The most radical thing Kepler did was to remove the assumption of circular motions, a motion viewed by the Greeks and Copernicus as sacred. This simple generalization allowed Kepler to make a model which was consistent the the data acquired by Tycho.
Law I: Law of Ellipses
The orbits are nearly circular, however. The distortions are quite small and visually hard to see, in general:
Law III: Harmonic Law
![]() The above is a log-log plot, log P vs. log a |
In tabular form,
![]() Note that the last two entries in the above table are discrepant. |
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The asteroid belt sits between the orbits of Mars and Jupiter. Compare the orbital period for an object that has orbit of size 4 A.U. to the orbital period of the Earth. Using Kepler's 3rd Law we have that the square of the orbital period measured in years isSo the orbital period of the asteroid measured in years is the square root of 64, that is, the orbital period of the asteroid is 8 years.
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