eWith a fine 2µm pixel size, the ASI676MM is built for high-resolution imaging, allowing you to achieve critical sampling on telescopes with shorter focal lengths without aggressive use of Barlow lenses. The sensor's 83% peak QE means the vast majority of incoming photons are converted to signal, which is critical for capturing faint planetary details or guiding on dim stars. This sensitivity, combined with its BSI structure, makes it exceptionally effective in the near-infrared, ideal for methane band imaging of Jupiter and Saturn.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e0.56e Read Noise with Zero Amp Glow\u003c\/h3\u003e\n\u003cp\u003eFor planetary imagers using \"lucky imaging\" techniques, the camera's 0.56e read noise is a defining feature, preserving signal-to-noise ratio across thousands of stacked short exposures. Unlike many CMOS sensors, the ASI676MM produces zero amplifier glow, regardless of gain or exposure settings. This eliminates a major source of noise and simplifies post-processing, as dark frames become easier to match and subtract perfectly.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003e256MB DDR3 Buffer:\u003c\/strong\u003e Ensures no frames are dropped during high-speed planetary runs, providing a stable and reliable data stream to your computer.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003e12-bit ADC:\u003c\/strong\u003e Captures over 4,000 grayscale levels, providing smooth tonal gradations across bright lunar surfaces and the faint cloud bands of gas giants.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003e10.55Ke Full Well:\u003c\/strong\u003e A deep full well capacity for an uncooled camera with small pixels, reducing the risk of saturating bright stars or planetary limbs during longer exposures.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eZWO ASI676MM vs. ASI178MM\u003c\/h3\u003e\n\u003cp\u003eWhile both are high-resolution monochrome cameras, the ASI676MM and ASI178MM serve different primary roles. The ASI178MM has a slight advantage in sensitivity due to its larger 2.4µm pixels, making it a strong performer for solar and lunar imaging where light is plentiful. It also uses a rectangular sensor, which can be more efficient for framing elongated galaxies.\u003c\/p\u003e\n\u003cp\u003eThe ASI676MM's primary advantages are its modern sensor architecture and specialized format. Its 12.6 MP square sensor is objectively better for all-sky imaging and mosaic construction, and its complete lack of amp glow is a significant quality-of-life improvement, simplifying calibration. For imagers focused on planets, meteors, or building large-scale mosaics, the ASI676MM's feature set is more specifically tailored to the task.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat makes the ZWO ASI676MM's square sensor good for all-sky imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e3552 x 3552 pixel\u003c\/strong\u003e square sensor of the ASI676MM perfectly matches the circular image produced by an all-sky or fisheye lens. This means you utilize the entire sensor area for capturing the sky, unlike a rectangular sensor which would leave the corners of the frame empty, wasting resolution.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow do the 2µm pixels on the ASI676MM affect telescope choice for planetary imaging of Jupiter?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe small \u003cstrong\u003e2µm pixels\u003c\/strong\u003e are ideal for high-resolution work. For optimal sampling of planets like Jupiter, you should aim for a final focal ratio between f\/10 (2µm * 5) and f\/14 (2µm * 7). This means an f\/10 Schmidt-Cassegrain can use the ZWO ASI676MM at its native focal length, while an f\/5 Newtonian would pair well with a 2x or 2.5x Barlow lens to reach the target f-ratio.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan the uncooled ZWO ASI676MM be used for deep-sky objects like the Orion Nebula (M42)?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, but with limitations. As an \u003cstrong\u003euncooled camera\u003c\/strong\u003e, thermal noise will build up on long exposures (over 30-60 seconds), which can impact faint details. However, for bright deep-sky objects like the Orion Nebula (M42) or the Hercules Cluster (M13), you can achieve excellent results by stacking hundreds of very short exposures (5-10 seconds), a technique where the ASI676MM's low \u003cstrong\u003e0.56e read noise\u003c\/strong\u003e and zero amp glow are major assets.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the benefit of the 256MB DDR3 buffer in the ZWO ASI676MM?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e256MB DDR3 memory buffer\u003c\/strong\u003e acts as a temporary storage space for image data before it's sent to the computer. This prevents data loss and maintains a stable, high frame rate (like its max of \u003cstrong\u003e31.2 FPS\u003c\/strong\u003e), especially if the host computer's USB bus is temporarily busy. It's a critical feature for reliable planetary and solar imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the monochrome sensor of the ZWO ASI676MM better than a color one for planets?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor achieving maximum detail, yes. A monochrome sensor like the one in the ASI676MM uses every pixel to capture light, resulting in higher effective resolution and sensitivity compared to a color camera of the same pixel count. To create a color image, you capture separate videos through Red, Green, and Blue filters and combine them in software, a technique which produces sharper and more detailed results than a one-shot-color camera.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the ZWO ASI676MM require dark frames for calibration?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eBecause the ASI676MM has \u003cstrong\u003eZero Amplifier Glow\u003c\/strong\u003e, the need for dark frames is greatly reduced for short-exposure planetary imaging. While darks are still best practice to remove thermal noise, the absence of amp glow means you can often get clean results with just flat frames, significantly simplifying your workflow.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003e1\/1.6\" Sony IMX676 BSI CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e12.6 MP (3552 x 3552)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Dimensions\u003c\/td\u003e\n\u003ctd\u003e7.1 mm x 7.1 mm (10 mm diagonal)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQuantum Efficiency (Peak)\u003c\/td\u003e\n\u003ctd\u003e83%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e0.56e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e10.55Ke\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e31.2 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBit Depth\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAmplifier Glow Control\u003c\/td\u003e\n\u003ctd\u003eZero Amplifier Glow\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Buffer\u003c\/td\u003e\n\u003ctd\u003e256MB DDR3\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Type\u003c\/td\u003e\n\u003ctd\u003eMonochrome, Uncooled\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eInterface\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Connection\u003c\/td\u003e\n\u003ctd\u003eM42x0.75 Threads, 1.25\" Nosepiece\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Window\u003c\/td\u003e\n\u003ctd\u003eAR Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDimensions\u003c\/td\u003e\n\u003ctd\u003e62 mm diameter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e0.28 lb\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCamera Series\u003c\/td\u003e\n\u003ctd\u003eZWO ASI676\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSKU\u003c\/td\u003e\n\u003ctd\u003eZWO-ASI676MM\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eASI676MM Camera Body\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e1.25\" Nosepiece\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eCamera Cover\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e2m USB 3.0 Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eST-4 Guide Cable\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eQuick Guide\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/www.zwoastro.com\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\u003ca href=\"https:\/\/davidastro.com\/pages\/zwo-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eZWO 2-Year Limited Warranty\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":50843600781597,"sku":"ZWO-ASI676MM","price":699.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/ZWO-ASI676MM-Mono-Camera-1.jpg?v=1768505603"},{"product_id":"ioptron-icam462c-planetary-camera","title":"iOptron iCAM462C Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003eSony IMX462 Color CMOS Sensor\u003c\/li\u003e\n\u003cli\u003e2.1 Megapixel Resolution (1944 x 1096)\u003c\/li\u003e\n\u003cli\u003e2.9µm Pixel Size\u003c\/li\u003e\n\u003cli\u003eUp to 136 FPS Frame Rate\u003c\/li\u003e\n\u003cli\u003eUSB 3.0 and ST-4 Ports\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eiOptron iCAM462C Planetary Camera\u003c\/h2\u003e\n\u003cp\u003eThe iOptron iCAM462C planetary camera centers on the 2.1MP Sony IMX462 color sensor, using 2.9µm pixels to resolve fine detail on planetary targets. It achieves a maximum frame rate of 136 fps at full resolution, supported by a low read noise floor of 0.7e and a full well capacity of 12K e. Data is transferred over a high-speed USB3.0 port, capturing a 12-bit dynamic range with a peak quantum efficiency of approximately 80%.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e136 FPS Capture with the 2.1MP Sony IMX462 Sensor\u003c\/h3\u003e\n\u003cp\u003eThe core of modern planetary imaging is \"lucky imaging\"—capturing thousands of frames in a short period to freeze moments of stable atmospheric seeing. The iCAM462C delivers a blistering 136 fps at its full 1944 x 1096 resolution, ensuring you can acquire vast amounts of data during brief windows of clarity. The 2.9µm pixels are optimally sized for sampling the fine details resolved by long focal-length telescopes like Schmidt-Cassegrains and Maksutovs, often without requiring a Barlow lens.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e0.7e Read Noise and ~80% QE for High Signal-to-Noise\u003c\/h3\u003e\n\u003cp\u003eHigh frame rates require short exposures, where sensor noise can easily overwhelm faint signals. The iCAM462C utilizes a low-noise architecture, including a supported HCG mode, to drop read noise as low as 0.7e. Combined with a peak Quantum Efficiency of ~80%, this ensures that a high percentage of incoming photons are converted to signal, producing clean, high-contrast images of faint planetary cloud belts and lunar rilles. The camera's rolling shutter is perfectly suited for astronomical targets but may introduce distortion on fast-moving terrestrial objects.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eUSB 3.0 Data Transfer and ST-4 Autoguiding Port\u003c\/h3\u003e\n\u003cp\u003eTo sustain its high frame rates, the iCAM462C uses a USB 3.0 data port, which provides the necessary bandwidth to transfer uncompressed video streams to your computer without dropping frames. This camera also serves a dual purpose for deep-sky imagers; the integrated ST-4 compatible guide port allows it to function as a highly sensitive autoguider. The standard 1.25” adapter provides direct compatibility with most focusers and accessories right out of the box.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eiOptron iCAM462C vs. ZWO ASI462MC: A Head-to-Head Comparison\u003c\/h3\u003e\n\u003cp\u003eThe most direct competitor to the iCAM462C is the ZWO ASI462MC, as both cameras are built around the identical Sony IMX462 sensor. Consequently, their core imaging specifications—resolution, pixel size, read noise, and quantum efficiency—are virtually indistinguishable. The choice between them often comes down to software integration and existing equipment.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eZWO ASI462MC Advantage:\u003c\/strong\u003e ZWO has a more established ecosystem with broad third-party support in capture software and hardware like the ASIAIR. If you are already invested in the ZWO ecosystem, the ASI462MC offers seamless integration.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eiOptron iCAM462C Advantage:\u003c\/strong\u003e For users of iOptron mounts and software, the iCAM462C is designed for native compatibility. It presents a strong, manufacturer-supported option that consolidates driver and hardware support within a single brand.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the iOptron iCAM462C best for?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe iOptron iCAM462C excels at high-frame-rate solar system imaging. Its combination of a fast \u003cstrong\u003e136 fps rate\u003c\/strong\u003e, small \u003cstrong\u003e2.9µm pixels\u003c\/strong\u003e, and high sensitivity makes it ideal for capturing detailed images of \u003cstrong\u003eJupiter, Saturn, Mars, and the Moon\u003c\/strong\u003e by overcoming atmospheric turbulence.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow would the iCAM462C perform on Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThis is an excellent pairing. The \u003cstrong\u003e2.9µm pixels\u003c\/strong\u003e of the iCAM462C provide near-optimal image sampling for an 8\" SCT at its native f\/10 focal ratio, resolving fine cloud bands in Jupiter's atmosphere without needing a Barlow lens. The high frame rate is crucial for capturing moments of steady seeing to produce a sharp final image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the iOptron iCAM462C for autoguiding?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. The iCAM462C includes a standard \u003cstrong\u003eST-4 compatible guide port\u003c\/strong\u003e. This allows it to connect directly to the autoguider port on most equatorial mounts, making it a very capable and sensitive guide camera for long-exposure deep-sky astrophotography.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the iCAM462C suitable for deep-sky imaging of galaxies or nebulae?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWhile its low read noise and high sensitivity are beneficial, the iCAM462C's small \u003cstrong\u003e2.1MP sensor\u003c\/strong\u003e is not designed for capturing large deep-sky objects like the Andromeda Galaxy (M31). It can be effective for \"electronically-assisted astronomy\" (EAA) or imaging smaller, brighter targets like the Ring Nebula (M57) or other planetary nebulae.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat kind of exposure times should I use for imaging the lunar surface with the iCAM462C?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Moon is extremely bright, so you will use very short exposures. With the iCAM462C, exposures will typically be in the millisecond range (e.g., 5ms to 20ms), with gain adjusted to prevent bright highland areas from being overexposed. The camera supports exposures as short as \u003cstrong\u003e32µs\u003c\/strong\u003e, ensuring no part of the Moon is too bright to capture.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat software do I need to use the iOptron iCAM462C?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYou will need an astronomical capture program that supports the camera, such as SharpCap or FireCapture, along with the appropriate drivers from iOptron. For post-processing the video files, standard planetary imaging software like AutoStakkert!, RegiStax, or PixInsight is used.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSony IMX462 CMOS (Color)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003e1\/2.8” (5.6 x 3.2 mm)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Resolution\u003c\/td\u003e\n\u003ctd\u003e1944 x 1096 (2.1MP)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9 µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e136 fps (at 10-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32µs to 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e0.7e to 2.6e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePeak QE\u003c\/td\u003e\n\u003ctd\u003e~80%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e12K e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eHCG Mode\u003c\/td\u003e\n\u003ctd\u003eSupported\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOptical Window\u003c\/td\u003e\n\u003ctd\u003eAR Coated Glass\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4 Compatible\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Connection\u003c\/td\u003e\n\u003ctd\u003e1.25\" Adapter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e0.75 lbs\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eiOptron iCAM462C Camera Body\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/ioptron-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eiOptron 2-Year Limited Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"iOptron","offers":[{"title":"Default Title","offer_id":50862920466717,"sku":"IOP-3372","price":385.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/iOptron-iCAM462C-Planetary-Camera.jpg?v=1768943717"},{"product_id":"player-one-apollo-m-pro-mono-imx432-cooled-solar-camera","title":"Player One Apollo-M MAX Pro Mono IMX432 Cooled Solar Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e1.7 Megapixel Sony IMX432 Mono Sensor\u003c\/li\u003e\n\u003cli\u003eLarge 9µm Pixel Size\u003c\/li\u003e\n\u003cli\u003eMassive 100k e- Full Well Capacity\u003c\/li\u003e\n\u003cli\u003eGlobal Shutter for Distortion-Free Imaging\u003c\/li\u003e\n\u003cli\u003e126 FPS at Full 1608x1104 Resolution\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Apollo-M MAX Pro Mono IMX432 Cooled Solar Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Apollo-M MAX Pro redefines high-resolution solar imaging by pairing a Sony IMX432 monochrome sensor with a powerful 2-stage TEC cooling system. Its large 9µm pixels and enormous 100k e- full well capacity are engineered to capture extreme dynamic range, from the brightest sunspots to faint prominences, in a single exposure. This camera achieves a blistering 126 FPS at its full 1608x1104 resolution, while the global shutter ensures every frame is perfectly sharp, and the 2-stage cooling system provides a 35°C-40°C delta-T for ultra-low-noise results.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eIMX432 Global Shutter Sensor: 9µm Pixels and 100k e- Full Well\u003c\/h3\u003e\n\u003cp\u003eAt the heart of the Apollo-M MAX Pro is the 1.1-inch IMX432 sensor, a chip purpose-built for the challenges of solar astronomy. The large 9µm pixels are exceptionally well-suited for long focal ratio instruments, such as SCTs paired with Daystar filters, providing ideal image sampling without needing a Barlow. Its massive 100k e- full well capacity is over three times that of previous-generation solar sensors, allowing you to capture incredible detail on the solar disk and in the faint corona simultaneously, minimizing the need for composite images.\u003c\/p\u003e\n\u003cp\u003eThe Sony Pregius 3rd generation global shutter is non-negotiable for high-resolution imaging through atmospheric turbulence. By reading the entire 1.7MP sensor at once, it completely eliminates the wobble and distortion that rolling shutters can introduce, ensuring that even during fleeting moments of good seeing, your data is geometrically perfect.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e2-Stage Cooling: 40°C Delta-T and Active Anti-Dew Control\u003c\/h3\u003e\n\u003cp\u003eThis camera integrates a 2-stage TEC cooling system capable of reducing the sensor temperature by 35°C-40°C below ambient. This aggressive cooling dramatically reduces thermal noise, a critical factor for teasing out low-contrast details in H-alpha, like spicules and plages. Unlike uncooled planetary cameras, the Apollo-M MAX Pro delivers clean, stable data suitable for both lucky imaging and longer exposures.\u003c\/p\u003e\n\u003cp\u003eTo combat dew formation, a common issue with cooled cameras, the Apollo-M MAX Pro includes an integrated, software-adjustable anti-dew heater for the protective window. This, combined with adjustable fan speed and target temperature settings in the ASCOM driver, gives you complete control over the camera's thermal environment for consistent results night after night.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eAdvanced Mechanics: 420g Carbon Fiber Body and Dual Tilter Plates\u003c\/h3\u003e\n\u003cp\u003eThe Apollo-M MAX Pro features a housing constructed with carbon fiber, reducing its weight to just 420g. This lightweight design minimizes strain on your focuser and makes balancing your imaging setup easier. The camera also includes a versatile sensor tilting mechanism to achieve a perfectly flat field.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eFront 3-Point Tilter:\u003c\/strong\u003e The default configuration allows for quick and easy tilt adjustments for most standard imaging setups.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eRear 4-Point Tilter:\u003c\/strong\u003e An included alternate plate, essential for complex image trains involving filter wheels or an OAG, allowing you to make precise adjustments without disassembling your setup.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e126 FPS Capture with 512MB DDR3 Buffer\u003c\/h3\u003e\n\u003cp\u003eTo ensure flawless data transfer at its maximum frame rate of 126 FPS, the Apollo-M MAX Pro is equipped with a 512MB DDR3 memory buffer. This onboard cache prevents dropped frames, even when connected to less powerful computers or over a USB 2.0 connection. The buffer secures the data stream from the camera to your PC, greatly reducing readout noise and ensuring that every valuable moment of stable seeing is captured without compromise.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eApollo-M MAX Pro vs. IMX174-Based Cameras: Pixel Size and Full Well\u003c\/h3\u003e\n\u003cp\u003eWhile cameras using the popular Sony IMX174 sensor have been a standard for solar imaging, the Apollo-M MAX Pro's IMX432 sensor presents a significant technological leap forward. The primary differences lie in pixel scale and dynamic range.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eIMX174 Advantage:\u003c\/strong\u003e The IMX174's smaller 5.86µm pixels can achieve critical sampling with shorter focal length telescopes, and it remains a proven, high-QE performer.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eApollo-M MAX Pro Advantage:\u003c\/strong\u003e The IMX432's 9µm pixels are 1.5x larger, making it a perfect match for the long effective focal lengths of SCTs and dedicated solar telescopes. More importantly, its 100k e- full well capacity is more than triple the ~32k e- of the IMX174, delivering vastly superior dynamic range for capturing both surface and prominence detail in a single shot.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy is the Apollo-M MAX Pro's 9µm pixel size ideal for solar imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe large \u003cstrong\u003e9µm pixels\u003c\/strong\u003e are an excellent match for the long focal lengths common in solar astronomy, especially when using Schmidt-Cassegrains with Daystar Quark or other H-alpha filters that increase the effective focal ratio. This combination provides an optimal image scale for capturing fine detail without needing an additional Barlow lens, simplifying the optical train.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the 100k e- full well on the Apollo-M MAX Pro help with imaging the Sun?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Sun has an enormous brightness range between features on the surface (like sunspots and granulation) and the much fainter prominences at the limb. The Apollo-M MAX Pro's massive \u003cstrong\u003e100k e- full well capacity\u003c\/strong\u003e allows the sensor to capture both bright and dim details in a single exposure without saturating the pixels, dramatically increasing the dynamic range of your final image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is a global shutter, and why is it important for the Apollo-M MAX Pro?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eA \u003cstrong\u003eglobal shutter\u003c\/strong\u003e exposes and reads out every pixel on the 1.7MP sensor at the exact same time. This is critical for solar, lunar, and planetary imaging, as it freezes motion caused by atmospheric turbulence. Unlike a rolling shutter which can cause distortion and \"wobble\" effects, a global shutter ensures that your target's geometry is perfectly preserved in every frame.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Apollo-M MAX Pro for deep-sky imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, while optimized for solar, the Apollo-M MAX Pro can be used for deep-sky imaging. Its monochrome sensor, 2-stage cooling, and low readout noise (down to \u003cstrong\u003e2.6e\u003c\/strong\u003e) make it suitable for imaging smaller, bright DSOs like planetary nebulae or globular clusters. However, its 1.1\" sensor is smaller than typical dedicated deep-sky cameras, making it less ideal for wide-field targets.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow would the Apollo-M MAX Pro perform on solar prominences with a Lunt H-alpha telescope at f\/7?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Apollo-M MAX Pro would be an excellent choice. On an f\/7 system, its 9µm pixels provide a good image scale for resolving fine prominence detail. The camera's high QE of \u003cstrong\u003e≈79%\u003c\/strong\u003e and low read noise, combined with its \u003cstrong\u003e100k e- full well\u003c\/strong\u003e, would allow you to capture the delicate, faint structures of prominences with high contrast and minimal noise.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat's the benefit of the Apollo-M MAX Pro's sensor for creating a full-disk solar mosaic with a Celestron 8\" SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWith an 8\" SCT at its native f\/10 or longer with a solar filter, the Apollo-M MAX Pro's large \u003cstrong\u003e1.1\" sensor (17.5mm diagonal)\u003c\/strong\u003e captures a significantly larger field of view per frame compared to smaller-chip cameras. This means you can complete a full-disk mosaic of the Sun in fewer panels, which saves time during capture and simplifies processing later on.