On solving Kepler's equation for nearly rectilinear hyperbolic orbits

DOI10.1023/A:1015283119522zbMath1085.70004OpenAlexW2069226939MaRDI QIDQ1610305

Richard A. Serafin

Publication date: 19 August 2002

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1023/a:1015283119522

zbMATH Keywords

Newton's methodquadratic convergencemethod of successive approximationstellar passages

Mathematics Subject Classification ID

Computational methods for problems pertaining to mechanics of particles and systems (70-08) Numerical computation of solutions to single equations (65H05) Two-body problems (70F05) Galactic and stellar dynamics (85A05)

Related Items (1)

Methods for the Study of the Dynamics of the Oort Cloud Comets I: Modelling the Stellar Perturbations

This page was built for publication: On solving Kepler's equation for nearly rectilinear hyperbolic orbits