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Probing general relativity with radar astrometry in the inner solar system

Published online by Cambridge University Press:  06 January 2010

Jean-Luc Margot  and
Jon D. Giorgini
Jean-Luc Margot
Affiliation:
University of California, Los Angeles, 595 Charles Young Drive East, Los Angeles, CA 90095, USA email: jlm@ess.ucla.edu
Jon D. Giorgini
Affiliation:
Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA email: jdg@tycho.jpl.nasa.gov
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Abstract

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We describe a long-term program designed to obtain and interpret high-precision radar range measurements of a number of near-Earth objects (NEOs) that have trajectories reaching deep inside the gravitational well of the Sun. Objects in our sample have perihelion shift rates 1.5 to 2.5 times that of (1566) Icarus (10″/cy) and span a wide range of inclinations and semi-major axes, allowing for an unambiguous separation of general relativistic and solar oblateness effects. Four objects have been observed at Arecibo on at least two apparitions since 2000, with typical uncertainties of a few hundred meters. Within the next three years, we anticipate securing a total of 15 observations of 5 different NEOs. This program is expected to provide a purely dynamical measurement of the oblateness of the Sun (J2 at the 10−8 level) and to constrain the Eddington parameter β at the 10−4 level. Although our objects are selected to minimize Yarkovsky orbital drift, we also anticipate measuring Yarkovsky drift rates, which are orthogonal to the GR and J2 signatures.

Keywords

general relativitysolar quadrupole momentYarkovsky driftasteroidsradar
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S261: Relativity in Fundamental Astronomy: Dynamics, Reference Frames, and Data Analysis , April 2009 , pp. 183 - 188
Copyright
Copyright © International Astronomical Union 2010

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