An automatic
celestial navigation system for navigating both night and day by observation of K-band or H-band
infrared light from multiple
stars. In a first set of preferred embodiments three relatively
large aperture telescopes are rigidly mounted on a movable platform such as a ship or
airplane with each
telescope being directed at a substantially different portion of
sky. Embodiments in this first set tend to be relatively large and heavy, such as about one cubic meter and about 60 pounds. In a second set of preferred embodiments one or more smaller aperture telescopes are pivotably mounted on a movable platform such as a ship,
airplane or
missile so that the
telescope or telescopes can be pivoted to point toward specific regions of the
sky. Embodiments of this second set are mechanically more complicated than those of the first set, but are much smaller and lighter and are especially useful for guidance of aircraft and missiles.
Telescope optics focus (on to a
pixel array of a sensor) H-band or K-band light from one or more
stars in the
field of view of each
telescope. Each
system also includes a GPS sensor and a computer processor having access to catalogued
infrared star charts. The processor for each
system is programmed with special algorithms to use image data from the
infrared sensors, position and timing information from the GPS sensor, and the catalogued star charts information to determine orientation (attitude) of the platform.
Direction information from two
stars is needed for locating the platform with respect to the
celestial sphere. The computer is also preferably programmed to calculate further information which may be used by a
guidance control system. These systems provide efficient alternatives to inertial navigation systems when such systems are too expensive and can be used for periodic augmentation and calibration of inertial navigation systems.