To Mars via the Moon: An Astronomical Story — John Shaqi
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
"We are looking at it now under a high sun, but when the sun has only
just risen sufficiently high to illuminate all those high mountains,
whilst the lower surroundings are still in shadow, the great bay
presents in the telescope the appearance of a brilliant luminous arch
springing from the lighted part of the moon and extending far out over
the dark part of the disc.
"Farther eastward, and lower down on the Ocean of Storms, you will
observe what is admitted by all to be the very brightest large formation
upon the moon, viz. Aristarchus--a ring-plain nearly thirty miles in
diameter, the floor of which is 5000 feet below the surface level. It
possesses a central mountain, very difficult to measure on account of
the general brightness, but believed to be about 1300 feet high.
Well-defined terraces are seen on the mountain walls enclosing the area,
and many external ridges are connected with the walls, especially to the
south. This formation is evidently covered with some substance which
reflects light to a greater extent than that on similar formations;
indeed it appears so bright that when the moon is new and the whole of
this part of the disc is dark, Aristarchus can still be seen with a
telescope, and this gave rise in the past to the idea that it was a
volcano in actual eruption. The explanation is, however, more prosaic,
because the mountain is really brought into view by earthshine on its
bright covering. When the moon is new the earth is almost fully lighted
on the side toward the moon, and sheds a faint light on the dark portion
of its disc, thus producing the phenomenon known as 'the old moon in the
new moon's arms.'
"Close to Aristarchus you will notice another ring-plain, which is
called Herodotus, about twenty-three miles in diameter, with a floor
7000 feet depressed; but this formation is not nearly so bright as its
neighbour. That high plateau between them is notable on account of the
T-shaped cleft in it, which runs into that other long zig-zag cleft (in
some parts two miles wide and 1600 feet in depth), whose direction
changes abruptly several times in its length of over one hundred miles.
Public-domain text, read in full here on John Shaqi.
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