Astrophysics (Index)About

equatorial coordinate system

(latitude/longitude-like system for the celestial sphere)

The equatorial coordinate system is a spherical coordinate system used for directions into the celestial sphere, fixed to the stars/constellations as seen from Earth. Elements:

Note that the relationship between right ascension and longitude shifts with time, its most obvious shift occurring over a daily cycle. In contrast, the relationship between declination and latitude is basically constant.

The equatorial coordinate system (and the closely related International Celestial Reference System) is commonly used for the position of planets in the celestial sphere and its coordinates are commonly used for identifying and naming objects beyond the solar system (e.g., J designators).

The Earth's precession of the equinoxes slowly changes the coordinates of points on the celestial sphere on the order of an arcsecond per month. This is a primary reason for specifying an epoch.


(coordinate system,equatorial,celestial sphere,Earth)
Further reading:
https://en.wikipedia.org/wiki/Equatorial_coordinate_system

Referenced by pages:
celestial coordinate system
celestial pole
celestial reference frame
celestial sphere
declination (dec)
ephemeris
epoch
equinox
Catalogues of Fundamental Stars
International Celestial Reference System (ICRS)
epoch J2000.0
J2000.0 equinox
J designator
precession of the equinoxes
right ascension (RA)
supergalactic coordinate system
zenith

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