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
EXAMPLE 1. If the centripetal force tending to the several particles of
the sphere be reciprocally as the distance; instead of V write PE the
distance, then 2PS × LD for PE2; and DN will become as
.
Suppose DN equal to its double ;
and 2SL the given part of the
ordinate drawn into the length AB will describe the rectangular area
2SL × AB; and the indefinite part LD, drawn perpendicularly into the
same length with a continued motion, in such sort as in its motion one
way or another it may either by increasing or decreasing remain always
equal to the length LD, will describe the area ,
that is, the area SL × AB; which taken from
the former area 2SL × AB, leaves the area SL × AB. But the third part
, drawn after the same manner with
a continued motion perpendicularly into the same length, will describe
the area of an hyperbola, which subducted from the area SL × AB will
leave ANB the area sought. Whence arises this construction of the
Problem. At the points, L, A, B, erect the perpendiculars Ll,
Aa, Bb; making Aa equal to LB, and Bb equal
to LA. Making Ll and LB asymptotes, describe through the points
a, b,[Pg 230] the hyperbolic curve ab. And the chord
ba being drawn, will inclose the area aba equal to the
area sought ANB.
EXAMPLE 2. If the centripetal force tending to the several particles
of the sphere be reciprocally as the cube of the distance, or
(which is the same thing) as that cube applied to any given
plane; write for V,
and 2PS × LD for PE2; and DN will become as
that is (because PS, AS, SI are continually proportional), as
.
If we draw then these three parts into the length AB, the first
will generate the area of
an hyperbola; the second the area
; the third
the
area ,
that is, . From the first
subduct the sum of the second and third, and there will remain ANB,
the area sought. Whence arises this construction of the problem. At
the points L, A, S, B, erect the perpendiculars Ll Aa,
Ss, Bb, of which suppose Ss equal to SI; and
through the point s, to the asymptotes Ll, LB, describe
the hyperbola asb meeting the perpendiculars Aa,
Bb, in a and b; and the rectangle 2ASI, subducted
from the hyperbolic area AasbB, will leave ANB the area sought.
EXAMPLE 3. If the centripetal force tending to the several particles
of the spheres decrease in a quadruplicate ratio of the distance
from the particles; write
for V, then
for PE, and DN will become as
.
These three parts drawn into the length AB, produce so many areas, viz.
into ;
into
; and
into .
And these after due
reduction come forth ,
[Pg 231], and .
And these by subducting the last from the first, become .
Therefore the entire force with which the corpuscle P
is attracted towards the centre of the sphere is as
, that is, reciprocally as
Q.E.I.
By the same method one may determine the attraction of a corpuscle
situate within the sphere, but more expeditiously by the following
Theorem.
PROPOSITION LXXXII. THEOREM XLI.
Public-domain text, read in full here on John Shaqi.
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