Mineralogical Composition of (25143) Itokawa 1998 SF36 from Visible and Near-Infrared Reflectance Spectroscopy: Evidence for Partial Melting

Details Mineralogical Composition of (25143) Itokawa 1998 SF36 from Visible and Near-Infrared Reflectance Spectroscopy: Evidence for Partial Melting Mineralogical Composition of (25143) Itokawa 1998 SF36 from Visible and Near-Infrared Reflectance Spectroscopy: Evidence for Partial Melting

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1513a&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1513

Physics

Scientific paper

Spectral reflectance ground-based observations of (25143) Itokawa were
obtained to support the Japanese Hayabusa mission. Detailed analyses of
the spectra indicate that this object is likely a primitive achondrite
with a 70:30 olivine/pyroxene ratio.

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