Kepler Orbit Propagation

Use when you must determine the time propagation of a spacecraft orbit from its classical orbital elements: mean motion from the semimajor axis, the Kepler equation M = E - e sin E solved by Newton iteration for the eccentric anomaly, the branch-safe half-angle conversion to true anomaly, the radius at any anomaly, the time since periapsis for a given true anomaly, and the inertial position and velocity vectors after an elapsed time from an element state (a, e, i, RAAN, argp, nu0). Produces the propagated mean, eccentric and true anomalies, radius, r vector, v vector and orbital period for ground-track and event timing. Trigger: keplerian propagation, kepler equation, mean anomaly, eccentric anomaly, time since periapsis, orbit propagation.

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