sidereal day
Noun
Meaning
the time for one complete rotation of the earth relative to a particular star, about 4 minutes shorter than a mean solar day
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Astronomy and Astrophysics 105(2), 361, 1982, see equation 19. defined UT1 such that the observed sidereal day at the beginning of 2000 would be times a UT1 day of main s, which gives main s of UT1.
Because its rotation is so slow, Venus is very close to spherical. citation A Venusian sidereal day thus lasts longer than a Venusian year (243 versus 224.7 Earth days).
A mean solar day is, therefore, nearly 4 minutes longer than a sidereal day.
A semi-synchronous orbit has an orbital period of ½ sidereal day, i.e., 11 h 58 min.
A sidereal day (the period of rotation) lasts about 58.7 Earth days.
Earth's sidereal day also differs from its rotation period relative to the background stars by the amount of precession in right ascension during one day (8.4 ms).