astrodynx#
Kepler Equations
Returns the Kepler's equation for elliptical orbits in the form f(E) = 0. |
|
Returns the Kepler's equation for hyperbolic orbits in the form f(H) = 0. |
|
Returns the universal Kepler's equation in the form f(chi) = 0. |
|
Returns the generalized anomaly. |
|
Returns the mean anomaly for an elliptical orbit. |
|
Returns the mean anomaly for a hyperbolic orbit. |
|
Returns the eccentric anomaly for an elliptical orbit. |
|
Returns the hyperbolic eccentric anomaly for a hyperbolic orbit. |
|
Returns the generalized anomaly for a universal orbit equation. |
|
Returns the derivative of Kepler's equation for elliptical orbits with respect to the eccentric anomaly. |
|
Returns the derivative of Kepler's equation for hyperbolic orbits with respect to the hyperbolic eccentric anomaly. |
Orbit Integrals
Returns the orbital period of a two-body system. |
|
Returns the semimajor axis of a two-body system from its orbital period. |
|
Returns the specific angular momentum of a two-body system. |
|
Returns the semimajor axis of a two-body orbit. |
|
Returns the eccentricity vector of a two-body orbit. |
|
Returns the semiparameter of a two-body orbit. |
|
Returns the mean motion of a two-body orbit. |
|
Returns the equation of the orbit in the two-body system. |
|
The equation of orbit using universal functions |
|
Returns the radius of periapsis of the orbit. |
|
Returns the radius of apoapsis of the orbit. |
|
Returns the semiparameter of the orbit from the semimajor axis and eccentricity. |
|
Returns the semimajor axis of the orbit from the semiparameter and eccentricity. |
Orbit State Conversions
Transfer position and velocity vectors to classical orbital elements. |
|
Transfer classical orbital elements to position and velocity vectors. |
|
Returns the inclination of a two-body orbit. |
|
Returns the true anomaly of a two-body orbit. |
|
Returns the right ascension of the ascending node of a two-body orbit. |
|
Returns the argument of periapsis of a two-body orbit. |