A Likely Formation Mechanism of the Hematite-rich Spherules in the Equatorial Region of Western Mars

Details A Likely Formation Mechanism of the Hematite-rich Spherules in the Equatorial Region of Western Mars A Likely Formation Mechanism of the Hematite-rich Spherules in the Equatorial Region of Western Mars

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1470f&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

We argue that the hematite-rich spherules were originally formed in
Valles Marineris and transported to Meridiani Planum accompanied with
accretion of finer volcanic materials, abrasion of basaltic fragments
and break down of the spherules during the wash-out flows.

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