Ni, S, and Cl in EETA79001 Lithology C

Details Ni, S, and Cl in EETA79001 Lithology C Ni, S, and Cl in EETA79001 Lithology C

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2814s&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2814

Computer Science

Scientific paper

We investigate EETA79001 impact melt using S, Ni, and Cl — all
strong indicator elements of martian soil. If soil is a contributor to
Lithology C’s S budget it should also contribute Ni and Cl. Our
work suggests no soil component is necessary to explain the Lithologu C
composition.

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