Radiolysis in the subsurface of rocky planets: An alternative to sunlight energy for life Lisa M....
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Transcript of Radiolysis in the subsurface of rocky planets: An alternative to sunlight energy for life Lisa M....
![Page 1: Radiolysis in the subsurface of rocky planets: An alternative to sunlight energy for life Lisa M. Pratt Provost’s Professor Department of Geological Sciences,](https://reader036.fdocuments.in/reader036/viewer/2022070403/56649f295503460f94c433c0/html5/thumbnails/1.jpg)
Radiolysis in the subsurface of rocky planets: An alternative to sunlight energy for life
Lisa M. PrattProvost’s Professor
Department of Geological Sciences, Indiana University
Astrobiology Short CourseLPSI
May 1, 2010
![Page 2: Radiolysis in the subsurface of rocky planets: An alternative to sunlight energy for life Lisa M. Pratt Provost’s Professor Department of Geological Sciences,](https://reader036.fdocuments.in/reader036/viewer/2022070403/56649f295503460f94c433c0/html5/thumbnails/2.jpg)
Head frame for the Evander gold mine near Johannesburg,
South Africa.
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Gold ore hosted by quartz-pebble conglomerate
deposited 2.5 billion years ago
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High-retention ceramic filters for sampling of cells, membranes, and
DNA.
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Anaerobic chamber for transfer of deep-groundwater samples into nutrient media to assess metabolic pathways.
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A single-species ecosystem in the deep subsurface
Groundwater sampled at a depth of 2.8 km below the surface in the
Witwatersrand Basin of South Africa has yielded a single, complete genome
of a bacterial microorganism.
Chivian et al. 2008 Science Magazine
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Vegetative cells and resting spores in
groundwater sample
Rod-like shape shown by scanning electron micrograph
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Radiolytic Splitting of Water as Energy for Microbes
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Some Crazy Radiolytic Chemistry
Within 10-10 to 10-8 seconds of a decay event, the initial species
(H2O+, e-, H2O*) react further to produce:
Chemically reactive species:
Hydrated electron (eaq-),
Hydrogen (H•) radicals,
Hydroxyl (HO•) radicals,
Superoxide (O2•) radicals
Molecules:
Molecular hydrogen (H2)
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Sealed silica tubes showing products of reaction between pyrite and hydrogen peroxide
Red and yellow minerals include iron oxide, elemental sulfur, and numerous iron sulfates
similar to minerals identified on Mars
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Estimated water content near surface of Marsneutron spectrometer on Mars Odyssey spacecraft.
http://marsprogram.jpl.nasa.gov/odyssey/gallery/science/PIA04907.html
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This view covers an area about 1.15 kilometers (0.7 mile) wide.
Individual layers in the scene average 3.6 meters (12 feet) thick.
http://www.nasa.gov/mission_pages/MRO/multimedia/20081204a.html
Rhythmic bedding in Martian sedimentary rocks (Becquerel crater) indicates climate cycles.
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Water is not a limiting molecular resource although liquid water may be a limiting physical state for life on Mars.
Energy sources (redox gradients) do not appear to be limiting near the surface and radioactive minerals could drive radiolysis in the deep subsurface.
High-obliquity (tilt 70o or more) warm intervals could allow for episodic surface blooms of microbes waiting in a subsurface refuge.