A View of Sir Isaac Newton's PhilosophyPemberton, Henry
Science
A View of Sir Isaac Newton's Philosophy
Pemberton, Henry
Newton, Isaac, 1642-1727. Principia
And by entering the atmospheres of the earth and other planets,
they may well be supposed to contribute to the renovation of the face
of things, in particular to supply the diminution caused in the humid
parts by vegetation and putrefaction. For vegetables are nourished by
moisture, and by putrefaction are turned in great part into dry earth;
and an earthy substance always subsides in fermenting liquors; by which
means the dry parts of the planets must continually increase, and the
fluids diminish, nay in a sufficient length of time be exhausted, if
not supplied by some such means. It is farther our great author’s
opinion, that the most subtile and active parts of our air, upon which
the life of things chiefly depends, is derived to us, and supplied
by the comets. So far are they from portending any hurt or mischief
to us, which the natural fears of men are so apt to suggest from the
appearance of any thing uncommon and astonishing.
20. THAT the tails of comets have some such important use seems
reasonable, if we consider, that those bodies do not send out those
fumes merely by their near approach to the sun; but are framed of a
texture, which disposes them in a particular manner to fume in that
sort: for the earth, without emitting any such steam, is more than half
the year at a less distance from the sun, than the comet of 1664 and
1665 approached it, when nearest; likewise the comets of 1682 and 1683
never approached the sun much above a seventh part nearer than Venus,
and were more than half as far again from the sun as Mercury; yet all
these emitted tails.
21. FROM the very near approach of the comet of 1680 our author draws
another speculation; for if the sun have an atmosphere about it, the
comet mentioned seems to have descended near enough to the sun to
enter within it. If so, it must have been something retarded by the
resistance it would meet with, and consequently in its next descent to
the sun will fall nearer than now; by which means it will meet with a
greater resistance, and be again more retarded. The event of which must
be, that at length it will impinge upon the sun’s surface, and thereby
supply any decrease, which may have happened by so long an emission of
light, or otherwise. And something like this our author conjectures
may be the case of those fixed stars which by an additional increase
of their lustre have for a certain time become visible to us, though
usually they are out of sight. There is indeed a kind of fixed stars,
which appear and disappear at regular and equal intervals: here some
more steady cause must be sought for; perhaps these stars turn round
their own axis’s, as our sun does[236], and have some part of their
body more luminous than the other, whereby they are seen, when the most
lucid part is next to us, and when the darker part is turned toward us,
they vanish out of sight.
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