Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent AstronomersOlmsted, Denison
Science
Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent Astronomers
Olmsted, Denison
Astronomy
It was once supposed, that we could never reason respecting the laws
that govern the heavenly bodies from what we observe in bodies around
us, but that motion is one thing on the earth and quite another thing in
the skies; and hence, that it is impossible for us, by any inquiries
into the laws of terrestrial Nature, to ascertain how things take place
among the heavenly bodies. Galileo and Newton, however, proceeded on the
contrary supposition, that Nature is uniform in all her works; that the
same Almighty arm rules over all; and that He works by the same fixed
laws through all parts of His boundless realm. The certainty with which
all the predictions of astronomers, made on these suppositions, are
fulfilled, attests the soundness of the hypothesis. Accordingly, those
laws, which all experience, endlessly multiplied and varied, proves to
be the laws of terrestrial motion, are held to be the laws that govern
also the motions of the most distant planets and stars, and to prevail
throughout the universe of matter. Let us, then, briefly review these
great laws of motion, which are three in number. The FIRST LAW is as
follows: _every body perseveres in a state of rest, or of uniform motion
in a straight line, unless compelled by some force to change its state_.
By _force_ is meant any thing which produces motion.
The foregoing law has been fully established by experiment, and is
conformable to all experience. It embraces several particulars. First, a
body, when at rest, remains so, unless some force puts it in motion; and
hence it is inferred, when a body is found in motion, that some force
must have been applied to it sufficient to have caused its motion. Thus,
the fact, that the earth is in motion around the sun and around its own
axis, is to be accounted for by assigning to each of these motions a
force adequate, both in quantity and direction, to produce these
motions, respectively.
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