Gravitational bending of light by planetary multipoles and its measurement with microarcsecond astronomical interferometers

Abstract

General relativistic deflection of light by mass, dipole, and quadrupole moments of gravitational field of a moving massive planet in the Solar system is derived. All terms of order 1 microarcsecond are taken into account, parametrized, and classified in accordance with their physical origin. We calculate the instantaneous patterns of the light-ray deflections caused by the monopole, the dipole and the quadrupole moments, and derive equations describing apparent motion of the deflected position of the star in the sky plane as the impact parameter of the light ray with respect to the planet changes due to its orbital motion. The present paper gives the physical interpretation of the observed light-ray deflections and discusses the observational capabilities of the near-future optical (SIM) and radio (SKA) interferometers for detecting the Doppler modulation of the radial deflection, and the dipolar and quadrupolar light-ray bendings by the Jupiter and the Saturn.

33 pages, 10 figures, accepted to Phys. Rev. D

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Cited by in corpus (4)

• Time-delay and Doppler tests of the Lorentz symmetry of gravity
• Time-Varying Gravitomagnetism
• Relativistic gravitational deflection of light and its impact on the modeling accuracy for the Space Interferometry Mission
• Constraining the parameters of binary systems through time-dependent light deflection