Procedures for Solving Kepler's Equation

Details Procedures for Solving Kepler's Equation Procedures for Solving Kepler's Equation

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986cemec..38..307o&link_type=abstract

Celestial Mechanics, Volume 38, Issue 4, pp.307-334

Computer Science

20

Scientific paper

The authors review starting formulae and iteration processes for the solution of Kepler's equation, and give details of two complete procedures. The first has been in use for a number of years, but the second is entirely new. The new procedure operates with an iterative process that always gives fourth-order convergence and is taken to only two iterations. The error in the resulting solution then never exceeds 7×10-15rad.

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