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Prospects for observations of relativistic effects in the solar system

Published online by Cambridge University Press:  04 August 2017

R. D. Reasenberg  and
I. I. Shapiro
R. D. Reasenberg
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138
I. I. Shapiro
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138

Abstract

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The solar system is the traditional laboratory for testing theories of gravitation. The results of all tests are consistent with the predictions of general relativity. The differences between these predictions and those of Newton's theory of gravitation have been confirmed with uncertainties as small as one part in a thousand. To enhance significantly the accuracy of such tests, one must investigate novel techniques. In this paper we concentrate on an experiment that promises a dramatic improvement in a classical test of general relativity – the deflection of light by solar gravity. The goal is to measure the post-post-Newtonian contribution of nearly 11 microarcseconds to this deflection. The technique we propose is based on use of an astrometric optical interferometer, POINTS, which could be operated from the bay of the Space Shuttle, mounted on the proposed Space Station, or supported by an independent spacecraft. POINTS should be able to measure the separation of stars about 90° apart with an uncertainty of only a few microarcseconds.

Type
Future Observations of Relativity Effects
Information
Symposium - International Astronomical Union , Volume 114: Relativity in Celestial Mechanics and Astrometry , 1986 , pp. 383 - 391
Copyright
Copyright © Reidel 1986 

References

Anderson, J.T., Cabrera, B., Everitt, C.W.F., Leslie, B.C., and Lipa, J.A., ‘Progress on the Relativity Gyroscope Experiment since 1976,’ in Proceedings of the Second Marcel Grossmann Meeting on General Relativity, edited by Ruffini, R., North-Holland, 939–957, 1982.Google Scholar
Epstein, R. and Shapiro, I.I., ‘Post-post-Newtonian Deflection of Light by the Sun,’ Phys. Rev. D, 22, 2947–2949, 1980.CrossRefGoogle Scholar
Fomalont, E. B. and Sramek, R. A., ‘The Deflection of Radio Waves by the Sun,’ Comments on Astrophys., 7, 19, 1977.Google Scholar
Kovalevsky, J., ‘Prospects for Space Stellar Astrometry,’ Sp. Sci. Rev., 39, 1–63. 1984.CrossRefGoogle Scholar
Reasenberg, R.D., Shapiro, I.I., MacNeil, P.E., Goldstein, R.B., Breidenthal, J.C., Brenkle, J.P., Cain, D.L., Kaufman, T.M., Komarek, T.A., and Zygielbaum, A.I., ‘Viking Relativity Experiment: Verification of Signal Retardation by Solar Gravity,’ Astrophys. J., 234, L219–L221, 1979.CrossRefGoogle Scholar
Reasenberg, R.D., ‘Microarcsecond Astrometric Interferometry,’ in Proceedings of the Workshop of High Angular Resolution Optical Interferometry From Space, edited by Boyce, P. B. and Reasenberg, R. D., BAAS , 16, 758–766. 1984.Google Scholar
Reasenberg, R.D., ‘Microarcsecond Astrometric Interferometry,’ in Astrometric Techniques, IAU Symposium 109, edited by Eichhorn, H. and Leacock, R. J., Reidel, Dordrecht, in press, 1986.CrossRefGoogle Scholar
Taylor, J.H. and Weisberg, J.M., ‘Observations of Post-Newtonian Timing Effects in the Binary Pulsar PSR 1913+16,’ Phys. Rev. Lett., 52, 1348–1350, 1984.Google Scholar