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSony IMX432 1.1\" CMOS (Monochrome)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Resolution\u003c\/td\u003e\n\u003ctd\u003e1608 × 1104 (1.7MP)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e9µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e17.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Size\u003c\/td\u003e\n\u003ctd\u003e14.5mm × 9.9mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eGlobal Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e126 FPS (at 1608×1104, 12-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e100,000 e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e2.6e to 22.9e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePeak QE\u003c\/td\u003e\n\u003ctd\u003e≈79%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32µs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCooling System\u003c\/td\u003e\n\u003ctd\u003e2-Stage Thermoelectric Cooler (TEC)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCooling Delta T\u003c\/td\u003e\n\u003ctd\u003e35°C - 40°C below ambient\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0 (Type-C)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePower Port (for cooler)\u003c\/td\u003e\n\u003ctd\u003e12V DC 5.5x2.1mm (min. 5A adapter required)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD32*2mm AR Plus Multi-Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e17.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMounting Adapter\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e78mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e420g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOperating Temperature\u003c\/td\u003e\n\u003ctd\u003e-10°C to 60°C\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOperating Humidity\u003c\/td\u003e\n\u003ctd\u003e0% to 80%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rates (USB 3.0)\u003c\/td\u003e\n\u003ctd\u003e1608×1104: 126 FPS (RAW8) \/ 109 FPS (RAW16)\u003cbr\u003e1280×720: 187 FPS\u003cbr\u003e800×600: 220 FPS\u003cbr\u003e640×480: 268 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eApollo-M MAX Pro Camera Body\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Apollo-M_MAX_Pro_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51111900184861,"sku":"POA-Apollo-M-MAX-Pro","price":1118.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Apollo-M-MAX-Pro-Mono-Camera.png?v=1775149855"},{"product_id":"player-one-apollo-428m-max-pro-mono-cooled-solar-camera","title":"Player One Apollo 428M MAX Pro Mono Cooled Solar Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003eSony IMX428 1.1\" monochrome CMOS sensor with global shutter\u003c\/li\u003e\n\u003cli\u003e7.1 Megapixel resolution (3216x2208) with 4.5μm pixels\u003c\/li\u003e\n\u003cli\u003eHigh frame rate of 51 FPS at full resolution (10-bit)\u003c\/li\u003e\n\u003cli\u003e2-stage TEC cooling provides a 35°C-40°C delta-T below ambient\u003c\/li\u003e\n\u003cli\u003eLow readout noise of 5.5e down to 1.4e\u003c\/li\u003e\n\u003cli\u003e25.3k e- full well capacity and 12-bit ADC\u003c\/li\u003e\n\u003cli\u003eLightweight 420g body with M42x0.75 threads\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Apollo 428M MAX Pro Mono Cooled Solar Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Apollo 428M MAX Pro combines a large-format Sony IMX428 1.1-inch sensor with a global shutter, delivering 7.1MP (3216x2208) images free of motion artifacts. Its 4.5μm pixels resolve fine solar granulation and chromospheric details, while the 2-stage TEC cooling system achieves a 35°C-40°C delta-T for low-noise, long-exposure DSO imaging. A readout noise floor as low as 1.4e and a 25.3k e- full well capacity ensure you capture maximum dynamic range in every frame, streamed reliably at up to 51 FPS over USB 3.0.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony IMX428 Global Shutter: 7.1MP for High-Resolution Solar\u003c\/h3\u003e\n\u003cp\u003eThe core of the Apollo 428M MAX Pro is its 1.1-inch Sony IMX428 monochrome sensor, which uses Pregius 3rd generation global shutter technology. This is critical for high-resolution solar and lunar imaging, as it reads out all 7.1 million pixels simultaneously, completely eliminating the distortion and warping that rolling shutters can introduce during moments of unsteady seeing. The 4.5μm pixels offer a significant increase in sampling resolution compared to older generation solar cameras, allowing you to capture incredibly fine detail in solar spicules, filaments, and granulation without needing an aggressive Barlow lens.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e2-Stage TEC Cooling: A 35-40°C Delta-T System\u003c\/h3\u003e\n\u003cp\u003eEngineered for both high-speed planetary and deep-sky imaging, the Apollo 428M MAX Pro integrates a powerful 2-stage thermoelectric cooling system. Capable of reducing the sensor temperature by 35°C to 40°C below ambient, this system dramatically lowers thermal noise for clean, long-exposure captures of faint nebulae and galaxies. An integrated, controllable anti-dew heater on the D32*2MM protective window prevents condensation during humid nights, ensuring your imaging sessions are uninterrupted.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e51 FPS Capture with 512MB DDR3 Cache\u003c\/h3\u003e\n\u003cp\u003eTo ensure stable, drop-free video capture at its maximum speed of 51 FPS, the Apollo 428M MAX Pro is equipped with a 512MB DDR3 memory buffer. This cache secures data transmission from the sensor before it's sent over the USB 3.0 connection, preventing lost frames even on PCs with slower hard drives. This onboard memory greatly reduces readout noise and makes the camera's high-speed capabilities accessible without requiring a top-tier computer.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e420g Carbon Fiber Body with Dual Tilter Plates\u003c\/h3\u003e\n\u003cp\u003eThe camera's housing is constructed with carbon fiber, reducing its weight to just 420g and making it easier to balance on any setup. A key innovation is the dual sensor-tilting mechanism. It ships with a 3-point front tilter for general use, but also includes a 4-point rear tilter. The rear tilter is essential for imagers using rigid accessories like a filter wheel or OAG, allowing precise tilt adjustments without introducing flexure into the image train.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eApollo 428M MAX Pro vs. Apollo-M MAX (IMX432): 4.5μm vs. 9μm Pixels\u003c\/h3\u003e\n\u003cp\u003eThe primary difference between the Apollo 428M MAX Pro (IMX428) and the classic Apollo-M MAX (IMX432) is pixel size and resolution. While both use a 1.1\" format sensor, the choice depends on your telescope and imaging goals.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eApollo 428M MAX Pro (IMX428):\u003c\/strong\u003e With 4.5μm pixels and a 7.1MP resolution, this camera is built for high-resolution imaging. It provides four times the pixel density, making it ideal for capturing fine details on the Sun and Moon with short to medium focal length refractors.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eApollo-M MAX (IMX432):\u003c\/strong\u003e This camera uses larger 9μm pixels and has a 1.7MP resolution. Its larger pixels offer a greater full well capacity per pixel, making it extremely sensitive and well-suited for capturing full-disc solar images with longer focal length telescopes or for applications where light-gathering is prioritized over raw resolution.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy is the Apollo 428M MAX Pro's global shutter so important for solar imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAtmospheric turbulence (seeing) causes solar details to shift and warp rapidly. A \u003cstrong\u003eglobal shutter\u003c\/strong\u003e exposes every one of the camera's 7.1 million pixels at the exact same instant, freezing the motion and preventing the \"jello\" effect common with rolling shutters. This results in sharper, more authentic details in solar prominences and surface granulation.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow do the 4.5μm pixels of the Apollo 428M MAX Pro perform with a dedicated H-alpha solar telescope?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e4.5μm\u003c\/strong\u003e pixels provide excellent image sampling for many solar telescopes. For example, on a Lunt LS80THa (f\/7, 560mm focal length), this camera achieves a resolution of 1.66 arcseconds per pixel, which is well-matched for capturing fine chromospheric details without needing a Barlow lens, simplifying your imaging train.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Apollo 428M MAX Pro for detailed lunar imaging, like capturing the rilles around crater Gassendi?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAbsolutely. The camera's high resolution and global shutter are perfect for lunar \"lucky imaging.\" The \u003cstrong\u003e3216x2208\u003c\/strong\u003e sensor can frame large regions of the lunar surface, while the 51 FPS frame rate allows you to capture thousands of frames in a short period, letting you select only the sharpest ones to stack and reveal fine details like the complex floor fractures of Gassendi.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the advantage of the rear 4-point tilter on the Apollo 428M MAX Pro?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe rear 4-point tilter allows you to adjust sensor tilt from behind the camera. This is crucial when you have a filter wheel, off-axis guider, or other accessories rigidly attached to the front M42 threads. It lets you correct for field tilt without having to disassemble your imaging train, a significant convenience especially for remote or automated setups.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the Apollo 428M MAX Pro require an external power supply?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor uncooled operation, the camera can be powered solely by the main USB 3.0 port. To activate the \u003cstrong\u003e2-stage TEC cooling system\u003c\/strong\u003e, you must connect a separate 12V DC power supply (minimum 5A rating) to the 5.5x2.1mm port. The power supply is not included.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the 512MB DDR3 cache benefit my imaging sessions?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e512MB DDR3 cache\u003c\/strong\u003e acts as a high-speed buffer, temporarily storing frames before they are transferred to your computer. This prevents data loss (\"frame dropping\") during high-speed video capture at \u003cstrong\u003e51 FPS\u003c\/strong\u003e, ensuring a smooth and stable data stream even if your computer's hard drive can't keep up in real-time.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSony IMX428 1.1\" Mono CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Resolution\u003c\/td\u003e\n\u003ctd\u003e3216×2208\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTotal Pixels\u003c\/td\u003e\n\u003ctd\u003e7.1 MP\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e4.5μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e17.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Size\u003c\/td\u003e\n\u003ctd\u003e14.5mm x 9.9mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eGlobal Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e51 FPS (10-bit), 27 FPS (12-bit) at 3216×2208\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e25.3k e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e5.5e to 1.4e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈79%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32μs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCooling System\u003c\/td\u003e\n\u003ctd\u003e2-Stage TEC\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCooling Delta T\u003c\/td\u003e\n\u003ctd\u003e35°C-40°C below ambient\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCooler Power Consumption\u003c\/td\u003e\n\u003ctd\u003e12V, 3A (requires 5A minimum adapter)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0 (Type-C)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eThreads\u003c\/td\u003e\n\u003ctd\u003eM42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e17.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD32*2mm AR Plus Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e78mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e420g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWorking Temperature\u003c\/td\u003e\n\u003ctd\u003e-10°C to 60°C\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWorking Humidity\u003c\/td\u003e\n\u003ctd\u003e0% to 80%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Apollo_428M_MAX_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51111916601629,"sku":"POA-Apollo-428M-MAX-Pro","price":1398.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Apollo-428M-MAX-Pro-Mono-Camera.png?v=1775149716"},{"product_id":"player-one-saturn-m-sqr-imx533-mono-planetary-camera","title":"Player One Saturn-M SQR IMX533 Mono Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e9 Megapixel Sony IMX533 monochrome sensor\u003c\/li\u003e\n\u003cli\u003e1-inch square format (11.31mm x 11.31mm)\u003c\/li\u003e\n\u003cli\u003e3.76μm pixel size\u003c\/li\u003e\n\u003cli\u003eHigh full well capacity of 73k e-\u003c\/li\u003e\n\u003cli\u003eUp to 43 FPS at full 3008x3008 resolution\u003c\/li\u003e\n\u003cli\u003e14-bit ADC\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Saturn-M SQR IMX533 Mono Planetary Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Saturn-M SQR camera leverages the 9 Megapixel Sony IMX533 monochrome sensor to deliver a unique combination of high-resolution lucky imaging and capture speed. Its 1-inch square format, 3.76μm pixels, and enhanced 73k e- full well capacity are optimized for detailed solar, lunar, and planetary imaging. At a full resolution of 3008x3008, the camera streams data at 43 FPS over USB 3.0, while maintaining a peak Quantum Efficiency of approximately 91% and read noise as low as 1e-.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eThe 9MP IMX533 Sensor: 73k Full Well and 91% QE\u003c\/h3\u003e\n\u003cp\u003eThe core of the Saturn-M SQR is Sony's back-illuminated IMX533 sensor, presented here in a 1-inch square format perfect for creating mosaics with no overlapping data. Player One has enhanced the sensor's native capabilities to achieve a deep 73k e- full well capacity, preventing saturated stars and preserving dynamic range in bright targets like the solar chromosphere or lunar terminator. Combined with a peak QE of ≈91%, the sensor efficiently converts photons to signal, critical for short-exposure \"lucky imaging\" of deep-sky objects.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e43 FPS Full-Resolution Capture over USB 3.0\u003c\/h3\u003e\n\u003cp\u003eDesigned for high-speed imaging, the Saturn-M SQR can capture full-frame 9MP images at 43 frames per second in 10-bit mode. This high frame rate is essential for freezing atmospheric turbulence when imaging planets. For even faster captures on smaller targets, you can window the sensor to achieve up to 272 FPS at 640x480 resolution. A built-in DDR3 cache ensures stable data transmission to your computer, eliminating dropped frames even over slower USB 2.0 connections.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eDual Sampling Modes and Non-Amp-Glow Signal\u003c\/h3\u003e\n\u003cp\u003eThe Saturn-M SQR features two distinct readout modes to match your target. Normal mode prioritizes speed, delivering the maximum 43 FPS for planetary work. Low Readout Noise (LRN) mode reduces read noise to its lowest levels (down to 1e-), ideal for DSO lucky imaging where maximizing signal-to-noise on faint targets is key. The IMX533 sensor is also known for its zero amp glow, which produces exceptionally clean calibration frames and a uniform background without the need to subtract complex thermal patterns.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSaturn-M SQR vs. ZWO ASI533MM Pro: Speed vs. Cooling\u003c\/h3\u003e\n\u003cp\u003eThe Saturn-M SQR and ZWO ASI533MM Pro are built around the same 9MP monochrome sensor but are engineered for different primary uses. The choice depends entirely on your imaging priorities.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003ePlayer One Saturn-M SQR Advantage:\u003c\/strong\u003e At 160g and with a max frame rate of 43 FPS, the Saturn is built for speed and portability. It excels at high-frame-rate lunar, solar, and planetary imaging where its passive cooling is sufficient.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eZWO ASI533MM Pro Advantage:\u003c\/strong\u003e The ZWO camera incorporates regulated two-stage TEC cooling for deep, long-exposure astrophotography. Its heavier body (470g) houses a system that can cool the sensor more than 35°C below ambient, making it the superior choice for traditional narrowband and LRGB imaging of faint nebulae.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eLightweight 160g Body with 12.5mm Back Focus\u003c\/h3\u003e\n\u003cp\u003eWeighing only 160g, the Saturn-M SQR adds minimal load to your focuser or mount, making it an excellent match for smaller telescopes or portable setups. The camera body features a Passive Cooling System (PCS) that draws heat away from the sensor to maintain thermal stability during a run. For demanding daylight solar imaging, an optional external Active Cooling System (ACS) can be added. The camera connects via standard M42x0.75 threads and has a 12.5mm back focal length.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the benefit of the Saturn-M SQR's 3008x3008 square sensor for mosaics?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eA square sensor simplifies the process of creating mosaics of the Moon or Sun. You can move the telescope in a simple grid pattern (up\/down, left\/right) without needing to rotate the camera. This ensures consistent panel orientation and makes stitching the final composite image significantly easier in post-processing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the 73k e- full well on the Saturn-M SQR help with solar imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eSolar features like prominences and surface granulation have an extremely high dynamic range. The \u003cstrong\u003e73k e- full well capacity\u003c\/strong\u003e prevents the brightest parts of the image from saturating (turning pure white), allowing you to capture detail in both the faint, extended prominences and the intensely bright solar surface in a single exposure.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhen should I use Normal mode vs. LRN (Low Readout Noise) mode on the Saturn-M SQR?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eUse \u003cstrong\u003eNormal mode\u003c\/strong\u003e for lunar, solar, and planetary imaging. This mode provides the fastest frame rates (up to 43 FPS), which is critical for \"freezing\" atmospheric seeing. Use \u003cstrong\u003eLRN mode\u003c\/strong\u003e for DSO \"lucky imaging.\" This mode lowers the camera's readout noise to as little as 1e-, maximizing the signal-to-noise ratio on faint targets where every photon counts.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan the Player One Saturn-M SQR be used for traditional long-exposure deep-sky imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWhile excellent for DSO lucky imaging (stacking thousands of very short exposures), the Saturn-M SQR is not designed for traditional long-exposure astrophotography (minutes-long subs). It lacks active thermoelectric cooling (TEC), so thermal noise will accumulate during long exposures. For that style of imaging, a TEC-cooled camera like the ZWO ASI533MM Pro is a better choice.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat do I need to achieve the maximum 43 FPS with the Saturn-M SQR?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eTo achieve the maximum frame rate, you need to connect the camera to a \u003cstrong\u003eUSB 3.0 port\u003c\/strong\u003e on your computer and use a \u003cstrong\u003eSolid State Drive (SSD)\u003c\/strong\u003e for storage. A traditional hard disk drive (HDD) may not have fast enough write speeds to keep up with the data stream, which can cause dropped frames.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the Saturn-M SQR perform on the Moon with an 8\" SCT at f\/10?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Saturn-M SQR is an excellent match for an 8\" SCT. The 1-inch sensor is large enough to frame significant regions of the lunar surface for creating high-resolution mosaics. The 3.76μm pixels provide a good image scale at f\/10, and the high 43 FPS frame rate allows you to capture sharp data even in average seeing conditions.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSony IMX533 1\" Monochrome CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e3008 x 3008 (9MP)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e3.76μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003e11.31mm x 11.31mm (16mm diagonal)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rate (Max)\u003c\/td\u003e\n\u003ctd\u003e43 FPS at 3008x3008 (10-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e14-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e73,000 e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQuantum Efficiency (Peak)\u003c\/td\u003e\n\u003ctd\u003e≈91%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRead Noise\u003c\/td\u003e\n\u003ctd\u003e4.46e- to 1e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32μs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD32*2MM AR Plus Multi-Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMechanical Interface\u003c\/td\u003e\n\u003ctd\u003e1.25″ Nosepiece \/ M42x0.75 Threads\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e160g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rates (USB 3.0)\u003c\/td\u003e\n\u003ctd\u003e3008×3008: 43 FPS (RAW8) \/ 19.5 FPS (RAW16)\u003cbr\u003e1920×1080: 125 FPS (RAW8) \/ 53 FPS (RAW16)\u003cbr\u003e1280×720: 185 FPS (RAW8) \/ 79 FPS (RAW16)\u003cbr\u003e640×480: 272 FPS (RAW8) \/ 115 FPS (RAW16)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Saturn-M_SQR_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51112828502301,"sku":"POA-Saturn-M-SQR","price":1048.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Saturn-M-SQR-Mono-Camera.png?v=1775181012"},{"product_id":"player-one-saturn-c-sqr-imx533-color-planetary-camera","title":"Player One Saturn-C SQR IMX533 Color Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e9 Mega Pixel 1-inch Square Color Sensor (IMX533)\u003c\/li\u003e\n\u003cli\u003e3.76µm Pixels and 73k e- Full Well Capacity\u003c\/li\u003e\n\u003cli\u003e43 FPS at Full 3008x3008 Resolution\u003c\/li\u003e\n\u003cli\u003e1.0e Minimum Readout Noise\u003c\/li\u003e\n\u003cli\u003eUSB 3.0 Data Port with 12.5mm Back Focus\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Saturn-C SQR IMX533 Color Planetary Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Saturn-C SQR camera centers on its 9MP Sony IMX533 1-inch square sensor, capturing full 3008x3008 resolution frames at up to 43 FPS. Its large 3.76µm pixels feed a massive 73k e- full well, while readout noise drops to just 1.0e in its low-noise mode, with all data processed through a 14-bit ADC for exceptional dynamic range on the brightest and faintest targets.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eThe 9MP IMX533 Square Sensor: 73k Full Well and Zero Amp Glow\u003c\/h3\u003e\n\u003cp\u003eThe Sony IMX533 is a 1-inch, 9MP back-illuminated sensor with a perfectly square 11.31mm x 11.31mm format, making the Saturn-C SQR ideal for lunar and solar mosaics without wasting pixels on an oblong field. Player One has engineered this camera to achieve an impressive 73k e- full well depth, which prevents bright features like Jupiter's Galilean moons or crater rims on the Moon from saturating, preserving detail where other cameras might clip to white. A key advantage for longer exposures is its zero amp-glow characteristic, ensuring a clean, uniform background for DSO lucky imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eDual-Mode Readout: 43 FPS Planetary vs. Sub-1.0e DSO Imaging\u003c\/h3\u003e\n\u003cp\u003eThe Saturn-C SQR incorporates a dual sampling mode to optimize performance for different targets. In Normal Mode, the camera prioritizes speed, delivering up to 43 FPS at full resolution to freeze atmospheric seeing during planetary encounters. For fainter targets, LRN (Low Readout Noise) Mode drops the read noise floor to a mere 1.0e, maximizing the signal-to-noise ratio for DSO lucky imaging. This low-noise capability is further enhanced by an HCG mode that engages automatically at higher gain settings to suppress read noise without sacrificing dynamic range.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eStable Data Transfer: USB 3.0 and Onboard DDR3 Cache\u003c\/h3\u003e\n\u003cp\u003eTo manage the high data rates from its 9MP sensor, the Saturn-C SQR includes an onboard DDR3 cache. This buffer is critical for preventing dropped frames during high-speed capture, ensuring a smooth and reliable data stream to your computer over the USB 3.0 interface. The cache reduces the demand on your host PC, maintaining stable performance even when connected to a USB 2.0 port or a less powerful computer at the scope.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003ePassive \u0026amp; Active Cooling: Maintaining a Stable 16mm Sensor\u003c\/h3\u003e\n\u003cp\u003eHeat is the enemy of low-noise imaging, and the Saturn-C SQR addresses this with a built-in Passive Cooling System (PCS) that uses a high-density sponge and thermally conductive materials to draw heat away from the 16mm diagonal sensor. For the most demanding applications like daytime solar imaging or long DSO sequences, an optional ACS (Active Cooling System) is available. This external fan unit integrates with the camera body to provide aggressive air cooling, keeping sensor temperatures stable and noise levels consistently low.