Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-28T17:24:52.955Z Has data issue: false hasContentIssue false
  • English
  • Français

Relativistic rotational effects: application to the Earth-Moon system

Published online by Cambridge University Press:  25 May 2016

David Vokrouhlický
David Vokrouhlický*
Affiliation:
Observatoire de la Côte d'Azur, Dept. CERGA, Av N. Copernic, 06130 Grasse, France1

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.

Relativistic spin effects involved in the Earth-Moon dynamics are reviewed. They enclose: (i) the coordinate system effects, and (ii) the relativistic physical librations. The geodetic precession is the only relativistic spin phenomenon which has been firmly detected so far. The best candidates of the effects which might be detected in the forthcoming period are the lunar physical librations and coordinate nutations. As for the latter, however, a fine cancellation between the geodetic and the Lense-Thirring coordinate effects results in decreasing their amplitude just below the possibility of the Lunar Laser Ranging technology.

Type
Part VIII - General Relativity. Physics
Information
Symposium - International Astronomical Union , Volume 172: Dynamics, Ephemerides and Astrometry of the Solar System , 1996 , pp. 321 - 324
Copyright
Copyright © Kluwer 1996 

References

Bizouard, C., Schastok, J., Soffel, M. and Souchay, J. (1992) Etude de la rotation de la Terre dans la cadre de la relativite generale: Premier approche, in: Journee 1992: Systemes de reference spatio-temporels ed. Capitaine, N., Paris Observatory, pp. 76–84.Google Scholar
Bois, E. and Vokrouhlický, D. (1995) The relativistic spin effects in the Earth-Moon system, Astron. Astrophys., 300, p. 559.Google Scholar
Brumberg, V.A., Bretagnon, P. and Francou, G. (1991) Analytical algorithms of relativistic reduction of astronomical observations, in: Journee 1991: Systemes de reference spatio-temporels ed. Capitaine, N., Paris Observatory, pp. 141–148.Google Scholar
Damour, T. (1987) chapter 6 of 300 years of gravitation , eds. Hawking, S.W. and Israel, W., Cambridge Univ. Press, Cambridge, pp. 128–198.Google Scholar
Damour, T. and Vokrouhlický, D. (1995), The equivalence principle and the Moon, Phys. Rev. D, in press.Google Scholar
Damour, T., Soffel, M. and Xu, C. (1991) Phys. Rev. D, 43, p. 3273; (1992) Phys. Rev. D, 45, p. 1017; (1993) Phys. Rev. D, 47, p. 1017; (1994) Phys. Rev. D, 49, p. 618; see also Damour, T. and Vokrouhlický, D. (1995) Phys. Rev. D, 52, p. 4455.Google Scholar
Dickey, J.O. et al., Science, 265, p. 482.Google Scholar
Fukushima, T. (1991) Astron. Astrophys., 244, p. L11.Google Scholar
Sitter, W. de (1916) Mon. Not. R. astr. Soc., 76, p. 699; (1916) Mon. Not. R. astr. Soc., 77, p. 155.Google Scholar
Vokrouhlický, D. (1995) The relativistic spin effects in the Earth-Moon system, Phys. Rev. D, in press.Google Scholar
Williams, J.G., Newhall, X.X. and Dickey, J.O. (1995) Relativity parameters determined from Lunar Laser Ranging, Phys. Rev. D, in press.Google Scholar