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IMPORTANT: Our store is located in Canada. All orders that include products manufactured outside of Canada or USA will be subject to tariffs and duties, regardless of the order value. US customers are responsible for all applicable duties and tariffs, and those will be billed by the carrier, except for the Lacerta upgrade kit, for which we collect them at checkout.

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Player One Apollo-M MAX IMX432 Mono Solar Camera

SKU POA-Apollo-M-MAX
Original price $599.00 - Original price $599.00
Original price
$599.00
$599.00 - $599.00
Current price $599.00
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  • 1.1" Sony IMX432 Monochrome CMOS Sensor
  • 9µm Pixel Size
  • 100,000 e- Full Well Capacity
  • 126 FPS at Full Resolution (1608x1104)
  • Global Shutter for Distortion-Free Images
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  • Player One Apollo-M MAX IMX432 Mono Solar Camera

    The 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.

    The 1.1" IMX432 Sensor: 9µm Pixels for Long Focal Ratios

    The 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.

    100k e- Full Well: Capture Prominences and Photosphere in One Frame

    With 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.

    Global Shutter at 126 FPS: Clean, Band-Free Solar Imaging

    The 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.

    Apollo-M MAX (IMX432) vs. The IMX174 Standard: A Generational Leap

    For 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.

    • Full Well Capacity: 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.
    • Pixel Size: 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.
    • Image Quality: The IMX432 delivers images without the horizontal banding that can be a persistent issue with the IMX174, resulting in a cleaner final product.
    • Sensor Size: 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.

    Player One Platform: DDR3 Cache, DPS, and Passive Cooling

    The 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.

  • Why are the Apollo-M MAX's 9µm pixels better for solar imaging with an SCT?

    A 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 9µm pixels 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.

    How does the Apollo-M MAX's 100k e- full well help when imaging a solar flare?

    A solar flare or prominence is thousands of times fainter than the solar disk (photosphere). The Apollo-M MAX's enormous 100k e- full well capacity 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.

    What is the benefit of the Apollo-M MAX's global shutter?

    Earth's atmosphere causes the image of the Sun to shimmer and distort rapidly. A global shutter 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.

    Does the Player One Apollo-M MAX suffer from the horizontal banding seen in other solar cameras?

    No. 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.

    What is the HCG mode on the Apollo-M MAX camera?

    The 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.

    What filters do I need to safely use the Apollo-M MAX for solar imaging?

    WARNING: 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).

  • Sensor SONY IMX432 1.1" CMOS (Monochrome)
    Max Resolution 1608×1104 (1.7 MP)
    Pixel Size 9µm
    Sensor Diagonal 17.5mm
    Image Size 14.5mm × 9.9mm
    Shutter Type Global Shutter
    Max Frame Rate 126 FPS (at 1608x1104, RAW8)
    Full Well Capacity 100k e-
    Readout Noise 22.9e to 2.6e
    QE Peak ≈79%
    ADC 12-bit
    Exposure Range 32μs - 2000s
    Data Port USB 3.0 / USB 2.0
    Back Focal Length 12.5mm
    Adapter 1.25″ / M42x0.75
    Protective Window D32*2MM AR Plus Multi-Layer Coating
    Diameter 66mm
    Weight 160g
    Frame Rate (USB 3.0) 1608×1104: 126FPS (RAW8) / 109FPS (RAW16)
    1280×720: 187FPS
    800×600: 220FPS
    640×480: 268FPS
  • Player One 2-Year Warranty