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003ePlayer One Saturn-C SQR vs. ZWO ASI585MC: A Tale of Two Sensors\u003c\/h3\u003e\n\u003cp\u003eWhen choosing a modern color planetary camera, the Saturn-C SQR and ZWO's ASI585MC are both strong contenders built around recent Sony sensors. The best choice depends on your telescope and primary targets.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eZWO ASI585MC Advantage:\u003c\/strong\u003e The ASI585MC uses smaller 2.9µm pixels, which can achieve critical sampling on telescopes with shorter focal lengths without a Barlow. It also has a slightly higher maximum frame rate at full resolution.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eSaturn-C SQR IMX533 Advantage:\u003c\/strong\u003e The Saturn-C SQR's larger 3.76µm pixels are more forgiving with longer focal length instruments like SCTs and Maksutovs. Its key advantages are the massive 73k e- full well (vs. ~50k e- on the ASI585MC) for superior dynamic range on bright targets, and its 1-inch square format, which is far more efficient for creating mosaics of the Moon and Sun.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat makes the Player One Saturn-C SQR's square sensor good for mosaics?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Saturn-C SQR's 3008x3008 pixel square sensor is highly efficient for building mosaics of the Moon or Sun. Unlike rectangular sensors that require careful, overlapping placement to cover a round disk, a square sensor minimizes the number of panels needed and simplifies the alignment process in software, saving you time both at the telescope and during processing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the LRN mode on the Saturn-C SQR help with DSO lucky imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eLRN (Low Readout Noise) mode is specifically designed for deep-sky object (DSO) lucky imaging. By prioritizing low noise over raw speed, it allows the Saturn-C SQR to achieve a \u003cstrong\u003ereadout noise as low as 1.0e\u003c\/strong\u003e. This is critical for capturing faint details in galaxies and nebulae using stacks of many short exposures, as it ensures the faint signal is not lost in the camera's electronic noise.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Player One Saturn-C SQR for planetary imaging with my 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, it's an excellent match. The 3.76µm pixels of the Saturn-C SQR are well-suited to the long focal length of an f\/10 Schmidt-Cassegrain Telescope (SCT). You will achieve a good image scale for planets like Jupiter and Saturn, often without needing an aggressive Barlow lens. The large 1-inch sensor also makes it much easier to find and center planets in the field of view.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the benefit of the 73k e- full well on the Saturn-C SQR when imaging Jupiter?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eJupiter has a vast range of brightness, from its dim cloud belts to its intensely bright moons. The Saturn-C SQR's exceptionally deep \u003cstrong\u003e73,000 e- full well\u003c\/strong\u003e prevents the brighter areas and moons from becoming overexposed and losing detail. This high dynamic range allows you to capture texture in the bright zones and subtle detail in the darker belts within the same exposure.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the Saturn-C SQR camera require an external power supply?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eNo, the Player One Saturn-C SQR is powered directly through the USB 3.0 cable connected to your computer. No separate 12V power supply is needed for standard operation. The optional ACS (Active Cooling System) fan unit also draws its power from the camera and does not require a separate power source.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the difference between the Saturn-C SQR Camera and the Camera + ACS bundle?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe standard camera purchase includes the Saturn-C SQR with its built-in Passive Cooling System (PCS). The \u003cstrong\u003eCamera + ACS bundle\u003c\/strong\u003e adds the Active Cooling System, an external fan that attaches to the camera body. The ACS is recommended for users who plan to do extensive solar imaging or DSO lucky imaging, where managing sensor heat over long sessions is critical for the lowest possible noise.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSony IMX533 1\" Color CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTotal Pixels\u003c\/td\u003e\n\u003ctd\u003e9 Mega Pixels\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Resolution\u003c\/td\u003e\n\u003ctd\u003e3008 x 3008\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e3.76µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003e11.31mm x 11.31mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e16mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e14-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Depth\u003c\/td\u003e\n\u003ctd\u003e73k e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e4.46e to 1.0e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈80%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32µs to 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAdapter Threads\u003c\/td\u003e\n\u003ctd\u003eM42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFocuser Compatibility\u003c\/td\u003e\n\u003ctd\u003e1.25\" Nosepiece\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD32*2MM AR Plus Multi-Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e160g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate (USB 3.0)\u003c\/td\u003e\n\u003ctd\u003e43 FPS at 3008x3008 (RAW8)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAdditional Frame Rates\u003c\/td\u003e\n\u003ctd\u003e95 FPS at 2560x1440\u003cbr\u003e125 FPS at 1920x1080\u003cbr\u003e185 FPS at 1280x720\u003cbr\u003e272 FPS at 640x480\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_2026_Planetary_Camera_Catalog_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51112867332381,"sku":"POA-Saturn-C-SQR","price":796.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Saturn-C-SQR-Color-Camera.png?v=1775181377"},{"product_id":"player-one-uranus-m-imx585-mono-planetary-camera","title":"Player One Uranus-M IMX585 Mono Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e8.3 MP Monochrome IMX585 Sensor\u003c\/li\u003e\n\u003cli\u003e3856 x 2180 Resolution\u003c\/li\u003e\n\u003cli\u003e1\/1.2\" Sensor Format\u003c\/li\u003e\n\u003cli\u003e47 FPS at Full Resolution\u003c\/li\u003e\n\u003cli\u003e12-bit ADC\u003c\/li\u003e\n\u003cli\u003eUSB 3.0 and ST-4 Ports\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Uranus-M IMX585 Mono Planetary Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Uranus-M IMX585 Mono Planetary Camera pairs a large 1\/1.2-inch format IMX585 sensor with a native 8.3 MP resolution of 3856x2180 for capturing expansive, high-resolution views of the Moon and planets. This monochrome camera streams uncompressed frames at up to 47 FPS over USB 3.0, capturing moments of steady seeing with 12-bit analog-to-digital conversion for smoother tonal gradations and greater flexibility in post-processing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e8.3 MP at 47 FPS: High-Resolution Planetary Imaging\u003c\/h3\u003e\n\u003cp\u003eThe Uranus-M is built for \"lucky imaging,\" where high frame rates are essential to counteract atmospheric turbulence. Capturing 47 frames per second at a full 8.3 MP resolution allows you to select only the sharpest frames from a video stream, revealing fine details in Jupiter's cloud bands or the Cassini Division in Saturn's rings. The large 1\/1.2\" sensor also provides a generous field of view, making it ideal for creating detailed multi-pane mosaics of the lunar surface without requiring hundreds of panels.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eThe 12-bit Monochrome Advantage: Deeper Data for LRGB and Narrowband\u003c\/h3\u003e\n\u003cp\u003eAs a monochrome camera, the Uranus-M's sensor is inherently more sensitive than its color counterparts because no light is lost to a Bayer color filter array. Every pixel contributes to the luminance signal, resulting in a sharper, more detailed base image. The 12-bit ADC captures over 4,000 grayscale levels, providing the deep data needed to pull out faint details from planetary atmospheres or wispy lunar rays when combined with LRGB or narrowband filters.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eUranus-M vs. Color IMX585: The 8.3 MP Resolution Showdown\u003c\/h3\u003e\n\u003cp\u003eWhile a one-shot-color camera using the same IMX585 sensor offers a simpler workflow, the monochrome Uranus-M delivers superior final resolution. A color camera must interpolate color from its Bayer matrix, sacrificing some fine detail in the process. The Uranus-M captures a true, full-resolution 8.3 MP luminance layer. When you combine this sharp luminance with data from red, green, and blue filters, the resulting color image is fundamentally more detailed than what a color camera can produce from a single exposure.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eEssential Connectivity: USB 3.0 Data and ST-4 Guiding\u003c\/h3\u003e\n\u003cp\u003eThe Player One Uranus-M uses a USB 3.0 interface to handle the high data throughput required for its 47 FPS capture rate at 8.3 MP resolution, preventing dropped frames during critical imaging sessions. An integrated ST-4 guide port provides standard connectivity to almost any equatorial mount, allowing the Uranus-M to also serve as a highly sensitive guide camera for deep-sky imaging with a separate telescope.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy choose the Uranus-M mono over a color camera with the same IMX585 sensor?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003emonochrome Uranus-M\u003c\/strong\u003e provides higher sensitivity and ultimate resolution. By capturing separate luminance, red, green, and blue filtered images, you create a final color image that is sharper and more detailed than what a one-shot-color camera can achieve through its Bayer matrix. It also allows for narrowband imaging, which is impossible with a color camera.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the main advantage of the Uranus-M's 8.3 MP resolution for planetary imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e8.3 MP resolution (3856x2180)\u003c\/strong\u003e allows you to capture planets at a large image scale without needing aggressive Barlow lenses, which can dim the image and introduce optical aberrations. This high resolution records finer details directly on the sensor, preserving the quality of your data for processing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the Uranus-M's 47 FPS frame rate help when imaging Jupiter with an 8\" SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eJupiter rotates quickly, limiting video captures to just a few minutes before details smear. In an 8\" SCT at f\/10 or f\/20, the \u003cstrong\u003e47 FPS\u003c\/strong\u003e rate of the Uranus-M allows you to capture thousands of frames in that short window. This greatly increases the probability of catching moments of excellent atmospheric seeing, which you can then stack into a single, sharp final image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Player One Uranus-M for deep-sky imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWhile designed for planetary work, the Uranus-M's sensitive IMX585 sensor can be used for brighter deep-sky objects like the Orion Nebula (M42) or the Hercules Cluster (M13). As an uncooled camera, long exposures will show thermal noise, so it is best suited for taking many short exposures (a technique known as \"live stacking\" or EAA) rather than traditional long-duration astrophotography.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the Uranus-M a good choice for creating high-resolution lunar mosaics with a 100mm refractor?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, it's an excellent choice. The large \u003cstrong\u003e1\/1.2\" format sensor\u003c\/strong\u003e captures a wide swath of the lunar surface in each frame, reducing the number of panels needed for a full mosaic. The 8.3 MP resolution will capture fine craterlet detail even in a smaller 100mm telescope.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat accessories do I need to get started with the Uranus-M for color imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eTo produce color images with the Uranus-M, you will need two key accessories: a \u003cstrong\u003efilter wheel\u003c\/strong\u003e and an \u003cstrong\u003eLRGB filter set\u003c\/strong\u003e (Luminance, Red, Green, Blue). You will capture separate videos through each filter and then combine them in software to create a full-color, high-resolution image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eMonochrome IMX585\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFormat\u003c\/td\u003e\n\u003ctd\u003e1\/1.2\"\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e3856 x 2180\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Count\u003c\/td\u003e\n\u003ctd\u003e8.3 MP\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e47 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Uranus-M_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51112956985629,"sku":"POA-Uranus-M","price":614.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Uranus-M-Mono-Camera.png?v=1775181440"},{"product_id":"player-one-uranus-c-imx585-color-planetary-camera","title":"Player One Uranus-C IMX585 Color Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e8.3 Megapixel Sony IMX585 Color CMOS Sensor\u003c\/li\u003e\n\u003cli\u003e1\/1.2\" Format with 12.85mm Diagonal\u003c\/li\u003e\n\u003cli\u003e2.9μm Pixel Size\u003c\/li\u003e\n\u003cli\u003e47 FPS at Full 3856x2180 Resolution\u003c\/li\u003e\n\u003cli\u003eExtremely Low 0.7e Read Noise\u003c\/li\u003e\n\u003cli\u003e47k e- Full Well Capacity\u003c\/li\u003e\n\u003cli\u003eUSB 3.0 Data Port\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Uranus-C IMX585 Color Planetary Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Uranus-C camera pairs Sony's latest IMX585 STARVIS 2 sensor with an engineering focus on eliminating noise sources common in high-speed imaging. Its 8.3 MP resolution at 3856x2180 captures expansive planetary and lunar surfaces, while the 1\/1.2\" format sensor with 2.9μm pixels resolves fine detail. This camera sustains a full-resolution frame rate of 47 FPS, supported by a deep 47k e- full well and a minimal read noise of 0.7e for clean, high-dynamic-range captures.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony IMX585 STARVIS 2: A 1\/1.2\" Sensor with 8.3MP\u003c\/h3\u003e\n\u003cp\u003eAt the core of the Uranus-C is the Sony IMX585, a large 1\/1.2\" format color sensor with a 12.85mm diagonal. This large sensor size, combined with an 8.3 MP resolution of 3856x2180, makes capturing the entire lunar disc or creating large planetary mosaics significantly more efficient. The back-illuminated STARVIS 2 architecture and 2.9μm pixels achieve a peak Quantum Efficiency of approximately 91%, ensuring that faint signals from planetary cloud bands or deep-sky targets are registered effectively.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eNoise Control: A 47k e- Full Well with Zero Amp Glow\u003c\/h3\u003e\n\u003cp\u003eThe Uranus-C is engineered for exceptionally clean images, even in demanding EAA (Electronically Assisted Astronomy) and lucky imaging applications. Its standout feature is a complete absence of amplifier glow, providing a uniformly dark background that simplifies processing. This is complemented by a deep 47,000 e- full well capacity and read noise as low as 0.7 electrons, delivering a high dynamic range to capture both the bright core of Jupiter and the subtle detail in its surrounding moons in a single exposure.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e47 FPS Capture with Onboard DDR3 Cache\u003c\/h3\u003e\n\u003cp\u003eTo ensure stable, high-speed video capture, the Uranus-C integrates a DDR3 cache. This buffer prevents frame dropping during planetary imaging sessions by securing data transmission before it's written to your computer. The camera can maintain 47 FPS at its full 8.3 MP resolution over USB 3.0, and can reach up to 418 FPS at reduced resolutions like 640x480, allowing you to freeze moments of excellent seeing. The cache also reduces the demand on the host computer, ensuring reliable operation even when connected to a USB 2.0 port.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003ePassive Cooling System and 12.5mm Back Focus\u003c\/h3\u003e\n\u003cp\u003eThe Uranus-C features a Passive Cooling System (PCS) that uses the camera's metal housing to dissipate heat from the sensor, maintaining thermal stability during long imaging sessions. The camera body has a 66mm diameter, weighs only 160g, and provides a standard 12.5mm back focal length. It connects to your telescope using either the included 1.25\" nosepiece or its native M42x0.75 threads, offering flexible integration with filter wheels and other accessories.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003ePlayer One Uranus-C vs. ZWO ASI585MC: Key Differentiators\u003c\/h3\u003e\n\u003cp\u003eWhile both cameras use the excellent Sony IMX585 sensor, they differ in design philosophy and features. The ZWO ASI585MC is a well-established camera with a large user base and offers dual 6.5mm\/17.5mm back focus options for greater hardware flexibility.\u003c\/p\u003e\n\u003cp\u003eThe Player One Uranus-C, however, distinguishes itself with specific anti-noise technologies that directly impact image quality.\n\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eZero Amp Glow:\u003c\/strong\u003e Player One guarantees a completely amp-glow-free sensor, which is a significant advantage for EAA and lucky imaging, resulting in cleaner, easier-to-process backgrounds.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eDPS Technology:\u003c\/strong\u003e The camera features Dead Pixel Suppression (DPS), which analyzes and corrects for fixed abnormal pixels in-camera, reducing post-processing work.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eDDR3 Cache:\u003c\/strong\u003e While both cameras have a buffer, Player One was the first to implement it across their planetary line, ensuring robust data transfer without dropped frames.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the Uranus-C's 1\/1.2\" sensor benefit lunar imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe large 1\/1.2\" sensor, with its 12.85mm diagonal, allows you to capture a much larger portion of the Moon's surface in a single frame compared to smaller planetary cameras. This significantly reduces the number of panels needed to create a full lunar mosaic, saving time during both capture and processing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the advantage of the Uranus-C's \"Zero Amp Glow\" for EAA on M13?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor EAA or lucky imaging on targets like the Hercules Cluster (M13), amp glow can introduce a bright, uneven pattern in the background, especially during longer exposures or high-gain captures. The Uranus-C's zero-amp-glow design provides a perfectly flat, dark background, making it much easier to stack short exposures and pull out faint stars at the edge of the cluster without complex calibration frames.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Player One Uranus-C with my 8\" f\/10 SCT for imaging Jupiter?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, the Uranus-C is an excellent match for an 8\" f\/10 SCT. The 2.9μm pixels are well-sized for sampling planetary detail at this focal length, often without needing a Barlow lens. The high frame rate of 47 FPS will allow you to capture thousands of frames in a short period, maximizing your chances of catching moments of steady seeing to resolve fine details in Jupiter's cloud belts.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does the DDR3 cache in the Uranus-C camera actually do?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe DDR3 cache is an internal memory buffer. When you are capturing video at high frame rates like 47 FPS, the camera temporarily stores the image data in this fast cache before sending it to your computer over the USB cable. This prevents data bottlenecks and lost frames, ensuring a smooth, stable video stream, which is critical for planetary imaging software like SharpCap or FireCapture.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the difference between the Player One Uranus-C (IMX585) and Neptune series cameras?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe primary difference is the sensor format. The Uranus-C uses the large 1\/1.2\" IMX585 sensor (12.85mm diagonal), making it ideal for wide-field lunar, solar, and planetary imaging. The Neptune series uses smaller 1\/2\" format sensors, which provide a more magnified view at the same focal length, often preferred for high-magnification views of planets like Saturn and Mars without a Barlow lens.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the Passive Cooling System (PCS) work on the Uranus-C?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Passive Cooling System (PCS) uses the camera's metal body as a heat sink. It conducts heat generated by the sensor during operation to the outer casing, where it radiates away into the air. This helps stabilize the sensor's temperature, reducing thermal noise during longer exposures for EAA or lucky imaging. For even greater cooling, an optional external Active Cooling System (ACS) fan is also available.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSony IMX585 1\/1.2\" Color CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e3856 x 2180 (8.3 MP)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e12.85mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Size\u003c\/td\u003e\n\u003ctd\u003e11.2mm x 6.3mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e47 FPS (at 3840x2160, 10-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e47k e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e7.2e to 0.7e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈91%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32μs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTelescope Adapter\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD32*2MM AR Plus Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e160g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBayer Matrix\u003c\/td\u003e\n\u003ctd\u003eRGGB\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rate Options\u003c\/td\u003e\n\u003ctd\u003e46FPS @ 3856x2180 (RAW8), 187FPS @ 1920x1080 (RAW8), 418FPS @ 640x480 (RAW8)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePurchase Options\u003c\/td\u003e\n\u003ctd\u003eCamera, Camera + ACS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Uranus-C_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113067708701,"sku":"POA-Uranus-C","price":516.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Uranus-C-Color-Camera.png?v=1775181959"},{"product_id":"player-one-neptune-664c-color-planetary-camera","title":"Player One Neptune 664C Color Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003eAdopts the 4.2MP Sony IMX664 color CMOS sensor\u003c\/li\u003e\n\u003cli\u003eHigh-speed capture at 93 FPS at full 2704x1540 resolution\u003c\/li\u003e\n\u003cli\u003eExtremely low read noise, down to 0.67e\u003c\/li\u003e\n\u003cli\u003eLarge 38.5k e- full well capacity\u003c\/li\u003e\n\u003cli\u003eSTARVIS 2 technology provides zero amplifier glow\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Neptune 664C Color Planetary Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Neptune 664C camera leverages Sony's latest STARVIS 2 technology to deliver frames with zero amplifier glow. Its 1\/1.8\" IMX664 sensor features 4.2 megapixels with 2.9µm pixels, achieving a peak QE of approximately 91% for exceptional sensitivity. The camera sustains a capture rate of 93 FPS at its full 2704x1540 resolution, while a deep 38.5k e- full well and read noise as low as 0.67e ensure high dynamic range on the brightest planetary targets.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony STARVIS 2 Sensor: 4.2 MP Resolution and 91% QE\u003c\/h3\u003e\n\u003cp\u003eAt the core of the Neptune 664C is the Sony IMX664 color sensor, a back-illuminated chip designed for low-light sensitivity. The 2.9µm pixel size is well-suited for sampling planetary detail with a wide range of telescopes, while the 4.2 megapixel resolution captures a generous field of view on the Moon and Sun. With a peak Quantum Efficiency of ~91% and a large 38.5k e- full well capacity, the sensor gathers light efficiently and avoids saturation on bright targets like Jupiter's cloud belts or Saturn's rings, preserving subtle color and brightness variations.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eZero Amp Glow \u0026amp; HCG Mode: Clean Data at Gain 180\u003c\/h3\u003e\n\u003cp\u003eA significant advancement of the STARVIS 2 architecture is the complete elimination of amplifier glow, resulting in perfectly dark calibration frames. This camera also features a High Conversion Gain (HCG) mode that automatically activates at a gain setting of 180 or higher. This function drastically reduces read noise to as low as 0.67e, allowing you to use higher gain settings to capture faint details without sacrificing dynamic range.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eDDR3 Cache:\u003c\/strong\u003e An internal cache ensures stable, drop-free data transmission to your computer, even over slower USB 2.0 connections.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eDPS Technology:\u003c\/strong\u003e Dead Pixel Suppression (DPS) analyzes dark frames to identify and correct for hot or cold pixels during image capture, producing cleaner raw files.