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    Radio Interferometric Test of the General Relativistic Light Bending Near the Sun

    D. O. Muhleman, R. D. Ekers, and E. B. Fomalont

    • Owens Valley Radio Observatory, California Institute of Technology, Pasadena, California 91109

    Phys. Rev. Lett. 24, 1377 – Published 15 June, 1970

    DOI: https://doi.org/10.1103/PhysRevLett.24.1377

    Abstract

    We have used radio interferometry to measure the deflection of a radio source as it passed the sun. This deflection is a separable combination of refraction in the coronal electron plasma and the general relativistic effect. The observed deflection was 1.04−0.10+0.15 times that predicted by Einstein's theory of general relativity. The observation also yielded a reasonable value for the coronal electron density.

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