Biology
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufm.p12a..03z&link_type=abstract
American Geophysical Union, Fall Meeting 2010, abstract #P12A-03
Biology
[0406] Biogeosciences / Astrobiology And Extraterrestrial Materials, [0424] Biogeosciences / Biosignatures And Proxies, [0454] Biogeosciences / Isotopic Composition And Chemistry, [0456] Biogeosciences / Life In Extreme Environments
Scientific paper
The Atacama Desert, one of the driest places on Earth, is considered a suitable analog for the extremely arid, oxidizing conditions on the surface of Mars. Recent observations suggest the presence of evaporitic deposits on the surface of Mars, such as those found in the Atacama. Halites in the Atacama have been shown to be hygroscopic and are colonized by photosynthetic microbes. While there is considerable evidence for the decrease in abundance and diversity of microbes closer to the hyper-arid core of the Atacama, experimental studies have thus far have yet to estimate the sources of carbon to these communities and the rate at which they cycle. To address these questions, we characterized the isotopic composition (13C and 14C) microbial community biomarkers from four distinct sites in the Atacama. Sites ranged from halites in the hyper-arid core (Yungay, Salar Grande) to volcanic rock and gypsum near the Monturaqui Crater. Our analysis of the phospholipids fatty acids (PLFA) and glycolipid fatty acid (GLFA) methyl esters of the endoliths agreed with previous studies: the abundance and diversity of microbes decreases approaching the hyper-arid core. The total PLFA and GLFA concentrations were lower at Yungay than Salar Grande and higher in the gypsum and volcanic rock samples. Changes in the mole percentage distribution of the PLFA and GLFA illustrated that the endolithic communities inhabiting the volcanic rock and gypsum were more complex than those inhabiting the halites. ∂13C of both PLFA and GLFA showed that non-halite lipids were less depleted in 13C than halite-lipids. This suggested a difference in carbon source or cycling. The 14C content of PLFA and GLFA varied by up to 250 per mil. Endolith PLFA and GLFA from the gypsum had radiocarbon signatures comparable to the modern atmosphere, which suggests that the predominant source of carbon to the system is the modern atmosphere and that lipids are cycling rapidly in this system. However, at the other three locations both PLFA and GLFA were more depleted in 14C relative to the gypsum, indicative of a difference in carbon sources and cycling. This may relate to the presence of inputs of older carbon to these endolithic environments, or to the persistence of biosignature compounds for significant lengths of time notwithstanding the generally oxidizing nature of the Atacama environment. This persistence may be related to differences in moisture levels and therefore hydrolysis of these compounds. Applied to Mars, our results suggest the potential that biosignatures of photosynthesis may be preserved in low-moisture, high salt endolithic environments. Ongoing work to understand the sources of isotopic variation within the Atacama analogue system will help identify the potential for target biosignatures in similar systems on Mars.
Davila Alberto
Slater Greg F.
Wierzchos Jacek
Ziolkowski Lori A.
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