Zenith cameras are astronomic or geodetic instruments which are directed exactly to the zenith. The stars are recorded either by photographic plates or by CCD sensors.
The main tasks in using these instruments are:
The small differences between the instrumental axis and the vertical is controlled by spirit levels or by vertical sensors.
Whereas the focal lengths of the astronomical instruments range from about 1 to 3 meters,
the geodetic zenith cameras are much more smaller (f ≈ 0.2 to 0.5 m). Some special instruments were developed in the 1990s by the Technical University of Hannover (northern Germany) and of the TU Wien (Austria).
See also: Geodetic astronomy, Position astronomy, Geoid, IERS, time service