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eHigh-Speed Planetary Capture: 93 FPS at Full 2704x1540 Resolution\u003c\/h3\u003e\n\u003cp\u003eTo freeze atmospheric turbulence—the key to sharp planetary imaging—high frame rates are essential. The Neptune 664C uses a USB 3.0 interface to stream data at up to 93 frames per second at its full 4.2 MP resolution. By selecting a smaller region of interest (ROI), you can increase this rate significantly, reaching up to 398 FPS at a 640x480 resolution, ideal for capturing fine detail on Jupiter, Mars, and Saturn during moments of steady seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eUV\/NIR Enhanced Optical Window and 12.5mm Back Focus\u003c\/h3\u003e\n\u003cp\u003eThe Neptune 664C is equipped with a high-quality AR Plus coated protective window that provides high light transmission from ultraviolet (310nm) to near-infrared (1100nm). This makes the camera highly effective for UV imaging of Venus's cloud tops and for methane band or IR-pass imaging of Jupiter and Saturn, which can reveal detail not visible in the visual spectrum. The camera body features standard M42x0.75 threads and a 1.25\" nosepiece, with a sensor distance of 12.5mm from the front flange for straightforward integration with accessories.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eNeptune 664C vs. Neptune-C II: 38.5k Full Well and STARVIS 2\u003c\/h3\u003e\n\u003cp\u003eWhile its predecessor, the Neptune-C II (IMX464), set a high standard for planetary imaging, the Neptune 664C introduces key upgrades with its IMX664 sensor. The primary advantages stem from the move to Sony's STARVIS 2 technology.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eAmplifier Glow:\u003c\/strong\u003e The Neptune 664C has zero amp glow, a significant improvement over the first-generation STARVIS sensor in the Neptune-C II, simplifying calibration and producing cleaner data.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eFull Well Depth:\u003c\/strong\u003e The Neptune 664C boasts a full well capacity of 38.5k e-, more than three times that of the Neptune-C II. This provides vastly superior dynamic range, preventing clipping of highlights on bright planets and capturing a wider range of tones in a single exposure.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eRead Noise:\u003c\/strong\u003e Both cameras feature very low read noise, but the combination of zero amp glow and HCG mode in the 664C makes it easier to achieve clean, noise-free results at high gain settings.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the main advantage of the Player One Neptune 664C's STARVIS 2 sensor?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe primary advantage is the complete \u003cstrong\u003eelimination of amplifier glow\u003c\/strong\u003e. This means your dark frames are truly dark, which simplifies image calibration and results in cleaner, higher-quality final images, especially on long exposures or high-gain planetary captures.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the HCG mode on the Neptune 664C work?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe High Conversion Gain (HCG) mode automatically activates when the camera's gain is set to \u003cstrong\u003e180 or higher\u003c\/strong\u003e. When enabled, it significantly reduces the camera's read noise to as low as 0.67e while preserving the full dynamic range you would expect at low gain. This is ideal for pulling out faint details on planets or moons without introducing excess noise.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow will the Neptune 664C perform on Jupiter with an 8\" SCT at f\/10?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Neptune 664C is an excellent match for this setup. The \u003cstrong\u003e2.9µm pixels\u003c\/strong\u003e provide good image sampling at the long focal length of an f\/10 SCT, often without needing a Barlow lens. The high frame rate (up to 93 FPS at full resolution) is crucial for \"lucky imaging\" of Jupiter, allowing you to capture thousands of frames quickly to overcome atmospheric seeing. The large \u003cstrong\u003e38.5k e- full well\u003c\/strong\u003e will prevent the bright zones of the planet from overexposing while still capturing detail in the darker belts.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the Neptune 664C a good choice for imaging the Sun in H-alpha?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, it's a very capable solar camera. Its high sensitivity in the near-infrared includes the H-alpha wavelength (656nm). The camera also incorporates a mechanism to adjust the sensor tilt, which can help eliminate Newton's rings—an interference pattern often seen when imaging the Sun's flat, monochromatic disk. The high frame rates are also beneficial for capturing sharp details of prominences and surface granulation.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy is the DDR3 cache important in the Player One Neptune 664C?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe DDR3 cache acts as a high-speed buffer for image data before it's sent to your computer. This ensures a stable data stream, \u003cstrong\u003epreventing dropped frames\u003c\/strong\u003e during high-speed video capture. It also reduces the processing load on your computer, meaning the camera performs reliably even when connected to a less powerful PC or a USB 2.0 port.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the Neptune 664C a color or mono camera? What are the trade-offs?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Neptune 664C is a \u003cstrong\u003eone-shot color (OSC) camera\u003c\/strong\u003e. The main advantage is simplicity; you can capture full-color images immediately without the need for filter wheels and LRGB filter sets. The trade-off is that a mono camera will always be more sensitive and provide higher resolution, as it doesn't have the Bayer matrix covering the pixels. For advanced imagers wanting to use specialized filters (like methane or UV), a monochrome camera is generally preferred, but the 664C offers a much faster and easier path to excellent color planetary images.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX664 1\/1.8\" Color CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTotal Pixels\u003c\/td\u003e\n\u003ctd\u003e4.2 Mega Pixels\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Resolution\u003c\/td\u003e\n\u003ctd\u003e2704×1540\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e9mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Size\u003c\/td\u003e\n\u003ctd\u003e7.8mm × 4.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rate (Max)\u003c\/td\u003e\n\u003ctd\u003e136FPS (10bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32μs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e6.1e to 0.67e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈91%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e38.5k e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12 bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAdapter\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42X0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eAR Plus Multi-Layer Coating (310nm-1100nm)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e180g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax FPS (RAW8 \/ RAW16) at 2704×1540\u003c\/td\u003e\n\u003ctd\u003e93 FPS \/ 46.5 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax FPS (RAW8 \/ RAW16) at 1920×1080\u003c\/td\u003e\n\u003ctd\u003e187 FPS \/ 93 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax FPS (RAW8 \/ RAW16) at 640×480\u003c\/td\u003e\n\u003ctd\u003e398 FPS \/ 294 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Neptune_664C_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113136062749,"sku":"POA-Neptune-664C","price":390.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Neptune-664C-Color-Camera.png?v=1775182299"},{"product_id":"player-one-neptune-c-ii-imx464-color-planetary-camera","title":"Player One Neptune-C II IMX464 Color Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e4.2 Megapixel Sony IMX464 Color Sensor\u003c\/li\u003e\n\u003cli\u003e9mm Sensor Diagonal (1\/1.8\" Format)\u003c\/li\u003e\n\u003cli\u003e2.9µm Pixel Size\u003c\/li\u003e\n\u003cli\u003e93 FPS at Full 2712x1538 Resolution\u003c\/li\u003e\n\u003cli\u003eRead Noise as low as 0.7e\u003c\/li\u003e\n\u003cli\u003e12-bit ADC\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Neptune-C II IMX464 Color Planetary Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Neptune-C II camera centers its design on Sony's IMX464 sensor, delivering 4.2 megapixels of resolution across a 9mm diagonal format. Its 2.9µm pixels and 12k e full well capacity are optimized for capturing fine details on planetary surfaces. At a full resolution of 2712x1538, the Neptune-C II sustains a capture rate of 93 FPS, while its low-noise architecture achieves a read noise floor of just 0.7e and a peak Quantum Efficiency of approximately 90%.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony IMX464 Sensor: 4.2MP at a 9mm Diagonal\u003c\/h3\u003e\n\u003cp\u003eThe Neptune-C II employs a 1\/1.8\" format Sony IMX464 color sensor, a significant step up in size and resolution from smaller 1\/3\" class planetary imagers. With a 4.2 MP resolution of 2712x1538 and a 9mm diagonal, this sensor provides a larger field of view to easily frame Jupiter with its Galilean moons or capture expansive lunar surface mosaics. The 2.9µm pixel size offers a sharp image scale on Schmidt-Cassegrains and other long-focal-length telescopes typically used for high-magnification planetary work.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e0.7e Read Noise and 90% QE: Capturing Low-Contrast Detail\u003c\/h3\u003e\n\u003cp\u003eSuccess in planetary imaging depends on pulling faint, low-contrast features out of the noise. The Neptune-C II's sensor architecture achieves a peak Quantum Efficiency of approximately 90% and a read noise that drops from 2.9e to an exceptionally low 0.7e. This camera features an HCG (High Conversion Gain) mode that automatically activates at a gain setting of 83 or higher, drastically reducing read noise without sacrificing dynamic range. This combination ensures that subtle details like Jupiter's cloud bands and Martian dust features are cleanly captured.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e93 FPS at Full Resolution with Onboard DDR3 Cache\u003c\/h3\u003e\n\u003cp\u003eTo freeze atmospheric turbulence, high-speed capture is essential. The Neptune-C II delivers 93 FPS at its full 4.2MP resolution over a USB 3.0 connection. For even faster rates, you can use a smaller region of interest (ROI) to achieve up to 299 FPS at 640x480. Player One includes a DDR3 cache to ensure stable, drop-free data transmission at these high speeds, preventing corrupted frames and reducing the computational load on your capture computer.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eAdvanced Imaging Tools: DPS, Tilt Plate, and IR Sensitivity\u003c\/h3\u003e\n\u003cp\u003eThe Neptune-C II incorporates several features for advanced imagers. Onboard Dead Pixel Suppression (DPS) technology analyzes dark frames to create an internal map of abnormal pixels, correcting them in every frame you capture. For solar imagers, a built-in sensor tilt plate allows you to adjust the focal plane to eliminate distracting Newton's rings. The IMX464 sensor also possesses strong infrared sensitivity, making it highly effective with IR-pass filters to enhance contrast and cut through atmospheric seeing for sharper lunar and planetary images.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eNeptune-C II (IMX464) vs. IMX462 \u0026amp; IMX178 Sensors\u003c\/h3\u003e\n\u003cp\u003eThe IMX464 sensor in the Neptune-C II offers a distinct set of advantages over other popular planetary sensors.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003evs. IMX462-based cameras:\u003c\/strong\u003e While both sensors share exceptional sensitivity and low read noise, the IMX464 provides double the resolution (4.2MP vs. 2.1MP) and a significantly larger 1\/1.8\" sensor format. This gives you a wider field of view and more imaging real estate.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003evs. IMX178-based cameras:\u003c\/strong\u003e The Neptune-C II's 2.9µm pixels are larger than the 2.4µm pixels of the IMX178, giving each pixel a greater light-gathering area for improved sensitivity. More importantly, the Neptune-C II achieves a much higher frame rate at full resolution (93 FPS vs. ~60 FPS), allowing you to capture more frames in the same period of stable seeing.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat makes the Player One Neptune-C II's IMX464 sensor good for planetary imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe IMX464 provides an ideal combination of specifications for planetary work. Its \u003cstrong\u003e4.2MP resolution\u003c\/strong\u003e and \u003cstrong\u003e2.9µm pixels\u003c\/strong\u003e resolve fine detail on typical f\/10 telescopes, while the \u003cstrong\u003e9mm diagonal\u003c\/strong\u003e offers a generous field of view. Critically, its \u003cstrong\u003e≈90% QE\u003c\/strong\u003e and read noise as low as \u003cstrong\u003e0.7e\u003c\/strong\u003e ensure maximum sensitivity for capturing low-contrast atmospheric features.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the DDR3 cache in the Neptune-C II improve my imaging sessions?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe DDR3 cache acts as a high-speed buffer, ensuring stable data transfer from the camera to your computer, especially at high frame rates like 93 FPS. This prevents dropped frames, which can ruin a capture sequence, and reduces read noise by ensuring a clean data stream. It also makes the camera less demanding on your computer's resources.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Player One Neptune-C II for solar imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, with a dedicated and safe solar telescope or filter. The Neptune-C II is well-suited for solar imaging due to its high frame rates, which help counteract daytime atmospheric turbulence. It also includes a built-in sensor tilt plate, allowing you to adjust the sensor's angle to eliminate Newton's rings, a common artifact in solar imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the benefit of the Neptune-C II's low 0.7e read noise?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eRead noise is the electronic noise introduced when the sensor's signal is read out. A very low read noise of \u003cstrong\u003e0.7e\u003c\/strong\u003e means that extremely faint details are not lost in the electronic background noise of the camera. This is crucial for capturing subtle cloud variations on Jupiter, faint festoons on Saturn, or delicate features within lunar rilles.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow will the Neptune-C II perform on Jupiter with an 8\" SCT at f\/10?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Neptune-C II is an excellent match for an 8\" SCT. The camera's 2.9µm pixels will provide a well-sampled image scale for resolving details in the Great Red Spot and major cloud bands. The high frame rate of 93 FPS (and higher with ROI) will allow you to run very short exposures, effectively freezing moments of good seeing and maximizing the data you can capture during Jupiter's rapid rotation.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the Neptune-C II a good choice for high-resolution lunar mosaics with a 120mm refractor?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAbsolutely. The 4.2MP resolution and 9mm diagonal sensor provide a wide enough field to capture large sections of the lunar surface in each panel, reducing the total number of panes needed for a full mosaic. The camera's high sensitivity and low noise will excel at capturing the subtle gray tones and fine details along the terminator of the Moon.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX464 1\/1.8\" Color CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e4.2 MP (2712×1538)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Dimensions\u003c\/td\u003e\n\u003ctd\u003e7.9mm × 4.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e9mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePeak QE\u003c\/td\u003e\n\u003ctd\u003e≈90%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e2.9e ~ 0.7e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e12k e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32µs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rate\u003c\/td\u003e\n\u003ctd\u003e93 FPS at 2712×1538\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rate (ROI)\u003c\/td\u003e\n\u003ctd\u003e105 FPS @ 2560x1440\u003cbr\u003e138 FPS @ 1920x1080\u003cbr\u003e204 FPS @ 1280x720\u003cbr\u003e299 FPS @ 640x480\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMounting Adapter\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42 x 0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD21 x 1.1mm AR Plus Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e180g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Neptune-C_II_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113167257885,"sku":"POA-Neptune-C-II","price":278.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Neptune-C-II-Color-Camera.png?v=1775182482"},{"product_id":"player-one-neptune-c-imx178-color-planetary-camera","title":"Player One Neptune-C IMX178 Color Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003eSensor: Sony IMX178 1\/1.8\" Color CMOS\u003c\/li\u003e\n\u003cli\u003eResolution: 6.4 MP (3096x2078)\u003c\/li\u003e\n\u003cli\u003ePixel Size: 2.4µm\u003c\/li\u003e\n\u003cli\u003eMax Frame Rate: 60 FPS (at full resolution)\u003c\/li\u003e\n\u003cli\u003eRead Noise: 1.3e (Minimum)\u003c\/li\u003e\n\u003cli\u003eFull Well Capacity: 15k e\u003c\/li\u003e\n\u003cli\u003eADC: 14-bit\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Neptune-C IMX178 Color Planetary Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Neptune-C IMX178 Color Planetary Camera is built around Sony's 6.4 Megapixel IMX178 sensor, using small 2.4µm pixels to resolve fine detail on planetary surfaces and intricate lunar features. Its 14-bit ADC and 15k e full well capacity capture a wide dynamic range in a single frame, while the USB 3.0 interface delivers full-resolution 3096×2078 video at up to 60 FPS. An automatic High Conversion Gain (HCG) mode engages at higher gain settings to drop read noise as low as 1.3e, preserving faint signals during high-speed lucky imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e6.4 MP IMX178 Sensor: High-Resolution Planetary and Lunar Imaging\u003c\/h3\u003e\n\u003cp\u003eWith a resolution of 3096x2078, the Neptune-C provides enough imaging scale to capture stunning detail on Jupiter, Saturn, and Mars, even with moderate focal length telescopes. The 1\/1.8\" sensor format, with a 9mm diagonal, is perfectly suited for creating high-resolution mosaics of the Moon and Sun (with a proper solar filter). A peak Quantum Efficiency of approximately 80% ensures that most incoming photons are converted to signal, making for efficient data collection.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e60 FPS Capture with Onboard DDR3 Cache\u003c\/h3\u003e\n\u003cp\u003eTo ensure reliable data transfer at high frame rates, the Neptune-C incorporates a DDR3 cache. This buffer prevents frame dropping, a common issue during high-speed planetary imaging that can corrupt video files and waste valuable time during moments of steady seeing. The cache also reduces the processing load on your computer, ensuring smooth performance even when connected to a USB 2.0 port.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eStable Data Stream:\u003c\/strong\u003e The DDR3 cache acts as a high-speed buffer, guaranteeing every captured frame is successfully transferred to your computer.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eReduced System Demands:\u003c\/strong\u003e By managing data flow internally, the camera performs reliably without requiring a top-tier PC.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eMax Frame Rate:\u003c\/strong\u003e Achieves up to 60 FPS at full 6.4 MP resolution in RAW8 mode, ideal for lucky imaging techniques.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eLow-Noise Architecture: HCG Mode and 1.3e Read Noise\u003c\/h3\u003e\n\u003cp\u003eThe Neptune-C features a switchable High Conversion Gain (HCG) mode that automatically activates when gain is increased. This technology significantly reduces read noise to as low as 1.3e without compromising the sensor's native dynamic range, a critical advantage for teasing out low-contrast details like Martian dust storms or subtle Jovian cloud features. Player One's Dead Pixel Suppression (DPS) technology further cleans the image by analyzing dark frames and correcting for fixed pattern noise in real-time.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e12.5mm Back Focus: Tilt Plate, UV\/IR Filter, and ST4 Port\u003c\/h3\u003e\n\u003cp\u003eThe Neptune-C integrates several features to streamline your imaging train and improve results. An innovative sensor tilt plate is built into the camera body, allowing you to adjust the sensor's angle to eliminate Newton's rings, a common artifact in solar imaging. For accurate color, a high-quality UV\/IR cut filter is integrated as the protective window, removing the need for an external filter and ensuring natural color balance right out of the box. Standard connectivity includes an ST4 autoguiding port, M42x0.75 threads, and a 1.25\" nosepiece, providing a standard 12.5mm back focus distance.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003ePlayer One Neptune-C vs. ZWO ASI178MC: Key Differentiators\u003c\/h3\u003e\n\u003cp\u003eBoth the Neptune-C and the ZWO ASI178MC are built around the same excellent 6.4 MP Sony IMX178 color sensor, offering nearly identical resolution, pixel size, and frame rates. While the ASI178MC is a well-established camera from a market leader, the Player One Neptune-C includes several hardware features aimed at the advanced imager.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eZWO ASI178MC Advantage:\u003c\/strong\u003e Backed by a mature and widely adopted software ecosystem (ASICAP, ASIStudio) and a long track record of driver stability.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003ePlayer One Neptune-C Advantages:\u003c\/strong\u003e The primary differentiator is the onboard DDR3 cache, which provides superior data transfer stability and prevents dropped frames. The Neptune-C also incorporates a user-accessible sensor tilt plate to combat Newton's rings and features Dead Pixel Suppression (DPS) technology.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy does the Player One Neptune-C have a DDR3 cache?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe DDR3 cache is a high-speed memory buffer built into the camera. Its main purpose is to prevent dropped frames during high-speed video capture by ensuring stable data transmission. This means your video files are less likely to be corrupted, which is critical when imaging planets during brief moments of excellent atmospheric seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the HCG mode on the Neptune-C camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eHCG (High Conversion Gain) mode is a feature of the IMX178 sensor that automatically activates at high gain settings. It significantly reduces the camera's read noise (down to \u003cstrong\u003e1.3e\u003c\/strong\u003e) while preserving the full dynamic range you would get at low gain. This is essential for capturing faint, low-contrast details without introducing excessive noise.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the Neptune-C's 6.4MP sensor perform on lunar mosaics with an 8\" SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Neptune-C is an excellent choice for lunar mosaics with an 8\" f\/10 SCT. The \u003cstrong\u003e6.4 MP resolution (3096x2078)\u003c\/strong\u003e provides a large enough field of view to capture significant sections of the lunar surface in each panel, reducing the total number of panes needed for a full mosaic. The small \u003cstrong\u003e2.4µm pixels\u003c\/strong\u003e are well-matched to the focal length of an SCT, allowing you to sample details at high resolution without needing an aggressive Barlow lens.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the Neptune-C a good camera for imaging Jupiter's Great Red Spot?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, the Neptune-C is very well-suited for imaging features like Jupiter's Great Red Spot. Its ability to capture video at \u003cstrong\u003e60 FPS\u003c\/strong\u003e allows you to use \"lucky imaging\" to freeze atmospheric turbulence. The built-in UV\/IR cut filter ensures correct color balance, and the low \u003cstrong\u003e1.3e read noise\u003c\/strong\u003e helps pull out subtle color variations and textures within the storm system.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhen should I use the built-in tilt plate on the Neptune-C?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe sensor tilt plate is primarily designed to eliminate \u003cstrong\u003eNewton's rings\u003c\/strong\u003e. These are interference patterns that can appear when imaging the Sun through a Hydrogen-alpha telescope like a Lunt or Coronado. By making small adjustments to the sensor's tilt, you can change the light path just enough to make these rings disappear, resulting in a smooth, artifact-free solar image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the Neptune-C need a separate UV\/IR cut filter for color imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eNo, it does not. The Player One Neptune-C has a high-quality, multi-coated \u003cstrong\u003eUV\/IR cut filter\u003c\/strong\u003e integrated directly into the camera as its protective window. This simplifies your imaging train and ensures that the sensor receives only visible light, producing accurate and natural colors for planets and other celestial objects.