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[[File:Celestial_Sphere_-_Eq_w_Label_figures.png|Celestial Sphere - Eq w Label figures|thumb]] [[File:JostBurgi-MechanisedCelestialGlobe1594.jpg|JostBurgi-MechanisedCelestialGlobe1594|thumb|left]] '''Celestial Sphere'''

The '''celestial sphere''' is an imaginary sphere of arbitrarily large radius, concentric with [[Earth]]. It is a practical tool for [[astronomy]], where the stars are considered to be fixed on the sphere's inner surface, and it moves around the Earth in a way that represents the [[sky]] as seen from Earth. The concept of the celestial sphere provides a way to describe the position of objects in the sky, despite the Earth's rotation and orbit around the [[Sun]].

==Concept==
The idea of the celestial sphere is rooted in the [[Ancient Greek astronomy|ancient Greek]] understanding of the cosmos. To the ancient astronomers, the stars appeared to be fixed on a sphere rotating once per day around an axis through the geographic poles of the Earth. This model explained the apparent daily motion of the stars and was central to the development of the methods of [[spherical astronomy]], which allows astronomers to determine the position of objects in the sky.

==Components==
The celestial sphere has several important components that are key to its understanding and use in astronomy:

* '''[[Celestial Equator]]''': The projection of the Earth's equator onto the celestial sphere. It divides the celestial sphere into the northern and southern celestial hemispheres.
* '''[[Celestial Poles]]''': Points where the Earth's axis of rotation, if extended infinitely, intersects the celestial sphere. The North Celestial Pole is directly above the Earth's North Pole, and the South Celestial Pole is directly above the Earth's South Pole.
* '''[[Ecliptic]]''': The apparent path of the Sun across the celestial sphere over the course of a year. It is inclined to the celestial equator because the Earth's axis is tilted relative to its orbit around the Sun.
* '''[[Equinoxes]] and [[Solstices]]''': Points on the celestial sphere where the ecliptic intersects the celestial equator (equinoxes) and points of greatest separation from the celestial equator (solstices), marking the change of seasons on Earth.

==Usage==
The celestial sphere is used in various ways in astronomy:

* To define the positions of stars and other celestial objects. Positions are given in terms of [[right ascension]] (analogous to longitude on Earth) and [[declination]] (analogous to latitude on Earth).
* To explain the apparent motion of the stars, Sun, Moon, and planets across the sky.
* In the creation of star charts and celestial globes, which represent the celestial sphere in a two-dimensional or three-dimensional form, respectively.

==Modern Relevance==
Despite the advent of more complex models of the universe, the celestial sphere remains a useful abstraction for astronomers. It simplifies the visualization of celestial phenomena and aids in the teaching of astronomical concepts. The celestial sphere is also used in [[navigational astronomy]], helping navigators to determine their position at sea or in the air by observing the stars.

==See Also==
* [[Astronomical coordinate systems]]
* [[Stellar navigation]]
* [[History of astronomy]]

[[Category:Astronomy]]
[[Category:Celestial navigation]]
[[Category:Celestial mechanics]]

Celestial sphere - Revision history

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