The Moon: A Popular TreatiseServiss, Garrett Putman
Science
The Moon: A Popular Treatise
Serviss, Garrett Putman
Moon
“Thank you, and now I will ask you one more question,” said my friend.
“I have often heard of the ‘Harvest Moon’ and the ‘Hunter’s Moon.’ Will
you not kindly explain what is meant by these terms and when the
‘Harvest Moon’ can be seen? There is a poetic suggestiveness in the name
that appeals to me.”
“I will try with pleasure,” I said, “but I fear that I shall have to
trouble you with another diagram, or perhaps with two.”
“Oh, I shall not mind that at all. I have grown used to diagrams as well
as to the nomenclature of the moon.”
“Well, if my diagrams conduct your thoughts to things as interesting as
many that lie concealed behind the prosaic names on the moon I shall be
content. To begin, then, I must remind you that in her monthly journey
around the earth the moon moves from west toward east in her orbit, and
thus she gets a little over 12° farther east every twenty-four hours, as
reckoned from the position of the sun. The earth turning on its axis in
the same direction causes the moon to appear to rise in the east and set
in the west once every twenty-four hours. But in consequence of the
constant eastward motion of the moon she rises at a later hour every
night. Here is a graphic representation of what I mean:
“The earth is turning on its axis in the direction represented by the
arrows, and simultaneously the moon is moving in its orbit in the same
direction, as is shown by the large arrow. Suppose that some night the
moon is seen rising at a particular hour from the point A on the earth.
Then, the following night, when the observer has again arrived at A,
with the rotation of the earth, the moon will have advanced from M^1 to
M^2, and will not be seen rising until the point occupied by the
observer has arrived at B. This retardation of the hour of moonrise is
variable on account of changes in the position of the moon, arising from
the inclination of her orbit to the plane of the equator, and from the
inequalities of her motion, to which I have before referred. On the
average it amounts to fifty-one minutes daily. It varies also with the
distance of the observer from the equator, the variation being greater
in high latitudes. In the latitude of New York the retardation of
moonrise may be as great as an hour and a quarter, or as little as
twenty-three minutes.
[Illustration:
Diagram Showing Why Moon Rises Later Every Night.
]
Public-domain text, read in full here on John Shaqi.
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