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Present problems in relativistic Celestial Mechanics

Published online by Cambridge University Press:  04 August 2017

V. A. Brumberg*
Affiliation:
Institute for Theoretical Astronomy, 191187 Leningrad, U.S.S.R.

Abstract

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Review of the present problems of relativistic celestial mechanics. Advantage is taken of the method suggested earlier by the author and based on using quasi-Galilean coordinates with arbitrary coordinate functions or parameters. As compared with the previous papers the new elements are post-post-Newtonian approximation for the circular motion in the Schwarzschild problem and reduction of the artificial satellite problem including the main solar perturbations to the Schwarzschild problem. Some current questions of time scales definitions, reference frames and reduction of observations are briefly discussed.

Type
Dynamical Effects in General Relativity
Copyright
Copyright © Reidel 1986 

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