One of the most common questions in astrophotography is which camera to use. The answer depends largely on the type of object being photographed. Nebulae, galaxies, the Sun and the Moon all require different sensor sizes, pixel scales and capture methods.
My own imaging is centred on deep-sky objects, with regular solar and lunar work. Over time, this has led to a three-camera setup where each sensor type is matched to a specific kind of target.
The ASI2600MC Pro uses a back-illuminated APS-C Sony CMOS sensor designed for long-exposure imaging. Its relatively large sensor area allows wide fields of view, which is useful for extended nebulae and large star fields.
The camera includes regulated cooling, which keeps the sensor at a stable temperature during long exposures. This reduces thermal noise and allows consistent calibration with dark frames over multiple sessions.
The ASI174MM is based on the Sony IMX174 sensor, widely used in solar and lunar imaging. It uses a global shutter, meaning the entire sensor is exposed at once.
The camera can capture thousands of short exposures which are stacked using lucky imaging to improve detail in turbulent atmospheric conditions.
The ASI585MC Pro is a compact colour CMOS camera with a modern back-illuminated sensor. It offers high resolution and low read noise, making it suitable for short-exposure imaging.
It is commonly used for planetary and lunar colour imaging, and for smaller deep-sky objects where a compact sensor is appropriate.
| Target | Camera |
|---|---|
| Nebulae, galaxies, clusters | ASI2600MC Pro |
| Sun | ASI174MM |
| High-resolution Moon | ASI174MM |
| Lunar colour images | ASI585MC Pro |
Sensor size and focal length determine the field of view and image scale of any astrophotography setup. Using a planning tool can help you choose a camera that frames your subject correctly.
Open Field of View Calculator