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. 5. In the same figure, or even in different figures, whose
principal latera recta are equal, the velocity of a body is
reciprocally as the perpendicular let fall from the focus on the
tangent.
COR. 6. In a parabola, the velocity is reciprocally in the subduplicate
ratio of the distance of the body from the focus of the figure; it
is more variable in the ellipsis, and less in the hyperbola, than
according to this ratio. For (by Cor. 2, Lem. XIV) the perpendicular
let fall from the focus on the tangent of a parabola is in the
subduplicate ratio of the distance. In the hyperbola the perpendicular
is less variable; in the ellipsis more.
COR. 7. In a parabola, the velocity of a body at any distance from the
focus is to the velocity of a body revolving in a circle, at the same
distance from the centre, in the subduplicate ratio of the number 2
to 1; in the ellipsis it is less, and in the hyperbola greater, than
according to this ratio. For (by Cor. 2 of this Prop.) the velocity
at the vertex of a parabola is in[Pg 123] this ratio, and (by Cor. 6 of this
Prop. and Prop. IV) the same proportion holds in all distances. And
hence, also, in a parabola, the velocity is everywhere equal to the
velocity of a body revolving in a circle at half the distance; in the
ellipsis it is less, and in the hyperbola greater.
COR. 8. The velocity of a body revolving in any conic section is to
the velocity of a body revolving in a circle, at the distance of half
the principal latus rectum of the section, as that distance to the
perpendicular let fall from the focus on the tangent of the section.
This appears from Cor. 5.
COR. 9. Wherefore since (by Cor. 6, Prop. IV), the velocity of a body
revolving in this circle is to the velocity of another body revolving
in any other circle reciprocally in the subduplicate ratio of the
distances; therefore, ex æquo, the velocity of a body revolving
in a conic section will be to the velocity of a body revolving in a
circle at the same distance as a mean proportional between that common
distance, and half the principal latus rectum of the section, to the
perpendicular let fall from the common focus upon the tangent of the
section.
PROPOSITION XVII. PROBLEM IX.
Supposing the centripetal force to be reciprocally proportional to
the squares of the distances of places from the centre, and that the
absolute quantity of that force is known; it is required to determine
the line which a body will describe that is let go from a given place
with a given velocity in the direction of a given right line.
Public-domain text, read in full here on John Shaqi.
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