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Looking up into the night sky, one can imagine that the stars and planets are fixed to an imaginary sphere surrounding our planet. To specify locations on this Celestial Sphere, astronomers use a system of coordinates similar to the latitude and longitude measurements used to map Earth. The equatorial guides show this imaginary celestial sphere mapped onto the sky. They are based upon the celestial equator (a projection of the Earth's equator onto the Celestial Sphere), and the celestial poles (a projection of the north and south geographic poles). Declination measures an object's angular distance north or south of the celestial equator (an object of 0 declination is directly on the celestial equator). Declination is usually given in degrees minutes and seconds of arc. The east-west measurement is called the right ascension (RA), and is most often measured in hours, minutes, and seconds. The zero-point of right ascension is based upon the Vernal Equinox, the point at which the Sun crosses the celestial equator on its way north in the Spring. Since the vernal equinox slowly changes over time due to the precession of the Earth, the equatorial coordinate system upon which it is based also changes. This means that an object's position given in RA and Dec will change depending on the date. To standardize astronomical positions astronomers will often refer to an object's position using the coordinate system of a particular date. For example you will often see positions given in J2000 coordinates, that is using the equatorial coordinate system of Jan 1, 2000.
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