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Gravitational bending of light by planetary multipoles

2007/12/04 by Sergei M. Kopeikin, Sergei Kopeikin, В. В. Макаров +3 · 1 citation
Physics and Astronomy · #Astro and Planetary Science #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Historical Astronomy and Related Studies #Planetary Science and Exploration #gr-qc

paper · pdf · doi:10.48550/arxiv.0712.0417

4 pages, contributed talk submitted to the proceedings of the IAU 248 Symp. "A Giant Step: from Milli- to Micro-arcsecond Astrometry" (Shanghai, October 2007)

arxiv created 2007/12/04 · openalex publication_date 2007/12/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

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 in the approximation of the linearized Einstein equations. All terms of order 1 microarcsecond are taken into account, parametrized, and classified in accordance with their physical origin. We discuss the observational capabilities of the near-future optical and radio interferometers for detecting the Doppler modulation of the radial deflection, and the dipolar and quadrupolar light-ray bendings by Jupiter and the Saturn.

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