ZWO ASI676MC Color
- 12.6 Megapixel 3552 x 3552 Square Sensor
- 2.0µm Pixel Size
- 83% Peak Quantum Efficiency
- Zero Amplifier Glow Circuitry
- 256MB DDR3 Internal Buffer
The ZWO ASI676MC combines a high-resolution 12.6 MP Sony IMX676 sensor with small 2µm pixels, resolving fine detail on planetary surfaces and small deep-sky targets. Its perfectly square 3552 x 3552 pixel array simplifies mosaic construction, while the 83% peak QE and back-illuminated structure capture faint signal efficiently. With a maximum frame rate of 31.2 FPS at full resolution and a 256MB DDR3 buffer, you can capture sharp frames during moments of steady seeing without dropping data.
The ASI676MC's defining feature is its 1/1.6" format, 3552 x 3552 square CMOS sensor. This format eliminates the need for rotating the camera between mosaic panels, streamlining the capture of large targets like the lunar surface or sprawling solar active regions. The 12.6 megapixel resolution gives you the image scale to create vast, high-definition composites without sacrificing detail.
With a pixel size of just 2µm, the ASI676MC is built for high-resolution imaging on long focal length instruments like Schmidt-Cassegrains and Maksutovs. The back-illuminated Sony sensor achieves a peak Quantum Efficiency of 83%, ensuring that a high percentage of incoming photons are converted to signal. This sensitivity is critical for reducing exposure times on planets, which helps freeze atmospheric turbulence.
ZWO engineered the ASI676MC with circuitry that completely eliminates amplifier glow, a common source of noise in CMOS sensors that typically requires dark frame subtraction. This results in cleaner raw data and a more streamlined processing workflow. The onboard 256MB DDR3 buffer ensures stable, high-speed data transfer over USB 3.0, preventing dropped frames during critical planetary video captures.
The ASI676MC represents a significant evolution from its popular predecessor, the ASI178MC, primarily for planetary and lunar imagers.
As an uncooled camera, the ASI676MC is optimized for short-exposure "lucky imaging" of the Moon, planets, and Sun (with a proper solar filter). Its lightweight body and ST-4 port also make it a capable, high-resolution autoguider. The lack of a cooling system means thermal noise will become a factor on multi-second exposures, making it less suitable for imaging faint deep-sky objects than a dedicated cooled camera.
The 3552 x 3552 square sensor is ideal for creating mosaics of large areas like the Moon or Sun. You can capture adjacent panels without rotating the camera, which simplifies both the acquisition process at the telescope and the image stitching process in software.
An 8" f/10 SCT has a focal length of around 2000mm. With 2µm pixels, this provides good image sampling, but for optimal planetary resolution, you typically want to image between f/10 and f/14 (5 to 7 times the pixel size). We recommend using a 1.5x Barlow lens with your SCT to bring the focal ratio to f/15, which will allow the ASI676MC to resolve the finest details in Jupiter's cloud bands under good seeing conditions.
Whether the ASI676MC can capture the full Moon depends on your telescope's focal length. On a short refractor with a focal length of 400-500mm, you can easily frame the entire disc. On a longer instrument like an SCT, the 10mm sensor diagonal will only show a portion of the Moon, making it a perfect candidate for creating a high-resolution mosaic.
No. The ZWO ASI676MC features a Zero Amplifier Glow hardware design. The circuitry is engineered to prevent the light leakage that causes amp glow, so you do not need to subtract dark frames to remove it, even on longer exposures for guiding.
Yes. The ASI676MC is an excellent high-resolution guide camera. It includes a standard ST-4 guide port to connect directly to your mount. Its high sensitivity and small pixels can detect very faint guide stars and register minute star movements for precise tracking corrections.
The choice depends on your primary target. The ASI462MC has extreme sensitivity in near-infrared light, making it a specialist for imaging methane bands on Jupiter and Saturn. The ASI676MC, however, offers a much higher 12.6 MP resolution (vs 2.1 MP) and a square sensor, making it far superior for high-resolution lunar, solar, and general planetary color imaging.
| Sensor | 1/1.6" Sony IMX676 BSI CMOS |
| Resolution | 12.6 MP (3552 x 3552) |
| Pixel Size | 2µm |
| Sensor Dimensions | 7.1mm x 7.1mm |
| Sensor Diagonal | 10mm |
| Quantum Efficiency (Peak) | 83% |
| Full Well Capacity | 10.55Ke |
| Bit Depth | 12-bit |
| Max Frame Rate | 31.2 FPS |
| Amp Glow Control | Zero Amplifier Glow |
| Image Buffer | 256MB DDR3 |
| Camera Type | Color, Uncooled |
| Guide Port | ST-4 |
| Computer Interface | USB 3.0 |
| Telescope Interface | M42x0.75 Threads, 1.25" Nosepiece |
| Camera Window | IR-Cut |
| Series | ZWO ASI676 |
| SKU | ZWO-ASI676MC |
ASI676MC Camera Body
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1.25" Nosepiece
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1.25" Cover
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2m USB 3.0 Cable
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ST-4 Guide Cable
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Quick Guide
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