The Trouvelot astronomical drawings manualTrouvelot, E. L. (Etienne Leopold)
Science
The Trouvelot astronomical drawings manual
Trouvelot, E. L. (Etienne Leopold)
Astronomy -- Pictorial works
The well-known fact that the continents, and especially the mountainous
and denuded districts of our globe, reflect much more light than the
surfaces covered by water, has led astronomers to suppose that the dark
spots on Mars are produced by a liquid strongly absorbing the rays of
light, like the liquids on the surface of the Earth. According to this
theory the dark spots observed are supposed to be lakes, seas, and
oceans, similar to our own seas and oceans, while the reddish and
whitish surfaces separating these dark spots, are supposed to be
islands, peninsulas, and continents. This supposition seems certainly to
have a great deal of probability in its favor, although some of the
lighter markings may have a different origin, and perhaps be due to
vegetation; but no observer has yet seen in them any of the changes
which ought to result from change of seasons. Some of the changes in the
dark spots might also be attributed to the flooding or drying up of
marshes and low land. The change which I have observed lately might be
attributed to such a cause, especially as my observation was made
shortly after the spring equinox of the northern hemisphere of Mars,
which occurred on December 8th.
Besides the dark spots just described, there are markings of a different
character and appearance. Among the most conspicuous are two very
brilliant white oval spots, which always occupy opposite sides of the
planet. These two bright spots, which correspond very closely with the
poles of rotation of Mars, have been called "polar spots."
On account of the inclination of the axis of rotation of this planet to
the ecliptic, it is rare that both of these spots are visible on the
disk at the same time; and when this occurs, they are seen considerably
foreshortened, as they are then both on the limb of the planet. Usually
only one spot is visible, and it appears to its best advantage when the
region to which it belongs attains its maximum of inclination towards
the Earth.
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