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CHAPTER II - ON THE LAW OF UNIVERSAL GRAVITATION, DEDUCED FROM OBSERVATION

Published online by Cambridge University Press:  29 August 2010

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Summary

309. The three laws of Kepler furnish the data from which the principle of gravitation is established, namely :—

  1. i. That the radii vectores of the planets and comets describe areas proportional to the time.

  2. ii. That the orbits of the planets and comets are conic sections, having the sun in one of their foci.

  3. iii. That the squares of the periodic times of the planets are proportional to the cubes of their mean distances from the sun.

310. It has been shown, that if the law of the force which acts on a moving body be known, the curve in which it moves may be found; or, if the curve in which the body moves be given, the law of the force may be ascertained. In the general equation of the motion of a body in article 144, both the force and the path of the body are indeterminate; therefore in applying that equation to the motion of the planets and comets, it is necessary to know the orbits in which they move, in order to ascertain the nature of the force that acts on them.

311. In the general equation of the motion of a body, the forces acting on it are resolved into three component forces, in the direction of three rectangular axes ; but as the paths of the planets, satellites, and comets, are proved by the observations of Kepler to be conic sections, they always move in the same plane: therefore the component force in the direction perpendicular to that plane is zero, and the other two component forces are in the plane of the orbit.

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Publisher: Cambridge University Press
Print publication year: 2009
First published in: 1831

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