The Trouvelot astronomical drawings manualTrouvelot, E. L. (Etienne Leopold)
Science
The Trouvelot astronomical drawings manual
Trouvelot, E. L. (Etienne Leopold)
Astronomy -- Pictorial works
Mars is a very difficult object to observe, the atmosphere surrounding
it being sometimes so cloudy and foggy that the sight can hardly
penetrate through its vapors. When this planet is observed under
favorable atmospheric conditions, and with sufficient magnifying power,
its surface, which is of a general reddish tint, is found to be
diversified by white, gray and dark markings. The dark markings, which
are the most conspicuous, almost completely surround the planet. They
are of different forms and sizes, and very irregular, as can be seen on
Plate VIII., which represents one of the hemispheres of this planet.
Many of them, especially those situated in the tropical regions of the
planet, form long narrow bands, whose direction is in the main parallel
to the Martial equator.
The dusky spots differ very much, both from one another and in their
several parts, as regards intensity of shade. Some appear almost black,
while others which appear grayish, are so faint, that they can seldom be
seen. In the southern hemisphere, the darkest part of the spots is
generally found along their northern border; especially where there are
deep indentations.
Some observers have described these spots as being greenish or bluish,
but I have never been able to see the faintest trace of these colors in
them, except when they were observed close to the limb, and involved in
the greenish tinted ring which is always to be seen there. It is
probably an effect of contrast, since green and red are complementary
colors, and since this greenish tinge around the limb covers all kinds
of spots, whether white or dark. When such dark spots, involved in the
greenish tint, are carried by the rotation towards the centre of the
disk, they no longer show this greenish color. To me, these spots have
always appeared dark, and of such tints as would result from a mixture
of white and black in different proportions; except that on their
lighter portions they show some of the prevalent reddish tint of the
Martial surface. It is to be remarked that in moments of superior
definition of the telescopic image, the intensity of darkness of all the
spots is considerably increased--some of them appearing almost perfectly
black.
The markings on the surface of Mars are now tolerably well
known--especially those of its southern hemisphere, which, owing to the
greater proximity of the planet to our globe when this hemisphere is
inclined towards the earth, have been better studied. Those of the
northern hemisphere are not so well known, since when this hemisphere is
inclined towards us, the distance of Mars from the Earth is 26,000,000
miles greater, so that the occasions for observing them are not so
favorable.
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