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
COR. 6. Hence from the given time there is given the space described in
the ascent or descent. For the greatest velocity of a body descending
in infinitum is given (by Corol. 2 and 3, Theor. VI, of this
Book); and thence the time is given in which a body would acquire that
velocity by falling in a non-resisting space. And taking the sector
ADT or ADt to the triangle ADC in the ratio of the given time
to the time just now found, there will be given both the velocity AP
or Ap, and the area ABNK or ABnk, which is to the sector
ADT, or ADt, as the space sought to the space which would, in
the given time, be uniformly described with that greatest velocity
found just before.
[Pg 268]
COR. 7. And by going backward, from the given space of ascent or
descent ABnk or ABNK, there will be given the time ADt or
ADT.
PROPOSITION X. PROBLEM III.
Suppose the uniform force of gravity to tend directly to the plane
of the horizon, and the resistance to be as the density of the medium
and the square of the velocity conjunctly: it is proposed to find the
density of the medium in each place, which shall make the body move in
any given curve line; the velocity of the body and the resistance of
the medium in each place.
Let PQ be a plane perpendicular to the plane of the scheme itself;
PFHQ a curve line meeting that plane in the points P and Q; G, H, I,
K four places of the body going on in this curve from F to Q; and
GB, HC, ID, KE four parallel ordinates let fall from these points to
the horizon, and standing on the horizontal line PQ at the points
B, C, D, E; and let the distances BC, CD, DE, of the ordinates be
equal among themselves. From the points G and H let the right lines
GL, HN, be drawn touching the curve in G and H, and meeting the
ordinates CH, DI, produced upwards, in L and N: and complete the
parallelogram HCDM. And the times in which the body describes the
arcs GH, HI, will be in a subduplicate ratio of the altitudes LH, NI,
which the bodies would describe in those times, by falling from the
tangents; and the velocities will be as the lengths described GH, HI
directly, and the times inversely. Let the times be expounded by T and
t, and the velocities by and
; the decrement of the velocity produced in
the time t will be expounded by .
This decrement arises from the
resistance which retards the body, and from the gravity which
accelerates it. Gravity, in a falling body, which in its fall describes
the space NI, produces a velocity with which it would be able to
describe twice that space in the same time, as Galileo has
demonstrated; that is, the velocity :
but if the body describes the arc HI, it augments that arc only by
the length or
;
and therefore generates only the velocity
.
Let this velocity be added to the before-mentioned
decrement, and we shall have the decrement of the velocity arising
from the resistance alone, that is,
.[Pg 269]
Therefore since, in the same time, the
action of gravity generates, in a falling body, the velocity
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