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX178 1\/1.8\" Color CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Format\u003c\/td\u003e\n\u003ctd\u003e7.4mm × 5.0mm (9mm diagonal)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e6.4 MP (3096 × 2078)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.4µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e14-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rate (Max)\u003c\/td\u003e\n\u003ctd\u003e60 FPS at 3096×2078 (10-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e15k e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e2.2e to 1.3e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈80%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32µs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST4 Compatible\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD21 x 1.1mm UV\/IR Cut Coated Glass\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAdapters\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e180g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rates (USB 3.0)\u003c\/td\u003e\n\u003ctd\u003e3096×2078: 60FPS (RAW8) \/ 30FPS (RAW16)\u003cbr\u003e2560x1440: 89.5FPS (RAW8) \/ 43FPS (RAW16)\u003cbr\u003e1920×1080: 118FPS (RAW8) \/ 57FPS (RAW16)\u003cbr\u003e1280×720: 175FPS (RAW8) \/ 85FPS (RAW16)\u003cbr\u003e800×600: 208FPS (RAW8) \/ 101FPS (RAW16)\u003cbr\u003e640×480: 257FPS (RAW8) \/ 124.5FPS (RAW16)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003ePlayer One Neptune-C Camera\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Neptune-C_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113172467997,"sku":"POA-Neptune-C","price":250.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Neptune-C-Color-Camera.png?v=1775182594"},{"product_id":"player-one-neptune-m-imx178-mono-planetary-camera","title":"Player One Neptune-M IMX178 Mono Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e6.4 Megapixel Resolution (3096 x 2078)\u003c\/li\u003e\n\u003cli\u003e2.4µm Pixel Size\u003c\/li\u003e\n\u003cli\u003e60 FPS at Full Resolution (10-bit)\u003c\/li\u003e\n\u003cli\u003e15,000e- Full Well Capacity\u003c\/li\u003e\n\u003cli\u003e1.3e Minimum Read Noise\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Neptune-M IMX178 Mono Planetary Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Neptune-M planetary camera pairs a high-resolution 6.4 MP Sony IMX178 monochrome sensor with a fast USB 3.0 interface, delivering 60 FPS at its full 3096x2078 resolution. Its 2.4µm pixels are sized for detailed lunar and solar imaging, while the 15k e- full well capacity and peak Quantum Efficiency of approximately 80% capture a wide dynamic range in a single frame. With a readout noise as low as 1.3e, this 14-bit camera extracts faint surface details on planets like Jupiter and Saturn with exceptional clarity.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e6.4MP IMX178 Sensor: High-Resolution Lunar and Solar Imaging\u003c\/h3\u003e\n\u003cp\u003eAt the core of the Neptune-M is the Sony IMX178 monochrome sensor, a 1\/1.8\" format chip with a 9mm diagonal. The sensor's 6.4-megapixel resolution across a 3096x2078 array allows you to capture expansive lunar landscapes and full-disk solar images without requiring large, complex mosaics. The small 2.4µm pixels provide excellent image sampling on short-to-medium focal length refractors and imaging Newtonians, resolving fine details without the need for an aggressive Barlow lens.\u003c\/p\u003e\n\u003cp\u003eCombined with a high peak QE of ≈80% and a 15k e- full well depth, the sensor gathers significant signal before saturation. The rolling shutter is standard for this class of sensor, providing high frame rates that are ideal for \"lucky imaging\" techniques to freeze atmospheric seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e60 FPS Capture: Onboard DDR3 Cache for Flawless Data Transfer\u003c\/h3\u003e\n\u003cp\u003eThe Neptune-M is capable of capturing full-resolution 10-bit frames at 60 FPS, and even faster rates like 118 FPS at 1920x1080 when using a smaller region of interest. To ensure this high-speed data stream is transferred to your computer without errors, Player One includes an onboard DDR3 cache. This buffer prevents dropped frames and data corruption, a common issue when imaging at high speeds, especially on systems with slower hard drives or shared USB bus resources.\u003c\/p\u003e\n\u003cp\u003eThis cache greatly reduces the processing demand on the host computer, ensuring stable and reliable performance even when connected via a USB 2.0 port. You can focus on capturing the perfect moment of seeing, confident that every frame is being saved correctly.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eLow-Noise Architecture: 1.3e Read Noise, HCG Mode, and DPS\u003c\/h3\u003e\n\u003cp\u003eExtracting maximum detail requires minimizing noise, and the Neptune-M integrates several technologies to achieve this. The sensor's native read noise ranges from 2.2e down to just 1.3e at higher gain settings. When the gain is increased, the camera automatically activates HCG (High Conversion Gain) mode, which significantly reduces read noise without sacrificing the sensor's full dynamic range—a critical advantage for low-contrast planetary detail.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eDead Pixel Suppression (DPS):\u003c\/strong\u003e The camera features a built-in DPS technology that analyzes dark frames to map and correct abnormal pixels on the fly, saving you from correct them in post-processing.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eOvervoltage Protection:\u003c\/strong\u003e Circuits for overvoltage and overcurrent protection are included to safeguard the camera and connected equipment.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSolar-Ready Design: 12.5mm Back Focus and Newton's Ring Suppression\u003c\/h3\u003e\n\u003cp\u003eThe Neptune-M is housed in a 66mm diameter, 180g body designed for practical use. It includes a built-in sensor tilt plate, a key feature for dedicated solar imagers. This allows you to adjust the sensor's angle relative to the incoming light path, effectively canceling out the distracting interference patterns known as Newton's rings that often appear in monochromatic H-alpha solar imaging.\u003c\/p\u003e\n\u003cp\u003eStandard connectivity includes a 1.25\" nosepiece and M42x0.75 threads, ensuring compatibility with most focusers, filter wheels, and off-axis guiders. The camera's sensor is set at a 12.5mm back focal distance, a common standard that simplifies spacing calculations in your imaging train.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eNeptune-M vs. ZWO ASI178MM: A Feature-Driven Comparison\u003c\/h3\u003e\n\u003cp\u003eBoth the Player One Neptune-M and the ZWO ASI178MM are built around the same excellent 6.4 MP Sony IMX178 mono sensor, offering identical resolution, pixel size, and sensitivity. While ZWO benefits from a vast and mature software and driver ecosystem, Player One distinguishes the Neptune-M with several hardware-level features aimed at serious planetary imagers.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eCompetitor Advantage (ZWO ASI178MM):\u003c\/strong\u003e ZWO's cameras are supported by a wider range of third-party applications and have a longer track record in the community, which can simplify software integration.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eNeptune-M Advantage (DDR Cache):\u003c\/strong\u003e The Neptune-M includes an onboard DDR3 cache, which the ASI178MM lacks. This buffer is critical for preventing dropped frames during high-speed captures, resulting in more reliable data acquisition.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eNeptune-M Advantage (Sensor Tilt Plate):\u003c\/strong\u003e For solar imagers, the Neptune-M's built-in tilt plate is a decisive feature, offering a hardware solution to Newton's rings that the ASI178MM cannot provide.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eNeptune-M Advantage (DPS):\u003c\/strong\u003e The onboard Dead Pixel Suppression handles pixel defects in-camera, a convenience not offered at the hardware level by the competing model.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat makes the Player One Neptune-M a good choice for lunar and solar imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003eNeptune-M\u003c\/strong\u003e is ideal for lunar and solar work due to its \u003cstrong\u003e6.4 MP resolution\u003c\/strong\u003e, which captures wide fields of view, and its small \u003cstrong\u003e2.4µm pixels\u003c\/strong\u003e that resolve fine detail. As a monochrome camera, it excels with narrowband filters used for solar imaging (like H-alpha), and its built-in sensor tilt plate is a major advantage for eliminating Newton's rings.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the benefit of the DDR3 cache in the Neptune-M camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe onboard \u003cstrong\u003eDDR3 cache\u003c\/strong\u003e acts as a high-speed buffer for image data. It ensures stable data transmission from the camera to your computer, effectively preventing \u003cstrong\u003edropped frames\u003c\/strong\u003e during high-speed recording sessions. This makes captures more reliable and less demanding on your computer's CPU and hard drive speed.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the HCG mode on the Neptune-M work?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003e\u003cstrong\u003eHCG (High Conversion Gain) mode\u003c\/strong\u003e automatically activates when the camera's gain is set above a certain level. This mode alters the way the sensor converts light into a signal, drastically reducing \u003cstrong\u003ereadout noise\u003c\/strong\u003e while preserving the sensor's full \u003cstrong\u003e15k e- dynamic range\u003c\/strong\u003e. This allows you to use higher gain to capture faint details without introducing excessive noise.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow would the Neptune-M perform on Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Neptune-M's \u003cstrong\u003e2.4µm pixels\u003c\/strong\u003e are a great match for an 8\" f\/10 SCT when used with a 2x Barlow lens, which brings the focal ratio to f\/20 and achieves optimal image sampling for Jupiter's fine cloud bands. The camera's high frame rate (up to \u003cstrong\u003e175 FPS at 1280x720\u003c\/strong\u003e) is perfect for \"lucky imaging,\" allowing you to capture thousands of frames in a short period to freeze moments of steady atmospheric seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Player One Neptune-M for imaging the solar chromosphere with a Lunt H-alpha scope?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAbsolutely. The \u003cstrong\u003eNeptune-M\u003c\/strong\u003e is an excellent choice for H-alpha solar imaging. Its monochrome sensor is essential for narrowband work, and its most significant feature for this task is the \u003cstrong\u003ebuilt-in sensor tilt plate\u003c\/strong\u003e. This allows you to precisely adjust the sensor angle to mitigate or eliminate Newton's rings, a common and frustrating artifact when imaging the sun through highly parallel optical systems like a Lunt.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan the Neptune-M be used as a guide camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, the \u003cstrong\u003eNeptune-M\u003c\/strong\u003e has an ST4 guide port and the necessary sensitivity for guiding. However, its high 6.4 MP resolution produces very large files, which can be inefficient for the rapid, short exposures used in guiding. While it can work, a dedicated guide camera with a smaller sensor is often more practical and responsive for autoguiding.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX178 1\/1.8\" CMOS (Mono)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e3096×2078 (6.4 Megapixels)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.4µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Size\u003c\/td\u003e\n\u003ctd\u003e7.4mm × 5.0mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e9mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e60 FPS (at 10-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e15,000 e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e2.2e- to 1.3e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈80%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e14-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32µs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST4 Compatible\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAdapter\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42X0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD21*1.1MM AR Plus Multi-Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e180g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rates (USB 3.0)\u003c\/td\u003e\n\u003ctd\u003e3096×2078: 60fps (RAW8) \/ 30fps (RAW16)\u003cbr\u003e2560x1440: 89.5fps \/ 43fps\u003cbr\u003e1920×1080: 118fps \/ 57fps\u003cbr\u003e1280×720: 175fps \/ 85fps\u003cbr\u003e800×600: 208fps \/ 101fps\u003cbr\u003e640×480: 257fps \/ 124.5fps\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Neptune-M_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113207333149,"sku":"POA-Neptune-M","price":376.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Neptune-M-Mono-Camera.png?v=1775182755"},{"product_id":"player-one-mars-662m-mono-planetary-camera","title":"Player One Mars 662M Mono Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e2.1 Megapixel Sony IMX662 monochrome sensor\u003c\/li\u003e\n\u003cli\u003e108 FPS capture rate at full 1936x1100 resolution\u003c\/li\u003e\n\u003cli\u003eLarge 54k e- full well capacity\u003c\/li\u003e\n\u003cli\u003eExtremely low readout noise, down to 0.7e-\u003c\/li\u003e\n\u003cli\u003e12.5mm back focal length\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Mars 662M Mono Planetary Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Mars 662M Mono Planetary Camera leverages Sony's latest STARVIS 2 technology to set a new benchmark for planetary imaging. Its IMX662 sensor delivers a full 1936x1100 resolution at a blistering 108 FPS, capturing moments of perfect seeing with its sensitive 2.9μm pixels. A massive 54k e- full well capacity prevents saturation on bright targets, while peak QE of approximately 91% and readout noise as low as 0.7e ensure that even the faintest details are recorded with exceptional clarity.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony IMX662 Sensor: 2.1MP at 108 FPS\u003c\/h3\u003e\n\u003cp\u003eAt the core of the Mars 662M is the Sony IMX662, a 1\/2.8\" back-illuminated monochrome sensor designed for high-speed capture. The camera streams 12-bit data at up to 108 frames per second, allowing you to acquire thousands of frames in a short window to overcome atmospheric turbulence. The 2.1 megapixel resolution is ideal for framing planets like Jupiter and Saturn with a variety of telescope focal lengths, while the 2.9μm pixels provide a good balance of resolution and sensitivity.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e54k e- Full Well and Zero Amp Glow\u003c\/h3\u003e\n\u003cp\u003eThe Mars 662M's standout feature is its complete elimination of amplifier glow, resulting in perfectly dark and clean background calibration frames. This non-amp-glow characteristic, combined with a deep 54k e- full well, makes processing easier and produces higher quality final images. The high full well is critical for preventing the bright equatorial zones of Jupiter or the polar caps of Mars from clipping, preserving the full dynamic range of the target.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSuper AR Plus Window: UV \u0026amp; NIR Sensitivity for Advanced Imaging\u003c\/h3\u003e\n\u003cp\u003eEquipped with a D21*1.1MM protective window featuring a Super AR Plus multi-layer coating, the Mars 662M offers superb light transmission across a wide spectrum. This advanced coating is optimized for high transmittance from ultraviolet (UV) through near-infrared (NIR). This makes the Mars 662M an exceptional tool for advanced scientific imaging, such as capturing cloud details on Venus in UV or imaging the methane bands of Jupiter and Saturn in NIR.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eDDR3 Cache and Dead Pixel Suppression\u003c\/h3\u003e\n\u003cp\u003ePlayer One integrates a DDR3 cache into all their planetary cameras, and the Mars 662M is no exception. This buffer ensures stable, high-speed data transmission to your computer, eliminating dropped frames that can ruin an imaging run. The camera also features on-board Dead Pixel Suppression (DPS), which analyzes dark frames to map and correct for abnormal pixels, delivering cleaner raw data before it ever reaches your hard drive.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eMars 662M vs. IMX462 Cameras: A Generational Leap in Planetary Imaging\u003c\/h3\u003e\n\u003cp\u003eWhile cameras based on the previous-generation IMX462 sensor are highly capable, the IMX662 sensor in the Mars 662M represents a significant upgrade. The most critical difference is the full well capacity.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eMars 662M (IMX662):\u003c\/strong\u003e The 54k e- full well is roughly 4.5 times larger than its predecessor. This dramatically increases dynamic range, allowing for longer exposures on planets without saturating highlights, which is key for capturing faint moons or cloud features near the bright planetary disk.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eIMX462-based Cameras:\u003c\/strong\u003e These cameras typically have a full well of around 12k e-. While excellent for short exposures, they are more prone to clipping bright details, forcing the use of lower gain settings which can impact the signal-to-noise ratio of fainter regions.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eAmp Glow:\u003c\/strong\u003e The Mars 662M's complete lack of amp glow provides a cleaner, more uniform background than many previous-generation sensors, simplifying dark frame calibration.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat makes the Mars 662M's lack of amp glow important for planetary imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAmp glow is a faint illumination that appears in the corners of an image sensor during longer exposures. Its absence in the \u003cstrong\u003ePlayer One Mars 662M\u003c\/strong\u003e means your dark frames are perfectly dark. This results in a cleaner, flatter background in your final stacked image, making it easier to pull out low-contrast details without introducing gradients or artifacts during processing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the 54k e- full well on the Mars 662M help when imaging Jupiter?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eJupiter has both very bright zones and much dimmer belts and polar regions. The \u003cstrong\u003eMars 662M's\u003c\/strong\u003e large \u003cstrong\u003e54k e- full well\u003c\/strong\u003e prevents the bright equatorial zones from becoming overexposed and \"clipping\" to pure white. This allows you to use a gain setting that captures faint, low-contrast detail in the belts and the Great Red Spot (GRS) without losing data in the brightest areas, resulting in an image with superior dynamic range.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Player One Mars 662M for imaging in ultraviolet or infrared?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. The camera's monochrome IMX662 sensor has native sensitivity into the near-infrared (NIR), and the Super AR Plus protective window is specifically coated for high transmission from UV to NIR. This makes the \u003cstrong\u003eMars 662M\u003c\/strong\u003e an excellent choice for advanced planetary work, such as using an IR-pass filter for methane band imaging of Jupiter or a UV filter to reveal cloud patterns on Venus.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the benefit of the DDR3 cache in the Mars 662M?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe onboard DDR3 cache acts as a high-speed buffer for image data. It ensures stable data transfer from the camera to your computer, even if the PC is busy with other tasks. For the user, this means \u003cstrong\u003eno dropped frames\u003c\/strong\u003e during high-speed video capture at \u003cstrong\u003e108 FPS\u003c\/strong\u003e, which is critical for lucky imaging. It also reduces readout noise and allows the camera to perform well even when connected to a slower USB 2.0 port.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the Mars 662M suitable for solar imaging in an H-alpha telescope?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, the \u003cstrong\u003ePlayer One Mars 662M\u003c\/strong\u003e is an excellent camera for high-resolution solar imaging. Its high frame rate of \u003cstrong\u003e108 FPS\u003c\/strong\u003e is ideal for freezing moments of good seeing to capture fine details in prominences and surface granulation. The monochrome sensor is essential for narrowband H-alpha work, and the complete lack of amp glow ensures a perfectly flat field for revealing subtle surface features.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does HCG mode do on the Mars 662M camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eHCG (High Conversion Gain) mode automatically activates at a gain setting of 210 on the \u003cstrong\u003eMars 662M\u003c\/strong\u003e. When engaged, it significantly reduces the camera's readout noise without sacrificing dynamic range. This is particularly useful for imaging fainter targets where higher gain is needed to bring out detail, ensuring the signal remains well above the noise floor.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX662 1\/2.8\" Mono CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e1936×1100 (2.1 MP)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Dimensions\u003c\/td\u003e\n\u003ctd\u003e5.6mm × 3.2mm (6.44mm Diagonal)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e108 FPS (at 1936x1100, 10-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32μs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e6.7e- to 0.7e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈91%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e54k e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAdapter Threads\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD21*1.1MM Super AR Plus Multi-Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e150g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Mars_662M_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113228468509,"sku":"POA-Mars-662M","price":376.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Mars-662M-Mono-Camera.png?v=1775182916"},{"product_id":"player-one-mars-m-ii-imx462-mono-planetary-camera","title":"Player One Mars-M II IMX462 Mono Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e2.1 Megapixel Monochrome IMX462 Sensor\u003c\/li\u003e\n\u003cli\u003e2.9μm Pixel Size\u003c\/li\u003e\n\u003cli\u003e136 FPS at Full Resolution (10-bit)\u003c\/li\u003e\n\u003cli\u003e≈91% Peak Quantum Efficiency\u003c\/li\u003e\n\u003cli\u003e12.5mm Back Focal Length\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Mars-M II IMX462 Mono Planetary Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Mars-M II camera centers on the monochrome Sony IMX462 sensor, delivering a full 1944×1096 resolution at up to 136 FPS for high-speed planetary imaging. Its 2.9μm pixels are optimized for resolving fine detail, while a peak Quantum Efficiency of ≈91% and read noise as low as 0.7e ensure that faint signals from planetary moons and atmospheric features are captured cleanly. With a deep 12k e full well, the Mars-M II captures a wide dynamic range in a single frame, preserving highlights on bright targets like Jupiter's Galilean moons and Saturn's rings.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eThe IMX462 Mono Sensor: 136 FPS at 2.1MP\u003c\/h3\u003e\n\u003cp\u003eAt the heart of the Mars-M II is the 1\/2.8\" Sony IMX462 monochrome sensor, a chip renowned for its sensitivity and speed. The 2.1-megapixel resolution provides enough field to easily center planets while its 2.9μm pixels offer a high-resolution sampling for telescopes with focal lengths common in planetary work, such as SCTs, Maksutovs, and long-focus refractors. Over a USB 3.0 connection, the camera streams 12-bit data at a rate that allows you to capture thousands of frames in minutes, maximizing your chances of freezing moments of perfect seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eHCG Mode and 0.7e Read Noise\u003c\/h3\u003e\n\u003cp\u003eThe Mars-M II features an exceptionally low read noise floor, dropping to just 0.7e at high gain settings. This ultra-low noise is critical for pulling faint details out of the background, especially when imaging lower-contrast targets or using narrowband filters. When the gain is set to 80 or higher, the camera automatically engages High Conversion Gain (HCG) mode. This technology drastically cuts read noise while preserving the full dynamic range you would expect at low gain, giving you clean, low-noise images without sacrificing contrast.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e91% QE and Extended UV\/IR Sensitivity\u003c\/h3\u003e\n\u003cp\u003eWhile its peak QE of ≈91% is impressive, the Mars-M II's true strength lies in its broad spectral response. The sensor is protected by a Super AR Plus coated window that transmits light from the ultraviolet (310nm) deep into the infrared (1100nm). This makes the Mars-M II a powerful tool for advanced scientific imaging. You can capture sharp details on Jupiter and Mars using an IR-pass filter to defeat atmospheric turbulence, or target the methane absorption bands on giant planets with a CH4 filter to reveal high-altitude storms.