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2005 Annual Science Report

Indiana University, Bloomington Reporting  |  JUL 2004 – JUN 2005

Radiolysis as a Source of Chemical Energy for Microbial Metabolism in the Deep Subsurface

Project Summary

Radiolysis of water can accelerate water/rock interaction through production of radicals (e.g., hydrogen, hydroperoxyl, hydroxyl), ions (e.g., superoxide, protons, hydroxide), and reactive molecules (e.g., hydrogen, hydrogen peroxide, oxygen)

4 Institutions
3 Teams
0 Publications
0 Field Sites
Field Sites

Project Progress

Radiolysis of water can accelerate water/rock interaction through production of radicals (e.g., hydrogen, hydroperoxyl, hydroxyl), ions (e.g., superoxide, protons, hydroxide), and reactive molecules (e.g., hydrogen, hydrogen peroxide, oxygen). Radiolytic oxidation can be observed in modern groundwater associated with uranium ore bodies and can be inferred for ancient groundwater based on the composition and isotopic signature of minerals. Prior to development of an oxygen-rich atmosphere on Earth, radiolytically generated oxidants could have reacted with pyrite and provided local plumes of partially to fully oxidized sulfur species suitable for microbial metabolism.

We evaluated sulfur isotope effects associated with reactions between pyrite and radiolytic oxidants using a series of sealed-quartz-tube experiments run with 60 mg of acid-cleaned pyrite, 10 milliliters of deoxygenated water, and concentrations of hydrogen peroxide (H2O2 ) at millimolar levels (Figure 1). Experiments ranged in temperature from 4 to 150 degrees Celsius with durations from 1 to 10 days.

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In initial experiments, primary oxidation products were dissolved sulfate, elemental sulfur, iron sulfate minerals, and iron oxyhydroxide minerals. X-ray diffraction patterns and images from scanning electron microscopy reveal anhedral to subhedral hydrated iron sulfates in globular clusters of about 10-30 micrometers in diameter forming on pyrite surfaces (Figure 2). Sulfur isotopic compositions remained unchanged for pyrite but showed distinct enrichment of 34S in produced sulfate and elemental sulphur. The isotopic difference between sulfate and pyrite was 0.5-1 permil and between elemental sulfur and pyrite was 1-2 permil. Our results indicate that pyrite oxidation by H2O2 induces greater fractionation that has been recognized in previous studies. Although difference in isotopic composition for produced sulfate and elemental sulfur compared to starting pyrite are not large but compensating depletion of 34S in undetected products could be substantial if proportional yields are small. Preliminary isotope results from high-temperature experiments indicate that the missing 34S-depleted fraction might be held in iron sulfate and/or iron oxyhydroxides. Similar fractionation in ancient terrestrial samples or in extraterrestrial samples could be mistaken as evidence for microbial activity.

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Highlights:


  • Recently published paper by Lin and others (Geochemistry Geophysics, and Geosystems, 2005) presents an exciting and controversial hypothesis for the crucial of radiolytic hydrogen production in sustaining deep-subsurface microbial communities on Earth and, potentially, on other planets.
  • Laboratory experiments simulating radiolysis in the deep subsurface yield distinctive non-biogenic isotope signatures for sulfate and elemental sulfur produced by oxidation of pyrite.
  • Radiolysis of groundwater in uranium-rich deposits can provide oxidized and reduced chemical species suitable for sustaining diverse communities of microbes.
  • PROJECT INVESTIGATORS:
    Edward Ripley Edward Ripley
    Project Investigator
  • PROJECT MEMBERS:
    Lisa Pratt
    Co-Investigator

    David Bish
    Collaborator

    Tullis Onstott
    Collaborator

    Liliana Lefticariu
    Postdoc

  • RELATED OBJECTIVES:
    Objective 3.3
    Origins of energy transduction

    Objective 4.1
    Earth's early biosphere

    Objective 4.2
    Foundations of complex life

    Objective 5.1
    Environment-dependent, molecular evolution in microorganisms

    Objective 5.2
    Co-evolution of microbial communities

    Objective 5.3
    Biochemical adaptation to extreme environments

    Objective 6.1
    Environmental changes and the cycling of elements by the biota, communities, and ecosystems

    Objective 7.2
    Biosignatures to be sought in nearby planetary systems