Gravitational bending of light by planetary multipoles
| dc.creator | Kopeikin, Sergei | |
| dc.creator | Makarov, Valeri | |
| dc.date | 2007-12-04 | |
| dc.date.accessioned | 2026-07-07T08:47:08Z | |
| dc.date.available | 2026-07-07T08:47:08Z | |
| dc.description | 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. | |
| dc.description | 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) | |
| dc.identifier | https://arxiv.org/abs/0712.0417 | |
| dc.identifier | http://arxiv.org/abs/0712.0417 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/143493 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Gravitational bending of light by planetary multipoles | |
| dc.type | text |