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Kepler law with numerical problems
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Kepler law with numerical problems
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Sep 25, 2021
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Kepler law with numerical problems
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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.
Surge
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Sep 29, 2021
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