The Moon: A Popular TreatiseServiss, Garrett Putman
Science
The Moon: A Popular Treatise
Serviss, Garrett Putman
Moon
“The globe, half bright and half black, in the center,” I said,
“represents the earth. The large circle surrounding the earth we will
call the moon’s orbit, which she traverses once every month. The smaller
globe, also half white and half black, shown in four successive
positions in the orbit, is the moon. Suppose the sun to be away off here
on the left. It illuminates the earth and the moon only on the side
turned toward it. The opposite side of both is buried in night. Now, let
us begin with the moon at the point A. She is then between the earth and
the sun, the bright side being necessarily toward the sun and the dark
side toward the earth. In that position we do not see the moon at all
from the earth, unless she happens to come so exactly in a line with the
sun as to cover the latter, in which event we have an eclipse of the
sun. Now, suppose the moon to move in her orbit toward B. In a little
more than seven days she will arrive at B. In the meantime, while moving
away from the position of the sun, she begins to present a part of her
illuminated hemisphere toward the earth. This part appears in the form
of a sickle, or crescent, which grows gradually broader, until, at B, it
has grown to a half circle. In other words, when the moon is in the
position B we on the earth see one half of her illuminated surface. This
phase is called First Quarter. The narrow crescent, which appears as
soon as the moon begins to move from A toward B, is the New Moon. As the
moon continues on from B toward C, more and more of her illuminated half
is visible from the earth, and when she arrives at C, just opposite to
the position of the sun, she becomes a Full Moon. We then see, as occurs
to-night, the whole of that face of the moon which is presented sunward.
The upper half of the diagram shows how the moon moves from the position
of Full Moon back again to New Moon, or conjunction with the sun. During
this latter part of her course the moon rises later and later every
night, until, when she assumes the form of a waning crescent, she is
visible only in the morning sky just before sunrise.[1]
“Now, there is another interesting thing shown by this diagram,” I
continued—but my companion, who had followed my explanations thus far
with flattering attention, here suddenly ran to the door exclaiming:
“For mercy’s sake, what is happening to the moon?”
Footnote 1:
[Illustration:
The Moon’s Path with Respect to the Sun and the Earth.
]
Public-domain text, read in full here on John Shaqi.
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