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eOnboard DDR3 Cache and Dead Pixel Suppression (DPS)\u003c\/h3\u003e\n\u003cp\u003ePlayer One integrates a DDR3 cache into all its planetary cameras to ensure data integrity during high-speed capture. This buffer prevents dropped frames by stabilizing data transmission, ensuring every frame you capture is saved to your computer, even on systems with slower hard drives or when using a USB 2.0 connection. The camera also features Dead Pixel Suppression (DPS) technology, which analyzes dark frames to map and correct for abnormal pixels automatically, resulting in cleaner raw data and reducing your post-processing workload.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eMars-M II (Mono) vs. Mars-C (Color): The Infrared Advantage\u003c\/h3\u003e\n\u003cp\u003eThe primary difference between the Mars-M II and its color sibling, the Mars-C, is the sensor type. While the Mars-C offers the convenience of one-shot-color imaging without a filter wheel, the Mars-M II provides superior raw performance for the dedicated planetary imager.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eHigher Sensitivity:\u003c\/strong\u003e Without a Bayer color filter array, the monochrome sensor of the Mars-M II captures all incoming photons at each pixel, delivering a brighter, more detailed image than its color counterpart.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eInfrared Dominance:\u003c\/strong\u003e The key advantage of the Mars-M II is its exceptional performance in near-infrared light. Paired with an IR-pass filter (like an IR685 or IR850), it can cut through atmospheric seeing to produce dramatically sharper images of planetary surfaces and cloud features.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the main advantage of the Player One Mars-M II's mono sensor?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe primary advantage is its exceptional sensitivity in the near-infrared (NIR) spectrum. This allows you to use IR-pass filters to significantly reduce the blurring effects of atmospheric turbulence (\"seeing\"), resulting in much sharper images of planets like Jupiter, Saturn, and Mars.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the HCG mode on the Mars-M II camera work?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe High Conversion Gain (HCG) mode automatically activates when the camera's gain setting is 80 or higher. It significantly reduces read noise to as low as \u003cstrong\u003e0.7e\u003c\/strong\u003e while preserving the full dynamic range of the sensor. This gives you the benefit of high-gain sensitivity without the typical noise penalty.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the purpose of the DDR3 cache in the Mars-M II?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe onboard DDR3 cache acts as a high-speed buffer. It ensures stable data transmission and prevents dropped frames during high-speed video capture, even if your computer's hard drive has slow write speeds or you are connected via a USB 2.0 port. This guarantees that all captured data is reliably saved.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow would the Mars-M II perform for imaging Jupiter with an 8\" SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Mars-M II is an excellent match for an 8\" f\/10 SCT. Its \u003cstrong\u003e2.9μm pixels\u003c\/strong\u003e provide ideal image sampling with a 2x Barlow lens. More importantly, its high infrared sensitivity allows you to use an IR-pass filter to cut through poor seeing, dramatically sharpening details in Jupiter's cloud bands and the Great Red Spot (GRS).\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Player One Mars-M II for imaging methane bands on Saturn?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, absolutely. The Mars-M II's strong sensitivity deep into the near-infrared makes it a perfect camera for methane band (CH4) imaging. This technique reveals high-altitude features in the atmospheres of Jupiter and Saturn that are invisible in other wavelengths.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eShould I choose the Mars-M II (mono) or the Mars-C (color) camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eChoose the \u003cstrong\u003eMars-C\u003c\/strong\u003e for simplicity and a faster workflow, as it captures color images in a single shot. Choose the \u003cstrong\u003eMars-M II\u003c\/strong\u003e if you want the absolute highest resolution and sensitivity. It requires a filter wheel and LRGB filters but offers superior performance, especially for advanced techniques like infrared and ultraviolet imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX462 1\/2.8\" CMOS (mono)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTotal Pixels\u003c\/td\u003e\n\u003ctd\u003e2.1 Mega Pixels\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Resolution\u003c\/td\u003e\n\u003ctd\u003e1944×1096\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e6.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003e5.6mm × 3.2mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e136 FPS (10-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32μs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e2.6e ~ 0.7e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈91%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e12k e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAdapter Threads\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD21×1.1mm Super AR Plus Multi-Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e180g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution \u0026amp; FPS (USB 3.0)\u003c\/td\u003e\n\u003ctd\u003e1944×1096: 136FPS (RAW8) \/ 62.5FPS (RAW16)\u003cbr\u003e1920×1080: 138FPS (RAW8) \/ 63.5FPS (RAW16)\u003cbr\u003e1280×720: 205FPS (RAW8) \/ 94.1FPS (RAW16)\u003cbr\u003e800×600: 245FPS (RAW8) \/ 112.4FPS (RAW16)\u003cbr\u003e640×480: 304FPS (RAW8) \/ 139.3FPS (RAW16)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Mars-M_II_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113242657053,"sku":"POA-Mars-M-II","price":348.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Mars-M-II-Mono-Camera.png?v=1775183251"},{"product_id":"player-one-mars-m-imx290-mono-planetary-camera","title":"Player One Mars-M IMX290 Mono Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003eSensor: Sony IMX290 1\/2.8\" Mono CMOS\u003c\/li\u003e\n\u003cli\u003eResolution: 1944x1096 (2.1 Megapixels)\u003c\/li\u003e\n\u003cli\u003ePixel Size: 2.9µm\u003c\/li\u003e\n\u003cli\u003eMax Frame Rate: 136 FPS (10-bit)\u003c\/li\u003e\n\u003cli\u003eRead Noise: 0.98e (Minimum)\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Mars-M IMX290 Mono Planetary Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Mars-M IMX290 Mono Planetary Camera combines a 2.1 Megapixel Sony IMX290 sensor with 2.9µm pixels, a combination purpose-built for high-resolution lunar and planetary imaging. It achieves a maximum frame rate of 136 FPS at full resolution, while its high-sensitivity design reaches a peak QE of approximately 80% with read noise as low as 0.98e. The 1\/2.8\" CMOS sensor features a 6.5mm diagonal and a full well capacity of 14.6k e, captured through a 12-bit ADC for smooth tonal gradations on bright targets like Jupiter and Saturn.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony IMX290 Sensor: 2.1 MP, 2.9µm Pixels, and ~80% QE\u003c\/h3\u003e\n\u003cp\u003eAt the core of the Mars-M is the monochrome Sony IMX290 sensor, prized for its high sensitivity and extremely low read noise. Its 2.9µm pixels create a sharp image scale on long focal length Schmidt-Cassegrains and Maksutovs, resolving fine detail in cloud bands and crater rims without requiring aggressive Barlow lenses. As a monochrome camera, it captures significantly more light than its color counterparts, resulting in brighter, higher-contrast images that are essential for lucky imaging.\u003c\/p\u003e\n\u003cp\u003eWith a peak Quantum Efficiency of ≈80% and read noise that drops to just 0.98e, the Mars-M extracts faint details with minimal noise, even during very short exposures. While its 6.5mm diagonal sensor is optimized for planets, the Moon, and sunspots, its primary trade-off is a smaller field of view, making it less suited for capturing large nebulae or galaxies in a single frame.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e136 FPS Capture with Onboard DDR3 Cache\u003c\/h3\u003e\n\u003cp\u003eThe Mars-M can stream full-resolution 1944×1096 video at up to 136 FPS in 10-bit mode. This high frame rate is critical for freezing moments of atmospheric stability, allowing you to select only the sharpest frames for stacking. To ensure every one of those frames is captured without corruption, Player One includes an onboard DDR3 cache.\u003c\/p\u003e\n\u003cp\u003eThis cache acts as a high-speed buffer, preventing dropped frames that can occur when the host computer's hard drive cannot keep up. It stabilizes data transmission, reduces read noise, and lowers the computational demand on your PC. This makes high-speed capture reliable even on older laptops or when using a USB 2.0 connection.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eDPS Technology and a D21*1.1MM AR-Coated Window\u003c\/h3\u003e\n\u003cp\u003eThe Mars-M incorporates several features to ensure clean, high-contrast images. Dead Pixel Suppression (DPS) is an onboard technology that analyzes dark frames to map and correct for hot or cold pixels automatically. This correction happens inside the camera before the data is sent to your computer, saving you a post-processing step.\u003c\/p\u003e\n\u003cp\u003eThe sensor is protected by a D21*1.1MM window with a multi-layer anti-reflection coating (AR Plus), maximizing light transmission and preventing internal reflections. For solar imagers, an adjustable focal plate helps mitigate Newton's rings, a common frustration when imaging through narrowband solar telescopes.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003ePlayer One Mars-M vs. ZWO ASI290MM: A Head-to-Head Comparison\u003c\/h3\u003e\n\u003cp\u003eBoth the Mars-M and ZWO's popular ASI290MM camera are built around the same excellent Sony IMX290 monochrome sensor, giving them nearly identical resolution, pixel size, and quantum efficiency. The primary differences lie in the features Player One has engineered around the sensor.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eZWO ASI290MM Advantage:\u003c\/strong\u003e ZWO offers a mature and extensive software ecosystem, including native support in their ASIAIR devices, which is a significant factor for many imagers.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003ePlayer One Mars-M Advantage:\u003c\/strong\u003e The Mars-M includes an onboard DDR3 cache, which the standard ASI290MM lacks. This buffer provides more stable data transfer and prevents dropped frames, a critical asset in high-speed planetary work. The Mars-M also specifies a slightly lower minimum read noise (0.98e vs. 1.3e) and features onboard Dead Pixel Suppression (DPS).\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the advantage of the Player One Mars-M's monochrome IMX290 sensor?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eA monochrome sensor is significantly more sensitive than a color sensor because every pixel is used to detect light, rather than being filtered for red, green, or blue. This results in brighter, sharper, and higher-contrast images of the Moon and planets. For color imaging, you can use a separate filter wheel to create superior LRGB composites.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the DDR3 cache on the Mars-M camera improve planetary imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe DDR3 cache acts as a buffer to prevent data loss during high-speed video capture. When you're recording at 136 FPS, your computer's hard drive can sometimes lag, causing \"dropped frames.\" The cache stores the data temporarily, ensuring a smooth and stable transfer, so you never lose critical data during a moment of perfect seeing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan the Player One Mars-M be used for guiding?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. The Player One Mars-M is equipped with a standard ST4 guide port. Its high sensitivity and low read noise make it an excellent autoguider for deep-sky imaging when you are not using it for planetary work.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat kind of performance can I expect from the Mars-M on Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe 2.9µm pixels of the Mars-M are an excellent match for a typical 8\" f\/10 SCT, providing a well-sampled image scale for Jupiter's cloud bands and Great Red Spot. At this focal length, you can capture detailed video at high frame rates (over 60 FPS) to \"freeze\" atmospheric turbulence, allowing software like AutoStakkert! to produce a sharp final image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the Player One Mars-M suitable for imaging solar prominences or sunspots?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAbsolutely. The Mars-M's monochrome sensor is highly sensitive to the H-alpha wavelength used in most dedicated solar telescopes. Its high frame rate is ideal for capturing sharp detail in active regions and prominences. The camera also features an adjustable focal plate to help reduce Newton's rings, a common artifact in solar imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does the Dead Pixel Suppression (DPS) on the Mars-M camera do?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eDPS is a built-in feature that automatically identifies and corrects for defective pixels on the sensor. It analyzes dark frames to create a map of these pixels and then replaces their values with an average of the surrounding pixels during imaging. This provides a cleaner image straight from the camera, reducing the need for manual cosmetic correction in software.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX290 1\/2.8\" CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTotal Pixels\u003c\/td\u003e\n\u003ctd\u003e2.1 Megapixels\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Resolution\u003c\/td\u003e\n\u003ctd\u003e1944×1096\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e6.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Size\u003c\/td\u003e\n\u003ctd\u003e5.6mm × 3.2mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e136 FPS (10bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32μs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e3.2e ~ 0.98e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈80%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well\u003c\/td\u003e\n\u003ctd\u003e14.6k e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12 bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD21*1.1MM High Quality AR Plus (Anti Reflection) Multi-Layer Coating\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAdapter\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42 x 0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e180g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution \u0026amp; Frame Rate (USB 3.0)\u003c\/td\u003e\n\u003ctd\u003e1944×1096: 136 FPS (RAW8) \/ 62.5 FPS (RAW16)\u003cbr\u003e1920×1080: 138 FPS (RAW8) \/ 63.5 FPS (RAW16)\u003cbr\u003e1280×720: 205 FPS (RAW8) \/ 94.1 FPS (RAW16)\u003cbr\u003e800×600: 245 FPS (RAW8) \/ 112.4 FPS (RAW16)\u003cbr\u003e640×480: 304 FPS (RAW8) \/ 139.3 FPS (RAW16)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Mars-M_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113269854493,"sku":"POA-Mars-M","price":250.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Mars-M-Mono-Camera.png?v=1775183420"},{"product_id":"player-one-mars-c-imx462-mono-planetary-camera","title":"Player One Mars-C IMX462 Mono Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003eFeatures a 2.1 Megapixel Sony IMX462 color sensor\u003c\/li\u003e\n\u003cli\u003eAchieves a maximum frame rate of 136 FPS at full 1944x1096 resolution\u003c\/li\u003e\n\u003cli\u003e2.9μm pixels and 12k e- full well capacity capture fine details\u003c\/li\u003e\n\u003cli\u003eExtremely low readout noise, from 2.6e down to 0.7e\u003c\/li\u003e\n\u003cli\u003eExceptional near-infrared sensitivity with a QE peak around 90%\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section-center\"\u003e\n      \u003ch2\u003ePlayer One Mars-C IMX462 Mono Planetary Camera\u003c\/h2\u003e\n      \u003cp\u003eThe Player One Mars-C camera leverages the Sony IMX462 color sensor to deliver high-speed planetary performance, capturing full-resolution 1944x1096 images at up to 136 FPS. Its 2.9μm pixels are well-suited for resolving fine details on Jupiter and Saturn, while the extremely low 0.7e read noise and 12k e- full well capacity ensure a clean signal during short exposures. With a peak Quantum Efficiency of approximately 90% in the near-infrared, the Mars-C excels at specialized imaging, such as capturing methane band detail, behaving like a monochrome camera with the appropriate filter.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eA 2.1 MP Color Sensor with Monochrome IR Capability\u003c\/h3\u003e\n      \u003cp\u003eAt its core, the Mars-C uses a 2.1 Megapixel Sony IMX462 sensor with an RGGB Bayer matrix for color imaging. However, its unique strength lies in its sensitivity beyond the visible spectrum, where its QE peaks at ≈90%. This allows you to use it as a high-performance monochrome camera for IR-pass or methane band (CH4) imaging, revealing details in planetary atmospheres that are invisible in RGB.\u003c\/p\u003e\n      \u003cp\u003eThis dual-purpose capability makes the Mars-C a highly flexible tool. You can capture traditional color images of Mars's polar caps or Jupiter's Great Red Spot, then switch to an IR-pass filter to cut through atmospheric haze and dramatically increase surface contrast on the same targets.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n    \n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003e136 FPS Capture with Onboard DDR3 Cache\u003c\/h3\u003e\n      \u003cp\u003eTo freeze moments of perfect atmospheric seeing, planetary imaging demands high frame rates. The Mars-C delivers up to 136 FPS at its full 1944x1096 resolution over USB 3.0. For even faster capture, windowing the sensor allows for rates up to 304 FPS at 640x480 resolution.\u003c\/p\u003e\n      \u003cp\u003eTo ensure these high-speed data streams are stable, Player One includes a DDR3 cache. This onboard memory acts as a buffer, preventing dropped frames that can occur from USB bus contention or slow hard drive write speeds. This makes your capture sessions more reliable, even on computers that are not top-of-the-line.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n    \n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003e0.7e Read Noise, HCG Mode, and DPS\u003c\/h3\u003e\n      \u003cp\u003eThe Mars-C features an exceptionally low read noise floor, bottoming out at just 0.7e. This is activated by the camera's High Conversion Gain (HCG) mode, which automatically engages at a gain of 80 and above. HCG mode significantly reduces read noise without sacrificing the sensor's dynamic range, preserving subtle details in your images.\u003c\/p\u003e\n      \u003cp\u003ePlayer One also implements Dead Pixel Suppression (DPS) technology. The camera maps any fixed-pattern abnormal pixels during factory calibration. During an imaging session, the DPS system automatically corrects these pixels by calculating a median value from surrounding pixels, resulting in cleaner raw frames before you even begin stacking.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003ePlayer One Mars-C vs. ZWO ASI462MC: The Same Sensor, Different Features\u003c\/h3\u003e\n      \u003cp\u003eBoth the Player One Mars-C and the ZWO ASI462MC are built around the excellent Sony IMX462 sensor, offering nearly identical imaging potential in terms of resolution, pixel size, and IR sensitivity. The decision between them often comes down to key hardware and firmware features.\u003c\/p\u003e\n      \u003cul\u003e\n        \u003cli\u003e\n\u003cstrong\u003eZWO ASI462MC Advantage:\u003c\/strong\u003e The ASI462MC has a strong market presence and a long track record of driver compatibility and support within the astrophotography community. Its hardware and software are a known quantity for many imagers.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003ePlayer One Mars-C Advantage:\u003c\/strong\u003e The Mars-C includes an onboard DDR3 cache, which the ASI462MC lacks. This buffer is critical for preventing frame drops during high-speed captures, ensuring more stable performance on a wider range of PCs. The Mars-C also features built-in Dead Pixel Suppression (DPS) to clean up frames in real-time.\u003c\/li\u003e\n      \u003c\/ul\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n    \n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eImaging with the 180g Mars-C: Connections and Back Focus\u003c\/h3\u003e\n      \u003cp\u003eWeighing only 180g, the Mars-C adds minimal weight to your focuser, making it easy to balance. The camera body provides both a standard 1.25\" nosepiece and female M42x0.75 threads, allowing direct connection to most focusers, Barlow lenses, and filter wheels.\u003c\/p\u003e\n      \u003cp\u003eThe sensor is positioned at a 12.5mm back focal distance from the front M42 threads. This standard spacing is compatible with most common imaging accessories, ensuring you can easily reach focus without needing a complex set of extenders. The camera also includes an ST-4 guide port for use as a high-sensitivity autoguider.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n\u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the Player One Mars-C's IR sensitivity help when imaging Jupiter?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe Mars-C's ≈90% QE in near-infrared light makes it exceptionally powerful for methane band imaging of Jupiter. Using a CH4 filter, you can capture high-contrast images of the planet's upper-atmospheric cloud structures, which are typically faint or invisible in visible light. This allows you to highlight features like high-altitude plumes and track atmospheric dynamics separately from the lower cloud decks.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat frame rate can I expect from the Mars-C on an 8\" f\/10 SCT for lunar imaging?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eOn a typical 8\" f\/10 SCT, you will likely be using a region of interest (ROI) to frame specific lunar features like the Vallis Alpes or the crater Copernicus. With the Player One Mars-C, you can expect frame rates well over 200 FPS using a smaller ROI (e.g., 1280x720 at 205 FPS or 800x600 at 245 FPS). This high rate is crucial for \"lucky imaging\" to capture fleeting moments of steady air.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the benefit of the DDR3 cache in the Mars-C camera?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe DDR3 cache is an onboard memory buffer that temporarily stores image data before it's sent to your computer. This prevents data loss (dropped frames) if your computer's USB port or hard drive can't keep up with the camera's high frame rate of 136 FPS. It ensures a stable, reliable data stream, which is critical for planetary imaging.\u003c\/p\u003e\n  \u003c\/div\u003e\n    \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eIs the Player One Mars-C a color or monochrome camera?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe Mars-C has a \u003cstrong\u003eSony IMX462 color sensor\u003c\/strong\u003e with an RGGB Bayer matrix. However, it possesses extremely high sensitivity in the near-infrared portion of the spectrum. When used with an IR-pass filter (like an IR850), it effectively ignores the Bayer matrix and acts as a very sensitive monochrome camera, making it a dual-purpose instrument.\u003c\/p\u003e\n  \u003c\/div\u003e\n    \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is HCG mode on the Player One Mars-C?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003e\u003cstrong\u003eHCG (High Conversion Gain)\u003c\/strong\u003e mode is a feature of the Mars-C's sensor that automatically activates when the gain is set to 80 or higher. It significantly reduces read noise (down to 0.7e) while preserving the full dynamic range of the sensor. This allows you to use higher gain settings to capture faint details without introducing excessive noise.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Player One Mars-C for autoguiding?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eYes. The Mars-C is equipped with a standard \u003cstrong\u003eST-4 guide port\u003c\/strong\u003e. Its high sensitivity, especially in the near-infrared where many stars are bright, makes it an excellent autoguider for capturing long-exposure deep-sky images with a separate telescope.\u003c\/p\u003e\n  \u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003ctable class=\"DAV-specifications\"\u003e\n    \u003ctbody\u003e\n      \u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX462 1\/2.8\" CMOS (color)\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e1944×1096 (2.1 MP)\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9μm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e6.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eImage Size\u003c\/td\u003e\n\u003ctd\u003e5.6mm × 3.2mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e136 FPS (at 1944x1096, 10-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e12k e-\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e2.6e to 0.7e\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈90%\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32μs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eGuide Port\u003c\/td\u003e\n\u003ctd\u003eST-4\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eAdapter Threads\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eAR Plus Multi-Coated (D21*1.1mm)\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e180g\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eBayer Matrix\u003c\/td\u003e\n\u003ctd\u003eRGGB\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003c\/tbody\u003e\n  \u003c\/table\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cul class=\"DAV-grid\"\u003e\n    \u003c!-- whats_in_the_box was empty in the source data --\u003e\n  \u003c\/ul\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Mars-C_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113289679133,"sku":"POA-Mars-C","price":194.