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Origin & Evolution of Life: June 2010


Workshop Dates: October 11-13, 2010

NAI, together with the Agouron Institute and the Canadian Institute for Advanced Research, are again sponsoring a field workshop of the Early Earth Focus Group following upon the very successful BAR (Biosignatures in Ancient Rocks) workshop of 2007. The topic of this workshop is Anoxygenic Phototrophic Ecosystems (APE): Ancient and Modern. This workshop will bring together approximately 40 microbial ecologists, astro- and geobiologists; including ~10 senior scientists who have made significant contributions to our understanding of modern and ancient anaerobic ecosystems and of the chemistry of ancient oceans, ~15 early career researchers (assistant professors and postdocs) who have been actively conducting forefront research, and ~15 future leaders (current graduate students) in this field. The workshop is scheduled for Oct. 11-13 in Fayetteville, New York, at the scenic and biogeochemically stratified Green Lake. Travel awards are available. Please contact Linda Altamura (Penn State Astrobiology Research Center: lxg2@psu.edu) for further information.

For more information about the Early Earth Focus Group, visit: http://astrobiology.nasa.gov/nai/focus-groups/current/early-earth/intro/ [Source: NAI Newsletter]

Date/Time: Monday, June 21, 2010 11:00AM Pacific Speaker: Lee Kump (Pennsylvania State University) Title: "Evolution of the Oceans: Pale Pink Dot"

Although uniformitarian views dominated early thinking of ocean chemical evolution over geologic time, today we recognize that the composition of seawater has varied significantly over Earth's history. Some changes are ingrained in our thinking (for example, that the Archean ocean was anoxic and iron-rich) while others are rarely considered. For example, if sulfate was a trace constituent of the Archean ocean, then the chemistry of hydrothermal fluids would have been significantly different (more reduced, with high hydrogen partial pressures and iron concentrations but low concentrations of hydrogen sulfide); this may be of significance to those considering such environments as the locus for the origin of life and for early ecosystems. Refinement of radiometric ages of banded iron formations suggest that their deposition was episodic, not continuous, and this may require us to rethink the notion of a persistently Fe-replete Archean ocean. The rise of atmospheric oxygen in the earliest Proterozoic ironically created the potential for highly reducing marine conditions with free hydrogen sulfide in the upper water column supporting anoxygenic phototrophs. The persistence of these conditions through the Proterozoic is uncertain, but when they occurred, the "pale blue dot" may have been pink. Strategies for life detection on distant planets is based in part on our interpretation of Earth's oceanic and atmospheric evolution, and we have some way to go before we can confidently describe the evolutionary history and persistence of particular conditions on Earth.

For more information and participation instructions: http://astrobiology.nasa.gov/nai/seminars/detail/174 [Source: NAI Newsletter]