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

DIURNAL REVOLUTION. 21 lengths of the days and nights. All these points will be readily understood by inspecting figure 5. 5 7. Most of the phenomena of the diurnal revolution can be explained, either on the supposition that the celestial sphere actually all turns around the earth once in 24 hours, or that this motion of the heavens is merely apparent, arising from the revolution of the earth on its axis in the opposite direction,-a motion of which we are insensible, as we sometimes lose the consciousness of our own motion in a ship or a steamboat, and observe all external objects to be receding from us with a commdn motion. Proofs entirely conclusive and satisfactory, establish the fact, that it is the earth and not the celestial sphere that turns; but these proofs are drawn from various sources, and the student is not prepared to appreciate their value, or even to understand some of them, until he has made considerable proficiency in the study of astronomy, and become familiar with a great variety of astronomical phenomena. To such a period of our course of instruction we therefore postpone the discussion of the hypothesis of the earth's rotation on its axis. 58. While we retain the same place on the earth, the diurnal revolution -occasions no change in our horizon, but our horizon goes round as well as ourselves. Let us first take our station on the equator at sunrise; our horizon now passes through both the poles, and through the sun, which we are to conceive of as at a great distance from the earth, and therefore as cut, not by the terrestrial but by the celestial horizon. As the earth turns, the horizon dips more and more below the sun, at the rate of 15 degrees for every hour; and, as in the case of the polar star (Art. 50), the sun appears to rise at the same rate. In six hours, therefore, it is depressed 90 degrees below the sun, which brings us directly under the sun, which, for our present purpose, we may consider as having all the while maintained the same fixed position in space. The earth continues to turn, and in six hours more, it completely reverses the -position of our horizon, so that the western part of the horizon which at sunrise was diametrically opposite to the sun now cuts the sun, and soon afterwards it rises above the level

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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 21
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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