An introduction to astronomy: designed as a text-book for the use of students in college. By Denison Olmsted ...

TIME. 39 ages of the world, show that they all perform their diurnal revolutions in the same time, and that their motion during any part of the revolution is perfectly uniform. 101. Solar time is reckoned by the apparent revolution of the sun, from the meridian round to the same meridian again. Were the sun stationary in the heavens, like a fixed star, the time of its apparent revolution would be equal to the revolution of the earth on its axis, and the solar and the sidereal days would be equal. But since the sun passes from west to east, through 360~ in 365k- days, it moves eastward nearly 1~ a day (59' 8".3). While, therefore, the earth is turning round on its axis, the sun is moving in the same direction, so that when we have come round under the same celestial meridian from which we started, we do not find the sun there, but he has moved eastward nearly a degree, and the earth must perform so much more than one complete revolution, in order to come under the sun again. Now since a place on the earth gains 360~ in 24 hours, how long will it take to gain 1~? 360: 24:: 1: =4 nearly. Hence the solar day is about 4 minutes longer than the sidereal; and if we were to reckon the sidereal day 24 hours, we should reckon the solar day 24h. 4:m. To suit the purposes of society at large, however, it is found most convenient to reckon the solar day 24 hours, and to throw the fraction into the sidereal day. Then, 24h. 4m.: 24: 24: 23h. 56m. (23h. 56m 4".09)=the length of a sidereal day. 102. The solar days, however, do not always differ from the sidereal by precisely the same fraction, since the increments of right ascension (Art. 37), which measure the difference between a sidereal and a solar day, are not equal to each other. Apparent time is time reckoned by the revolutions of the sun from the meridian to the meridian again. These intervals being unequal, of course the apparent solar days are unequal to each other. 103. lean time is time reckoned by the average length of

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Title
An introduction to astronomy: designed as a text-book for the use of students in college. By Denison Olmsted ...
Author
Olmsted, Denison, 1791-1859.
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Page 39
Publication
New York,: Collins & brother,
1865.
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Astronomy

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"An introduction to astronomy: designed as a text-book for the use of students in college. By Denison Olmsted ..." In the digital collection Making of America Books. https://name.umdl.umich.edu/ajn0587.0001.001. University of Michigan Library Digital Collections. Accessed June 7, 2025.
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