Results from a Mössbauer and VNIR Study of Dust Generated from Olivine Basalt: Application to Mars

Details Results from a Mössbauer and VNIR Study of Dust Generated from Olivine Basalt: Application to Mars Results from a Mössbauer and VNIR Study of Dust Generated from Olivine Basalt: Application to Mars

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1622m&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

Scientific paper

It is shown that VNIR spectroscopy can greatly underestimate the ratio
of olivine to pyroxene and olivine may be more abundant on Mars than
hitherto believed. The possibilities of using electrodes to collect
samples on Mars are discussed.

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