Physics — Kepler's Laws
The three laws of planetary motion.
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\text{1: elliptical orbit, Sun at a focus}
\text{2: equal areas in equal times}
T^2 \propto a^3
\frac{T^2}{a^3} = \frac{4\pi^2}{GM}
The three laws of planetary motion.
\text{1: elliptical orbit, Sun at a focus}
\text{2: equal areas in equal times}
T^2 \propto a^3
\frac{T^2}{a^3} = \frac{4\pi^2}{GM}