title: Microbial production of isotopically light iron(II) in a modern chemically precipitated sediment and implications for isotopic variations in ancient rocks.
abstract: The inventories and Fe isotope composition of aqueous Fe(II) and solid-phase Fe compounds were quantified in neutral-pH, chemically precipitated sediments downstream of the Iron Mountain acid mine drainage site in northern California, USA. The sediments contain high concentrations of amorphous Fe(III) oxyhydroxides [Fe(III)(am)] that allow dissimilatory iron reduction (DIR) to predominate over Fe-S interactions in Fe redox transformation, as indicated by the very low abundance of Cr(II)-extractable reduced inorganic sulfur compared with dilute HCl-extractable Fe. delta(56)Fe values for bulk HCl- and HF-extractable Fe were approximately 0. These near-zero bulk delta(56)Fe values, together with the very low abundance of dissolved Fe in the overlying water column, suggest that the pyrite Fe source had near-zero delta(56)Fe values, and that complete oxidation of Fe(II) took place prior to deposition of the Fe(III) oxide-rich sediment. Sediment core analyses and incubation experiments demonstrated the production of millimolar quantities of isotopically light (delta(56)Fe approximately -1.5 to -0.5 per thousand) aqueous Fe(II) coupled to partial reduction of Fe(III)(am) by DIR. Trends in the Fe isotope composition of solid-associated Fe(II) and residual Fe(III)(am) are consistent with experiments with synthetic Fe(III) oxides, and collectively suggest an equilibrium Fe isotope fractionation between aqueous Fe(II) and Fe(III)(am) of approximately -2 per thousand. These Fe(III) oxide-rich sediments provide a model for early diagenetic processes that are likely to have taken place in Archean and Paleoproterozoic marine sediments that served as precursors for banded iron formations. Our results suggest pathways whereby DIR could have led to the formation of large quantities of low-delta(56)Fe minerals during BIF genesis.
authors.affiliation: Department of Geoscience and NASA Astrobiology Institute, University of Wisconsin, Madison, WI, USA.
authors.forename: G E
authors.initials: GE
authors.lastname: Tangalos
authors.forename: B L
authors.initials: BL
authors.lastname: Beard
authors.forename: C M
authors.initials: CM
authors.lastname: Johnson
authors.forename: C N
authors.initials: CN
authors.lastname: Alpers
authors.forename: E S
authors.initials: ES
authors.lastname: Shelobolina
authors.forename: H
authors.initials: H
authors.lastname: Xu
authors.forename: H
authors.initials: H
authors.lastname: Konishi
authors.forename: E E
authors.initials: EE
authors.lastname: Roden
mesh_terms: D002140:California; D005290:Ferric Compounds / Q000032:analysis; D005296:Ferrous Compounds / Q000378:metabolism*; D019015:Geologic Sediments / Q000737:chemistry / Q000382:microbiology*; D007503:Iron Isotopes / Q000378:metabolism*; D010084:Oxidation-Reduction; D013455:Sulfur / Q000032:analysis
chemical_list: D005290:Ferric Compounds; D005296:Ferrous Compounds; D007503:Iron Isotopes; D013455:Sulfur