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
The confused network of streaks round Copernicus seem to respond more
happily to the requirements of Professor Pickering's hypothesis, for here
there is an absence of that definiteness of direction so manifestly
displayed in the case of the Tycho rays, and we can well imagine that
with an area of condensation surrounding this magnificent object beyond
the limits of the streaks, and a number of active little craters on and
about its rim, the white material ejected might be drawn outwards in
every direction by wind currents, which possibly once existed, and,
settling down, assume forms such as we see.
Nasmyth's well-known hypothesis attributes the radiating streaks to
cracks in the lunar globe caused by the action of an upheaving force, and
accounts for their whiteness by the outwelling of lava from them which
has spread to a greater or less distance on either side. If the moon has
been fractured in this way, we can easily suppose that the craters formed
on these fissures, being in communication with the interior, might eject
some pulverulent white matter long after the rest of the surface with its
other types of craters had attained a quiescent stage.
The Tycho rays, when viewed under ordinary conditions, appear to extend
in unbroken bands to immense distances. One of the most remarkable,
strikes along the eastern side of Fracastorius, across the Mare Nectaris
to Guttemberg, while another, more central, extends, with local
variations in brightness, through Menelaus, over the Mare Serenitatis
nearly to the north-west limb. This is the ray that figures so
prominently in rude woodcuts of the moon, in which the Mare Serenitatis
traversed by it is made to resemble the Greek letter PHI. The Kepler,
Aristarchus, and Copernicus systems, though of much smaller extent, are
very noteworthy from the crossing and apparent interference of the rays;
while those near Byrgius, round Aristarchus, and the rays from Proclus,
are equally remarkable.
[Nichol found that the rays from Kepler cut through rays from Copernicus
and Aristarchus, while rays from the latter cut through rays from the
former. He therefore inferred that their relative ages stand in the
order,--Copernicus, Aristarchus, Kepler.]
As no branch of selenography has been more neglected than the observation
of these interesting but enigmatical features, one may hope that, in
spite of the exacting conditions as to situation and instrumental
requirements necessary for their successful scrutiny, the fairly equipped
amateur in this less favoured country will not be deterred from
attempting to clear up some of the doubts and difficulties which at
present exist as to their actual nature.
Public-domain text, read in full here on John Shaqi.
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