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

REFRACTION. 3 5 observed the altitude of the sun's center at Paris to be 50 0' 14". The latitude of Paris being 48~ 50' 10", and the sun's declination at that time being 15~ O' 25": Requiirecl the refraction. By spherical trigonometry, Zx will be found equal to 850 10' 8"; consequently, the true altitude was 4~ 49' 52". Now to 50 0' 14", the apparent altitude, 9" must be added for parallax, and we have 5~ 0' 23'", the apparent altitude corrected for parallax. Hence, 5~ 0' 23"-4~ 49' 52"=10' 31", the refraction at the apparent altitude 5~ 0' 14".*92. By these and similar methods, we could easily determine the refraction due to any elevation above the horizon, provided the refracting mediumn (the atmosphere) were always uniform. But this is not the fact: the refracting power of the atmosphere is altered by changes in density and temperature.t Hence, in delicate observations, it is necessary to take into the account the state of the barometer and of the thermometer, the influence of the variations of each having been very carefully investigated, and rules having been given accordingly. With every precaution to insure accuracy, on account of the variable character of the refracting medium, the tables are not considered as entirely accurate to a greater distance from the zenith than 74~; but almost all astronomical observations are made at a greater altitude than this. 93. Since the whole amount of refraction near the horizon exceeds 33', and the diameters of the sun and moon are severally less than this, these luminaries are in view both before they have actually risen and after they have set. 94. The rapid increase of refraction near the horizon is strikingly evinced by the ovalc figure which the sun assumes when near the horizon, and which is seen to the greatest advantage when light clouds enable us to view the solar disk. Were all parts of the sun equally raised by refraction, there * Gregory's Ast., p. 65. t It is said that the effects of humidity are insensible; for the most accurate experiments seem to prove that watery vapor diminishes the density of air in the same ratio as its own refractive power is greater than that of air. (New Encyc. Brit., iii., 762.)

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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 35
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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