- Celestial sphere
[
celestial equator .]In
astronomy andnavigation , the celestial sphere is an imaginary rotatingsphere of "giganticradius ", concentric andcoaxial with theEarth . All objects in thesky can be thought of as lying upon the sphere. Projected from their correspondinggeographic equivalents are thecelestial equator and thecelestial pole s. The celestial sphere projection is a very practical tool forpositional astronomy .The celestial sphere can be used
geocentric ally andtopocentric ally. The former means that it is centred upon an imaginary observer in the centre of the Earth, and noparallax effects need to be taken into account. In the latter case it is centred upon an observer on the surface of the Earth and then horizontalparallax cannot always be ignored; especially not for the Moon.In the Aristotelic and
Ptolemaic models, the celestial sphere was imagined as a physical reality rather than a geometrical projection (seeCelestial spheres ).The celestial sphere is divided by projecting the
equator into space. This divides the sphere into the north celestial hemisphere and the south celestial hemisphere. Likewise, one can locate the Celestial Tropic of Cancer, Celestial Tropic of Capricorn, North Celestial Pole, and South Celestial Pole. The directions toward various objects in the sky can be quantified by constructing acelestial coordinate system .As the Earth rotates from
west toeast around its axis once every 23 hours 56 minutes, the celestial sphere and all objects on it appear to rotate fromeast towest around thecelestial pole s in the same time. This is thediurnal motion . Therefore stars will rise in the east, culminate on the north-south line (meridian) and set in the west, (unless a star is circumpolar). On the next night a particular star will rise again, but with our normal clocks running a 24 hour 0 minutes cycle, it will do so 4 minutes earlier. By the following night the difference will be 8 minutes, and so forth with every following night (or day).The reason for this apparent misadjustment of our clocks is that the Sun is not standing still on the celestial sphere, as the stars do, but moves about 1° per day eastwards over a
great circle known as theecliptic (which is 360° or a full circle in one year, theannual motion of the Sun). As an angle of 1° corresponds to 4 minutes in time (360° = 24 hours), we need therefore 4 extra minutes of diurnal motion to see the Sun back on (for example) the meridian again, making the duration of one rotation just 24 hours exactly (on the average, ignoring small seasonal variations, seeequation of time )Normal clocks therefore indicate
solar time .Astronomers studying the movements of stars may want clocks indicatingsidereal time , going around once in 23h56m (solar time units).A celestial sphere can also refer to a physical model of the celestial sphere. Also known as a star globe, this sort of celestial sphere will indicate which constellations are visible at a given time and place.
See also
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*Armillary sphere
*Celestial coordinate system
*Celestial equator
*Celestial horizon
*Celestial pole
*Celestial spheres
*Conformal geometry
*Equinox
*Geocentric universe
*North Star
*Pole Star
*Prograde and retrograde motion
*Setting circles
*Solstice
*South Star
*Spherical Earth
*Zodiac External links
* [http://skyandtelescope.com/observing/skychart/# SkyandTelescope.com SkyChart]
* [http://astroclub.tau.ac.il/skymaps/monthly/ Monthly skymaps for every location on Earth]
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