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
As the satellites of Jupiter are continually revolving around him, they
will often pass behind or across his disc. Such occultations and
transits of satellites can be well observed in the telescope.
There is, however, a way in which the light of a celestial body may be
obscured without the necessity of its being hidden from us by one
nearer. It will no doubt be granted that any opaque object casts a
shadow when a strong light falls directly upon it. Thus the earth, under
the powerful light which is directed upon it from the sun, casts an
extensive shadow, though we are not aware of the existence of this
shadow until it falls upon something. The shadow which the earth casts
is indeed not noticeable to us until some celestial body passes into it.
As the sun is very large, and the earth in comparison very small, the
shadow thrown by the earth is comparatively short, and reaches out in
space for only about a million miles. There is no visible object except
the moon, which circulates within that distance from our globe, and
therefore she is the only body which can pass into this shadow. Whenever
such a thing happens, her surface at once becomes dark, for the reason
that she never emits any light of her own, but merely reflects that of
the sun. As the moon is continually revolving around the earth, one
would be inclined to imagine that once in every month, namely at what is
called _full moon_, when she is on the other side of the earth with
respect to the sun, she ought to pass through the shadow in question.
But this does not occur every time, because the moon's orbit is not
quite _upon the same plane_ with the earth's. It thus happens that time
after time the moon passes clear of the earth's shadow, sometimes above
it, and sometimes below it. It is indeed only at intervals of about six
months that the moon can be thus obscured. This darkening of her light
is known as an _eclipse of the moon_. It seems a great pity that custom
should oblige us to employ the one term "eclipse" for this and also for
the quite different occurrence, an eclipse of the sun; in which the
sun's face is hidden as a consequence of the moon's body coming directly
_between_ it and our eyes.
The popular mind seems always to have found it more difficult to grasp
the causes of an eclipse of the moon than an eclipse of the sun. As Mr.
J.E. Gore[4] puts it: "The darkening of the sun's light by the
interposition of the moon's body seems more obvious than the passing of
the moon through the earth's shadow."
Eclipses of the moon furnish striking spectacles, but really add little
to our knowledge. They exhibit, however, one of the most remarkable
evidences of the globular shape of our earth; for the outline of its
shadow when seen creeping over the moon's surface is always circular.
Public-domain text, read in full here on John Shaqi.
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