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Player One Uranus-M Pro Mono IMX585 Cooled Astrophotography Camera

Player One Uranus-M Pro Mono IMX585 Cooled Astrophotography Camera

par Player One
UGC POA-Uranus-M-Pro
CA$908.00 - CA$908.00
CA$908.00
CA$908.00 - CA$908.00
CA$908.00
Égalisation de prix!
  • Sony IMX585 Monochrome CMOS Sensor
  • 8.3 Megapixel Resolution (3856 x 2180)
  • High-Speed Capture up to 47 FPS
  • 12-bit ADC Depth
  • Thermoelectric Cooling System
  • USB 3.0 Type-C Main Data Port
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  • Description
  • FAQ
  • Specifications
  • In the Box
  • Downloads
  • Warranty

  • Player One Uranus-M Pro Mono IMX585 Cooled Astrophotography Camera

    The Player One Uranus-M Pro combines the high-resolution 8.3 MP Sony IMX585 monochrome sensor with deep thermoelectric cooling, creating a camera capable of both high-speed planetary imaging and long-exposure deep-sky work. Capturing full-resolution frames at 47 FPS allows you to freeze atmospheric turbulence for lunar and solar detail, while the 1/1.2" format sensor provides a generous field of view. Data is handled by a 12-bit ADC and transferred over a modern USB 3.0 Type-C connection, powered by a standard 12V DC input for stable cooled performance.

    IMX585 Mono Sensor: 8.3 Megapixels at 47 FPS

    At the core of the Uranus-M Pro is Sony's IMX585, a monochrome sensor with a 3856 x 2180 pixel array. This 8.3 MP resolution is ideal for capturing fine detail on Jupiter's cloud bands or resolving craterlets along the lunar terminator. The camera can stream this high-resolution data at up to 47 FPS, a critical speed for lucky imaging techniques that overcome atmospheric seeing.

    The sensor's 1/1.2" format provides a substantial field of view, making it easier to frame large targets like the full solar disk with the right telescope, or to mosaic large lunar landscapes. As a monochrome sensor, it captures all incoming light without the resolution loss inherent in a color filter array, delivering maximum detail for luminance data or narrowband imaging.

    Thermoelectric Cooling for Long-Exposure Astrophotography

    While its high frame rate excels at planetary work, the Uranus-M Pro's integrated thermoelectric cooling system makes it a capable deep-sky imager. Cooling the sensor significantly reduces thermal noise, the primary obstacle in long exposures of faint nebulae and galaxies. This allows you to take multi-minute sub-exposures to capture faint details that would be lost in the noise of an uncooled camera.

    This dual-purpose design means a single camera can serve your entire imaging workflow. You can shoot high-speed AVI files of Mars at opposition one night and switch to long-exposure FITS files of the Orion Nebula (M42) the next, all with the same instrument.

    Modern Connectivity: Dual USB Type-C and 12V DC Input

    The Uranus-M Pro features a modern and robust connection suite designed for reliability in the field. The main data connection is a USB 3.0 Type-C port, ensuring high-speed, stable data transfer to your capture computer. A secondary USB 2.0 Type-C port is also included, often used for powering accessories like an electronic filter wheel, simplifying your cable management.

    The cooling system is powered by a separate, standard 12V DC 5.5x2.1mm input. This isolates the power-hungry cooling electronics from the sensitive data lines, preventing potential noise and ensuring the camera maintains stable sensor temperatures throughout an imaging session.

    Uranus-M Pro vs. Color IMX585 Cameras: The Monochrome Advantage

    Cameras using the color version of the IMX585 sensor offer the convenience of capturing a full-color image in a single shot. However, the monochrome Uranus-M Pro holds a distinct advantage in two key areas: resolution and sensitivity, especially for specific types of astrophotography.

    • Higher Effective Resolution: A mono sensor uses every pixel to capture light, whereas a color sensor dedicates pixels to red, green, or blue, losing some resolving power in the process. For the sharpest possible lunar and planetary images, a mono camera shooting through RGB filters will always produce a more detailed final image.
    • Narrowband Imaging Capability: The primary advantage of a mono camera is its ability to work with narrowband filters (H-alpha, OIII, SII). This is impossible with a color camera. By isolating specific emission lines, you can cut through light pollution and capture dramatic, high-contrast images of emission nebulae like the Veil Nebula (NGC 6960).

    The trade-off is the added complexity of using a filter wheel and processing multiple data channels. For imagers seeking the highest possible detail and the flexibility to shoot in heavy light pollution, the monochrome Uranus-M Pro is the superior choice.

  • Is the Player One Uranus-M Pro good for deep-sky imaging?

    Yes. The integrated thermoelectric cooling system is the key feature that makes the Uranus-M Pro a capable deep-sky camera. Cooling reduces thermal noise, enabling the long exposures (30 seconds to several minutes) required to capture faint detail in galaxies and nebulae. As a monochrome camera, it is especially powerful when paired with LRGB and narrowband filters.

    What is the advantage of the Uranus-M Pro's monochrome IMX585 sensor?

    A monochrome sensor delivers higher effective resolution and sensitivity compared to its color counterpart. Every one of the 8.3 million pixels on the Uranus-M Pro's sensor captures light, whereas a color camera's pixels are filtered red, green, or blue. This makes a mono camera sharper for planetary imaging and enables the use of narrowband filters for cutting through light pollution to image emission nebulae.

    How does the Uranus-M Pro perform on Jupiter with an 8" SCT?

    The Uranus-M Pro is an excellent match for an 8" SCT for imaging Jupiter. The 8.3 MP resolution provides ample pixels across the planet's disk, and the 47 FPS frame rate is fast enough to "freeze" moments of good seeing. Using an LRGB filter set with this camera will produce a final image with more detail and color accuracy than a one-shot color camera could achieve.

    What do I need to power the Player One Uranus-M Pro?

    You will need two power sources. The camera's data transfer and basic operation are powered by the USB 3.0 Type-C connection to your computer. To run the thermoelectric cooling system for deep-sky imaging, you must connect a separate 12V DC power supply (with a 5.5*2.1mm plug) to the dedicated power port.

    Can I use the Uranus-M Pro for imaging galaxies like Andromeda (M31)?

    Yes. The 1/1.2" sensor format and cooled architecture make it suitable for larger targets like the Andromeda Galaxy (M31), though you will likely need to create a mosaic to capture its full extent. The monochrome sensor's sensitivity is a major benefit for capturing faint outer dust lanes and star-forming regions in M31's spiral arms when shooting luminance (L) frames.

    What is the second USB Type-C port on the Uranus-M Pro for?

    The main USB 3.0 Type-C port is for high-speed data transfer. The secondary USB 2.0 Type-C port acts as a USB hub, allowing you to connect and power other accessories, such as a Player One filter wheel or a guide camera, directly to the Uranus-M Pro. This helps to simplify cable management at the telescope.

  • Sensor Sony IMX585 Monochrome CMOS
    Format 1/1.2"
    Resolution 3856 x 2180 (8.3 MP)
    Max Frame Rate 47 FPS
    ADC 12-bit
    Main Data Port USB 3.0 Type-C
    Accessory Port USB 2.0 Type-C
    Power Input (Cooling) 12V DC (5.5mm x 2.1mm)
    Camera Type Cooled Monochrome
  • Player One 2-Year Warranty