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
LOHRMANN.--This ring-plain, with Hevel and Cavalerius on the N. of it, is
a member of a linear group, which, but for its propinquity to the limb,
would be one of the most imposing on the moon's surface. Lohrmann, about
28 miles in diameter, is surrounded by a bright wall, which, to all
appearance, is devoid of detail. Two prominent ridges, with a fine
intervening valley, connect it with the N. end of Grimaldi. It has a
large but not conspicuous central mountain. On the rugged surface,
between the ring-plain and the E. edge of the Oceanus Procellarum, lies a
very interesting group of crossed clefts, some of which run from N.E. to
S.W., and others from N.W. to S.E. Three of the latter proceed from
different points in a coarse valley extending from W. to E., and cross
the ridges just mentioned. They follow a parallel course, and terminate
on the S. side of a crater-row, consisting of three bright craters
ranging in a line parallel to the coarse valley. On the N. side of these
objects, and tangential to them, is another cleft, which traverses the W.
and E. walls of Lohrmann, and, crossing the region between it and
Riccioli, terminates apparently at the W. wall of the latter formation.
No map shows this cleft, though it is obvious enough; and, when the E.
wall of Hevel is on the morning terminator, the notches made by it in the
border of Lohrmann are easily detected. Capt. Noble, F.R.A.S., aptly
compares two of the crossed clefts to a pair of scissors, the craters at
which they terminate representing the oval handles. On the grey surface
of the Mare W. of Lohrmann is the bright crater Lohrmann A, from which,
running N., proceeds a rill-like valley ending at a large white spot,
which has a glistening lustre under a high light.
HEVEL.--A great walled-plain, 71 miles in diameter, adjoining Lohrmann on
the N., with a broad western rampart, rising at one peak to a height
above the interior of nearly 6000 feet, and presenting a steep bright
face to the Oceanus Procellarum. There are three prominent craters near
its crest, and one or two breaks in its continuity. It is not so lofty
and is more broken on the E., where three conspicuous craters stand on
its inner slope. The floor is slightly convex, and includes a triangular
central mountain, on which there is a small crater. The S. half of the
interior is crossed by four clefts: (l) running from a little crater N.
of the central mountain, on the W. side of it, to a hill at the foot of
the S.W. wall; (2) originating near the most southerly of the three
craters on the inner slope of the E. wall, and crossing 1, terminates at
the foot of the W. wall; (3) has the same origin as 2, crosses 1, and,
passing over a craterlet W. of the central mountain, also runs up to the
W. wall at a point considerably N. of that where 2 joins the latter; (4)
runs from the craterlet just mentioned to the W. end of 2.
Public-domain text, read in full here on John Shaqi.
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