Astronomy of To-day: A Popular Introduction in Non-Technical LanguageDolmage, Cecil Goodrich Julius
Science
Astronomy of To-day: A Popular Introduction in Non-Technical Language
Dolmage, Cecil Goodrich Julius
Astronomy
But the reader will surely ask the question: "How is it possible to
determine the actual height of a lunar mountain, if one cannot go upon
the moon to measure it?" The answer is, that we can calculate its height
from noting the length of the shadow which it casts. Any one will allow
that the length of a shadow cast by the sun depends upon two things:
firstly, upon the height of the object which causes the shadow, and
secondly, upon the elevation of the sun at the moment in the sky. The
most casual observer of nature upon our earth can scarcely have failed
to notice that shadows are shortest at noonday, when the sun is at its
highest in the sky; and that they lengthen out as the sun declines
towards its setting. Here, then, we have the clue. To ascertain,
therefore, the height of a lunar mountain, we have first to consider at
what elevation the sun is at that moment above the horizon of the place
where the mountain in question is situated. Then, having measured the
actual length in miles of the shadow extended before us, all that is
left is to ask ourselves the question: "What height must an object be
whose shadow cast by the sun, when at that elevation in the sky, will
extend to this length?"
There is no trace whatever of water upon the moon. The opinion, indeed,
which seems generally held, is that water has never existed upon its
surface. Erosions, sedimentary deposits, and all those marks which point
to a former occupation by water are notably absent.
Similarly there appears to be no atmosphere on the moon; or, at any
rate, such an excessively rare one, as to be quite inappreciable. Of
this there are several proofs. For instance, in a solar eclipse the
moon's disc always stands out quite clear-cut against that of the sun.
Again during occultations, stars disappear behind the moon with a
suddenness, which could not be the case were there any appreciable
atmosphere. Lastly, we see no traces of twilight upon the lunar surface,
nor any softening at the edges of shadows; both which effects would be
apparent if there were an atmosphere.
Public-domain text, read in full here on John Shaqi.
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