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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）

Cited 20|Views36
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Abstract
•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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Key words
Asteroids,Composition,Satellites of asteroids,Photometry,Spectroscopy
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