Page:A short history of astronomy(1898).djvu/107

This page has been validated.
§§ 46, 47]
Ptolemy
63

star appears to the observer at B nearer to the zenith Z than it actually is, i.e. the light appears to come from S' instead of from S; it is shewn further that this effect must be greater for bodies near the horizon than for those near the zenith, the light from the former travelling through a greater extent of atmosphere; and these results are shewn to account for certain observed deviations in the daily paths of the stars, by which they appear unduly raised up when near the horizon. Refraction also explains the well-known flattened appearance of the sun or moon when rising or setting, the lower edge being raised by

Fig. 32.—Refraction by the atmosphere.

refraction more than the upper, so that a contraction of the vertical diameter results, the horizontal contraction being much less.[1]

47. The Almagest is avowedly based largely on the world of earlier astronomers, and in particular on that of Hipparchus, for whom Ptolemy continually expresses the greatest admiration and respect. Many of its contents have therefore already been dealt with by anticipation, and need not be discussed again in detail. The book plays, however, such an important part in astronomical history, that it may be worth while to give a short outline of its contents,

  1. The better known apparent enlargement of the sun or moon when rising or setting has nothing to do with refraction. It is an optical illusion not very satisfactorily explained, but probably due to the lesser brilliancy of the sun at the time.