Images of Asteroid 21 Lutetia: A Remnant Planetesimal from the Early Solar System - Archive ouverte HAL
Article Dans Une Revue Science Année : 2011

Images of Asteroid 21 Lutetia: A Remnant Planetesimal from the Early Solar System

Jean-Loup Bertaux
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B. Carry
Pedro J. Gutiérrez
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Wing-Huen Ip
Laurent Jorda
Michael Küppers
Nicolas Thomas
P. Vernazza

Résumé

Images obtained by the Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) cameras onboard the Rosetta spacecraft reveal that asteroid 21 Lutetia has a complex geology and one of the highest asteroid densities measured so far, 3.4 ± 0.3 grams per cubic centimeter. The north pole region is covered by a thick layer of regolith, which is seen to flow in major landslides associated with albedo variation. Its geologically complex surface, ancient surface age, and high density suggest that Lutetia is most likely a primordial planetesimal. This contrasts with smaller asteroids visited by previous spacecraft, which are probably shattered bodies, fragments of larger parents, or reaccumulated rubble piles.
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Dates et versions

hal-00641442 , version 1 (15-11-2011)

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Citer

Holger Sierks, Philippe Lamy, Cesare Barbieri, Detlef Koschny, Hans Rickman, et al.. Images of Asteroid 21 Lutetia: A Remnant Planetesimal from the Early Solar System. Science, 2011, 334 (6055), pp.487-490. ⟨10.1126/science.1207325⟩. ⟨hal-00641442⟩
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