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A common unit of time in astronomy is the solar day. Paradoxically, in the northern hemisphere solar days are longer in winter than they are in the summer. Can you see how this comes about?
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#25458. Asked by Nude Dude.
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Gnomon
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A solar day is 24 hours as reckoned by the Sun, so it is the time from midnight to midnight or noon to noon based on the position of the sun in the sky. As the earth goes around the sun, it spins on its axis. It turns one full revolution on its axis in 23 hours and 56 minutes. But because the earth goes around the sun, the position of the sun against the background of other stars will have changed so the earth has to turn for another 4 minutes approximately in order to catch up and complete the solar day. Exactly how much it has to turn extra depends on the speed of the earth around the sun. The earth moves in an ellipse around the sun, with the sun at one of the two focuses of the ellipse. Not only is the Earth closer to the sun in Northern Hemisphere Winter, it moves faster as well. So the sun will appear to have moved further in the 23 hours 56 minutes and the earth will have to turn a little bit more to catch up, hence the solar days are longer in the (northern Hemisphere) winter.
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