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Player One Poseidon-M Pro Mono IMX571 Cooled Astrophotography Camera

SKU POA-Poseidon-M-Pro
Original price CA$2,658.00 - Original price CA$2,658.00
Original price
CA$2,658.00
CA$2,658.00 - CA$2,658.00
Current price CA$2,658.00
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  • Sensor: Sony IMX571 APS-C Mono
  • Resolution: 6252×4176 (26MP)
  • Pixel Size: 3.76μm
  • Full Well Capacity: 71.7k e-
  • Cooling: 40°C Delta-T below ambient
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  • Description
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  • Player One Poseidon-M Pro Mono IMX571 Cooled Astrophotography Camera

    The Player One Poseidon-M Pro centers on the Sony IMX571, an APS-C monochrome sensor delivering 26MP resolution with 3.76μm pixels. Its 16-bit ADC and massive 71.7k e- full well capacity capture immense dynamic range, while the two-stage TEC cooling achieves a 40°C Delta-T to eliminate thermal noise in long exposures. A peak Quantum Efficiency of ≈91% ensures that the majority of incoming photons are converted to signal, and the camera can sustain 10FPS at 10-bit output for high-speed applications.

    The IMX571 Sensor: 26MP, 16-bit ADC, and 71.7k Full Well

    The Poseidon-M Pro is built for advanced deep-sky imaging, leveraging the Sony IMX571's 26MP resolution across a large 23.5mm×15.7mm APS-C sensor. With 3.76μm pixels, it is well-suited for a wide range of telescope focal lengths, from wide-field refractors to large SCTs. The sensor's back-illuminated architecture and ≈91% peak QE maximize sensitivity, especially in the critical H-alpha and OIII wavelengths.

    A true native 16-bit ADC provides 65,536 levels of gray, giving you enormous flexibility in post-processing without introducing banding or posterization. This is complemented by an exceptionally deep 71.7k e- full well, which allows you to capture long exposures of bright targets like the Orion Nebula (M42) without saturating the core stars, preserving detail in both the brightest and faintest regions simultaneously.

    Advanced Cooling and Signal Integrity: 40°C Delta-T and 512MB Buffer

    To produce clean, long-exposure data, the Poseidon-M Pro integrates a 2-stage TEC cooling system capable of reducing the sensor temperature by 40°C ± 2°C below ambient. This aggressive cooling virtually eliminates thermal noise, resulting in a smooth, clean background that makes faint details easier to process. An integrated, adjustable anti-dew heater on the protective window prevents condensation during humid nights.

    Data transfer is managed by a 512MB DDR3 memory buffer, which prevents frame dropping during high-speed captures and ensures stable data transmission to your computer. This buffer also reduces readout noise and makes the camera less dependent on a high-speed USB connection, maintaining reliable operation even over a USB 2.0 port. The sensor's Non-Amp-Glow design further ensures that your background remains pristine and free of artifacts.

    Precision Mechanics: 4-Point Tilt Plate and 17.5mm/12.5mm Back Focus

    The Poseidon-M Pro features a 4-point, rear-adjusting sensor tilt plate, allowing for precise correction of field curvature introduced by the optical train. Adjusting from the rear is more intuitive than front-side plates, making it simpler to achieve perfectly sharp stars across the entire 28.3mm sensor diagonal. A built-in light-blocking sponge prevents any light leaks from the adjustment slits.

    The camera offers two native back focus distances to accommodate different imaging setups. The standard 17.5mm distance is ideal for use with filter wheels and off-axis guiders. By removing the sensor tilt plate, the back focus is reduced to 12.5mm, providing additional flexibility for custom optical configurations or systems with tight spacing requirements.

    Optimizing for 15 FPS Planetary or Low-Noise DSO Imaging

    The Poseidon-M Pro incorporates dual sampling modes to tailor its performance to your target. In Normal mode, the camera prioritizes speed, reaching up to 15 FPS at full 6252×4176 resolution (RAW8) and 150 FPS at 640x480. This makes it a capable high-resolution lunar and planetary imager.

    For deep-sky objects, the Low Noise (LRN) mode reduces read noise to as low as 1.0e, maximizing dynamic range for faint targets. The High Conversion Gain (HCG) mode engages automatically, dropping read noise significantly while preserving dynamic range, ensuring that even the faintest signals from distant galaxies are captured with clarity.

    Poseidon-M Pro vs. ZWO ASI2600MM Pro: A Head-to-Head on the IMX571

    Both the Poseidon-M Pro and the ZWO ASI2600MM Pro are built around the excellent Sony IMX571 monochrome sensor, but they differ in key design philosophies.

