Hints on Lutetia's surface composition

Details Hints on Lutetia's surface composition Hints on Lutetia's surface composition

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1772b&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1772

Computer Science

Scientific paper

All the information available from space missions (Rosetta and Herschel) and ground observations has been put together to interpret the Lutetia's surface composition. During the close encounter with (21) Lutetia on July 10, 2010, the instruments OSIRIS, VIRTIS, ALICE, and MIRO were turned on to characterize the surface properties of the asteroid and they provided important inputs to reach this goal. We present a complete overview on the data obtained by Rosetta (Sierks et al, 2011, Coradini et al. 2011) and those from ground observations collected during more than 30 years with many different techniques (Barucci & Fulchignoni 2009), which give constrains to the surface composition of Lutetia.

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