ZWO ASI6200MM Pro V2 Mono
- 61.2 Megapixel Full-Frame Sony IMX455 Monochrome Sensor
- 3.76µm Pixel Size
- 91% Peak Quantum Efficiency
- 1.2e Minimum Read Noise
- 16-Bit ADC and 51,400e Full Well Capacity
- 512MB DDR3 Image Buffer
- Two-Stage TEC Cooling
The ZWO ASI6200MM Pro V2 combines a massive 61.2 MP full-frame monochrome sensor with professional-grade imaging architecture for deep-sky astrophotography. Its 3.76µm pixels resolve fine detail in distant galaxies, while the back-illuminated sensor achieves a peak Quantum Efficiency of 91% to capture faint, outlying nebulosity. The upgraded 512MB DDR3 buffer reliably handles the huge 9576 x 6388 pixel files without dropping frames, and read noise as low as 1.2e keeps the background smooth on multi-hour exposures.
At the core of the ASI6200MM Pro V2 is Sony's back-illuminated IMX455 sensor, delivering an immense 9576 x 6388 pixel array on a 35mm full-frame format. This large sensor area allows you to frame entire nebulae complexes, such as the full expanse of the Andromeda Galaxy (M31) or the Veil Nebula, in a single shot with wide-field refractors. The monochrome design bypasses the Bayer matrix, ensuring that every one of the 61.2 million pixels contributes directly to capturing luminance detail.
This camera's back-illuminated structure and 91% peak QE mean it captures incoming photons with extreme efficiency, critical for imaging faint targets. This high sensitivity is paired with exceptionally low read noise, ranging from 3.5e down to just 1.2e, keeping the signal from faint objects well above the noise floor. Combined with a native 16-bit ADC and a deep 51,400e full well capacity, you can capture smooth gradations in bright cores and faint outer structures simultaneously, preserving the full dynamic range of the target.
The ASI6200MM Pro V2 builds on the legacy of its predecessor with a key electronic upgrade. While both cameras share the same exceptional IMX455 sensor, the V2 doubles the onboard memory buffer.
This memory upgrade makes the V2 a more robust choice for automated and remote observatories where data integrity is paramount.
ZWO's design completely eliminates amplifier glow, a common source of noise in long-exposure astrophotography. The ASI6200MM Pro V2 produces exceptionally clean, uniform dark frames, simplifying your calibration process. This is supported by a powerful two-stage TEC cooler capable of reducing the sensor's temperature to 35°C below ambient, minimizing thermal noise and ensuring consistent results throughout an imaging session.
The camera provides a standard 17.5mm of back focus from its front plate to the sensor, simplifying integration into complex imaging trains. The native telescope interface is a wide M54 thread, which helps to minimize vignetting with full-frame optics and large filter wheels. This robust connection standard ensures your imaging train remains rigid and perfectly aligned, preventing tilt and flexure during long exposures.
The 35mm full-frame sensor provides a massive field of view. When paired with a wide-field refractor, the ZWO ASI6200MM Pro V2 can capture enormous deep-sky objects like the entire North America Nebula (NGC 7000) or the Rho Ophiuchi cloud complex in a single frame, something impossible for smaller APS-C or Micro Four Thirds sensors at the same focal length.
The ZWO ASI6200MM Pro V2 has a hardware design that produces Zero Amplifier Glow. This means that even on exposures lasting many minutes, the characteristic brightening around the edge of the frame caused by amplifier heat is completely absent, resulting in cleaner raw data and easier image processing.
At a native focal length of around 2000mm, an 8" f/10 SCT would be poorly matched with the ASI6200MM Pro V2's 3.76µm pixels, resulting in severe oversampling. However, with a 0.63x or 0.7x reducer, the focal ratio becomes f/6.3-f/7, which provides a much better image scale for this camera. This combination would be excellent for resolving details in medium-sized galaxies like the Whirlpool Galaxy (M51) or the Sombrero Galaxy (M104).
To run the two-stage TEC cooler and internal electronics, the ASI6200MM Pro V2 requires a 12V DC power supply capable of delivering at least 3A. The camera itself consumes 650mA at 5V via the USB connection, but the cooler requires the external 12V supply for deep-sky imaging.
The ZWO ASI6200MM Pro V2 is designed for modern autoguiding setups that use "pulse guiding" via ASCOM or INDI drivers. Instead of connecting the guide camera to the mount with an ST-4 cable, you connect your guide camera and mount directly to your control computer or an ASIAIR. The guiding software (like PHD2) then sends correction commands to the mount directly, which is a more reliable and precise method than ST-4.
No, the anti-dew heater for the sensor window is integrated and can be controlled through the camera's driver software. You can turn it on to prevent moisture from forming on the IR window during humid nights and turn it off to conserve power when conditions are dry.
| Sensor | 35mm Full-Frame Sony IMX455 BSI CMOS |
| Resolution | 9576 x 6388 (61.2 MP) |
| Pixel Size | 3.76 µm |
| Sensor Dimensions | 35.91mm x 23.96mm |
| Sensor Diagonal | 43.3 mm |
| Peak Quantum Efficiency (QE) | 91% |
| Bit Depth | 16-bit |
| Full Well Capacity | 51,400 e- |
| Read Noise | 1.2e - 3.5e |
| Cooling | Two-Stage TEC, Cooled |
| Amp Glow Control | Zero Amplifier Glow |
| Image Buffer | 512MB DDR3 |
| Max Frame Rate | 6.3 FPS (at full resolution) |
| Shutter Type | Electronic Rolling Shutter |
| Exposure Range | 32µs to 2000s |
| ROI Support | Yes |
| Dew Heater | Yes, integrated |
| Computer Interface | USB 3.0 / USB 2.0 |
| Telescope Interface | M54 Thread |
| Back Focus | 17.5 mm |
| Guide Port | No (Pulse Guiding Only) |
| Camera Window | IR |
| Dimensions | 90mm Diameter |
| Weight | 1.4 lb. |
| Power Requirement (Cooler) | 12V @ 3A Max |
| Operating Temperature | -5°C to 45°C |
| OS Compatibility | Mac, Windows, Linux |
ZWO ASI2400 and ASI6200 5 Connection Methods Guide (11.30 MB)
× 1