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Mars-C-Color-Camera.png?v=1775183553"},{"product_id":"player-one-mars-c-ii-imx662-color-planetary-camera","title":"Player One Mars-C II IMX662 Color Planetary Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003eSensor: Sony IMX662 1\/2.8\" Color CMOS\u003c\/li\u003e\n\u003cli\u003eResolution: 2.1 Megapixels (1936x1100)\u003c\/li\u003e\n\u003cli\u003eMax Frame Rate: 108 FPS at full resolution\u003c\/li\u003e\n\u003cli\u003eFull Well Capacity: 54,000 e-\u003c\/li\u003e\n\u003cli\u003eRead Noise: 6.7e- to 0.7e-\u003c\/li\u003e\n\u003cli\u003ePixel Size: 2.9μm\u003c\/li\u003e\n\u003cli\u003eSpecial Feature: Zero Amplifier Glow\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Mars-C II IMX662 Color Planetary Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Mars-C II IMX662 Color Planetary Camera pairs Sony's latest IMX662 STARVIS 2 sensor with a massive \u003cstrong\u003e54k e-\u003c\/strong\u003e full well capacity and a peak QE of \u003cstrong\u003e≈91%\u003c\/strong\u003e. It captures full-resolution \u003cstrong\u003e1936x1100\u003c\/strong\u003e frames at up to \u003cstrong\u003e108 FPS\u003c\/strong\u003e over USB 3.0, while its \u003cstrong\u003e2.9µm\u003c\/strong\u003e pixels are ideal for resolving fine detail on planets. With readout noise as low as \u003cstrong\u003e0.7e\u003c\/strong\u003e, this \u003cstrong\u003e2.1 MP\u003c\/strong\u003e camera delivers exceptionally clean images free of amplifier glow, a critical advantage for both planetary imaging and Electronically-Assisted Astronomy (EAA).\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eThe IMX662 Sensor: 2.1 MP at 108 FPS\u003c\/h3\u003e\n\u003cp\u003eAt the heart of the Mars-C II is the Sony IMX662, a \u003cstrong\u003e1\/2.8\"\u003c\/strong\u003e format color sensor that delivers a \u003cstrong\u003e1936x1100\u003c\/strong\u003e resolution image. This sensor size is an excellent match for the corrected image circle of most Barlow lenses and Schmidt-Cassegrains, minimizing field curvature issues. The camera's ability to stream \u003cstrong\u003e12-bit\u003c\/strong\u003e data at \u003cstrong\u003e108 FPS\u003c\/strong\u003e allows you to leverage lucky imaging techniques, capturing thousands of frames in a short period to freeze moments of steady atmospheric seeing and resolve intricate details in the cloud bands of Jupiter or the Cassini Division in Saturn's rings.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eZero Amp Glow and a 54k e- Full Well\u003c\/h3\u003e\n\u003cp\u003eA standout feature of the Mars-C II is its complete lack of amplifier glow. Unlike many CMOS sensors that produce a bright pattern on dark frames, the IMX662's background is entirely dark, even when stretched. This produces a perfectly clean foundation for your images, simplifying processing and making the camera highly effective for EAA where live stacking benefits from a uniform background.\u003c\/p\u003e\n\u003cp\u003eThe sensor's deep \u003cstrong\u003e54k e-\u003c\/strong\u003e full well capacity provides immense dynamic range. This prevents brighter planetary features, like Mars' polar caps or Jupiter's Galilean moons, from saturating while you expose for fainter details, resulting in richer color and more nuanced images in a single capture session.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eOnboard Hardware: DDR3 Cache and Dead Pixel Suppression (DPS)\u003c\/h3\u003e\n\u003cp\u003ePlayer One integrates a DDR3 cache into the Mars-C II to ensure stable, drop-free data transmission. This buffer protects your imaging session from lost frames, a common issue during high-speed capture, and reduces the demand on your computer's CPU. The camera maintains reliable performance even when connected to a USB 2.0 port.\u003c\/p\u003e\n\u003cp\u003eThe camera also features onboard Dead Pixel Suppression (DPS) technology. It analyzes the sensor and maps any abnormal pixels, automatically correcting them in each frame you capture. This saves significant time in post-processing by delivering cleaner raw data from the start.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eMars-C II (IMX662) vs. IMX462 Cameras: A 4x Full Well Advantage\u003c\/h3\u003e\n\u003cp\u003eWhile cameras based on the previous-generation IMX462 sensor are noted for their high infrared sensitivity, the Mars-C II with the IMX662 offers a decisive advantage for mainstream color planetary imaging. The primary difference is dynamic range.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eIMX462 Full Well:\u003c\/strong\u003e Typically around 13k e-.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eMars-C II (IMX662) Full Well:\u003c\/strong\u003e A massive \u003cstrong\u003e54k e-\u003c\/strong\u003e, over four times greater.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cp\u003eThis larger capacity means the Mars-C II is far less likely to saturate bright targets. You can use higher gain settings to capture faint moons or surface details without blowing out the highlights on the planet itself, yielding a more balanced and data-rich final image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the main advantage of the Player One Mars-C II's IMX662 sensor over the older IMX462?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe IMX662 sensor in the Mars-C II has a \u003cstrong\u003e54k e- full well capacity\u003c\/strong\u003e, over four times larger than the IMX462. This provides superior dynamic range, preventing saturation on bright targets and capturing more subtle color gradations. It also features \u003cstrong\u003ezero amplifier glow\u003c\/strong\u003e, resulting in exceptionally clean images without complex calibration.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow will the Player One Mars-C II perform on Jupiter with an 8\" f\/10 SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWith an 8\" f\/10 SCT, the Mars-C II's \u003cstrong\u003e2.9µm pixels\u003c\/strong\u003e provide excellent sampling for high-resolution planetary imaging, especially when used with a 2x Barlow lens. The camera's high frame rate of \u003cstrong\u003e108 FPS\u003c\/strong\u003e is ideal for \"lucky imaging\" to freeze atmospheric seeing, and the \u003cstrong\u003e54k e- full well\u003c\/strong\u003e will prevent the bright Galilean moons from blowing out when imaging them alongside the planet's disk.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does \"No Amp Glow\" mean for my Player One Mars-C II images?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003e\"No Amp Glow\" means the camera's sensor does not produce the typical bright pattern in the corners of dark frames that is common in many CMOS cameras. This gives you a perfectly dark, clean background, making it much easier to process your images and requiring fewer calibration frames for EAA or planetary work.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Player One Mars-C II for EAA on bright objects like the Orion Nebula (M42)?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, the Mars-C II is well-suited for EAA on brighter deep-sky objects. Its high peak QE of \u003cstrong\u003e≈91%\u003c\/strong\u003e and low \u003cstrong\u003e0.7e read noise\u003c\/strong\u003e make it very sensitive. The zero amp glow is a major benefit for EAA, as it provides a clean background for live stacking without needing dark frame subtraction.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the purpose of the DDR3 cache in the Mars-C II camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe onboard DDR3 cache acts as a high-speed buffer for image data. It ensures stable data transmission to your computer, effectively eliminating dropped frames during high-speed capture. This makes the camera's performance reliable even if your computer's hard drive is slow or you are connected via a USB 2.0 port.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDo I need an IR-cut filter with the Player One Mars-C II?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. Like most color astronomy cameras, the Mars-C II is sensitive to infrared light, which can affect color balance. To achieve accurate colors for planetary imaging, a UV\/IR Cut filter is essential. The camera has standard \u003cstrong\u003eM42X0.75\u003c\/strong\u003e threads on its \u003cstrong\u003e1.25\" adapter\u003c\/strong\u003e for easy filter attachment.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX662 1\/2.8\" Color CMOS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Resolution\u003c\/td\u003e\n\u003ctd\u003e1936×1100 (2.1 Megapixels)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e2.9μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e6.44mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Size\u003c\/td\u003e\n\u003ctd\u003e5.6mm × 3.2mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rate\u003c\/td\u003e\n\u003ctd\u003e108 FPS (1936×1100, 10bit), 110 FPS (1920x1080), 162 FPS (1280x720)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eRolling shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32μs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e6.7e ~ 0.7e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈91%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e54k e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12 bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAdapter\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD21 x 1.1mm AR Plus Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e150g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Mars-C_II_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113320644893,"sku":"POA-Mars-C-II","price":278.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Mars-C-II-Color-Camera.png?v=1775183678"},{"product_id":"player-one-apollo-428m-max-mono-solar-camera","title":"Player One Apollo 428M MAX Mono Solar Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003eFeatures a Sony IMX428 1.1-inch monochrome CMOS sensor\u003c\/li\u003e\n\u003cli\u003eDelivers 7.1 Megapixel resolution (3216×2208) for detailed solar imaging\u003c\/li\u003e\n\u003cli\u003e4.5μm pixels provide high-resolution sampling of fine surface features\u003c\/li\u003e\n\u003cli\u003eCaptures up to 51 FPS at 10-bit for freezing atmospheric seeing\u003c\/li\u003e\n\u003cli\u003eGlobal shutter design eliminates motion artifacts on the Sun's turbulent surface\u003c\/li\u003e\n\u003cli\u003e25.3k e full well capacity captures a wide dynamic range\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Apollo 428M MAX Mono Solar Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Apollo 428M MAX is engineered specifically for high-resolution solar imaging, built around a Sony IMX428 1.1-inch monochrome sensor that resolves 7.1 megapixels with its 3216×2208 array. Its 4.5μm pixels are sized for critically sampling fine solar granulation, while the global shutter captures distortion-free images at up to 51 FPS. A deep 25.3k e full well and low read noise down to 1.4e ensure you capture the full dynamic range from bright sunspots to the subtle photosphere, with a peak QE of approximately 79% maximizing signal.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSony IMX428 Global Shutter: 7.1 MP at 51 FPS\u003c\/h3\u003e\n\u003cp\u003eThe core of the Apollo 428M MAX is its 7.1 MP Sony IMX428 sensor, whose global shutter architecture is essential for solar astronomy. Unlike a rolling shutter, a global shutter exposes every one of the 3216×2208 pixels simultaneously, eliminating the wobble and distortion caused by atmospheric seeing. This allows you to capture incredibly sharp, artifact-free images of the Sun's dynamic surface.\u003c\/p\u003e\n\u003cp\u003eAt a full-resolution frame rate of 51 FPS (10-bit), you can employ lucky imaging techniques to select only the sharpest frames captured during moments of steady seeing. The camera's low read noise, which drops to just 1.4e in HCG mode, combined with a 25.3k e full well depth, provides the dynamic range needed to record faint prominences and bright surface features in a single exposure.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSolar-Specific Hardware: D32*2mm AR Coated Window and Passive Cooling\u003c\/h3\u003e\n\u003cp\u003eDesigned for daytime operation, the Apollo 428M MAX incorporates features to manage heat and improve contrast. The sensor is protected by a D32*2mm window with a multi-layer Anti-Reflection (AR Plus) coating, which maximizes light transmission and prevents internal reflections that can reduce the contrast of delicate solar features like spicules.\u003c\/p\u003e\n\u003cp\u003eTo combat the heat generated by the sensor during prolonged solar sessions, the camera includes a Passive Cooling System (PCS). This system conducts heat away from the sensor to the camera body, helping to stabilize thermal noise. For even more demanding conditions, the camera is compatible with an optional Active Cooling System (ACS) to maintain optimal sensor temperature.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e12-bit Data Integrity: DDR3 Cache and Dead Pixel Suppression\u003c\/h3\u003e\n\u003cp\u003eTo ensure every frame is captured without corruption, the Apollo 428M MAX is equipped with an onboard DDR3 cache. This buffer prevents frame drops during high-speed data transfer over its USB 3.0 port, which is critical when writing 51 frames per second. The cache ensures a stable data stream, even if your computer's hard drive has momentary slowdowns.\u003c\/p\u003e\n\u003cp\u003eThe camera also features Dead Pixel Suppression (DPS) technology. This system identifies and corrects for non-responsive pixels directly in the camera's hardware, delivering cleaner raw frames and reducing the need for extensive post-processing. Combined with a 12-bit ADC, these features ensure your final data is clean, complete, and has the bit-depth needed for aggressive sharpening.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eApollo 428M MAX vs. Apollo-M MAX: 4.5µm Pixels for High Resolution\u003c\/h3\u003e\n\u003cp\u003eWhile both cameras use a 1.1-inch sensor format, they are optimized for different goals. The primary advantage of the classic Apollo-M MAX (IMX432) is its larger native pixel size, which provides an enormous full well capacity for maximum dynamic range on lower-magnification, full-disk images.\u003c\/p\u003e\n\u003cp\u003eThe Apollo 428M MAX, with its 4.5µm pixels, offers four times the spatial resolution. This makes it the superior choice for imagers using long focal length telescopes to resolve the finest details in sunspot umbra, granulation cells, and chromospheric plages. For versatility, the 428M MAX also offers a hardware BIN2 mode, effectively creating 9µm pixels with a much larger full well, allowing it to perform in scenarios where the IMX432 would traditionally excel.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the Apollo 428M MAX's 4.5µm pixel size perform with a DayStar Quark filter on a 1000mm refractor?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe 4.5µm pixels of the Apollo 428M MAX are an excellent match for a long focal length solar setup. With a DayStar Quark (which has a 4.2x Barlow effect), a 1000mm refractor operates at f\/42, yielding a fine image scale perfect for resolving intricate details in solar prominences and the chromosphere without needing an additional Barlow lens.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan the Apollo 428M MAX capture a full solar disk in a single frame?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThis depends on your telescope's focal length. The Apollo 428M MAX has a 17.5mm sensor diagonal. To fit the entire sun (which is about 0.5 degrees) onto this sensor, you would need a telescope with a focal length of approximately 2000mm or less. For longer focal lengths, you will need to capture a mosaic to create a full-disk image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the main advantage of the Apollo 428M MAX's global shutter?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003eglobal shutter\u003c\/strong\u003e exposes the entire 7.1 MP sensor at the same instant. This is critical for solar imaging because it prevents the \"wobble\" or distortion seen with rolling shutters when imaging through atmospheric turbulence. The result is sharper, more stable images of the sun's surface, making it easier to capture fine details.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDo I need special filters to use the Apollo 428M MAX for solar imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003e\u003cstrong\u003eYes, absolutely.\u003c\/strong\u003e You must use a dedicated, professional-grade solar filter, such as a white-light filter (like Baader AstroSolar film) or a Herschel wedge for photosphere imaging, or a Hydrogen-alpha telescope for chromosphere imaging. Pointing the camera at the sun without proper energy rejection will instantly destroy the sensor and can cause permanent eye damage.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the HCG mode on the Apollo 428M MAX work?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe High Conversion Gain (HCG) mode automatically activates at a gain setting of 70 or higher. When enabled, it significantly reduces the camera's read noise (down to 1.4e) without sacrificing its high dynamic range. This is beneficial for imaging lower-contrast features on the solar disk where you need to increase gain to see detail.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWill the Apollo 428M MAX work if I only have a USB 2.0 port?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. While a USB 3.0 port is required to achieve the maximum frame rate of 51 FPS, the camera is backward compatible with USB 2.0. The onboard DDR3 cache helps ensure stable data transfer even at the lower speeds of USB 2.0, though your maximum frame rate will be reduced.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX428 1.1\" CMOS (mono)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003e14.5mm × 9.9mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiagonal\u003c\/td\u003e\n\u003ctd\u003e17.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Resolution\u003c\/td\u003e\n\u003ctd\u003e3216×2208\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTotal Pixels\u003c\/td\u003e\n\u003ctd\u003e7.1 Mega Pixels\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e4.5μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eGlobal shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate (10-bit)\u003c\/td\u003e\n\u003ctd\u003e51 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate (12-bit)\u003c\/td\u003e\n\u003ctd\u003e27 FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e25.3k e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e5.5e ~ 1.4e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈79%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12 bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32μs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAdapter\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD32*2mm AR Plus Multi-Layer Coating\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e160g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePurchase Option\u003c\/td\u003e\n\u003ctd\u003eCamera, Camera + ACS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Apollo_428M_MAX_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113496576285,"sku":"POA-Apollo-428M-MAX","price":1118.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Apollo-428M-MAX-Mono-Camera.png?v=1775184669"},{"product_id":"player-one-apollo-m-max-imx432-mono-solar-camera","title":"Player One Apollo-M MAX IMX432 Mono Solar Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e1.1\" Sony IMX432 Monochrome CMOS Sensor\u003c\/li\u003e\n\u003cli\u003e9µm Pixel Size\u003c\/li\u003e\n\u003cli\u003e100,000 e- Full Well Capacity\u003c\/li\u003e\n\u003cli\u003e126 FPS at Full Resolution (1608x1104)\u003c\/li\u003e\n\u003cli\u003eGlobal Shutter for Distortion-Free Images\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Apollo-M MAX IMX432 Mono Solar Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Apollo-M MAX is engineered specifically for high-resolution solar imaging, built around the large 1.1\" Sony IMX432 monochrome sensor. Its 1.7 MP resolution of 1608x1104 is captured by massive 9µm pixels, which are exceptionally well-suited for long focal length solar telescopes. With an enormous 100k e- full well capacity, a peak QE of ≈79%, and read noise as low as 2.6e, this camera captures an unprecedented dynamic range in a single exposure. The global shutter operates at up to 126 FPS, delivering perfectly sharp, distortion-free images of the turbulent solar surface across its 17.5mm diagonal sensor.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eThe 1.1\" IMX432 Sensor: 9µm Pixels for Long Focal Ratios\u003c\/h3\u003e\n\u003cp\u003eThe Apollo-M MAX uses a large-format 1.1-inch sensor, but its defining feature is the 9µm pixel size. These large pixels are ideal for sampling the solar disk at the long focal lengths typical of dedicated solar setups, such as a Schmidt-Cassegrain with a DayStar Quark or other front-mounted etalon. This allows you to achieve critical sampling without aggressive Barlow lenses, preserving image brightness and contrast.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e100k e- Full Well: Capture Prominences and Photosphere in One Frame\u003c\/h3\u003e\n\u003cp\u003eWith a full well depth of 100,000 electrons, the Apollo-M MAX can handle the extreme brightness differences between the solar photosphere and faint, ethereal prominences in a single subframe. This massive capacity significantly reduces the need for complex composite images. When the camera gain is set to 145 or higher, an automatic High Conversion Gain (HCG) mode activates, dropping read noise dramatically while preserving this huge dynamic range.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eGlobal Shutter at 126 FPS: Clean, Band-Free Solar Imaging\u003c\/h3\u003e\n\u003cp\u003eThe IMX432's global shutter exposes every one of its 1.7 million pixels simultaneously, eliminating the distortion and wobble that rolling shutters can introduce when imaging through atmospheric turbulence. At a full-resolution speed of 126 FPS, you can effectively \"freeze\" the seeing for sharper results. Critically, the IMX432 sensor architecture produces exceptionally smooth images, free from the horizontal banding or row noise that can plague other popular sensors, ensuring your post-processing is focused on detail, not artifact removal.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eApollo-M MAX (IMX432) vs. The IMX174 Standard: A Generational Leap\u003c\/h3\u003e\n\u003cp\u003eFor years, the IMX174 sensor was the benchmark for serious solar imaging. The Apollo-M MAX's IMX432 represents a significant step forward in every key metric.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eFull Well Capacity:\u003c\/strong\u003e The IMX432's 100k e- capacity is more than three times larger than the ~32k e- of the IMX174, enabling true high-dynamic-range captures.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003ePixel Size:\u003c\/strong\u003e At 9µm, the IMX432's pixels have over twice the surface area of the IMX174's 5.86µm pixels, making them better suited for longer focal ratios.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eImage Quality:\u003c\/strong\u003e The IMX432 delivers images without the horizontal banding that can be a persistent issue with the IMX174, resulting in a cleaner final product.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eSensor Size:\u003c\/strong\u003e The 1.1\" format of the IMX432 provides a larger field of view compared to the 1\/1.2\" IMX174, making it easier to frame the entire solar disk.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003ePlayer One Platform: DDR3 Cache, DPS, and Passive Cooling\u003c\/h3\u003e\n\u003cp\u003eThe Apollo-M MAX includes Player One's signature features for stable and reliable imaging. A 256MB DDR3 cache acts as a high-speed buffer, preventing frame drops during 126 FPS capture and ensuring consistent data transfer even over USB 2.0. Onboard Dead Pixel Suppression (DPS) technology analyzes and corrects for abnormal pixels automatically, while the Passive Cooling System (PCS) conducts heat away from the sensor to maintain thermal stability during long daytime imaging sessions.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy are the Apollo-M MAX's 9µm pixels better for solar imaging with an SCT?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eA Schmidt-Cassegrain (SCT) paired with a solar filter like a DayStar Quark often results in a very long effective focal length (f\/30 or more). The large \u003cstrong\u003e9µm pixels\u003c\/strong\u003e of the Apollo-M MAX provide a more appropriate image scale at these focal lengths without requiring additional focal reducers, which helps maintain image brightness and contrast for a stronger signal.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the Apollo-M MAX's 100k e- full well help when imaging a solar flare?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eA solar flare or prominence is thousands of times fainter than the solar disk (photosphere). The Apollo-M MAX's enormous \u003cstrong\u003e100k e- full well capacity\u003c\/strong\u003e allows you to expose long enough to capture the faint flare detail without completely saturating and blowing out the much brighter solar surface in the same frame. This makes it possible to create stunning high-dynamic-range images with less processing effort.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the benefit of the Apollo-M MAX's global shutter?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eEarth's atmosphere causes the image of the Sun to shimmer and distort rapidly. A \u003cstrong\u003eglobal shutter\u003c\/strong\u003e exposes all 1.7 million pixels at the exact same instant, producing a snapshot that is free from the wobble or \"jello\" effect common with rolling shutters. This is essential for achieving the sharpest possible solar details.