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
right line with a spiral, since this is but one simple curve and not
reducible to more curves, require equations infinite in number of
dimensions and roots, by which they may be all exhibited together.
For the law and calculus of all is the same. For if a perpendicular
is let fall from the pole upon that intersecting right line, and that
perpendicular together with the intersecting line revolves about the
pole, the intersections of the spiral will mutually pass the one into
the other; and that which was first or nearest, after one revolution,
will be the second; after two, the third; and so on: nor will the
equation in the mean time be changed but as the magnitudes of those
quantities are changed, by which the position of the intersecting line
is determined. Wherefore since those quantities after every revolution
return to their first magnitudes, the equation will return to its first
form; and consequently one and the same equation will exhibit all the
intersections, and will therefore have an infinite number of roots,
by which they may be all exhibited. And therefore the intersection of
a right line with a spiral cannot be universally found by any finite
equation; and of consequence there is no oval figure whose area cut off
by right lines at pleasure, can be universally exhibited by any such
equation.
[Pg 156]
By the same argument, if the interval of the pole and point by which
the spiral is described is taken proportional to that part of the
perimeter of the oval which is cut off, it may be proved that the
length of the perimeter cannot be universally exhibited by any finite
equation. But here I speak of ovals that are not touched by conjugate
figures running out in infinitum.
COR. Hence the area of an ellipsis, described by a radius drawn from
the focus to the moving body, is not to be found from the time given
by a finite equation; and therefore cannot be determined by the
description of curves geometrically rational. Those curves I call
geometrically rational, all the points whereof may be determined by
lengths that are definable by equations; that is, by the complicated
ratios of lengths. Other curves (such as spirals, quadratrixes, and
cycloids) I call geometrically irrational. For the lengths which are or
are not as number to number (according to the tenth Book of Elements)
are arithmetically rational or irrational. And therefore I cut off an
area of an ellipsis proportional to the time in which it is described
by a curve geometrically irrational, in the following manner.
PROPOSITION XXXI. PROBLEM XXIII.
To find the place of a body moving in a given elliptic trajectory at
any assigned time.
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