QHYCCD QHY5III568C Color
- Color CMOS Sensor
- Planetary Imaging Camera
- Autoguiding Camera
- USB 3.0 Interface
- ST-4 Guide Port
Simulate the exact field of view of the QHYCCD QHY5III568C Color with your specific telescope.
Launch Imaging AssistantThe QHYCCD QHY5III568C is engineered as a versatile, dual-purpose camera, serving as both a high-frame-rate planetary imager and a sensitive autoguider. Its color sensor simplifies the process of capturing planets, the Moon, and the Sun (with a proper solar filter), delivering vibrant images in a single shot. This same sensitivity makes it a reliable guide camera, capable of tracking faint stars to ensure sharp, pinpoint results during long-exposure deep-sky astrophotography.
The QHY5III568C is designed for high-resolution imaging of our solar system neighbors. The built-in color sensor array eliminates the need for a filter wheel and monochrome imaging sequences, streamlining your workflow at the telescope. This one-shot-color capability is ideal for capturing fleeting moments of steady seeing, allowing you to record detailed images of Jupiter's cloud bands, Saturn's rings, and Martian surface features with straightforward acquisition and processing.
Beyond its planetary role, the QHY5III568C functions as a capable autoguider. When connected to your mount's guide port, it can detect and lock onto faint guide stars, issuing precise corrections to counteract tracking errors from your mount's drive system. This is critical for obtaining sharp, round stars in multi-minute exposures of nebulae and galaxies with a separate imaging telescope.
The QHY5III568C is designed for planetary work, which involves capturing thousands of frames in a short time (a technique called "lucky imaging"). Its color sensor simplifies this process by capturing full-color data in every frame, eliminating the complexity of using separate red, green, and blue filters.
As an autoguider, the QHY5III568C connects to an off-axis guider or a separate guide scope. It takes short, continuous exposures of a star near your imaging target. Guiding software like PHD2 analyzes the star's position and sends correction commands to the telescope mount via the camera's ST-4 port, ensuring your main camera captures sharp, untrailed images of faint targets like the Orion Nebula (M42).
Yes, this is an excellent combination. An 8" SCT provides the focal length needed to achieve a large image scale on Jupiter. The QHY5III568C would be used with a 2x or 3x Barlow lens to bring out fine details like the Great Red Spot and individual cloud bands. Its ability to capture high-speed video is essential for freezing moments of atmospheric stability.
For most planetary and guiding work, no color filters are needed since the QHY5III568C is a color camera. However, an IR/UV Cut filter is highly recommended to sharpen the image and improve color balance, as most telescopes are not designed to focus infrared and ultraviolet light at the same point as visible light. For solar imaging, a certified, full-aperture solar filter must be placed on the front of your telescope.
The QHY5III568C is supported by QHYCCD's own drivers and capture software. It is also compatible with a wide range of third-party astrophotography software via its ASCOM driver. For planetary capture, popular choices include FireCapture and SharpCap. For autoguiding, it works seamlessly with PHD2 Guiding.
The QHY5III series cameras typically use a 1.25" nosepiece form factor. This allows the QHY5III568C to be inserted directly into any standard 1.25" focuser or accessory, just like an eyepiece. It connects to a computer via a USB cable for data transfer and power, and has a separate ST-4 port for connecting to a telescope mount's autoguide input.