Possible Explanations for the 506 nm Feature in Telescopic Spectra of Vesta, Vestoids, and HED Meteorites

Details Possible Explanations for the 506 nm Feature in Telescopic Spectra of Vesta, Vestoids, and HED Meteorites Possible Explanations for the 506 nm Feature in Telescopic Spectra of Vesta, Vestoids, and HED Meteorites

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2174k&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2174

Computer Science

Scientific paper

On the basis of new high-resolution laboratory reflectance spectra,
variations in the wavelength position of the 506 nm feature seen in
reflectance spectra of Vesta, vestoids, and HED meteorites may be due to
variations in plagioclase feldspar abundances rather than changes in
pyroxene composition.

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