ZWO ASI183MM Mono
- 20.2 Megapixel (5496 x 3672) 1" Monochrome CMOS Sensor
- 2.4µm Pixel Size for High-Resolution Sampling
- 84% Peak Quantum Efficiency (BSI Sensor)
- 1.6e Low Readout Noise
- 19 FPS at Full 20.2 MP Resolution
- USB 3.0 and ST-4 Guiding Ports
The ZWO ASI183MM Mono combines a high-resolution 20.2 MP (5496 x 3672) Sony 1" CMOS sensor with small 2.4µm pixels, making it ideal for detailed imaging with short-focal-length instruments. Its back-illuminated design achieves a peak Quantum Efficiency of 84% and maintains low 1.6e read noise, capturing faint signals with high fidelity. At full resolution, the camera delivers 19 frames per second over its USB 3.0 interface, providing the speed needed for high-resolution lunar, solar, and planetary imaging.
The ASI183MM's 2.4µm pixels are perfectly suited for modern, short focal length refractors and imaging Newtonians. This combination allows you to achieve high-resolution image sampling without needing a Barlow lens, capturing fine details in nebulae and galaxies. The massive 20.2 MP resolution gives you the flexibility to frame large targets or crop aggressively on smaller objects without sacrificing image quality.
The Sony IMX183 sensor is a back-illuminated (BSI) design, which places the sensor's wiring behind the photodiodes. This architecture maximizes light collection, pushing the peak Quantum Efficiency to 84% and enabling over 60% sensitivity in the critical Hydrogen-alpha line. As an uncooled camera, the ASI183MM excels at shorter exposures for lucky imaging and narrowband work, though thermal noise will become a factor on multi-minute exposures of faint deep-sky objects.
While its color counterpart, the ASI183MC, simplifies imaging with one-shot-color convenience, the ASI183MM Mono holds a distinct advantage in sensitivity and resolution. The monochrome sensor captures every incoming photon, contributing to its higher 84% peak QE. Without a Bayer color filter array, the ASI183MM resolves finer detail and is the clear choice for advanced LRGB and narrowband imaging with separate filters.
While capable of deep-sky work, the ASI183MM is also a high-speed planetary and solar system imager. It can capture full-resolution 20.2 MP frames at 19 fps, fast enough to freeze moments of steady seeing. By defining a smaller Region of Interest (ROI), you can increase speeds dramatically, reaching 80.10 fps at 1920x1080 or 117.30 fps at 1280x720 to capture thousands of frames on Jupiter or Saturn in minutes.
The ASI183MM features a robust and standardized connection scheme for direct integration into your existing imaging train. The lightweight 0.26 lb. body minimizes focuser strain and balance issues.
Yes, the ASI183MM is a highly versatile camera. Its high frame rate of 19 fps at 20.2 MP makes it excellent for "lucky imaging" of the Moon, Sun, and planets. Its high sensitivity (84% QE) and low read noise (1.6e) also make it very capable for capturing deep-sky objects, especially with narrowband filters, though its uncooled design is best suited for shorter exposures.
The small 2.4µm pixels are an excellent match for short focal length instruments (e.g., 250mm-500mm). This combination achieves a high-resolution image scale, allowing you to capture fine detail without needing a Barlow or Powermate. It effectively turns a wide-field refractor into a high-resolution deep-sky imaging system.
The primary limitation is thermal noise. Without active cooling, the sensor's temperature will rise during long exposures (typically over 60-90 seconds), which increases noise in the final image. The ASI183MM is therefore best used for capturing many shorter exposures rather than single, very long ones. Using dark frame subtraction is essential to manage this thermal signal.
Choose the ASI183MM mono if your goal is maximum detail and sensitivity. It has a higher peak QE of 84% and resolves finer detail because it lacks a color filter array. This makes it the superior choice for LRGB imaging from dark skies or for narrowband imaging of emission nebulae (like the Horsehead Nebula, B33) from light-polluted locations.
Yes. While its large 1" sensor is overkill for many guide scopes, its high sensitivity and built-in ST-4 guide port make it a very capable autoguider. It can be particularly useful when guiding with an off-axis guider (OAG) on a longer focal length telescope, where the large sensor area makes it easier to find a suitable guide star.
The camera body has standard female M42x0.75 "T-threads". It typically ships with a 1.25" nosepiece (not listed in the provided manifest) that allows it to slide into any standard 1.25" focuser. You can also thread it directly to accessories like filter wheels or off-axis guiders that use the M42 standard.
| Sensor | 1" Sony IMX183 BSI CMOS (Monochrome) |
| Resolution | 5496 x 3672 (20.2 MP) |
| Pixel Size | 2.4 µm |
| Sensor Dimensions | 13.2 mm x 8.8 mm |
| Sensor Diagonal | 15.9 mm |
| Peak Quantum Efficiency (QE) | 84% |
| Full Well Capacity | 15,000e- |
| Readout Noise | 1.6e- |
| Bit Depth | 12-bit |
| Max Frame Rate | 19 fps at 5496x3672 |
| Shutter Type | Electronic Rolling Shutter |
| Minimum Exposure | 32 µs |
| Maximum Exposure | 2000 s |
| Back Focus | 6.5 mm |
| Data Interface | USB 3.0 |
| Guide Port | ST-4 |
| Telescope Connection | M42x0.75 |
| Camera Window | AR Coated |
| Cooling | Uncooled |
| Dimensions | 62 mm x 36 mm |
| Weight | 0.26 lb |
| Supported OS | Mac, Windows, Linux |
| Working Temperature | -5°C to 45°C |
| Storage Temperature | -20°C to 60°C |
| Working Relative Humidity | 20% to 80% |
ZWO ASI183 CMOS Camera User Manual
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