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The Apparent Motion of the Surn The sun rises in the east, moves across the south, and sets in the west much as stars in non-circumpolar constellations do. Just as for the stars, this apparent motion is really due to the rotation of the earth on its axis The Earths motion around the Sun adds a complication to the Suns apparent motion. In a full year, or 365 days, the Earth would go completely around the Sun so that the line-of- sight joining the Sun to the Earth would turn through 360 degrees. In one day, that line turns through approximately one degree. tions the Sun Solar and Sidereal Days The picture below shows the Earth rotating through a full 360 degrees relative to the distant stars. A vertical stick marks a spot that sees the Sun directly overhead when the rotation begins. tive to the Stars t of the Earths Axis
1° Noon Not noon yet. During that rotation, the line-of-sight between the Sun and the Earth turns through about one degree. As a result, the Sun is not directly overhead and the Earth needs to rotate one more degree to have the Sun directly overhead at the spot where the stick is. That takes about four minutes A solar day is defined to be the time from one solar noon to the next and is the time needed for the earth to rotate by about 361.That amount of time is defined to b8 24 hours. A sidereal day is the time needed for the earth to rotate by 360 and is four minutes shorter than 24 hours.
A sidereal day is O A a few minutes longer than a solar day 0 B afew minutes shorter than a solar day. ° C just the same as a solar day. O D several hours longer than a solar day OE several hours shorter than a solar day.
A time of 24 hours is O A almost exactly equal to a sidereal day (within a second). O B almost exactly equal to a solar day (within a second). ° C different by several minutes from both a solar day and a sidereal day.
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Option (B) is correct because in sidereal day earth have to to rotate 10 less

Option (B) is correct because a solar day have 24 hr duration

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