Test of General Relativity and Measurement of the Lense-Thirring Effect with Two Earth Satellites
Ignazio Ciufolini,
Erricos Pavlis,
Federico Chieppa,
Eduardo Fernandes-Vieira,
Juan Pérez-Mercader
The Lense-Thirring effect, a tiny perturbation of the orbit of a
particle caused by the spin of the attracting body, was accurately measured with the use of the data of two laser-ranged satellites, LAGEOS and LAGEOS II, and the Earth gravitational model EGM-96. The
parameter µ, which measures the strength of the Lense-Thirring effect, was found to be 1.1 ± 0.2; general relativity predicts µ
1. This result represents an accurate test and measurement of
one of the fundamental predictions of general relativity, that the spin
of a body changes the geometry of the universe by generating space-time
curvature.
I. Ciufolini, Istituto Fisica Spazio Interplanetario-Consiglio
Nazionale delle Ricerche, and Dipartimento Aerospaziale,
Universitá di Roma "La Sapienza," via Eudossiana 16, 00184 Rome, Italy.
E. Pavlis, Joint Center for Earth System Technology, University of
Maryland-Baltimore County, Baltimore, MD 21250, USA.
F. Chieppa, Scuola Ingegneria Aerospaziale, Universitá di Roma
"La Sapienza," Rome, Italy.
E. Fernandes-Vieira and J. Pérez-Mercader, Laboratorio de
Astrofisica Espacial y Fisica Fundamental (INTA-CSIC), Madrid, Spain.