Biology
Scientific paper
Oct 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009georl..3619201b&link_type=abstract
Geophysical Research Letters, Volume 36, Issue 19, CiteID L19201
Biology
11
Geochemistry: Planetary Geochemistry (5405, 5410, 5704, 5709, 6005, 6008), Mineralogy And Petrology: Planetary Mineralogy And Petrology (5410), Planetary Sciences: Astrobiology: Hydrothermal Systems And Weathering On Other Planets, Planetary Sciences: Solid Surface Planets: Composition (1060, 3672), Geochemistry: Sedimentary Geochemistry
Scientific paper
Studies of the origin of the Martian sulfate and phyllosilicate deposits have led to the hypothesis that there was a marked, global-scale change in the Mars environment from circum-neutral pH aqueous alteration in the Noachian to an acidic evaporitic system in the late Noachian to Hesperian. However, terrestrial studies suggest that two different geochemical systems need not be invoked to explain such geochemical variation. Western Australian acidic playa lakes have large pH differences separated vertically and laterally by only a few tens of meters, demonstrating how highly variable chemistries can coexist over short distances in natural environments. We suggest diverse and variable Martian aqueous environments where the coetaneous formation of phyllosilicates and sulfates at the Australian sites are analogs for regions where phyllosilicates and sulfates coexist on Mars. In these systems, Fe and alkali earth phyllosilicates represent deep facies associated with upwelling neutral to alkaline groundwater, whereas aluminous phyllosilicates and sulfates represent near-surface evaporitic facies formed from more acidic brines.
Baldridge Alice M.
Bridges Nathan T.
Brown Justin A.
Crowley James K.
de Souza Filho Carlos Roberto
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