Diogenite-like Features in the Spitzer IRS (5-35 µm) Spectrum of 956 Elisa

Details Diogenite-like Features in the Spitzer IRS (5-35 µm) Spectrum of 956 Elisa Diogenite-like Features in the Spitzer IRS (5-35 µm) Spectrum of 956 Elisa

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.2204l&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

2

Scientific paper

We report preliminary results from the Spitzer IRS (Infrared
Spectrograph) observations of the V-type asteroid 956 Elisa. Several
features of this spectrum suggest the presence of diogenitic material at
a relatively coarse particle size.

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