Mercury's Perihelion Advance: Determination by Radar

Irwin I. Shapiro, Gordon H. Pettengill, Michael E. Ash, Richard P. Ingalls, D. B. Campbell, and R. B. Dyce
Phys. Rev. Lett. 28, 1594 – Published 12 June 1972
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Abstract

Measurements of echo delays of radar signals transmitted from Earth to Mercury have yielded an accurate value for the advance of the latter's perihelion position. Given that the Sun's gravitational quadrupole moment is negligible, the result in terms of the Eddington-Robertson parameters is (2+2γβ)31.005±0.007, where γ=β=1 in general relativity, and where 0.007 represents the statistical standard error. Inclusion of the probable contribution of systematic errors raises the uncertainty to about 0.02.

  • Received 10 April 1972

DOI:https://doi.org/10.1103/PhysRevLett.28.1594

©1972 American Physical Society

Authors & Affiliations

Irwin I. Shapiro*,† and Gordon H. Pettengill*

  • Massachusetts Institute of Technology, Cambridge, Massachusetts 02139

Michael E. Ash

  • Massachusetts Institute of Technology Lincoln Laboratory Lexington, Massachusetts 02173

Richard P. Ingalls

  • Haystack Observatory, Northeast Radio Observatory Corporation, Westford, Massachusetts 01886

D. B. Campbell and R. B. Dyce

  • National Astronomy and Ionosphere Center, Arecibo, Puerto Rico 00612

  • *Department of Earth and Planetary Sciences.
  • Department of Physics.
  • Operated with support from the Department of the U. S. Air Force.

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Vol. 28, Iss. 24 — 12 June 1972

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