Kepler third law
= Kepler third law
{c}
{wiki}
= Kepler's third law
{c}
{synonym}
For two bodies with total mass $M$ and relative-orbit radius $r$, the Newtonian orbital period is
$$
T^2=\frac{4\pi^2r^3}{GM}.
$$
= Kepler third law
{c}
{wiki}
= Kepler's third law
{c}
{synonym}
For two bodies with total mass $M$ and relative-orbit radius $r$, the Newtonian orbital period is
$$
T^2=\frac{4\pi^2r^3}{GM}.
$$