Abstract: Mixtures of Silica and Disulfide Rocks Can Explain the Coeval Formation of Mineral Sequences on a Cold and Wet Early Mars (2016 AGU Fall Meeting)

Mixtures of Silica and Disulfide Rocks Can Explain the Coeval Formation of Mineral Sequences on a Cold and Wet Early Mars

Alberto G. Fairén^1,2, Eva Mateo³, Luis Gago-Duport⁴, Elisabeth Losa-Adams⁴, Vincent F Chevrier⁵ and Carolina Gil-Lozano⁶, (1)Cornell University, Ithaca, NY, United States, (2)Centro de Astrobiología (CSIC-INTA); and Dept. of Astronomy, Cornell University, Madrid, Spain, (3)Centro de Astrobiología (CAB), INTA-CSIC, Torrejón de Ardoz, Madrid, Spain, (4)Universidad de Vigo, Vigo, Spain, (5)University of Arkansas, Arkansas Center for Space and Planetary Sciences, Fayetteville, United States, (6)Centro de Astrobiologia (CSIC-INTA), Madrid, Spain

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