kepler
library
Functions
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kepler1(double e, double m, {int places = 8})
→ double
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Solves Kepler's equation by simple iteration.
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kepler2(double e, double m, {int places = 8})
→ double
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Solves Kepler's equation by Newton-like iteration.
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kepler2a(double e, double m, {int places = 8})
→ double
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Kepler2 with Leingärtner limiting to avoid divergence.
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kepler2b(double e, double m, {int places = 8})
→ double
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Kepler2 with Steele limiting to avoid divergence.
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kepler3(double e, double m)
→ double
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Solves Kepler's equation by binary search (53 iterations).
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kepler4(double e, double m)
→ double
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Approximate solution valid only for small eccentricity.
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radius(double eAnom, double e, double a)
→ double
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Radius distance from eccentric anomaly
eAnom, eccentricity e,
and semimajor axis a.
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trueAnomaly(double eAnom, double e)
→ double
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True anomaly ν from eccentric anomaly
e_anom and eccentricity e.
