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Sidereal day

An apparent sidereal day is the time it takes for the Earth to turn 360 degrees in its rotation; more precisely, is the time it takes the vernal equinox to make two successive upper meridian transit. This is slightly shorter than a solar day; there are 366.2422 sidereal days in a tropical year, but 365.2422 solar days, resulting in a sidereal day of 86,164.09 seconds (or: 23 hours, 56 minutes, 4.09 seconds).

The reason there is one more sidereal day than "normal" days in a year is that the Earth's orbit around the Sun cancels one sidereal day out, giving observers on Earth 365 (and a quarter) days, even though the planet itself rotated 366 (and a quarter) times.

Midnight, in sidereal time, is when the vernal equinox crosses the upper meridian.

A mean sidereal day is reckoned, not from the actual transit, but from the transit of the mean vernal equinox (see: mean sun).

See also: sidereal month, sidereal time, time

Referenced By

Ariel (moon) | Atlas (moon) | Atlas the moon | Charon (moon) | Dione (moon) | EartH | Earth (planet) | Enceladus (moon) | Epimetheus (moon) | Hyperion (moon) | Iapetus (moon) | Janus (moon) | List of astronomical topics | List of astronomical topics (N-Z) | Mimas (moon) | Outer core | Pan (moon) | Phoebe (moon) | Planet Earth | Sol 3 | Tethys (moon) | Titan (moon) | Triton (moon)

 

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This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Sidereal day".

 

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