Relative angular momentum
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In astrodynamics, the relative angular momentum () of an orbiting body () relative to a central body () is the moment of ()'s relative linear momentum:
where:
- is the orbital position vector of the orbiting body relative to the central body,
- is the orbital velocity vector of the orbiting body relative to the central body,
- is mass of the orbiting body.
For an body orbiting a central body is always perpendicular to the osculating orbital plane determined by orbital position and velocity vectors.
[edit] Uses
In astrodynamics relative angular momentum is usually used to derive specific relative angular momentum ():
where:
- is mass of the orbiting body.