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
But since the description of this curve is difficult, a solution by
approximation will be preferable. First, then, let there be found a
certain angle B which may be to an angle of 57,29578 degrees, which an
arc equal to the radius subtends, as SH, the distance of the foci, to
AB, the diameter of the ellipsis. Secondly, a certain length L, which
may be to the radius in the same ratio inversely. And these being
found, the Problem may be solved by the following analysis. By any
construction (or even by conjecture), suppose we know P the place of
the body near its true place p. Then letting fall on the axis
of the ellipsis the ordinate PR from the proportion of the diameters
of the ellipsis, the ordinate RQ of the circumscribed circle AQB will
be given; which ordinate is the sine of the angle AOQ, supposing AO to
be the radius, and also cuts the ellipsis in P. It will be sufficient
if that angle is found by a rude calculus in numbers near the truth.
Suppose we also know the angle proportional to the time, that is, which
is to four right angles as the time in which the body described the
arc Ap, to the time of one revolution in the ellipsis. Let this
angle be N. Then take an angle D, which may be to the angle B as the
sine of the angle AOQ to the radius; and an angle E which may be to
the angle N - AOQ + D as the length L to the same length L diminished
by the cosine of the angle AOQ, when that angle is less than a right
angle, or increased thereby when greater. In the next place, take an
angle F that may be to the angle B as the sine of the angle AOQ + E to
the radius, and an angle G, that may be to the angle N - AOQ - E + F
as the length L to the same length L diminished by the cosine of the
angle AOQ + E, when that angle is less than a right angle, or increased
thereby when greater. For the third time take an angle H, that may be
to the angle B as the sine of the angle AOQ + E + G to the radius; and
an angle I to the angle N - AOQ - E - G + H, as the[Pg 158] length L is to
the same length L diminished by the cosine of the angle AOQ + E + G,
when that angle is less than a right angle, or increased thereby when
greater. And so we may proceed in infinitum. Lastly, take the
angle AOq equal to the angle AOQ + E + G + I +, &c. and from
its and the ordinate pr, which is to its
as the lesser axis of the ellipsis to the greater, we
shall have p the correct place of the body. When the angle N
- AOQ + D happens to be negative, the sign + of the angle E must be
every where changed into -, and the sign - into +. And the same thing
is to be understood of the signs of the angles G and I, when the angles
N - AOQ - E + F, and N - AOQ - E - G + H come out negative. But the
infinite series AOQ + E + G + I +, &c. converges so very fast, that
it will be scarcely ever needful to proceed beyond the second term E.
And the calculus is founded upon this Theorem, that the area APS is as
the difference between the arc AQ and the right line let fall from the
Public-domain text, read in full here on John Shaqi.
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