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
The same things being supposed, I say, that the velocity of the body
before its incidence is to its velocity after emergence as the sine of
emergence to the sine of incidence.
Make AH and Id equal, and erect the perpendiculars AG, dK
meeting the lines of incidence and emergence GH, IK, in G and K.
In GH take TH equal to IK, and to the plane Aa let fall a
perpendicular Tv. And (by Cor. 2 of the Laws of Motion) let
the motion of the body be resolved into two, one perpendicular to the
planes[Pg 245] Aa, Bb, Cc, &c., and another parallel
to them. The force of attraction or impulse, acting in directions
perpendicular to those planes, does not at all alter the motion in
parallel directions; and therefore the body proceeding with this motion
will in equal times go through those equal parallel intervals that lie
between the line AG and the point H, and between the point I and the
line dK; that is, they will describe the lines GH, IK in equal
times. Therefore the velocity before incidence is to the velocity after
emergence as GH to IK or TH, that is, as AH or Id to vH,
that is (supposing TH or IK radius), as the sine of emergence to the
sine of incidence. Q.E.D.
PROPOSITION XCVI. THEOREM L.
The same things being supposed, and that the motion before incidence
is swifter than afterwards; I say, that if the line of incidence be
inclined continually, the body will be at last reflected, and the angle
of reflexion will be equal to the angle of incidence.
[Pg 246]
For conceive the body passing between the parallel planes Aa,
Bb, Cc, &c., to describe parabolic arcs as above; and
let those arcs be HP, PQ, QR, &c. And let the obliquity of the line
of incidence GH to the first plane Aa be such that the sine
of incidence may be to the radius of the circle whose sine it is, in
the same ratio which the same sine of incidence hath to the sine of
emergence from the plane Dd into the space DdeE; and
because the sine of emergence is now become equal to radius, the angle
of emergence will be a right one, and therefore the line of emergence
will coincide with the plane Dd. Let the body come to this plane
in the point R; and because the line of emergence coincides with that
plane, it is manifest that the body can proceed no farther towards the
plane Ee. But neither can it proceed in the line of emergence
Rd; because it is perpetually attracted or impelled towards the
medium of incidence. It will return, therefore, between the planes
Cc, Dd, describing an arc of a parabola QRq, whose
principal vertex (by what Galileo has demonstrated) is in R,
cutting the plane Cc in the same angle at q, that it did
before at Q; then going on in the parabolic arcs qp, ph,
&c., similar and equal to the former arcs QP, PH, &c., it will cut
the rest of the planes in the same angles at p, h, &c.,
as it did before in P, H, &c., and will emerge at last with the same
obliquity at h with which it first impinged on that plane at
H. Conceive now the intervals of the planes Aa, Bb,
Public-domain text, read in full here on John Shaqi.
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