SVBONY SV305C Color Telescope Camera IMX662
- 2.1 Megapixel SONY IMX662 Sensor
- 1920x1080 Max Resolution
- 2.9μm Pixel Size
- Up to 91% Peak Quantum Efficiency
- 128MB DDR Image Buffer
- USB 2.0 Data Port
Simulate the exact field of view of the SVBONY SV305C Color Telescope Camera IMX662 with your specific telescope.
Launch Imaging AssistantThe SVBONY SV305C astronomy camera centers its design on the SONY IMX662 sensor, delivering a max resolution of 1920x1080 with 2.1 Mega Pixels for detailed planetary and lunar imaging. Its back-illuminated architecture features 2.9μm pixels and a peak Quantum Efficiency of approximately 91%, capturing faint details with readout noise as low as 0.7e. A deep 38ke full well capacity, processed through a 12-bit ADC and supported by a 128M buffer, ensures high dynamic range and stable frame capture at up to 24 FPS over its USB 2.0 connection.
The SV305C is built for capturing fine details on solar system targets. The sensor's 2.9µm pixels are well-matched to the resolving power of many Schmidt-Cassegrains and Maksutovs, allowing you to sample atmospheric details on Jupiter or subtle rilles on the Moon without needing an aggressive Barlow lens. With a peak QE of 91%, the camera makes efficient use of every photon, which is critical for pulling out low-contrast features during short video captures.
A key challenge in planetary imaging is capturing the bright planetary disk without blowing out the highlights on its moons or cloud features. The SV305C's 38ke full well capacity provides the headroom to manage this contrast. This is complemented by the camera's HCG (High Conversion Gain) mode, which automatically engages at higher gain settings to reduce read noise to just 0.7e while preserving the sensor's full dynamic range, resulting in cleaner final images.
While the SV305C uses a USB 2.0 interface, it incorporates a 128MB DDR buffer to ensure your imaging sessions are free from dropped frames. The buffer caches image data, feeding it to the computer reliably even if the USB bus is momentarily interrupted. For physical integration into your optical train, the camera offers two back focus distances—7.5mm and 12.5mm—providing critical spacing flexibility for use with filter wheels, off-axis guiders, or other accessories.
The IMX662 sensor in the SV305C represents a significant upgrade over the previous-generation IMX462. While both are known for high sensitivity, the IMX662 provides distinct advantages for planetary imagers.
The SV305C combines a 1920x1080 resolution with small 2.9μm pixels, an ideal combination for achieving high-resolution images with common amateur telescopes. Its high sensitivity (≈91% QE) and low read noise (0.7e) allow it to capture faint, low-contrast details in short exposures, which is the core of the "lucky imaging" technique used for planets.
HCG (High Conversion Gain) mode automatically activates at high gain settings. It significantly reduces the camera's readout noise without sacrificing its dynamic range. This means you can increase the gain to capture fainter details without introducing the excessive noise that would typically degrade the image.
The 128MB DDR buffer is a critical feature that compensates for the slower speed of USB 2.0. It acts as a temporary storage for image frames, ensuring that data is transferred to your computer smoothly without being lost or corrupted, even if the connection is briefly interrupted. This results in more stable video capture and fewer ruined datasets.
This is an excellent pairing. The 2.9μm pixels of the SV305C would provide good image sampling at the native f/10 focal ratio, and even better with a 2x Barlow (f/20). The camera's high red sensitivity would help capture detail in Jupiter's Great Red Spot (GRS) and other atmospheric bands, while the 38ke full well helps prevent overexposure of the planet's disk relative to its dimmer moons.
Yes, it's very well-suited for it. The lunar terminator is an area of extreme contrast between brightly lit crater rims and deep black shadows. The SV305C's deep 38ke full well capacity and 12-bit ADC provide the high dynamic range needed to capture details in both the bright and dark regions simultaneously without clipping the data.
The dual back focus options provide flexibility for attaching different accessories. The 7.5mm distance is often used for direct connections or when minimal spacing is required, while the 12.5mm distance provides the necessary space to insert devices like filter drawers or certain correctors into the optical path while still reaching focus.
| Sensor Model | SONY IMX662 |
| Total Pixels | 2.1 Mega Pixels |
| Max Resolution | 1920×1080 |
| Pixel Size | 2.9μm X 2.9μm |
| Chip Size | 5.6mm×3.2mm |
| Diagonal | 6.44mm |
| Frame Rate | 24 FPS |
| Shutter | Rolling Shutter |
| Exposure Range | 32μs - 2000s |
| Readout Noise | 6.5e ~ 0.7e |
| QE Peak | ≈91% |
| Full Well Capacity | 38ke |
| ADC | 12 bit |
| Built-in Buffer | 128M |
| Data Port | USB 2.0 |
| Region of Interest (ROI) | Yes |
| Binning | 1x1, 2x2 |
| Digital Noise Reduction | HCG |
| Back Focal Length | 7.5mm / 12.5mm |
| Adapter Interface | 1.25″ / CS / C |
| Protective Window | UV/IR CUT Filter |
| Compatible Systems | Windows, Linux OS, Raspberry Pi, Mac OS, Chrome OS |