Martian Dust as an End-Member of Semi-Cosmic Weathering

Details Martian Dust as an End-Member of Semi-Cosmic Weathering Martian Dust as an End-Member of Semi-Cosmic Weathering

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.2020m&link_type=abstract

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

Computer Science

Scientific paper

The martian dust is a compound close to terrestrial amorphous
spinel’s minerals such as Hercynite, spinel ferrites. The
semi-cosmic weathering affects the mineral surface by both ways:
reduction (in the top layer) and oxidation (in the deeper layer).

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