Declination
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In astronomy, declination is one of the two coordinates of the equatorial coordinate system, the other being either right ascension or hour angle. Dec is comparable to latitude, projected onto the celestial sphere, and is measured in degrees north and south of the celestial equator. Therefore, points north of the celestial equator have positive declinations, while those to the south have negative declinations. An object on the celestial equator has a dec of 0°. An object at the celestial north pole has a dec of +90°. An object at the celestial south pole has a dec of 90°. The sign is…mehr

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In astronomy, declination is one of the two coordinates of the equatorial coordinate system, the other being either right ascension or hour angle. Dec is comparable to latitude, projected onto the celestial sphere, and is measured in degrees north and south of the celestial equator. Therefore, points north of the celestial equator have positive declinations, while those to the south have negative declinations. An object on the celestial equator has a dec of 0°. An object at the celestial north pole has a dec of +90°. An object at the celestial south pole has a dec of 90°. The sign is customarily included even if it is positive. Any unit of angle can be used for declination, but it is often expressed in degrees, minutes, and seconds of arc. 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 near to +90° or -90°