Astronomy Explained Upon Sir Isaac Newton's Principles: And made easy to those who have not studied mathematics — John Shaqi
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
102. We find the Moon moves round the Earth in an Orbit nearly circular.
The Moon therefore must be acted on by two powers or forces; one which
would cause her to move in a right line, another bending her motion from
that line into a curve. This attractive power must be seated in the
Earth; for there is no other body within the Moon’s Orbit to draw her.
The attractive power of the Earth therefore extends to the Moon; and, in
combination with her projectile force, causes her to move round the
Earth in the same manner as the circulating body above supposed.
[Sidenote: The Sun and Planets attract each other.]
103. The Moons of Jupiter and Saturn are observed to move round their
primary Planets: therefore there is such a power as gravity in these
Planets. All the Planets move round the Sun, and respect it for their
centre of motion: therefore the Sun must be endowed with attracting
force, as well as the Earth and Planets. The like may be proved of the
Comets. So that all the bodies or matter in the Solar System are
possessed of this power; and perhaps so is all matter whatsoever.
104. As the Sun attracts the Planets with their Satellites, and the
Earth the Moon, so the Planets and Satellites re-attract the Sun, and
the Moon the Earth: action and re-action being always equal. This is
also confirmed by observation; for the Moon raises tides in the ocean,
the Satellites and Planets disturb one another’s motions.
105. Every particle of matter being possessed of an attracting power,
the effect of the whole must be in proportion to the number of
attracting particles: that is, to the quantity of matter in the body.
This is demonstrated from experiments on pendulums: for, if they are of
equal lengths, whatever their weights be, they always vibrate in equal
times. Now, if one be double the weight of another, the force of gravity
or attraction must be double to make it oscillate with the same
celerity: if one is thrice the weight or quantity of matter of another,
it requires thrice the force of gravity to make it move with the same
celerity. Hence it is certain, that the power of gravity is always
proportional to the quantity of matter in bodies, whatever their bulks
or figures are.
106. Gravity also, like all other virtues or emanations issuing from a
centre, decreases as the square of the distance increases: that is, a
body at twice the distance attracts another with only a fourth part of
the force; at four times the distance, with a sixteenth part of the
force. This too is confirmed from observation, by comparing the distance
which the Moon falls in a minute from a right line touching her Orbit,
with the space which bodies near the Earth fall in the same time: and
also by comparing the forces which retain Jupiter’s Moons in their
Orbits. This will be more fully explained in the seventh Chapter.
[Sidenote: Gravitation and projection exemplified.]
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