Hostname: page-component-78c5997874-ndw9j Total loading time: 0 Render date: 2024-11-02T18:51:04.572Z Has data issue: false hasContentIssue false
  • English
  • Français

Relativistic equations of motion of celestial bodies

Published online by Cambridge University Press:  25 May 2016

Michael H. Soffel
Michael H. Soffel*
Affiliation:
Lohrmann Observatory, TU Dresden Mommsenstr. 13, 01062 Dresden e-mail: [email protected]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The problem of relativistic equations of motion for extended celestial bodies in the first post-Newtonian approximation is reviewed. It is argued that the problems dealing with kinematical aspects have been solved in a satisfactory way, but more work has to be done on the dynamical side. Concepts like angular velocity, moments of inertia, Tisserand axes etc. still have to be introduced in a rigorous manner at the 1PN level.

Type
Part VIII - General Relativity. Physics
Information
Symposium - International Astronomical Union , Volume 172: Dynamics, Ephemerides and Astrometry of the Solar System , 1996 , pp. 303 - 308
Copyright
Copyright © Kluwer 1996 

References

Brumberg, V.A.: 1991, Essential Relativistic Celestial Mechanics, Hilger.Google Scholar
Damour, T., Soffel, M. and Xu, C.: 1991–94 Phys. Rev. D 43, 3273 (1991) 45, 1017 (1992); 47, 3124 (1993); 49, 618 (1994). called DSX I - IV in the text.Google Scholar
Klioner, S.: 1996, these proceedings.Google Scholar
Thorne, K. and Gürsel, Y.: 1983 Mon. Not. Roy. Ast. Soc. 205, 809 Google Scholar