Kepler's equation
= Kepler's equation
{c}
{wiki}
For an elliptic <Kepler orbit>, <Kepler's equation> relates <mean anomaly> $M$ and <eccentric anomaly> $E$ by
$$
M=E-e\sin E.
$$
= Kepler's equation
{c}
{wiki}
For an elliptic <Kepler orbit>, <Kepler's equation> relates <mean anomaly> $M$ and <eccentric anomaly> $E$ by
$$
M=E-e\sin E.
$$