ZWO ASI462MM Mono
- 2.1MP Sony IMX462 Monochrome Sensor
- Exceptional Near-Infrared (NIR) Sensitivity
- 136.1 FPS at Full 1936x1096 Resolution
- Ultra-Low Read Noise as low as 0.47e-
- 256MB DDR3 Buffer for Stable Data Transfer
The 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.
The 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.
At 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.
The 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.
The ASI462MM is the direct successor to the legendary ASI290MM, offering significant improvements in key areas for planetary imagers.
For 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.
The 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.
Yes, 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.
For 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.
For 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.
The 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.
No. 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.
| Sensor | 1/2.8” Sony IMX462 CMOS (Monochrome) |
| Resolution | 2.1MP (1936 x 1096) |
| Pixel Size | 2.9µm |
| Quantum Efficiency (Peak) | ~89% |
| Read Noise | 0.47e- to 2.65e- |
| Full Well Capacity | 11.2ke- |
| Max Frame Rate | 136.1 fps at 1936x1096 |
| ADC | 12-bit |
| Data Buffer | 256MB DDR3 |
| Shutter Type | Rolling Shutter |
| Back Focus | 12.5mm |
| Protective Window | AR Coated |
| Data Interface | USB 3.0 / USB 2.0 |
| Guide Port | ST-4 |
ASI462MM Camera Body
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1.25" Nosepiece Adapter
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1.25" Dust Cover
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2 meter USB 3.0 Cable
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2 meter ST4 Guide Cable
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Quick Start Guide
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