pint.orbital.kepler
Functions for working with Keplerian orbits
All times are in days, distances in light-seconds, and masses in solar masses.
Functions
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Attempt to convert parameters from ELL1 to BTX. |
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Compute the eccentric anomaly from the mean anomaly. |
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Compute the Keplerian parameters for the osculating orbit. |
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Inverse Kepler one-body calculation. |
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Position and velocity of a particle in a Kepler orbit. |
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One-body Kepler problem in 3D. |
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Set up two bodies in a Keplerian orbit |
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Compute the mass of a particle in a Kepler orbit. |
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Compute the mass of a particle in a Kepler orbit, with partials. |
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Compute the true anomaly from the eccentric anomaly. |
Classes
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Parameters to describe a one-object 2D Keplerian orbit. |
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Parameters to describe a one-object 3D Keplerian orbit. |
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Parameters to describe a one-object 3D Keplerian orbit. |