Near-Infrared Spectra of Pyroxene- and Olivine-rich Asteroids

Details Near-Infrared Spectra of Pyroxene- and Olivine-rich Asteroids Near-Infrared Spectra of Pyroxene- and Olivine-rich Asteroids

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1777b&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1777

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To try to mineralogically characterize small (diameters<20 km)
asteroids, we have instituted a near-infrared (0.9 to 1.65 microns)
observational program called SMASSIR. We have focused on bodies with
visible spectra indicating pyroxene- or olivine-rich surface
assemblages.

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