HR: 1340h
AN: P23A-1096 [Abstracts]
TI: Assessing the Potential for Ancient Habitable Environments in Gusev Crater, Mars
AU: * Des Marais, D J
EM: David.J.DesMarais@nasa.gov
AF: NASA Ames Research Center, Mail Stop 239-4, Moffett Field, CA 94035-1000, United
States
AU: Athena Science Team, T
EM: David.J.DesMarais@nasa.gov
AB:
In order to be habitable for microbial life as we know it, an environment must provide nutrient elements, energy
and liquid water. We assess the potential for habitable environments in the areas explored by the MER rover
Spirit. These areas include the basaltic plains near Columbia Memorial Station, West Spur, Husband Hill, and the
inner basin south of Husband Hill. Little aqueous activity apparently occurred in Gusev crater since the basaltic
plains were emplaced in Hesperian times, therefore the basaltic plains were highly unlikely to have sustained
habitable environments. The Columbia Hills, located ~3 km southeast of the landing site, are older than the
surrounding basaltic plains. Aqueous processes have extensively altered bedrock in the Columbia Hills. Ferrous
iron in the original, unaltered parent rock of hills materials has typically been oxidized extensively to form ferric
oxides, hydroxides, and other ferric minerals. Migrating fluids have removed Ca and other cations, allowing
residual Al to become relatively more abundant, and fluids added sulfates and chlorides. In subsurface
environments on Earth, microorganisms can obtain key nutrients from the weathering of basalts. Materials
examined in the Columbia Hills have comparable or greater abundances of these elements than do MORB.
Wishstone rock and Watchtower outcrop have very high contents of phosphorous. Chemoautotrophs ("chemical-
feeders" that obtain energy from inorganic chemicals) can thrive in subsurface environments. Mixing oxidized
constituents from surface environments with generally more reduced constituents from subsurface rocks and
thermal emanations provides energy to sustain microorganisms. Ferrous iron in parent materials in the
Columbia Hills has been oxidized to form a variety of ferric minerals. On Earth, microbial processes have been
documented to contribute to the production of goethite, hematite and other iron oxides. Observations by Spirit are
consistent with the possibility that liquid water, nutrients and sources of chemical energy were simultaneously
available to sustain habitable conditions in subsurface Columbia Hills materials at least some time in the distant
(Noachian?) past. There is as yet no evidence that these conditions ever existed at the surface. Future research
must seek to determine whether ancient migrating fluids in Gusev ever achieved the water activity necessary to
sustain life.
DE: 0406 Astrobiology and extraterrestrial materials
DE: 0463 Microbe/mineral interactions
DE: 5220 Hydrothermal systems and weathering on other planets
DE: 6225 Mars
SC: Planetary Sciences [P]
MN: 2007 Fall Meeting