ZWO ASI662MC Color
- 2.1 Megapixel Sony IMX662 BSI Sensor
- 1920 x 1080 Resolution with 2.9µm Pixels
- 91% Peak Quantum Efficiency
- Ultra-Low 0.8e Read Noise
- 107.6 FPS at Full Resolution
- Zero Amplifier Glow Circuitry
- 256MB DDR3 Internal Buffer
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Open Barlow CalculatorThe ZWO ASI662MC combines a 2.1 MP Sony IMX662 back-illuminated sensor with 2.9µm pixels to resolve fine detail on planetary targets. Its exceptional 91% peak quantum efficiency and ultra-low 0.8e read noise capture faint atmospheric features, while the deep 38.2ke full well prevents bright planetary cores from saturating. A 256MB DDR3 buffer sustains a capture rate of 107.6 FPS over USB 3.0, ensuring no dropped frames during critical moments of stable seeing.
At the core of the ASI662MC is Sony's latest STARVIS 2 sensor technology, which delivers a peak quantum efficiency of 91% and heightened sensitivity in near-infrared wavelengths. This back-illuminated structure maximizes photon collection for a stronger signal. The sensor's 38.2ke full well capacity is a significant advantage for planetary imaging, allowing you to use longer exposures on targets like Jupiter and Saturn without blowing out highlights, retaining color data and detail in the brightest regions.
The ASI662MC integrates circuitry that completely eliminates amplifier glow, a common source of noise in CMOS sensors. This means your raw video files are free of glow from the start, simplifying your calibration and processing. Combined with a read noise of just 0.8e, the camera preserves faint, low-contrast details like Martian dust storms or subtle banding on Saturn, even with the very short exposures used in lucky imaging.
While the preceding ASI462MC was renowned for its high infrared sensitivity, the ASI662MC marks a major upgrade in core imaging fundamentals. The most critical improvement is in dynamic range, driven by a much deeper full well and lower noise.
To freeze moments of perfect atmospheric seeing, high-speed capture is essential. The ASI662MC streams full-resolution 1920x1080 video at 107.6 frames per second. The onboard 256MB DDR3 memory buffer ensures stable data transfer to your computer over USB 3.0, preventing dropped frames that can compromise your data set. Standard connectivity, including an ST-4 guide port and M42 threads, allows the camera to integrate easily into any imaging train.
The ZWO ASI662MC is an excellent match for an 8" f/10 SCT. To achieve the ideal image scale for its 2.9µm pixels, you should target a final focal ratio between f/15 and f/21. This is perfectly accomplished by adding a 1.5x or 2x Barlow lens to your f/10 optical train, which will allow you to resolve fine details like the Great Red Spot and intricate cloud bands.
Yes, but with limitations. The ASI662MC's high sensitivity makes it suitable for electronically-assisted astronomy (EAA) or short exposures on bright deep-sky objects like the Orion Nebula (M42) or the Hercules Cluster (M13). However, as an uncooled camera, thermal noise will become apparent on exposures longer than a few seconds. Its small 1/2.8" sensor also provides a very narrow field of view, making it better for smaller galaxies and planetary nebulae than large, extended targets.
The primary advantage is its significantly larger 38.2ke full well capacity, which is more than three times that of the ASI462MC. This provides greater dynamic range, preventing overexposure on bright planets and moons. A second key benefit is the zero amplifier glow circuitry, which produces cleaner raw data that is easier to calibrate.
Zero amp glow means the camera's circuitry prevents the sensor from producing a bright, noisy pattern on the edge of the frame during operation. For planetary imaging with its short exposures, this simplifies your workflow: there is no glow pattern to remove, so calibration is easier and faster, saving you time both at the telescope and during processing.
While the camera is backward-compatible with USB 2.0, a USB 3.0 port is highly recommended to take full advantage of its capabilities. Using USB 3.0 is necessary to achieve the maximum frame rate of 107.6 FPS. On a USB 2.0 connection, frame rates will be significantly lower, which limits your ability to capture enough frames during moments of good seeing.
Yes, it's an excellent choice. Its high sensitivity, low read noise, and zero amp glow make it very forgiving for a beginner. You can achieve high-quality results with a simplified workflow, allowing you to focus on capture techniques rather than complex calibration procedures.
| Sensor | 1/2.8" Sony IMX662 CMOS (Color) |
| Illumination | BSI (Back-Illuminated) |
| Resolution | 1920 x 1080 (2.1 MP) |
| Pixel Size | 2.9µm |
| Sensor Dimensions | 5.6mm x 3.1mm |
| Sensor Diagonal | 6.45mm |
| Quantum Efficiency (Peak) | 91% |
| Full Well Capacity | 38.2ke- |
| Read Noise | 0.8e- |
| Amp Glow Control | Zero Amplifier Glow |
| Max Frame Rate | 107.6 FPS |
| Bit Depth | 12-bit |
| Buffer | 256MB DDR3 |
| Exposure Range | 32µs to 2000s |
| Shutter Type | Electronic Rolling Shutter |
| ROI Support | Yes |
| Cooling | Uncooled |
| Computer Interface | USB 3.0 / USB 2.0 |
| Guide Port | ST-4 |
| Telescope Connection | M42x0.75 Thread, 1.25" Nosepiece |
| Back Focus | 12.5mm |
| Camera Window | AR Coated |
| Operating Temperature | -5°C to 50°C |
| Storage Temperature | -10°C to 60°C |
| Operating Humidity | 20% to 80% |
| Weight | 0.28 lbs |
| OS Compatibility | Windows, Mac, Linux |
ZWO ASI662MC Camera Body
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1.25" Nosepiece
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1.25" Cover
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USB 3.0 Cable (2m)
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ST-4 Autoguider Cable
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Quick Start Guide
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