Hostname: page-component-7bb8b95d7b-5mhkq Total loading time: 0 Render date: 2024-09-12T20:20:00.541Z Has data issue: false hasContentIssue false

New relativistic effects in the motion of the Moon

Published online by Cambridge University Press:  04 August 2017

Bahram Mashhoon*
Affiliation:
Institut für Theoretische Physik, Universität zu Köln, D-5000 Cologne 41, Federal Republic of Germany

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.

A summary of the main relativistic effects in the motion of the Moon is presented. The results are based on the application of a novel approach to the restricted three-body problem in general relativity to the lunar motion. It is shown that the rotation of the Sun causes a secular acceleration in the relative Earth-Moon motion. This might appear to be due to a temporal “variation” of the gravitational constant.

Type
Future Observations of Relativity Effects
Copyright
Copyright © Reidel 1986 

References

Baierlein, R.: Phys. Rev. 162, 1275 (1967).Google Scholar
Brumberg, V.A.: Bull. Inst. Theoret. Astron. (USSR), 6, 733 (1958).Google Scholar
de Sitter, W.: Mon. Not. Roy. Astron. Soc. 77, 155 (1916).Google Scholar
Fokker, A.D.: Proc. Roy. Acad. Amsterdam, 23, 729 (1920).Google Scholar
Lestrade, J.-F., Chapront, J., and Chapront-Touzé, M.: in “High-Precision Earth Rotation and Earth-Moon Dynamics”, Calame, O., ed. (Reidel, Dordrecht), p. 217 (1982).Google Scholar
Mashhoon, B.: Astrophys. J. 216, 591 (1977).Google Scholar
Mashhoon, B.: Gen. Rel. Grav. 16, 311 (1984).CrossRefGoogle Scholar
Mashhoon, B.: Found. Phys. 15, 497 (1985).Google Scholar
Mashhoon, B., and Theiss, D.S.: University of Cologne report (1982).Google Scholar
Schiff, L.I.: Phys. Rev. Lett. 4, 215 (1960).Google Scholar
Theiss, D.S.: , University of Cologne (1984).Google Scholar