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Biosignatures link microorganisms to iron mineralization in a paleoaquifer

  • Karrie A. Weber
  • , Trisha L. Spanbauer
  • , David Wacey
  • , Matthew R. Kilburn
  • , David B. Loope
  • , Richard M. Kettler

Producción científica: Articlerevisión exhaustiva

38 Citas (Scopus)

Resumen

Concretions, preferentially cemented masses within sediments and sedimentary rocks, are records of sediment diagenesis and tracers of pore water chemistry. For over a century, rinded spheroidal structures that exhibit an Fe(III) oxide-rich exterior and Fe-poor core have been described as oxidation products of Fe(II) carbonate concretions. However, mechanisms governing Fe(III) oxide precipitation within these structures remain an enigma. Here we present chemical and morphological evidence of microbial biosignatures in association with Fe(III) oxides in the Fe(III) oxide-rich rind of spheroidal concretions collected from the Jurassic Navajo Sandstone (southwest United States), implicating a microbial role in Fe biomineralization. The amount of total organic carbon in the exterior Fe(HI) oxides exceeded measured values in the friable interior. The mean delta C-13 value of organic carbon from the Fe(III) oxide-cemented exterior, delta C-13 of -20.55 parts per thousand, is consistent with a biogenic signature from autotrophic bacteria. Scanning electron micrographs reveal microstructures consistent with bacterial size and morphology, including a twisted-stalk morphotype that resembled an Fe(II)-oxidizing microorganism, Gallionella sp. Nanoscale associations of Fe, 0, C, and N with bacterial morphotypes demonstrate microorganisms associated with Fe(III) oxides. Together these results indicate that autotrophic microorganisms were present during Fe(III) oxide precipitation and present microbial catalysis as a mechanism of Fe(III) oxide concretion formation. Microbial biosignatures in rinded Fe(III) oxide-rich concretions within an exhumed, Quaternary aquifer has broad implications for detection of life within the geological record on Earth as well as other Fe-rich rocky planets such as Mars, where both Fe(II) carbonate and Fe(III) oxide-rich concretions have been identified.
Idioma originalEnglish
Páginas (desde-hasta)747-750
Número de páginas4
PublicaciónGeology
Volumen40
N.º8
DOI
EstadoPublished - ago 2012

Financiación

This study was carried out in Grand Staircase-Escalante National Monument with cooperation of the Bureau of Land Management and assistance of C. Shelton and A. Titus. We are grateful to C. Okafor, C. McFadden, A. Shultis, D. Snow, H. Chen, and K. Sun for assistance with sample preparation and analyses. The authors acknowledge facilities, scientific, and technical assistance of the Australian Microscopy and Microanalysis Research Facility at the Centre for Microscopy, Characterisation and Analysis for NanoSIMS analysis at UWA, facility funded by the University, State, and Commonwealth Governments. This research was supported by the UNL Research Office and Nebraska Tobacco Settlement Fund. Manuscript preparation was supported by NSF ADVANCE-Nebraska grant 0811250.

FinanciadoresNúmero del financiador
Government College University Faisalabad
KY State Government
Commonwealth Government
UNL Office of Research and Innovation
Nebraska Tobacco Settlement Biomedical Research Development Fund
NSF ADVANCE-Nebraska grant0811250

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