In astrophotography, celestial bodies, nebulae and other objects in the night sky are imaged in visible light and stored on various media. The camera is oriented on the geographic North Pole parallel to the Earth's axis. The inclination of the camera corresponds to the latitude. The exposure time for such photographs is several hours, which is why the camera must be adapted to the Earth's daily rotation. Otherwise only lines will be visible instead of the objects' actual shapes. An appropriate device, a tracker compensates for the Earth's rotation if the rotation speed corresponds exactly to one revolution per day. There are also different rotation speeds depending on the object to be tracked. For stars, one revolution takes 23 hours, 56 minutes and 4 seconds. The moon requires a revolution time of 24 hours, 52 minutes and 28 seconds, while the sun requires exactly 24 hours.