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
For BN, BD, NX, put A, O, C, respectively, and let VZ be to XZ or DN as
d to e, and VG be equal to ;
then DN will be equal to A - O,
,
,
and GD or NX - VZ - VG equal to
.
[Pg 274]Let the term
be resolved into an infinite series
,
&c., and GD will be equal to
,
&c. The second term
of this series is to be used for Qo, the third
for Roo,
the fourth
for . And thence the density of the
medium ,
in any place G, will be
and therefore if in VZ you take VY
equal to n × VG, that density is reciprocally as XY. For A2 and
are the squares of XZ and ZY. But the resistance in the same
place G is to the force of gravity as
to 4RR, that is, as XY to . And the
velocity there is the same wherewith the projected body would move in a
parabola, whose vertex is G, diameter GD, and latus rectum
or
. Q.E.I.
SCHOLIUM.
In the same manner that the density of the medium comes out to be
as ,
in Cor. 1, if the resistance is put as any power
Vn of the velocity V, the density of the medium will come out
to be as .
And therefore if a curve can be found, such that the ratio
[Pg 275]of to
or
of to
may be given; the body, in an uniform medium, whose resistance is as
the power Vn of the velocity V, will move in this curve. But let us
return to more simple curves.
Because there can be no motion in a parabola except in a non-resisting
medium, but in the hyperbolas here described it is produced by a
perpetual resistance; it is evident that the line which a projectile
describes in an uniformly resisting medium approaches nearer to these
hyperbolas than to a parabola. That line is certainly of the hyperbolic
kind, but about the vertex it is more distant from the asymptotes, and
in the parts remote from the vertex draws nearer to them than these
hyperbolas here described. The difference, however, is not so great
between the one and the other but that these latter may be commodiously
enough used in practice instead of the former. And perhaps these may
prove more useful than an hyperbola that is more accurate, and at the
same time more compounded. They may be made use of, then, in this
manner.
Complete the parallelogram XYGT, and the right line GT will touch
the hyperbola in G, and therefore the density of the medium in
G is reciprocally as the tangent GT, and the velocity there as
; and the resistance
is to the force of gravity as GT to .
Therefore if a body projected from the place A, in the direction
of the right line AH, describes the hyperbola AGK and AH produced
meets the asymptote NX in H, and AI drawn parallel to it meets
the other asymptote MX in I; the density of the medium in A
will be reciprocally as AH, and the velocity of the body as
, and the resistance
there to the force of gravity as AH to .
Hence the following rules are deduced.
Public-domain text, read in full here on John Shaqi.
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