The interval of time that elapses between two consecutive passages of a fixed star (other than the sun) across the meridian is called
A
mean solar day
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B
mean sidereal day
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C
mean solar year
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D
mean sidereal year
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Solution
The correct option is C mean sidereal day The time that the Earth takes to rotate about its axis so that the distant stars appear in the same position is called a sidereal day. Note that we treat the stars to be attached to the imaginary celestial sphere at a very large distance from the Earth. An Earth day is 24 hours and hence a sidereal day will be 4 minutes faster. The interval of time that elapses between two consecutive passages of a fixed star (other than the sun) across the meridian is called mean sidereal day.