Astronomy Explained Upon Sir Isaac Newton's Principles: And made easy to those who have not studied mathematicsFerguson, James
Science
Astronomy Explained Upon Sir Isaac Newton's Principles: And made easy to those who have not studied mathematics
Ferguson, James
Astronomy -- Early works to 1800
A bare view of the Figure is enough to shew, that as the Earth advances
from Capricorn toward Aries, and the Sun appears to move from Cancer
toward Libra, the north Pole recedes toward the dark, which causes the
days to decrease, and the nights to increase in length, till the Earth
comes to Aries, and then they are equal as before; for the boundary of
light and darkness cut the Equator and all it’s parallels equally, or in
halves. The north pole then goes into the dark, and continues therein
until the Earth goes half way round it’s Orbit; or, from the 23d of
_September_ till the 20th of _March_. In the middle between these times,
_viz._ on the 22d of _December_, the north Pole is as far as it can be
in the dark, which is 23-1/2 degrees, equal to the inclination of the
Earth’s Axis from a perpendicular to it’s Orbit: and then, the northern
parallels are as much in the dark as they were in the light on the 21 of
_June_; the winter nights being as long as the summer days, and the
winter days as short as the summer nights. It is needless to multiply
words on this subject, as we shall have occasion to mention the seasons
again in describing the _Orrery_, § 439. Only this must be noted, that
all that has been said of the northern Hemisphere, the contrary must be
understood of the southern; for on different sides of the Equator the
seasons are contrary, because, when the northern Hemisphere inclines
toward the Sun the southern declines from him.
[Sidenote: The Phenomena of Saturn’s Ring.
PLATE V.]
204. As Saturn goes round the Sun, his obliquely posited ring, like our
Earth’s Axis, keeps parallel to itself, and is therefore turned edgewise
to the Sun twice in a Saturnian year, which is almost as long as 30 of
our years § 81. But the ring, though considerably broad, is too thin to
be seen when it is turned round edgewise to the Sun, at which time it is
also edgewise to the Earth; and therefore it disappears once in every
fifteen years to us. As the Sun shines half a year on the north pole of
our earth, then disappears to it, and shines as long on the south pole;
so, during one half of Saturn’s year the Sun shines on the north side of
his ring, then disappears to it, and shines as long on it’s south side.
When the Earth’s Axis inclines neither to nor from the Sun, but sidewise
to him, he instantly ceases to shine on one pole, and begins to
enlighten the other; and when Saturn’s Ring inclines neither to nor from
the Sun, but sidewise to him, he ceases to shine on the one side of it,
and begins to shine upon the other.
[Sidenote: Fig. III.]
Public-domain text, read in full here on John Shaqi.
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