c с 5. In polar coordinates the orbit of the earth around the sun is described by the differential equations GM ř - rh2

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c с 5. In polar coordinates the orbit of the earth around the sun is described by the differential equations GM ř - rh2

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c с 5. In polar coordinates the orbit of the earth around the sun is described by the differential equations GM ř - rh2 p2 r2 Here, M = mass of the earth and G =Newton's gravitational constant. The origin is taken to be the center of the sun. Show that r(0) c2/(GM) 1- (Ac2/(GM)) cos(8) solves the given differential equation. Here, A and c are constants.
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