4.7 Article

Simulating Precambrian banded iron formation diagenesis

Journal

CHEMICAL GEOLOGY
Volume 362, Issue -, Pages 66-73

Publisher

ELSEVIER SCIENCE BV
DOI: 10.1016/j.chemgeo.2013.05.031

Keywords

Mineral diagenesis; Mineral transformations; Banded iron formations; Anoxygenic phototrophs; Biogenic minerals

Funding

  1. Wilhelm-Schuler Stiftung
  2. German Academic Exchange Service (DAAD)
  3. German Research Foundation (DFG) [PO 1624/1-1, PO 1624/2-1, KA 1736/4-1, KA 1736/12-1]
  4. Nachwuchsprogramm Universitat Tubingen
  5. Promotionsverbund Einblicke in die Bakterien-Material-Wechselwirkungen
  6. National Science Foundation [1064391]
  7. Natural Sciences and Engineering Research Council of Canada
  8. Office Of Internatl Science &Engineering
  9. Office Of The Director [1064391] Funding Source: National Science Foundation

Ask authors/readers for more resources

Post-depositional diagenetic alteration makes the accurate interpretation of key precipitation processes in ancient sediments, such as Precambrian banded iron formations (BIFs), difficult. While microorganisms are proposed as key contributors to BIF deposition, the diagenetic transformation of precursor Fe(III) minerals associated with microbial biomass had not been experimentally tested. We incubated mixtures of ferrihydrite (proxy for biogenic ferric oxyhydroxide minerals) and glucose (proxy for microbial biomass) in gold capsules at 1.2 kbar and 170 degrees C. Both wet chemical analysis and mineralogical methods (microscopy, X-ray diffraction and Mossbauer spectroscopy) were used to analyze the reaction products. Under these conditions, ferrihydrite (Fe-III(OH)(3)) transforms to hematite ((Fe2O3)-O-III), magnetite ((FeFe2O4)-Fe-II-O-III), and siderite ((FeCO3)-C-II). Silica-coated ferrihydrite prepared at conservative Si: Fe ratios (as predicted for the Precambrian oceans) and mixed with glucose yielded hematite and siderite, whereas magnetite could not be identified microscopically. Our results show that electron transfer from organic carbon to Fe(III) minerals during temperature/pressure diagenesis can drive the production of key BIF minerals. Our results also demonstrate that the post-depositional mineralogy of BIF does not directly archive the oceanic or atmospheric conditions present on Earth during their lithification. As a consequence, atmospheric composition regarding concentrations of methane and CO2 during the time of BIF mineral deposition cannot be directly inferred from BIF mineralogical data alone. (C) 2013 Elsevier B. V. All rights reserved.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.7
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available