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orbital motion

In astronomy the motion of a material body through space under the influence of its own inertia, a central force, and other forces. Johannes Kepler found empirically that the orbital motions of the planets about the Sun are ellipses. Isaac Newton, starting from his laws of motion, proved that an inverse-square gravitational field of force requires a body to move in an orbit that is a circle, ellipse, parabola, or hyperbola.

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