Kepler's 3rd law: Difference between revisions

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'''Johannes Kepler''' (b. 1571)
''''' Kepler's laws of planetary motion''''' 1609-1619
The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
: $$T^2 \propto a^3$$
: $$T^2 \propto a^3$$



Revision as of 08:25, 18 March 2020

Johannes Kepler (b. 1571)

Kepler's laws of planetary motion 1609-1619

The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.

$$T^2 \propto a^3$$

Resources:

Discussion: