Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent AstronomersOlmsted, Denison
Science
Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent Astronomers
Olmsted, Denison
Astronomy
Soon after this, an inhabitant of the moon would see a crescent,
resembling our new moon, which would in like manner increase and go
through all the changes, from new to full, and from full to new, as we
see them in the moon. There are, however, in the two cases, several
striking points of difference. In the first place, instead of
twenty-nine and a half days, all these changes occur in one lunar day
and night. During the first and last quarters, the changes would occur
in the day-time; but during the second and third quarters, during the
night. By this arrangement, the lunarians would enjoy the greatest
possible benefit from the light afforded by the earth, since in the half
of her revolution where she appears to them as full, she would be
present while the sun was absent, and would afford her least light while
the sun was present. In the second place, the earth would appear
thirteen times as large to a spectator on the moon as the moon appears
to us, and would afford nearly the same proportion of light, so that
their long nights must be continually cheered by an extraordinary degree
of light derived from this source; and if the full moon is hailed by our
poets as "refulgent lamp of night,"[10] with how much more reason might
a lunarian exult thus, in view of the splendid orb that adorns his
nocturnal sky! In the third place, the earth, as viewed from any
particular place on the moon, would occupy invariably the same part of
the heavens. For while the rotation of the moon on her axis from west to
east would appear to make the earth (as the moon does to us) revolve
from east to west, the corresponding progress of the moon in her orbit
would make the earth appear to revolve from west to east; and as these
two motions are equal, their united effect would be to keep the moon
apparently stationary in the sky. Thus, a spectator at E, Fig. 38, page
175, in the middle of the disk that is turned towards the earth, would
have the earth constantly on his meridian, and at E, the conjunction of
the earth and sun would occur at mid-day; but when the moon arrived at
G, the same place would be on the margin of the circle of illumination,
and will have the sun in the horizon; but the earth would still be on
his meridian and in quadrature. In like manner, a place situated on the
margin of the circle of illumination, when the moon is at E, would have
the earth in the horizon; and the same place would always see the earth
in the horizon, except the slight variations that would occur from the
librations of the moon. In the fourth place, the earth would present to
a spectator on the moon none of that uniformity of aspect which the moon
presents to us, but would exhibit an appearance exceedingly diversified.
The comparatively rapid rotation of the earth, repeated fifteen times
during a lunar night, would present, in rapid succession, a view of our
seas, oceans, continents, and mountains, all diversified by our clouds,
storms, and volcanoes.
FOOTNOTES:
Public-domain text, read in full here on John Shaqi.
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