To Mars via the Moon: An Astronomical StoryWicks, Mark
Science
To Mars via the Moon: An Astronomical Story
Wicks, Mark
Mars (Planet) -- Fiction; Science fiction
An enormous number of ring-plains and ring-mountains exists all over the
southern half of the moon's disc; in many cases there are rings within
rings, and others where they have overlapped or cut into previously
formed rings.
Moving almost due south, we passed the large but partially ruined walled
plain known as Maginus. This ring has a floor which is no less than
14,000 feet below the lunar surface. We then arrived at that favourite
object for telescopic observers which is named Clavius. This is an
enormous ring-plain, being over 142 miles in diameter, and encloses an
area of 16,000 square miles, thus being half the area of Scotland. It
has a very depressed floor, and some of the mountains are 16,000 to
17,000 feet in altitude.
Farther on, and close to the south pole, we saw the very deepest of the
lunar walled plains, which is named after Newton, who possessed probably
the deepest intellect of any of our astronomers. A smaller formation
south of Plato was originally named after him, but was not considered
worthy of a man of his scientific eminence, so the name was transferred
to the formation we were looking upon. It is about 143 miles long and
very irregular in shape, and its depth is about 24,000 feet--so deep, in
fact, that the sun's light never reaches to the bottom; thus, when we
look at it from the earth, the floor is always in shadow.
The Leibnitz Mountains, unfortunately, were not visible, as the sun had
set upon them. I, however, mentioned that this range comprises several
peaks which are believed to be the highest on the lunar surface,
reaching as they do an altitude of 30,000 feet, and, according to some
measurements, 40,000 feet. They are very difficult to measure, owing to
the fact that they are really situated on the farther side of the moon,
extending east and west of the south pole, and are only occasionally
brought into view by the moon's libration; even then they are seen in
profile, and so situated that they cannot be measured with certainty.
They are, however, so high that they blunt the southern cusp of the moon
when it is in crescent form.
Public-domain text, read in full here on John Shaqi.
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