Hostname: page-component-848d4c4894-jbqgn Total loading time: 0 Render date: 2024-06-26T06:49:13.189Z Has data issue: false hasContentIssue false
  • English
  • Français

Results from Lunar Laser Ranging Data Analysis

Published online by Cambridge University Press:  12 April 2016

J. O. Dickey ,
J. G. Williams  and
C. F. Yoder
J. O. Dickey
Affiliation:
Jet Propulsion Laboratory California Institute of Technology Pasadena, CA 91109 USA
J. G. Williams
Affiliation:
Jet Propulsion Laboratory California Institute of Technology Pasadena, CA 91109 USA
C. F. Yoder
Affiliation:
Jet Propulsion Laboratory California Institute of Technology Pasadena, 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.

The lunar laser range data taken at McDonald Observatory between August 1969 and May 1980 has been analyzed. The simple rms residual for the 2954 ranges is 31 cm. Results of the analysis include GMearth = 398600.45±0.02 km3/sec2 and a secular acceleration of the lunar orbital mean longitude of ṅ = −23.8±1.5“/century2 which yields a Q of 12.3 at semidiurnal frequencies. The lunar harmonic C30 is (−8.7 ± 1.1) × 10−6 and the lunar rotational dissipation k2mT = (4.7 ± 0.5) × 10−3 day. Also resulting from the solution are geocentric coordinates of McDonald accurate to 30 cm, including the first value for the longitude with the new IAU constants and a dynamical equinox.

Type
Part III
Information
International Astronomical Union Colloquium , Volume 63: High-Precision Earth Rotation and Earth-Moon Dynamics , May 1981 , pp. 209 - 216
Copyright
Copyright © Reidel 1982

References

Cappallo, R.J., Counselman, C.C. III, King, R.W., and Shapiro, I.I.: 1981, “The Tidal Dissipation in the Moon,” Submitted to J. Geophvs. Res.. CrossRefGoogle Scholar
Dickey, J. O., Fliegel, H.F., Williams, J.G.: 1981, “Comparison of Polar Motion Results Using Lunar Laser Ranging,” this volume, 125–137.Google Scholar
Esposito, , Pasquale, B.: 1979, private communication and Report of Special Study Group No. 5.39 of International Association of Geodesy, Fundamental Geodetic Constants XVII General Assembly of International union of Geodesy and Geophysics.Google Scholar
Ferrari, A.J., Sinclair, W. S., Sjogren, W.L., Williams, J.G., and Yoder, C.F.: 1981, J. Geophys. Res., 85, 3939–3951.Google Scholar
Fliegel, H.F., Dickey, J. O., and Williams, J.G.: 1982, “Intercomparison of Lunar Laser and Traditional Determinations of Earth Rotation,” this volume, 53-88.CrossRefGoogle Scholar
Fricke, W.: 1981, Astron. Astrophvs., in press.Google Scholar
King, R.W.: 1979, cited by Esposito, P. B. as a private communication in the above reference.Google Scholar
Lieske, J.H., Lederle, T., Fricke, W., and Morando, W.: 1977, Astron. Astrophvs. 55, 1.Google Scholar
Lieske, J.H.: 1979, Astron. Astrophvs. 73, 282.Google Scholar
Seidelmann, P.K., Abalakin, V.K., Kinoshita, H., Kovalevsky, J., Murray, C.A., Smith, M.L., Vicente, R. O., Williams, J.G., and Yatskiv, Ya. S.: 1982, Celestial Mechanics, in press.Google Scholar
Smith, David E.: 1981, “Further Estimations of GM and Inter-continental Baselines from the Tracking of LAGEOS,” Third Annual NASA Geodynamics Program Review, 62.Google Scholar
Williams, J.G., Sinclair, W.S., and Yoder, C.F.: 1978, Geophys. Res. Lett., 5, 943–946.CrossRefGoogle Scholar
Williams, J.G., Melbourne, W.G.: 1982, this volume, 293–303.Google Scholar
Yoder, , Charles, F.: 1981, “The Free Librations of a Dissipative Moon,” Philosophical Transactions of the Royal Sooiety, in press.Google Scholar