    • Full Well Capacity: The Poseidon-M Pro's key advantage is its 71.7k e- full well, which is significantly deeper than the 50k e- of the ZWO ASI2600MM Pro. This allows for longer sub-exposures without clipping stars, capturing more color and detail in bright star-forming regions.
    • Sensor Tilt Mechanism: The Poseidon-M Pro uses a 4-point, rear-adjust tilt plate, which many find easier for isolating and correcting tilt in a specific corner. The ASI2600MM Pro uses a 3-point, front-adjust plate.
    • Body Design: The octagonal body of the Poseidon-M Pro is designed to minimize diffraction artifacts when used with telescopes like the Celestron RASA, a benefit over the traditional round body of the ZWO.
    • ADC: Both cameras feature a true native 16-bit ADC, offering exceptional data quality and processing flexibility.
  • What is the main advantage of the Poseidon-M Pro's 71.7k e- full well?

    The 71.7k e- full well capacity allows the sensor's pixels to collect more photons before becoming saturated. This is a significant advantage when imaging targets with high dynamic range, such as the Orion Nebula (M42) or the Andromeda Galaxy (M31). You can take longer exposures to capture faint outer details without blowing out the bright core, resulting in a more detailed and nuanced final image.

    How do I choose between Normal and Low Noise (LRN) mode on the Poseidon-M Pro?

    Choose the mode based on your target:

    • Normal Mode: Use this for high-speed imaging of bright objects like the Moon and planets. It provides the fastest frame rates, reaching 15 FPS at full resolution, which is ideal for "lucky imaging" techniques.
    • Low Noise (LRN) Mode: Use this for deep-sky imaging of faint nebulae and galaxies. This mode prioritizes signal quality, reducing read noise to as low as 1.0e and maximizing dynamic range to capture the faintest details.

    What power supply do I need for the Poseidon-M Pro's cooling system?

    To run the two-stage TEC cooling system, you need an external 12V DC power adapter with a minimum rating of 5A, connected via the 5.5x2.1mm port. The camera's maximum power consumption is 3A, but a 5A supply ensures stable operation. A power supply is not included with the camera.

    How does the 4-point sensor tilt plate on the Poseidon-M Pro work?

    The 4-point rear-adjust tilt plate allows you to physically align the sensor so it is perfectly perpendicular to your telescope's focal plane. This corrects for any tilt in your imaging train, ensuring sharp stars across the entire APS-C frame. Because there is one adjustment screw near each corner, it is more intuitive to identify which part of the sensor needs to be moved to achieve a flat field.

    How would the Poseidon-M Pro perform on the Horsehead Nebula (Barnard 33) with an 80mm f/6 refractor?

    The Poseidon-M Pro is an excellent match for this setup. The 3.76μm pixels provide good sampling for a typical 480mm focal length refractor. The sensor's ≈91% peak QE and low read noise are critical for capturing the faint, glowing hydrogen gas of the Flame Nebula (NGC 2024) and the subtle details within the dark dust lanes of the Horsehead itself, especially when using narrowband filters.

    Is the Poseidon-M Pro's 15 FPS rate fast enough for imaging Jupiter?

    Yes, but with a caveat. While 15 FPS at full resolution is impressive for a DSO camera, you would typically use a smaller region of interest (ROI) for planetary imaging. At a 1280x720 ROI, the camera can achieve 103 FPS in RAW8 mode, which is more than fast enough to freeze atmospheric seeing and capture fine details like the Great Red Spot and cloud bands on Jupiter.

  • Sensor SONY IMX571 APS-C CMOS (mono)
    Resolution 6252×4176 (26 MP)
    Pixel Size 3.76μm
    Image Size 23.5mm × 15.7mm
    Diagonal 28.3mm
    Max Frame Rate 10FPS (10bit)
    Shutter Type Rolling shutter
    Exposure Range 32μs - 2000s
    Readout Noise 3.9e - 1.0e
    Full Well Capacity 71.7k e-
    Peak QE ≈91%
    ADC 16 bit
    Cooling System 2-Stage TEC, Delta T 40℃ ± 2℃ below ambient
    Power Consumption Max 3A (requires 12V 5A power adapter, not included)
    Protective Window D46*2MM AR Plus Multi-Layer Coating
    Data Port USB 3.0 / USB 2.0 (Type-C)
    Back Focus 17.5mm (with tilt plate), 12.5mm (without tilt plate)
    Adapters M48x0.75, 2", 1.25"
    Diameter 90mm
    Weight 650g
    Operating Temperature -10°C to 60°C
    Operating Humidity 0% to 80%
    Frame Rates (USB 3.0) 6252×4176: 15FPS (RAW8) / 7FPS (RAW16)
    3840x2160: 36FPS (RAW8) / 13FPS (RAW16)
    1920x1080: 70FPS (RAW8) / 25.5FPS (RAW16)
    640×480: 150FPS (RAW8) / 54.5FPS (RAW16)
    • Poseidon-M Pro Camera Body

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