The starry skies : $b or, First lessons on the sun, moon and starsGiberne, Agnes
General
The starry skies : $b or, First lessons on the sun, moon and stars
Giberne, Agnes
Astronomy -- Juvenile literature
At Full Moon _the Earth is between the Sun and the Moon_. On one side
of our Earth is the Sun; on the other side is the Moon. The Sun shines
full upon that side of the Moon which is turned towards us; and so
we see the whole of her round bright face. We know that her farther
side is in darkness, because it is turned away from the Sun: in almost
pitch-darkness, for it has not even our Earth to light it up, being
turned away from us also. It has only Stars on the farther side.
I am speaking of when the Sun has set, and is below our horizon, so
that we cannot see him, although his rays travel straight to the Moon.
The Sun having set means only that the solid body of our Earth is
between him and us. It does not interfere with his shining upon the
Moon.
If our Earth at Full Moon were _exactly_ between the Sun and the Moon,
that would interfere with his shining upon her. More commonly, however,
our Earth is not just in the line between, but only very nearly so.
Thus we get the best possible view of the Moon’s round face.
The Moon does not stay on one side of the Earth. She is always
travelling round from one side to the other side of us. At another part
of her monthly journey things are quite different.
A fortnight after Full Moon we have _New Moon_.
At Full Moon the Earth is between Sun and Moon; but at New Moon the
Moon has come right round to the opposite side, and is _between the Sun
and the Earth_. Not usually in the exact line between, so as to hide
the Sun from us, but very nearly so.
Then still the Moon has a bright round face; only we on Earth cannot
see it. For her bright side is, as always, towards the Sun; and her
_dark_ side is towards us.
Just at first we cannot see the New Moon at all, for it is entirely
dark. As she journeys on to one side we get a glimpse of a thin line of
light shaped like a sickle; and this widens every day. It is while we
see the sickle of light that we sometimes catch a glimpse of the dark
side of the Moon, dimly lighted up by Earth-shine.
[Illustration: _The Moon. Second quarter. 10½ days old._]
When the Moon gets half-way back to where she was at Full Moon we are
able to see _half_ of her bright face, and we call that the “First
Quarter.” The other half of the bright face is still turned away from
us, and half of the dark side is still towards us. We do not see the
whole round face till she gains once more the place of Full Moon--after
which, between Full Moon and New Moon, follows the Third Quarter, which
is much the same as the First Quarter.
You know that the rising and the setting of the Moon in our sky,
by night or by day, are not real movements. They are only seeming
movements, caused by our own Earth’s daily spinning on her axis.
Public-domain text, read in full here on John Shaqi.
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