Astronomical coordinate systems

From Wikipedia, the free encyclopedia

Astronomical coordinate systems are coordinate systems used in astronomy to describe the location of objects in the sky and in the universe. The most commonly occurring such systems are coordinate systems on the celestial sphere, but extragalactic coordinates systems are also important for describing more distant objects.

[edit] Coordinate systems on the celestial sphere

See Celestial coordinate system.

[edit] Extragalactic coordinate systems

See Extragalactic astronomy.