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Celestial bodies provide the basic standards for determining the periods of a calendar. Their movement as they rise and set is now known to be a reflection of the Earth’s rotation, which, although not precisely uniform, can conveniently be averaged out to provide a suitable calendar day. The day can be measured either by the stars or by the Sun. If the stars are used, then the interval is called the sidereal day and is defined by the period between two passages of a star (more precisely of the vernal equinox, a reference point on the celestial sphere) across the ...(100 of 21777 words)