The moon : $b a full description and map of its principal physical features — John Shaqi
The moon : $b a full description and map of its principal physical featuresElger, Thomas Gwyn
Science
The moon : $b a full description and map of its principal physical features
Elger, Thomas Gwyn
Moon
of the ring-plains would not frequently slide down in great masses, and
thus form irregular plateaus on the lower and flatter portions of the
slope; but this fails to explain the symmetrical arrangement of the
concentric terraces and intermediate valleys. The inner declivity of the
north-eastern wall of Plato exhibits what to all appearance is an
undoubted landslip, as does also that of Hercules on the northern side,
and numerous other cases might be adduced; but in all of them the
appearance is very different from that of the true terrace.
The _glacis_, or outer slope of a ring-plain, is invariably of a much
gentler inclination than that which characterises the inner declivity:
while the latter very frequently descends at an angle varying from 60
deg. to 50 deg. at the crest of the wall, to from 10 deg. to 2 deg. at
the bottom, where it meets the floor; the former extends for a great
distance at a very flat gradient before it sinks to the general level of
the surrounding country. It differs likewise from the inner descent, in
the fact that, though often traversed by valleys, intersected by deep
gullies and irregular depressions, and covered with humpy excrescences
and craters, it is only rarely that any features comparable to the
terraces, usually present on the inner escarpment, can be traced upon it.
Elongated depressions of irregular outline, and very variable in size and
depth, are frequently found on the outer slopes of the border. Some of
them consist of great elliptical or sub-circular cavities, displaying
many expansions and contractions, called "pockets," and suggesting the
idea that they were originally distinct cup-shaped hollows, which from
some cause or other have coalesced like rows of inosculating craters.
While many of these features are so deep that they remain visible for a
considerable time under a low sun, others, though perhaps of greater
extent, vanish in an hour or so.
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