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21 January, 15:03

Kepler law with numerical problems

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  1. 21 January, 15:32
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    First Law: Planetary orbits are elliptical with the sun at a focus.

    Second Law: The radius vector from the sun to a planet sweeps equal areas in equal times.

    Third Law: The ratio of the square of the period of revolution and the cube of the ellipse semimajor axis is the same for all planets.
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