Player One Apollo-M MAX IMX432 Mono Solar Camera
- 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
Simulez le champ de vision exact de Player One Apollo-M MAX IMX432 Mono Solar Camera avec votre télescope.
Lancer l'assistant d'imagerieThe 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 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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
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 |