Newton's Principia : $b The mathematical principles of natural philosophyNewton, Isaac
General
Newton's Principia : $b The mathematical principles of natural philosophy
Newton, Isaac
Celestial mechanics -- Early works to 1800; Mechanics -- Early works to 1800
Of the attractive forces of bodies which are not of a sphærical
figure.
PROPOSITION LXXXV. THEOREM XLII.
If a body be attracted by another, and its attraction be vastly
stronger when it is contiguous to the attracting body than when they
are separated from one another by a very small interval; the forces of
the particles of the attracting body decrease, in the recess of the
body attracted, in more than a duplicate ratio of the distance of the
particles.
For if the forces decrease in a duplicate ratio of the distances from
the particles, the attraction towards a sphærical body being (by Prop.
LXXIV) reciprocally as the square of the distance of the attracted
body from the centre of the sphere, will not be sensibly increased
by the contact, and it[Pg 234] will be still less increased by it, if the
attraction, in the recess of the body attracted, decreases in a still
less proportion. The proposition, therefore, is evident concerning
attractive spheres. And the case is the same of concave sphærical
orbs attracting external bodies. And much more does it appear in orbs
that attract bodies placed within them, because there the attractions
diffused through the cavities of those orbs are (by Prop. LXX)
destroyed by contrary attractions, and therefore have no effect even in
the place of contact. Now if from these spheres and sphærical orbs we
take away any parts remote from the place of contact, and add new parts
any where at pleasure, we may change the figures of the attractive
bodies at pleasure; but the parts added or taken away, being remote
from the place of contact, will cause no remarkable excess of the
attraction arising from the contact of the two bodies. Therefore the
proposition holds good in bodies of all figures. Q.E.D.
PROPOSITION LXXXVI. THEOREM XLIII.
If the forces of the particles of which an attractive body is
composed decrease, in the recess of the attractive body, in a
triplicate or more than a triplicate ratio of the distance from the
particles, the attraction will be vastly stronger in the point of
contact than when the attracting and attracted bodies are separated
from each other, though by never so small an interval.
For that the attraction is infinitely increased when the attracted
corpuscle comes to touch an attracting sphere of this kind, appears,
by the solution of Problem XLI, exhibited in the second and third
Examples. The same will also appear (by comparing those Examples
and Theorem XLI together) of attractions of bodies made towards
concavo-convex orbs, whether the attracted bodies be placed without
the orbs, or in the cavities within them. And by adding to or taking
from those spheres and orbs any attractive matter any where without
the place of contact, so that the attractive bodies may receive
any assigned figure, the Proposition will hold good of all bodies
universally. Q.E.D.
PROPOSITION LXXXVII. THEOREM XLIV.
Public-domain text, read in full here on John Shaqi.
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