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
Let a body descend from A through D and E, to the centre C; and let
another body move from V in the curve line VIKk. From the centre
C, with any distances, describe the concentric circles DI, EK, meeting
the right line AC in D and E, and the curve VIK in I and K. Draw IC
meeting KE in N, and on IK let fall the perpendicular NT; and let the
interval DE or IN between the circumferences of the circles be very
small; and imagine the bodies in D and I to have equal velocities.
Then because the distances CD and CI are equal, the centripetal
forces in D and I will be also equal. Let those forces be expressed
by the equal lineolæ DE and IN; and let the force IN (by Cor. 2 of
the Laws of Motion) be resolved into two others, NT and IT. Then the
force NT acting in the direction of the line NT perpendicular to the
path ITK of the body will not at all affect or change the velocity
of the body in that path, but only draw it aside from a rectilinear
course, and make it deflect perpetually from the tangent of the orbit,
and proceed in the curvilinear path ITKk. That whole force,
therefore, will be spent in producing this effect; but the other force
IT, acting in the direction of the course of the body, will be all
employed in accelerating it, and in the least given time will produce
an acceleration proportional to itself. Therefore the accelerations
of the bodies in D and I, produced in equal times, are as the lines
DE, IT (if we take the first ratios of the nascent lines DE, IN, IK,
IT, NT); and in unequal times as those lines and the times conjunctly.
But the times in which DE and IK are described, are, by reason of the
equal velocities (in D and I) as the spaces described DE and IK, and
therefore the accelerations in the course of the bodies through the
lines DE and IK are as DE and IT, and DE and IK conjunctly; that is, as
the square of DE to the rectangle IT into IK. But the rectangle IT × IK
is equal to the square of IN, that is, equal to the square of DE; and
therefore the accelerations generated in the passage of the bodies from
D and I to E and K are equal. Therefore the velocities of the bodies in
E and K are also equal: and by the same reasoning they will always be
found equal in any subsequent equal distances. Q.E.D.
By the same reasoning, bodies of equal velocities and equal distances
from the centre will be equally retarded in their ascent to equal
distances. Q.E.D.
Public-domain text, read in full here on John Shaqi.
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