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NASA NTRS ยท 19950021346

Kepler Equation solver

Abstract

Kepler's Equation is solved over the entire range of elliptic motion by a fifth-order refinement of the solution of a cubic equation. This method is not iterative, and requires only four transcendental function evaluations: a square root, a cube root, and two trigonometric functions. The maximum relative error of the algorithm is less than one part in 10(exp 18), exceeding the capability of double-precision computer arithmetic. Roundoff errors in double-precision implementation of the algorithm are addressed, and procedures to avoid them are developed.

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BibTeXRIS

Markley, F. Landis. 1995-05-01. Kepler Equation solver. https://ntrs.nasa.gov/citations/19950021346

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