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
21. When we speak of the Planets Orbits, all that is meant is their
Paths through the open and unresisting Space in which they move; and are
kept in, by the attractive power of the Sun, and the projectile force
impressed upon them at first: between which power and force there is so
exact an adjustment, that without any solid Orbits to confine the
Planets, they keep their courses, and at the end of every revolution
find the points from whence they first set out, much more truly than can
be imitated in the best machines made by human art.
[Sidenote: Mercury.
Fig. I.
May be inhabited.
PLATE I.]
22. MERCURY, the nearest Planet to the Sun, goes round him (as in the
circle marked ☿) in 87 days 23 hours of our time nearly; which is the
length of his year. But, being seldom seen, and no spots appearing on
his surface or disc, the time of his rotation on his axis, or the length
of his days and nights, is as yet unknown. His distance from the Sun is
computed to be 32 millions of miles, and his diameter 2600. In his
course, round the Sun, he moves at the rate of 95 thousand miles every
hour. His light and heat from the Sun are almost seven times as great as
ours; and the Sun appears to him almost seven times as large as to us.
The great heat on this Planet is no argument against it’s being
inhabited; since the Almighty could as easily suit the bodies and
constitutions of it’s inhabitants to the heat of their dwelling, as he
has done ours to the temperature of our Earth. And it is very probable
that the people there have such an opinion of us, as we have of the
inhabitants of Jupiter and Saturn; namely, that we must be intolerably
cold, and have very little light at so great a distance from the Sun.
[Sidenote: Has like phases with the Moon.]
23. This Planet appears to us with all the various phases of the Moon,
when viewed at different times by a good telescope; save only that he
never appears quite Full, because his enlightened side is never turned
directly towards us but when he is so near the Sun as to be lost to our
sight in it’s beams. And, as his enlightened side is always toward the
Sun, it is plain that he shines not by any light of his own; for if he
did, he would constantly appear round. That he moves about the Sun in an
Orbit within the Earth’s Orbit is also plain (as will be more largely
shewn by and by, § 141, _& seq._) because he is never seen opposite to
the Sun, nor above 56 times the Sun’s breadth from his center.
[Sidenote: His Orbit and Nodes.]
Public-domain text, read in full here on John Shaqi.
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