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- Dec 17, 2003
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Or the 1865 Comparative Geography Book (online)
www.gutenberg.org

Comparative geography

The daily revolution of the Earth on its axis is also of only medium swiftness, consuming 24 hours. This, of course, controls the periods of waking and sleep of the entire animate creation on our globe. Some planets revolve slower, some more rapidly than our own; Jupiter’s revolution, for example, is accomplished in little less than 10 hours. This extreme rapidity seems to account for the much greater flattening at the poles of the planets than the Earth exhibits, occasioned doubtless during the formation processes, while those immense revolving masses were passing from their primitive fluid state into the more rigid forms in which we know them. Of all the planets, however, the Earth has most perfectly retained the spherical shape; and the spherical form is in one sense a medium form; i.e. it is removed from all extremes of angularity, and so falls in with the analogies which I am endeavoring to establish, springing from[xi] the position of the Earth’s orbit midway between those of the inner and outer planets. According to Plato, the beauty of form lies in symmetry, and our Earth is the most symmetrical of planets, and, unquestionably, the spherical shape is the one best adapted to the display of the largest number of phenomena possible.
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