Geochemistry, Mineralogy and Diagenesis of the Burns Formation at Meridiani Planum: Insights into the Sedimentary Rock Cycle on Mars

Details Geochemistry, Mineralogy and Diagenesis of the Burns Formation at Meridiani Planum: Insights into the Sedimentary Rock Cycle on Mars Geochemistry, Mineralogy and Diagenesis of the Burns Formation at Meridiani Planum: Insights into the Sedimentary Rock Cycle on Mars

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3231m&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3231

Physics

Scientific paper

The Burns formation consists of sulfate-rich sandstones that experienced
an extended history of groundwater diagenesis. Sulfates appear common on
Mars and provide insight into a martian sedimentary rock cycle strongly
influenced by the sulfur cycle.

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