HR: 1340h
AN: B53B-0991 [Abstracts]
TI: Iron Isotope Analyses for the Origin of Fe-Bearing Minerals in the 3.46 Ga Marble Bar Chert, Pilbara
Craton, Western Australia, Recovered by Archean Biosphere Drilling Project (ABDP)
AU: * Yamaguchi, K E
EM: kosei@jamstec.go.jp
AF: Institute for Research on Earth Evolution, Japan Agency for Marine-Earth Science and Technology, 2-15
Natsushima, Yokosuka, 237-0061
Japan
AU: * Yamaguchi, K E
EM: kosei@jamstec.go.jp
AF: NASA Astrobiology In stitute, NASA, NASA, 00000
United States
AU: Hoashi, M
EM: hoashi@chan.co.jp
AF: Department of Physics, Kagoshima University, Korimoto, Kagoshima, 890
Japan
AU: Tanimizu, M
EM: mash@cc.kochi-u.ac.jp
AF: Institute for Research on Earth Evolution, Japan Agency for Marine-Earth Science and Technology, 2-15
Natsushima, Yokosuka, 237-0061
Japan
AU: Kakegawa, T
EM: kakegawa@mail.tains.tohoku.ac.jp
AF: NASA Astrobiology In stitute, NASA, NASA, 00000
United States
AU: Kakegawa, T
EM: kakegawa@mail.tains.tohoku.ac.jp
AF: Department of GeoEnvironmental Sciences, Tohoku University, Aramaki, Aoba, Sendai, 980-8570
Japan
AU: Nedachi, M
EM: nedachi@sci.kagoshima-u.ac.jp
AF: NASA Astrobiology In stitute, NASA, NASA, 00000
United States
AU: Nedachi, M
EM: nedachi@sci.kagoshima-u.ac.jp
AF: Graduate School of Science and Engineering, Kagoshima University, Korimoto, Kagoshima, 890
Japan
AU: Ohmoto, H
EM: ohmoto@geosc.psu.edu
AF: NASA Astrobiology In stitute, NASA, NASA, 00000
United States
AU: Ohmoto, H
EM: ohmoto@geosc.psu.edu
AF: Penn State Astrobiology Research Center and Department of Geosciences, Pennsylvania State University,
435 Deike Building, University Park, PA 16802
United States
AB:
In 2003, "Archean Biosphere Drilling Project" recovered 3.46 billion-years-old modern-weathering free banded chert of the
Marble Bar Chert Member of the Towers Formation of the Warrawoona Group in the East Pilbara Granite-Greenstone Terrane,
Western Australia. The chert samples contain variable abundance of Fe-bearing minerals such as hematite, magnetite, siderite
and pyrite. Hematite bands of mm or sub-mm order in thickness are composed of micro-crystals of hematite and cut by several
generations of quartz veins. Pyrite crystallization is found both in the quartz veins and the hematite bands. These
observations suggest that the hematite bands, probably syn-depositional, were formed earlier than the pyrite crystals. Iron
isotope analyses were performed on individual Fe-bearing minerals separated by micro-drilling of the chert samples. Such
data, when combined with published data for Fe isotope fractionation between minerals and fluids in natural environments and
laboratory experimental system, are expected to give information on (1) the Fe isotope compositions of the fluid or precursor
Fe-bearing minerals from which the Fe-bearing minerals were formed, (2) the degree of involvement of microbiological
processes such as bacterial Fe reduction / oxidation in the mineralization of Fe-bearing minerals, and (3) redox state of the
Early Archean deep marine environments. If hematite mineralization was primary and precipitation of Fe-(oxy)hydroxide as its
precursor occurred during sedimentation by oxidizing dissolved ferrous Fe by oxygen, or if microbes were involved in the
formation of Fe-bearing minerals, then far-reaching implications will emerge for the redox evolution of the atmosphere and
oceans and the evolution of biosphere in the Early Archean.
DE: 4805 Biogeochemical cycles (1615)
DE: 4851 Oxidation/reduction reactions
DE: 1040 Isotopic composition/chemistry
DE: 1050 Marine geochemistry (4835, 4850)
DE: 1615 Biogeochemical processes (4805)
SC: Biogeosciences [B]
MN: 2004 AGU Fall Meeting