Imaginary sphere of infinite radius used to define the positions of celestial bodies as seen from Earth
, the centre of the sphere. The sphere rotates, once in 24 hours, about a line that is an extension of the Earth's axis. The position of a celestial body is the point at which a radial line through it meets the surface of the sphere. The position is defined in terms of coordinates, such as declination and right ascension or altitude and azimuth
, which refer to great circles on the sphere, such as the celestial equator
or the ecliptic.
celestial sphere, imaginary sphere of infinite radius with the earth at its center. It is used for describing the positions and motions of stars and other objects. For these purposes, any astronomical object can be thought of as being located at the point where the line of sight from the earth through the object intersects the surface of the celestial sphere. In astronomical coordinate systems, the coordinate axes are great circles on the celestial sphere. In most systems of this type, the reference points are fixed on the sphere, so the two coordinates needed to locate a body are relatively constant.
an imaginary sphere of which the observer is the center and on which all celestial objects are considered to lie.