ZWO ASI 678 MC Color
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Vai al moduloZWO ASI678MC – Color Planetary Camera with Sony IMX678 Sensor
The ZWO ASI678MC is one of the latest color cameras designed for high-resolution planetary and solar imaging. Equipped with the advanced Sony IMX678 STARVIS 2 sensor, it delivers outstanding sensitivity, extremely low noise, and exceptional detail—ideal for astrophotographers who demand top performance and image precision.
Featuring a USB 3.0 interface, the ASI678MC ensures ultra-fast data transfer and prevents frame loss during high-speed captures. The 8.29 MP sensor with 2 µm pixels provides fine detail and high quantum efficiency, reaching a QE peak of 83%.
The new STARVIS 2 sensor is up to three times more efficient than the one used in the ASI178MC and offers significantly lower dark current. This results in excellent image quality even under low-light conditions and superior thermal noise control.
Main Features
- Sony IMX678 STARVIS 2 sensor with 8.29 MP resolution
- Perfect for high-resolution planetary and solar imaging
- 2 µm pixel size for ultra-fine details
- High-speed data transfer via USB 3.0
- Extremely low noise and wide dynamic range
- Compatible with Windows, Linux, and Mac systems
Technical Specifications
| Sensor | 1/1.8″ CMOS Sony IMX678AAQR1-C |
| Resolution | 8.29 MP (3840 × 2160) |
| Pixel Size | 2 µm |
| Bayer Pattern | R Gr Gb B |
| QE Peak | 83% |
| Back Focus | 12.5 mm |
| Full Well Capacity | 11.27 Ke |
| Shutter Type | Rolling Shutter |
| Maximum Frame Rate | 47.5 fps |
| Exposure Range | 32 μs – 2000 s |
| Interface | USB 3.0 / 2.0 Type-B |
| Protective Window | φ21-1.1 IR |
| ADC | 12 bit |
| Sensor Size | 7.68 mm × 4.32 mm |
| Weight | 126 g |
| Operating Temperature | -5°C ~ 50°C |
| Storage Temperature | -10°C ~ 60°C |
| Relative Humidity | 0 – 80% |
| Supported OS | Windows 7/8/10 (32 & 64 bit), Linux, Mac |
Included in the Box
- ZWO ASI678MC camera
- USB 3.0 cable
- Standard ZWO adapters and accessories
- User manual
The ZWO ASI678MC is the ideal choice for demanding astrophotographers looking for high-speed performance, precision, and superior imaging quality for solar and planetary observation.