Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-14T19:13:38.728Z Has data issue: false hasContentIssue false
  • English
  • Français

Determination of Precession and Nutation from Lunar Laser Ranging Analysis

Published online by Cambridge University Press:  30 March 2016

J.G. Williams ,
X.X. Newhall  and
J. O. Dickey
J.G. Williams
Affiliation:
Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena CA 91109, USA
X.X. Newhall
Affiliation:
Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena CA 91109, USA
J. O. Dickey
Affiliation:
Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena CA 91109, USA

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.

From the analysis of 24 yr of lunar laser ranges, the correction to the IAU luni-solar precession constant is found to be −3.2 ± 0.3 mas/yr for a total value of 50.3846˝/yr at J2000. The size of the 18.6 yr nutation of the pole needs to be increased by about 2 mas over the 1980 IAU theory.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 10: Highlights of Astronomy. As presented at the XXIInd General Assembly of the IAU, 1994 , 1995 , pp. 214 - 217
Copyright
Copyright © Kluwer 1995

References

Dickey, J.O. et al. (1994), Science, Vol. 265, pp. 482–490.CrossRefGoogle Scholar
Folkner, W.M., Chariot, P., Finger, M.H., Newhall, X.X., Williams, J.G., Sovers, O.J., and Standish, E.M. (1994), Astron. Astrophys., Vol. 287, pp. 279–289.Google Scholar
Gross, R.S. (1994), to appear in IERS Technical Notes.Google Scholar
Herring, T.A. (1991), in Proceedings of the 127th Colloquium of the International Astronomical Union, Reference Systems, eds. Hughes, J.A., Smith, C.A., and Kaplan, G.H. (U. S. Naval Obs., Washington), pp. 157–166.Google Scholar
Kinoshita, H., and Souchay, J. (1990), Celes. Mech. and Dyn. Astron., Vol. 48, pp. 187–265.CrossRefGoogle Scholar
Laskar, J. (1986), Astron. Astrophys., Vol. 157, pp. 59–70.Google Scholar
Lieske, J.H., Lederle, T., Fricke, W., and Morando, B. (1977), Astron. Astrophys., Vol. 58, pp. 1–16.Google Scholar
Seidelmann, P.K. (1982), Celestial Mech., Vol. 27, pp. 79–106.CrossRefGoogle Scholar
Simon, J.L., Bretagnon, P., Chapront, J., Chapront-Touzé, M., Francou, G., and Laskar, J. (1994), Astron. Astrophys., Vol. 282, pp. 663–683.Google Scholar
Williams, J.G. (1994), Astron. J., Vol. 108, pp. 711–724.CrossRefGoogle Scholar
Williams, J.G., Newhall, X.X., and Dickey, J.O. (1991), Astron. Astrophys., Vol. 241, pp. L9–L12.Google Scholar
Williams, J.G., Newhall, X.X., and Dickey, J.O. (1993), in Contributions of Space Geodesy to Geodynamics: Earth Dynamics, American Geophysical Union Geodynamics Series, Vol. 24, eds. Smith, D.E. and Turcotte, D.L., Washington, D. C., pp. 83–88.Google Scholar