Declination
Declination (dec) is an astronomical term associated with the equatorial coordinate system. Dec is comparable to latitude, projected unto the celestial sphere, and is measured in degrees north of the celestial equator. Therefore, points north of the celestial equator have positive declination, while those to the south have negative declination.
- An object on the celestial equator has a dec of 0°.
- An object above the north pole has a dec of +90°.
- An object above the south pole has a dec of −90°.
A celestial object that passes over zenith, has a declination equal to the observer's latitude, with northern latitudes yielding positive declinations. A pole star therefore has the declination +90° or -90°. Conversely, celestial objects with a declination higher than , where l is the latitude, are visible the whole sidereal day. Such stars are called circumpolar, while the phenomenon of a sun not setting is called midnight sun.
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See also: right ascension
Declination is occasionally and erroneously used to refer to the linguistic term declension.Varying declination
The declination of all celestial objects vary over time, in different periods.Sun

Moon
The Moon also has an annual cycle, with maximum declination at northern hemisphere midwinter and minimum at midsummer. There is also a approximately 19 year long cycle, varying the maximum declination from +28°35' to +18°18' and the minimum from -18°18' to -28°35'.Stars
The Stars have approximately the same declination from year to year, and vary in whole degrees after passing of centuries.
Declination is used in some contexts that rule out astronomical declination, to mean the same as magnetic declination.