ZWO ASI183MC Color
- 20.2 Megapixel 1" Sony IMX183 BSI CMOS Sensor
- 2.4µm pixels for high-resolution planetary and solar system imaging
- 19 FPS at full 5496 x 3672 resolution
- 1.6e low read noise and 84% peak QE
- USB 3.0 and ST-4 guide port connectivity
The ZWO ASI183MC combines a high-resolution 20.2 MP sensor with small 2.4µm pixels, making it a formidable tool for capturing fine detail on the Moon and planets. Its 1-inch back-illuminated Sony sensor achieves a peak Quantum Efficiency of 84% with only 1.6e of read noise, preserving faint signals in your raw data. At full 5496 x 3672 resolution, the camera streams at 19 FPS over its USB 3.0 interface, fast enough for lucky imaging techniques that freeze atmospheric turbulence.
The core of the ASI183MC is its Sony IMX183 back-illuminated CMOS sensor, which offers a massive 5496 x 3672 pixel array in a 1-inch format. This combination of high resolution and a large sensor diagonal of 15.86 mm lets you frame the entire lunar disc with a short refractor or capture intricate detail within Jupiter's cloud bands with a long focal-length SCT. The back-illuminated structure places wiring behind the photodiode, maximizing photon collection to reach a peak QE of 84%.
To overcome atmospheric seeing, planetary imagers rely on capturing thousands of frames in a short time, and the ASI183MC is built for this task. It delivers 19 FPS at its full 20.2 MP resolution and can be pushed to 80.10 FPS at a 1920x1080 Region of Interest (ROI). This speed, enabled by the USB 3.0 interface, is critical for capturing those fleeting moments of perfect seeing that reveal the sharpest details on planetary surfaces.
The ASI183MC is an uncooled camera, which makes it compact, lightweight at just 0.26 lbs, and simple to power in the field. This design is ideal for short-exposure solar, lunar, and planetary imaging where thermal noise is negligible. However, for multi-minute exposures of faint deep-sky objects, the lack of cooling will result in higher thermal noise compared to a dedicated cooled camera. The small 2.4µm pixels deliver exceptional resolution but require stable seeing and precise focusing to fully exploit their potential, and they pair best with telescopes operating at shorter focal ratios to avoid oversampling.
The primary difference between the ASI183MC and its monochrome sibling, the ASI183MM, is the sensor's Bayer matrix. The ASI183MM offers higher ultimate sensitivity and resolution because it lacks the color filter array, allowing every pixel to capture all incoming light. This makes it the superior choice for advanced imagers using filter wheels for LRGB or narrowband imaging. The ASI183MC, however, provides the significant advantage of one-shot color capture. You get a full-color image in a single exposure, drastically simplifying the acquisition and processing workflow, which is a major benefit for planetary imaging sessions where conditions can change rapidly.
For planetary imaging, the optimal focal ratio is typically 5 to 7 times the camera's pixel size. With the ASI183MC's 2.4µm pixels, you should aim for a focal ratio between f/12 and f/17. On an 8" f/10 SCT, you would use a 1.5x or 2x Barlow lens to achieve this ideal image scale, allowing you to resolve fine details in Jupiter's cloud bands under good seeing conditions.
Yes, the ASI183MC is sensitive enough to capture bright deep-sky objects like the Orion Nebula (M42) using a series of short exposures (e.g., 30-60 seconds) that can be stacked later. However, as an uncooled camera, it will exhibit more thermal noise on long exposures than a cooled model, which may limit its ability to capture the faintest outer nebulosity.
A Back-Illuminated Sensor (BSI) places the metal wiring layer below the light-sensitive photodiodes, rather than above them. This design prevents the wiring from blocking incoming photons, significantly increasing the sensor's light-gathering efficiency. For the ASI183MC, this contributes to its high peak Quantum Efficiency of 84%.
Yes. Like most color CMOS cameras, the ASI183MC's sensor is sensitive to infrared (IR) light that the human eye cannot see. To achieve accurate colors and prevent star bloat, it is essential to use an IR Cut or Luminance filter that blocks this unwanted wavelength. This filter is typically threaded onto the camera's 1.25" nosepiece.
While the ASI183MC has a standard ST-4 guide port and high sensitivity, making it technically capable of guiding, its 20.2 MP resolution is generally overkill for this purpose. Guiding requires finding and tracking a single star, and the large files generated by the ASI183MC would slow down the process unnecessarily. A dedicated guide camera with a smaller sensor is a more efficient choice.
The native back focus for the ZWO ASI183MC is 6.5 mm from the front of the M42 female threads to the sensor. This short distance is common for uncooled planetary cameras and is important to know if you plan to use it with accessories like filter drawers or off-axis guiders in a deep-sky setup.
| Sensor | 1" Sony IMX183 BSI CMOS |
| Resolution | 5496 x 3672 (20.2 MP) |
| Pixel Size | 2.4 µm |
| Sensor Dimensions | 13.19 mm x 8.81 mm |
| Sensor Diagonal | 15.86 mm |
| Peak Quantum Efficiency | 84% |
| Full Well Capacity | 15,000e- |
| Read Noise | 1.6e- |
| Shutter Type | Electronic Rolling Shutter |
| Max Frame Rate (12-bit) | 19 FPS at 5496x3672 |
| Bit Depth | 12-bit |
| Exposure Range | 32 µs to 2000 s |
| Camera Type | Color, Uncooled |
| Interface | USB 3.0 |
| Guide Port | ST-4 |
| Back Focus | 6.5 mm |
| Telescope Connection | 1.25", 2", M42x0.75 |
| Dimensions | 62 mm x 36 mm |
| Weight | 0.26 lb |
| Operating Temperature | -5°C to 45°C |
| OS Compatibility | Mac, Windows, Linux |
ZWO ASI183MC CMOS Camera User Manual
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