Physical, spectral, and dynamical properties of asteroid (107) Camilla and its satellites

Myriam Pajuelo,B. Carry,F. Vachier, M. Marsset,Jerome Berthier,P. Descamps,William Jon Merline,Peter Tamblyn,J. Grice,Al Conrad,Alex Storrs, B. Timerson,D. Dunham,S. Preston,A. Vigan,B. Yang,P. Vernazza, S. Fauvaud,L. Bernasconi, D. Romeuf, R. Behrend,Christophe Dumas,J.D. Drummond,Jean-Luc Margot,P. Kervella,Franck Marchis,J.H. Girard

Icarus（2018）

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摘要

•Exhaustive study of Camilla system with all available data: lightcurves, high angular resolution images, occultations, and spectra.•Orbit of largest satellite (sub-pixel accuracy): circular, equatorial and prograde.•Camilla’s analog material: IDPs.•Camilla’s surface properties and topography supports satellites origin by impact and reaccumulation of material.•Occultation predictions to refine characterization of the system.

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关键词

Asteroids,Composition,Satellites of asteroids,Photometry,Spectroscopy

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