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
borders, or, if the term may be allowed, their coast-line, is often
comparatively low and ill-defined, exhibiting many inlets and
irregularities in outline. Others, again, of considerable area, as, for
example, the Mare Serenitatis and the Mare Imbrium, are bounded more or
less completely by curved borders, consisting of towering mountain
ranges, descending with a very steep escarpment to their surface: thus in
form and other characteristics they resemble immense wall-surrounded
plains. Among the best examples of enclosed Maria is the Mare Crisium,
which is considered by Neison to be the deepest of all, and the Mare
Humboldtianum.
Though these great plains are described as level, this term must only be
taken in a comparative sense. No one who observes them when their surface
is thrown into relief by the oblique rays of the rising or setting sun
can fail to remark many low bubble-shaped swellings with gently rounded
outlines, shallow trough-like hollows, and, in the majority of them, long
sinuous ridges, either running concentrically with their borders or
traversing them from side to side. Though none of these features are of
any great altitude or depth, some of the ridges are as much as 700 feet
in height, and probably in many instances the other elevations often rise
to 150 feet or more above the low-lying parts of the plains on which they
stand. Hence we may say that the Maria are only level in the sense that
many districts in the English Midland counties are level, and not that
their surface is absolutely flat. The same may be said as to their
apparent smoothness, which, as is evident when they are viewed close to
the terminator, is an expression needing qualification, for under these
conditions they often appear to be covered with wrinkles, flexures, and
little asperities, which, to be visible at all, must be of considerable
size. In fact, were it possible to examine them from a distance of a few
miles, instead of from a standpoint which, under the most favourable
circumstances, cannot be reckoned at less than 300, and this through an
interposed aerial medium always more or less perturbed, they would
probably be described as rugged and uneven, as some modern lava sheets.
Public-domain text, read in full here on John Shaqi.
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