dc.contributor.author | Kopeikin, Sergei M. | eng |
dc.contributor.author | Makarov, Valeri V. | eng |
dc.date.issued | 2007 | eng |
dc.description.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. | eng |
dc.identifier.citation | arXiv:0712.0417v1 | eng |
dc.identifier.uri | http://hdl.handle.net/10355/6898 | eng |
dc.language | English | eng |
dc.publisher | arXiv | eng |
dc.relation.ispartofcollection | University of Missouri--Columbia. College of Arts and Sciences. Department of Physics and Astronomy. Physics and Astronomy publications | eng |
dc.source.uri | http://arxiv.org/PS_cache/arxiv/pdf/0712/0712.0417v1.pdf | eng |
dc.subject | gravitational lensing | eng |
dc.subject | astrometry | eng |
dc.subject | reference systems | eng |
dc.subject.lcsh | Gravitation | eng |
dc.subject.lcsh | Gravitational lenses | eng |
dc.subject.lcsh | Gravitational waves | eng |
dc.subject.lcsh | Relativity (Physics) | eng |
dc.title | Gravitational bending of light by planetary multipoles and its measurement with microarcsecond astronomical interferometers | eng |
dc.type | Article | eng |