The Moon: A Popular TreatiseServiss, Garrett Putman
Science
The Moon: A Popular Treatise
Serviss, Garrett Putman
Moon
“The supposed influence of the position of the New Moon on the weather,”
I replied, “is too gross a superstition to be worthy of any notice, but
the different attitudes of the sickle are interesting. They arise from
the changes in the position of the moon as seen from the earth with
respect to the direction of the sun, and these changes depend in turn on
the inclination of the moon’s path in the sky to the plane of the
earth’s equator as well as to the plane of the ecliptic or the earth’s
orbit. The ecliptic has an inclination of about 23½° to the plane of the
equator, and the moon’s orbit is inclined a little over 5° to the
ecliptic. The moon may, in consequence, appear more than 28° above or
below the equator. But since, as I told you in the beginning, the orbit
of the moon itself turns slowly about in space, the distance of the moon
above or below the equator is not constant. It may be only a little more
than 18°. In consequence of these changes of relative position the
situation of the horns of the crescent moon varies. But you need never
be in doubt as to what position they will occupy at any time if you will
simply remember that a straight line drawn from the point of one horn to
that of the other must always form a right angle with the direction of
the sun.
[Illustration:
Diagram Showing Why the Winter Moon Runs High.
]
“There is another very interesting fact about the position of the moon
in the sky which we should not neglect to notice. Did you ever observe
the superior brilliancy of the light of the Full Moon in winter? It is
one of the compensations that nature offers us. Since the Full Moon is
necessarily situated opposite to the point occupied by the sun, and
since the sun is far south of the equator in midwinter, it follows that
at the same season the Full Moon appears high above the equator in the
northern hemisphere. You will, perhaps, permit me to show you a diagram
intended to explain this phenomenon.
You observe that the sun being south of the equator, in the direction
indicated by the dotted line, the Full Moon is correspondingly situated
north of the equator, and must necessarily appear high in the sky at
midnight, when the sun is at its lowest declination. This is the reason
why the winter Full Moons are so brilliant, making the snow-clad hills
gleam with a splendor that sometimes dazzles the eyes of the beholders.
In the Arctic regions the long winter night, when the sun does not rise
for months, is periodically brightened by the presence of the Full Moon.
Just the opposite condition of affairs exists in summer. Then the sun
being north of the equator the Full Moon is south of it, and ‘runs low,’
appearing in high latitudes to skim along the southern horizon.”
Public-domain text, read in full here on John Shaqi.
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