

Calculation [edit]
Small body orbiting a central body [edit]
According to Kepler's Third Law, the orbital period (in seconds) of two bodies orbiting each other in a circular or elliptic orbit is:
where:
is the orbit's semi-major axis, in meters
is the standard gravitational parameter, in
is the gravitational constant,
is the mass of the more massive body.
For all ellipses with a given semi-major axis the orbital period is the same, regardless of eccentricity.
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This post was edited by saber_x3 on May 22 2013 04:09pm