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Title:ASTEROIDAL OCCULTATION OF REGULUS: DIFFERENTIAL EFFECT OF LIGHT BENDING
DOI No:10.1142/9789812834300_0469
Source:THE ELEVENTH MARCEL GROSSMANN MEETING
On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories
(pp 2594-2596)
Author(s):COSTANTINO SIGISMONDI
http://www.icra.it/solar ICRA, Piazzale Aldo Moro, 5 00185 Rome, Italy

University of Rome La Sapienza, Piazzale Aldo Moro, 5 00185 Rome, Italy

DAVIDE TROISE
http://www.icra.it/solar ICRA, Piazzale Aldo Moro, 5 00185 Rome, Italy

University of Rome La Sapienza, Piazzale Aldo Moro, 5 00185 Rome, Italy

Abstract:Asteroid 166 Rhodope moved at 14.4 milliarcsec/s during the occultation of Regulus of October 19, 2005. We made a 25 Hz frame rate video (resolution 0.6 mas per frame) near centerline in Vibo Valentia, Italy. Stellar and asteroidal diameters and relativistic light bending by solar field are outlined. The 0.16 mas differential effect of light bending (star-asteroid) is recovered fitting 7 observations with asteroid spherical model.
Keywords:Occultations; Fresnel diffraction; Gravitational light bending; Stellar diameter
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