A method solving Kepler's equation without transcendental function evaluations

Celestial Mechanics and Dynamical Astronomy

Volumn 66, Issue 3, 1996, Pages 309-319

  Fukushima, Toshio ^a  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

Kepler's equation; Newton Raphson method; Orbital motion

Indexed keywords

EID: 0041585960     PISSN: 09232958     EISSN: None     Source Type: Journal    
DOI: 10.1007/bf00049384     Document Type: Article

References (4)

1. Danby, J. M. A.: 1988, Fundamentals of Celestial Mechanics, 2nd ed., MacMillan, New York, NY.
2. Markley, F. L.: 1996, Kepler Equation Solver, Celest. Mech. and Dynam. Astronomy 63, 101-111.
3. Nijenhuis, A.: 1991, Solving Kepler's Equation with High Efficiency and Accuracy, Celest. Mech. 51, 319-330.
4. Odell, A. W. and Gooding, R. H.: 1986, Procedures for Solving Kepler's Equation, Celest. Mech. 38, 307-334.