The double-view field star sensing
detector and its
star chart distinguishing method belongs to the field of posture sensor technology. The double-view field star sensing
detector has one semi-transparent mirror in angle of 45 deg to the main optical axle installed before the lens
system of common star sensing
detector, and two lens hoods in the two incident light directions of the semi-transparent mirror to avoid spatial
stray light interference. The light rays of the two view fields are transmitted and reflected separately in the semi-transparent mirror, passed through the same lens
system and imaged in the same photosensitive detector. Compared with common
single view field star sensing detector, the double-view field star sensing detector has higher precision, high
chip utilization, small volume, low
power consumption, easy installation and use, and other features. In addition, the corresponding
star chart distinguishing method is also disclosed.