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Microbial Diversity in Surface Iron-Rich Aqueous Environments : Implications for Seeking Signs of Life on Mars

Author
Tringe, S. G.
Published
[2010].
Physical Description
1 electronic document
Additional Creators
Klatt, C. G., McKay, D. S., Sarkisova, S. A., Garrison, D. H., Brown, I. I., Bryant, D. A., and Allen, C. C.
Online Version

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Summary
The success of selecting future landing sites on Mars to discover extinct and/or extant extraterrestrial life is dependent on the correct approximation of available knowledge about terrestrial paleogeochemistry and life evolution to Martian (paleo) geology and geochemistry. It is well known that both Earth and Mars are Fe rich. This widespread occurrence suggests that Fe may have played a key role in early life forms, where it probably served as a key constituent in early prosthetic moieties in many proteins of ancient microbes on Earth and likely Mars. The second critical idea is the premise that Life on Mars could most likely have developed when Mars experienced tectonic activity [1] which dramatically decreased around 1 bin years after Martian creation. After that Martian life could have gone extinct or hibernated in the deep subsurface, which would be expensive to reach in contrast to the successful work of Martian surface rovers. Here we analyze the diversity of microbes in several terrestrial Fe rich surface environments in conjunction with the phylogeny and molecular timing of emergence of those microbes on Earth. Anticipated results should help evaluate future landing sites on Mars in searches for biosignatures.
Other Subject(s)
Collection
NASA Technical Reports Server (NTRS) Collection.
Note
Document ID: 20100005364.
JSC-CN-19784.
Astrobiology Science Conference; 26-29 Apr. 2010; League City, TX; United States.
Terms of Use and Reproduction
Copyright, Distribution as joint owner in the copyright.
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