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the Player One Apollo-M MAX suffer from the horizontal banding seen in other solar cameras?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eNo. One of the primary advantages of the Sony IMX432 sensor in the Apollo-M MAX is its exceptionally clean output. It is specifically noted for producing smooth images that are free from the horizontal banding (row noise) that can be a significant artifact in images from other sensors, such as the IMX174.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the HCG mode on the Apollo-M MAX camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe High Conversion Gain (HCG) mode is a feature of the Apollo-M MAX that automatically activates at a gain setting of 145 and above. When enabled, it dramatically reduces the camera's read noise while maintaining the high dynamic range from its large full well, ensuring low-noise images even at higher gain settings.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat filters do I need to safely use the Apollo-M MAX for solar imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003e\u003cstrong\u003eWARNING:\u003c\/strong\u003e You must use a certified and safe solar filter with the Apollo-M MAX. Never point the camera at the Sun without proper energy rejection. For white light, this means a full-aperture filter like Baader AstroSolar film or a Herschel wedge. For H-alpha, you must use it with a dedicated solar telescope or a system like a DayStar Quark, which has its own required energy rejection filter (ERF).\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX432 1.1\" CMOS (Monochrome)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Resolution\u003c\/td\u003e\n\u003ctd\u003e1608×1104 (1.7 MP)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e9µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e17.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Size\u003c\/td\u003e\n\u003ctd\u003e14.5mm × 9.9mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eGlobal Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e126 FPS (at 1608x1104, RAW8)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e100k e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e22.9e to 2.6e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈79%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32μs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAdapter\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD32*2MM AR Plus Multi-Layer Coating\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e160g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rate (USB 3.0)\u003c\/td\u003e\n\u003ctd\u003e1608×1104: 126FPS (RAW8) \/ 109FPS (RAW16)\u003cbr\u003e1280×720: 187FPS\u003cbr\u003e800×600: 220FPS\u003cbr\u003e640×480: 268FPS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Apollo-M_MAX_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113521545501,"sku":"POA-Apollo-M-MAX","price":838.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Apollo-M-MAX-Mono-Camera.png?v=1775184809"},{"product_id":"player-one-apollo-m-mini-imx429-mono-solar-camera","title":"Player One Apollo-M MINI IMX429 Mono Solar Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e2.8 Megapixel SONY IMX429 monochrome sensor\u003c\/li\u003e\n\u003cli\u003e4.5μm pixels for high-resolution solar and lunar imaging\u003c\/li\u003e\n\u003cli\u003eGlobal shutter eliminates motion artifacts from atmospheric turbulence\u003c\/li\u003e\n\u003cli\u003eUp to 84 FPS at full 1944×1472 resolution\u003c\/li\u003e\n\u003cli\u003ePassive Cooling System designed for daytime thermal stability\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Apollo-M MINI IMX429 Mono Solar Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Apollo-M MINI camera centers its design on the Sony IMX429 monochrome sensor, delivering a 1944×1472 resolution across its 2.8 million 4.5μm pixels. A global shutter captures the entire frame instantly at up to 84 FPS, while the sensor's high sensitivity is defined by a ≈79% peak QE and a low read noise of 1.45e. This combination of speed and low-noise architecture, supported by a 25k e full well depth, makes the Apollo-M MINI a dedicated tool for high-resolution solar imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eIMX429 Global Shutter: Capturing the Sun at 4.5μm Resolution\u003c\/h3\u003e\n\u003cp\u003eThe critical feature for any solar camera is its shutter, and the Apollo-M MINI's global shutter exposes every one of its 2.8 million pixels simultaneously. This completely eliminates the wobbly, distorted artifacts that rolling shutters produce when imaging through atmospheric turbulence, ensuring solar granulation and spicule details are captured without distortion. The 4.5μm pixel size provides a fine image scale, allowing you to resolve intricate details on the solar disk with shorter focal length telescopes.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e84 FPS Data Transfer: Stable High-Speed Capture with DDR3 Cache\u003c\/h3\u003e\n\u003cp\u003eAt its full 1944×1472 resolution, the Apollo-M MINI streams data over its USB 3.0 port at 84 frames per second. To ensure this high-speed data stream is stable and free of dropped frames, Player One includes a DDR3 cache. This buffer secures data transmission, reduces read noise, and ensures consistent performance even when connected to a less powerful computer or a USB 2.0 port.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eLow-Noise Signal: 1.45e Read Noise and 79% QE with HCG Mode\u003c\/h3\u003e\n\u003cp\u003eCapturing the subtle contrast of solar features requires a clean signal. The Apollo-M MINI achieves a low read noise of just 1.45e by using an automatic High Conversion Gain (HCG) mode. This system engages at higher gain settings to suppress noise without sacrificing the camera's dynamic range. Combined with a peak Quantum Efficiency of ≈79% and a 25k e full well capacity, the camera effectively captures the faint structures within prominences and the bright, detailed photosphere in the same session.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003ePassive Cooling System: Thermal Control for Daytime Solar Imaging\u003c\/h3\u003e\n\u003cp\u003eImaging during the day introduces significant thermal challenges that can increase sensor noise. The Apollo-M MINI incorporates a Passive Cooling System (PCS) that conducts heat away from the IMX429 sensor to the camera's exterior. For even more demanding conditions, an optional Active Cooling System (ACS) is available. The sensor is protected by a D32*2MM window with a multi-layer anti-reflection coating to maximize light transmission and protect against dust.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eApollo-M MINI vs. Apollo-M (IMX174): A Pixel-Scale Advantage\u003c\/h3\u003e\n\u003cp\u003eThe Apollo-M MINI (IMX429) is often compared to its sibling, the Apollo-M (IMX174). The choice between them depends entirely on your telescope and imaging goals.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003ePlayer One Apollo-M (IMX174):\u003c\/strong\u003e With its larger 1\/1.2\" sensor and 5.86µm pixels, the Apollo-M offers a wider field of view and is well-suited for full-disk solar imaging with shorter focal length instruments.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003ePlayer One Apollo-M MINI (IMX429):\u003c\/strong\u003e The MINI's smaller 4.5μm pixels give it a distinct advantage in resolution. On the same telescope, the MINI will deliver a more detailed, higher-magnification image, making it the superior choice for focusing on active regions, sunspots, and fine filamentary detail.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy is a global shutter critical for the Apollo-M MINI in solar imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eA \u003cstrong\u003eglobal shutter\u003c\/strong\u003e exposes the entire 1944×1472 sensor at once, freezing moments of steady seeing. This prevents the \"jello\" effect or distortion seen with rolling shutters, which read the sensor line by line. For the Sun, where atmospheric turbulence is constant, a global shutter is essential for sharp, artifact-free images of granulation and filaments.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the benefit of the Apollo-M MINI's 4.5μm pixels?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe relatively small \u003cstrong\u003e4.5μm pixels\u003c\/strong\u003e provide high sampling resolution. This means that for a given telescope, the Apollo-M MINI will produce a more magnified image and capture finer details compared to a camera with larger pixels. It's ideal for resolving small sunspots, spicules, and intricate prominence structures without needing an aggressive Barlow lens.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDo I need special filters to use the Apollo-M MINI for solar photography?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003e\u003cstrong\u003eYes, absolutely.\u003c\/strong\u003e You must use a certified solar filter, such as a white-light filter (like Baader film) over the front of your telescope or a Herschel wedge for refractors. For H-alpha imaging, it must be used with a dedicated solar telescope or H-alpha filter system. Pointing the camera at the Sun without proper energy rejection will permanently destroy the sensor and can cause severe eye injury.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the Apollo-M MINI perform for imaging solar prominences with a Lunt H-alpha telescope?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Apollo-M MINI is an excellent match for a Lunt H-alpha telescope. Its high sensitivity (\u003cstrong\u003e≈79% QE\u003c\/strong\u003e) and low read noise (\u003cstrong\u003e1.45e\u003c\/strong\u003e) are ideal for capturing the faint, detailed structures in solar prominences. The global shutter and high frame rate allow you to \"freeze\" moments of good seeing for the sharpest possible results.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Apollo-M MINI to image the International Space Station (ISS) transiting the sun with an 80mm f\/6 refractor?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, the Apollo-M MINI is perfect for this task. The \u003cstrong\u003eglobal shutter\u003c\/strong\u003e is critical for capturing a sharp, undistorted image of the fast-moving ISS. The high frame rate (up to \u003cstrong\u003e238 FPS\u003c\/strong\u003e at 640x480) gives you more chances to capture the perfect moment of transit against the solar disk. Remember to use a certified white-light solar filter on your refractor.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the HCG mode on the Apollo-M MINI camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003eHCG (High Conversion Gain)\u003c\/strong\u003e mode is a feature of the sensor that automatically activates at higher gain settings. It significantly reduces read noise while preserving the full dynamic range of the sensor. This allows you to increase the camera's sensitivity for fainter targets, like solar prominences, without introducing excessive noise into the image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX429 2\/3\" CMOS (mono)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Resolution\u003c\/td\u003e\n\u003ctd\u003e1944×1472\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTotal Pixels\u003c\/td\u003e\n\u003ctd\u003e2.8 Mega Pixels\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e4.5μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e11mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eImage Size\u003c\/td\u003e\n\u003ctd\u003e8.75mm × 6.6mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rate (Full Res)\u003c\/td\u003e\n\u003ctd\u003e84 FPS (12bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eGlobal shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32μs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e5.6e - 1.45e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈79%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e25k e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12 bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAdapter\u003c\/td\u003e\n\u003ctd\u003e1.25″ \/ M42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focal Length\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD32*2MM AR Plus Multi-Layer Coating\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e160g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution \u0026amp; FPS (USB 3.0)\u003c\/td\u003e\n\u003ctd\u003e1944×1472 @ 68FPS (RAW16)\u003cbr\u003e1920×1080 @ 111FPS (RAW8) \/ 94FPS (RAW16)\u003cbr\u003e1280×720 @ 163FPS (RAW8\/RAW16)\u003cbr\u003e800×600 @ 194FPS (RAW8\/RAW16)\u003cbr\u003e640×480 @ 238FPS (RAW8\/RAW16)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePurchase Option\u003c\/td\u003e\n\u003ctd\u003eCamera only, or Camera + ACS\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113547202845,"sku":"POA-Apollo-M-MINI","price":558.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Apollo-M-MINI-Mono-Camera.png?v=1775184968"},{"product_id":"player-one-apollo-m-imx174-mono-solar-camera","title":"Player One Apollo-M IMX174 Mono Solar Camera","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003eFeatures the 2.3MP Sony IMX174 monochrome CMOS sensor\u003c\/li\u003e\n\u003cli\u003eGlobal shutter design eliminates motion artifacts from atmospheric turbulence\u003c\/li\u003e\n\u003cli\u003eAchieves a maximum frame rate of 164 FPS at full 1936x1216 resolution\u003c\/li\u003e\n\u003cli\u003eLarge 5.86μm pixels provide a deep 24.8k e full well capacity\u003c\/li\u003e\n\u003cli\u003ePassive Cooling System (PCS) dissipates heat during daytime solar imaging\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eDownloads\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003ePlayer One Apollo-M IMX174 Mono Solar Camera\u003c\/h2\u003e\n\u003cp\u003eThe Player One Apollo-M IMX174 is engineered specifically for high-resolution solar imaging, built around a 1\/1.2-inch Sony IMX174 monochrome sensor that resolves 2.3 Megapixels. Its 5.86µm pixels and global shutter capture the sun's dynamic surface at up to 164 FPS without the wobble or distortion introduced by rolling shutters during moments of unsteady seeing. A deep 24.8k e- full well capacity and 12-bit ADC ensure you can record the vast brightness differences between the solar surface and faint prominences in a single exposure.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eThe IMX174 Global Shutter: 164 FPS at 2.3 MP Without Distortion\u003c\/h3\u003e\n\u003cp\u003eFor solar, lunar, and planetary imaging, atmospheric turbulence is the primary obstacle. The Apollo-M's Sony IMX174 sensor uses a global shutter, which exposes every one of its 2.3 million pixels simultaneously. This freezes motion instantly, eliminating the wavelike distortions that rolling shutters produce, resulting in significantly sharper raw frames of solar granulation, flares, and surface details.\u003c\/p\u003e\n\u003cp\u003eAt a full resolution of 1936×1216, the camera streams 10-bit data at 164 FPS over USB 3.0. This extreme speed is critical for \"lucky imaging,\" allowing you to capture thousands of frames in a short period to select the few captured during moments of perfect atmospheric stability. The sensor's peak Quantum Efficiency of approximately 77% ensures that even with very short exposures, you are collecting a strong signal.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eSolar-Optimized Engineering: Passive Cooling and 12.5mm Back Focus\u003c\/h3\u003e\n\u003cp\u003eOperating in direct daylight generates significant heat, which can increase sensor noise. The Apollo-M incorporates a Passive Cooling System (PCS) that conducts heat away from the sensor to the camera body, maintaining thermal stability. For even more demanding conditions, an optional Active Cooling System (ACS) accessory is available.\u003c\/p\u003e\n\u003cp\u003eTo combat Newton's rings—a common interference pattern in H-alpha solar imaging—the camera features a sensor tilt plate. This allows you to make micro-adjustments to the sensor's angle relative to the incoming light path, effectively canceling out the optical interference. A built-in light-blocking sponge prevents stray light from entering the sensor chamber, further enhancing contrast.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e12-bit Data Integrity with Onboard DDR Cache\u003c\/h3\u003e\n\u003cp\u003eTo manage the massive data stream from its high-speed sensor, the Apollo-M is equipped with a DDR3 cache. This buffer prevents frame dropping by ensuring a stable and consistent data flow to your computer, even if the host system experiences momentary slowdowns. This feature greatly reduces the demand on your PC and makes high-speed capture reliable.\u003c\/p\u003e\n\u003cp\u003eThe camera also features Dead Pixel Suppression (DPS) technology. Before shipping, the camera analyzes dark frames to map any non-responsive pixels. During an imaging session, these dead pixels are automatically corrected in-camera by calculating a median value from surrounding pixels, giving you cleaner raw data from the start.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eApollo-M vs. the Player One Lineup: Sensor Size and Speed\u003c\/h3\u003e\n\u003cp\u003eThe Apollo-M occupies a strategic position within Player One's solar camera series, offering a balance of resolution, field of view, and speed.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003evs. Xena-M (IMX249):\u003c\/strong\u003e While both cameras are based on Sony's Pregius 1st Generation global shutter technology and offer similar noise and sensitivity, the Apollo-M's IMX174 sensor is significantly faster, delivering 164 FPS compared to the slower rates of the IMX249.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003evs. Apollo-M MAX (IMX432) \u0026amp; MINI (IMX429):\u003c\/strong\u003e The Apollo-M's 1\/1.2-inch format (13.3mm diagonal) provides a larger field of view than the 2\/3-inch MINI, while being more manageable for many telescopes than the large 1.1-inch sensor in the MAX. This makes it an ideal match for a wide range of solar telescopes and focal lengths.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat filters are required to use the Player One Apollo-M for solar imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003e\u003cstrong\u003eWarning: Permanent eye and equipment damage will occur without proper filtration.\u003c\/strong\u003e The Apollo-M camera must \u003cstrong\u003eNEVER\u003c\/strong\u003e be used for solar imaging without a certified energy rejection filter (ERF) and a dedicated solar telescope or filter, such as a Herschel wedge for white light or a Hydrogen-alpha filter like a DayStar Quark or Lunt solar telescope.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the Apollo-M's global shutter help when imaging the Sun with an H-alpha telescope?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAtmospheric seeing causes the image of the sun to shimmer and distort rapidly. A \u003cstrong\u003eglobal shutter\u003c\/strong\u003e exposes the entire 1936x1216 sensor at the exact same instant, freezing the details of prominences and surface granulation without the \"jello-like\" effect a rolling shutter would create. This results in sharper, more detailed images, especially when combined with its 164 FPS capture rate for lucky imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat are Newton's rings and how does the Apollo-M camera help eliminate them?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eNewton's rings are an interference pattern of concentric circles that can appear in highly monochromatic light, such as from an H-alpha filter. They are caused by reflections between the camera sensor and other flat optical surfaces. The Apollo-M has a built-in \u003cstrong\u003esensor tilt plate\u003c\/strong\u003e, allowing you to slightly angle the sensor to change the reflection path and eliminate the interference pattern for a clean, uniform image.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Apollo-M for imaging Jupiter or the Moon?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. While optimized for solar, the Apollo-M is an excellent high-speed monochrome camera for lunar and planetary imaging. Its global shutter, high frame rate (164 FPS), and 5.86µm pixels are well-suited for capturing fine details on the Moon's surface and in the cloud belts of Jupiter, especially with telescopes of longer focal lengths.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the difference between the Apollo-M's PCS and the optional ACS?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Apollo-M includes a \u003cstrong\u003ePassive Cooling System (PCS)\u003c\/strong\u003e, which uses heat-conductive materials to draw heat from the sensor to the camera's body. The optional \u003cstrong\u003eActive Cooling System (ACS)\u003c\/strong\u003e is an external fan unit that attaches to the camera, providing forced airflow over the body to dissipate heat more effectively. The ACS is recommended for long imaging sessions or use in very warm climates.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy do I need a fast SSD with the Player One Apollo-M camera?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe Apollo-M can generate a massive amount of data, capturing at 164 frames per second at full resolution. To record this data stream without dropping frames, your computer's hard drive must be able to write data very quickly. A high-speed solid-state drive (SSD) is strongly recommended to keep up with the camera and ensure you don't lose any valuable data.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor\u003c\/td\u003e\n\u003ctd\u003eSONY IMX174 1\/1.2\" CMOS (Monochrome)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eResolution\u003c\/td\u003e\n\u003ctd\u003e1936×1216 (2.3 MP)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePixel Size\u003c\/td\u003e\n\u003ctd\u003e5.86μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Size\u003c\/td\u003e\n\u003ctd\u003e11.3mm × 7.1mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSensor Diagonal\u003c\/td\u003e\n\u003ctd\u003e13.3mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMax Frame Rate\u003c\/td\u003e\n\u003ctd\u003e164 FPS (at 1936x1216, 10-bit)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eShutter Type\u003c\/td\u003e\n\u003ctd\u003eGlobal Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFull Well Capacity\u003c\/td\u003e\n\u003ctd\u003e24.8k e-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eReadout Noise\u003c\/td\u003e\n\u003ctd\u003e6.3e to 3.5e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eQE Peak\u003c\/td\u003e\n\u003ctd\u003e≈77%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eADC\u003c\/td\u003e\n\u003ctd\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExposure Range\u003c\/td\u003e\n\u003ctd\u003e32μs - 2000s\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eData Port\u003c\/td\u003e\n\u003ctd\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eProtective Window\u003c\/td\u003e\n\u003ctd\u003eD32*2mm AR Plus Multi-Coated\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBack Focus\u003c\/td\u003e\n\u003ctd\u003e12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAdapter Threads\u003c\/td\u003e\n\u003ctd\u003eM42x0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eNosepiece\u003c\/td\u003e\n\u003ctd\u003e1.25\"\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eDiameter\u003c\/td\u003e\n\u003ctd\u003e66mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eWeight\u003c\/td\u003e\n\u003ctd\u003e160g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFrame Rates (USB 3.0)\u003c\/td\u003e\n\u003ctd\u003e1936×1216 @ 164 FPS (RAW8) \/ 82.5 FPS (RAW16)\u003cbr\u003e1920×1080 @ 184.5 FPS (RAW8) \/ 93.5 FPS (RAW16)\u003cbr\u003e1280×720 @ 272 FPS (RAW8) \/ 210 FPS (RAW16)\u003cbr\u003e640×480 @ 398 FPS (RAW8) \/ 311 FPS (RAW16)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player_One_Apollo-M_Camera_Manual.pdf\" target=\"_blank\"\u003e\u003csvg class=\"DAV-img-box\" viewbox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"\u003e\u003cpath d=\"M0 64C0 28.7 28.7 0 64 0L224 0l0 128c0 17.7 14.3 32 32 32l128 0 0 144-208 0c-35.3 0-64 28.7-64 64l0 144-48 0c-35.3 0-64-28.7-64-64L0 64zm384 64l-128 0L256 0 384 128zM176 352l32 0c30.9 0 56 25.1 56 56s-25.1 56-56 56l-16 0 0 32c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-48 0-80c0-8.8 7.2-16 16-16zm32 80c13.3 0 24-10.7 24-24s-10.7-24-24-24l-16 0 0 48 16 0zm96-80l32 0c26.5 0 48 21.5 48 48l0 64c0 26.5-21.5 48-48 48l-32 0c-8.8 0-16-7.2-16-16l0-128c0-8.8 7.2-16 16-16zm32 128c8.8 0 16-7.2 16-16l0-64c0-8.8-7.2-16-16-16l-16 0 0 96 16 0zm80-112c0-8.8 7.2-16 16-16l48 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 32 32 0c8.8 0 16 7.2 16 16s-7.2 16-16 16l-32 0 0 48c0 8.8-7.2 16-16 16s-16-7.2-16-16l0-64 0-64z\" fill=\"#0047a7\"\u003e\u003c\/path\u003e\u003c\/svg\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Manual\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\u003ca href=\"https:\/\/player-one-astronomy.com\/service\/software\/\" target=\"_blank\"\u003e\u003csvg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 640 512\" class=\"DAV-img-box\"\u003e\u003cpath fill=\"#0047a7\" d=\"M128 32C92.7 32 64 60.7 64 96l0 256 64 0 0-256 384 0 0 256 64 0 0-256c0-35.3-28.7-64-64-64L128 32zM19.2 384C8.6 384 0 392.6 0 403.2C0 445.6 34.4 480 76.8 480l486.4 0c42.4 0 76.8-34.4 76.8-76.8c0-10.6-8.6-19.2-19.2-19.2L19.2 384z\"\u003e\u003c\/path\u003e\u003c\/svg\u003e \n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eDownload Software\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/a\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/player-one-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003ePlayer One 2-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Player One","offers":[{"title":"Default Title","offer_id":51113561194781,"sku":"POA-Apollo-M","price":698.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Player-One-Apollo-M-Mono-Camera.png?v=1775185103"}],"url":"https:\/\/davidastro.com\/en-us\/collections\/planetary-cameras.oembed?page=2","provider":"David Astro","version":"1.0","type":"link"}