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Hydrogen in rocks: an energy source for deep microbial communitiesTo survive in deep subsurface environments, lithotrophic microbial communities require a sustainable energy source such as hydrogen. Though H2 can be produced when water reacts with fresh mineral surfaces and oxidizes ferrous iron, this reaction is unreliable since it depends upon the exposure of fresh rock surfaces via the episodic opening of cracks and fissures. A more reliable and potentially more voluminous H2 source exists in nominally anhydrous minerals of igneous and metamorphic rocks. Our experimental results indicate that H2 molecules can be derived from small amounts of H2O dissolved in minerals in the form of hydroxyl, OH- or O3Si-OH, whenever such minerals crystallized in an H2O-laden environment. Two types of experiments were conducted. Single crystal fracture experiments indicated that hydroxyl pairs undergo an in situ redox conversion to H2 molecules plus peroxy links, O3Si/OO\SiO3. While the peroxy links become part of the mineral structure, the H2 molecules diffused out of the freshly fractured mineral surfaces. If such a mechanism occurred in natural settings, the entire rock column would become a volume source of H2. Crushing experiments to facilitate the outdiffusion of H2 were conducted with common crustal igneous rocks such as granite, andesite, and labradorite. At least 70 nmol of H2/g diffused out of coarsely crushed andesite, equivalent at standard pressure and temperature to 5,000 cm3 of H2/m3 of rock. In the water-saturated, biologically relevant upper portion of the rock column, the diffusion of H2 out of the minerals will be buffered by H2 saturation of the intergranular water film.
Document ID
20040087963
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Freund, Friedemann
(SETI Institute and Department of Physics, San Jose State University San Jose, CA, United States)
Dickinson, J. Thomas
Cash, Michele
Date Acquired
August 21, 2013
Publication Date
March 1, 2002
Publication Information
Publication: Astrobiology
Volume: 2
Issue: 1
ISSN: 1531-1074
Subject Category
Geosciences (General)
Distribution Limits
Public
Copyright
Other

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