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
152. But if, whilst the projectile force carries the Planet from _B_ to
_b_, the Sun’s attraction (which constitutes the Planet’s gravitation)
should bring it down from _B_ to I, the gravitating power would then be
too strong for the projectile force; and would cause the Planet to
describe the curve _BC_. When the Planet comes to _C_, the gravitating
power (which always increases as the square of the distance from the Sun
_S_ diminishes) will be yet stronger for the projectile force; and by
conspiring in some degree therewith, will accelerate the Planet’s motion
all the way from _C_ to _K_; causing it to describe the arcs _BC_, _CD_,
_DE_, _EF_, &c. all in equal times. Having it’s motion thus accelerated,
it gains so much centrifugal force, or tendency to fly off at _K_ in the
line _Kk_, as overcomes the Sun’s attraction: and the centrifugal force
being too great to allow the Planet to be brought nearer the Sun, or
even to move round him in the Circle _Klmn_, &c. it goes off, and
ascends in the curve _KLMN_, &c. it’s motion decreasing as gradually
from _K_ to _B_ as it increased from _B_ to _K_, because the Sun’s
attraction acts now against the Planet’s projectile motion just as much
as it acted with it before. When the Planet has got round to _B_, it’s
projectile force is as much diminished from it’s mean state about _G_ or
_N_, as it was augmented at _K_; and so, the Sun’s attraction being more
than sufficient to keep the Planet from going off at _B_, it describes
the same Orbit over again, by virtue of the same forces or laws.
[Sidenote: Fig. IV.
The Planets describe equal Areas in equal times.]
153. A double projectile force will always balance a quadruple power of
gravity. Let the Planet at _B_ have twice as great an impulse from
thence towards _X_, as it had before: that is, in the same length of
time that it was projected from _B_ to _b_, as in the last example, let
it now be projected from _B_ to _c_; and it will require four times as
much gravity to retain it in it’s Orbit: that is, it must fall as far as
from _B_ to 4 in the time that the projectile force would carry it from
_B_ to _c_; otherwise it could not describe the curve _BD_, as is
evident by the Figure. But, in as much time as the Planet moves from _B_
to _C_ in the higher part of it’s Orbit, it moves from _I_ to _K_ or
from _K_ to _L_ in the lower part thereof; because, from the joint
action of these two forces, it must always describe equal areas in equal
times, throughout it’s annual course. These Areas are represented by the
triangles _BSC_, _CSD_, _DSE_, _ESF_, &c. whose contents are equal to
one another, quite round the Figure.
[Sidenote: A difficulty removed.]
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account