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
hundred times less; and so on. Now, it was known that the moon is about
sixty times as far from the centre of the earth as the surface of the
earth is from the centre, and consequently, the force of attraction at
the moon must be the square of sixty, or thirty-six hundred times less
than it is at the earth; so that a body at the distance of the moon
would fall towards the earth very slowly, only one thirty-six hundredth
part as far in a given time, as at the earth. Does the moon actually
fall towards the earth at this rate; or, what is the same thing, does
she depart at this rate continually from the straight line in which she
tends to move, and in which she would move, if no external force
diverted her from it? On making the calculation, such was found to be
the fact. Hence gravity, and no other force than gravity, acts upon the
moon, and compels her to revolve around the earth. By reasonings equally
conclusive, it was afterwards proved, that a similar force compels all
the planets to circulate around the sun; and now, we may ascend from the
contemplation of this force, as we have seen it exemplified in falling
bodies, to that of a universal power whose influence extends to all the
material creation. It is in this sense that we recognise the principle
of universal gravitation, the law of which may be thus enunciated; _all
bodies in the universe, whether great or small, attract each other, with
forces proportioned to their respective quantities of matter, and
inversely as the squares of their distances from each other_.
This law asserts, first, that attraction reigns throughout the material
world, affecting alike the smallest particle of matter and the greatest
body; secondly, that it acts upon every mass of matter, precisely in
proportion to its quantity; and, thirdly, that its intensity is
diminished as the square of the distance is increased.
Observation has fully confirmed the prevalence of this law throughout
the solar system; and recent discoveries among the fixed stars, to be
more fully detailed hereafter, indicate that the same law prevails
there. The law of universal gravitation is therefore held to be the
grand principle which governs all the celestial motions. Not only is it
consistent with all the observed motions of the heavenly bodies, even
the most irregular of those motions, but, when followed out into all its
consequences, it would be competent to assert that such irregularities
must take place, even if they had never been observed.
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