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Kepler law with numerical problems
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Kepler law with numerical problems

User Frank Hileman
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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.
User Surge
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