New test of general relativity: Measurement of de Sitter geodetic precession rate for lunar perigee

Bruno Bertotti, Ignazio Ciufolini, and Peter L. Bender
Phys. Rev. Lett. 58, 1062 – Published 16 March 1987
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Abstract

According to general relativity, the calculated rate of motion of lunar perigee should include a contribution of 19.2 msec/yr from geodetic precession. We show that existing analyses of lunarlaser-ranging data confirm the general-relativistic rate for geodetic precession with respect to the planetary dynamical frame. In addition, the comparison of Earth-rotation results from lunar laser ranging and from very-long-baseline interferometry (VLBI) shows that the relative drift of the planetary dynamical frame and the extragalactic VLBI reference frame is small. The estimated accuracy is about 10%.

  • Received 12 January 1987

DOI:https://doi.org/10.1103/PhysRevLett.58.1062

©1987 American Physical Society

Authors & Affiliations

Bruno Bertotti

  • Institute of Astronomy, University of Cambridge, Cambridge, United Kingdom

Ignazio Ciufolini

  • Center for Space Research, University of Texas at Austin, Austin, Texas 78712

Peter L. Bender

  • Joint Institute for Laboratory Astrophysics, University of Colorado and National Bureau of Standards, Boulder, Colorado 80309

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Vol. 58, Iss. 11 — 16 March 1987

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