Isotope and elemental geochemistry of black shale-hosted fossiliferous concretions from the Cretaceous Santana Formation fossil Lagerstätte (Brazil)

Research output: Contribution to journalArticleResearchpeer review

Authors

  • Ulrich Heimhofer
  • Patrick Meister
  • Stefano M. Bernasconi
  • Daniel Ariztegui
  • David M. Martill
  • Aristoteles M. Rios-Netto
  • Lorenz Schwark

Research Organisations

External Research Organisations

  • University of Vienna
  • Max Planck Institute for Marine Microbiology
  • ETH Zurich
  • University of Geneva
  • University of Portsmouth
  • Universidade Federal do Rio de Janeiro
  • Kiel University
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Details

Original languageEnglish
Pages (from-to)150-167
Number of pages18
JournalSedimentology
Volume64
Issue number1
Early online date21 Oct 2016
Publication statusPublished - 1 Jan 2017

Abstract

Carbonate concretions hosted within organic carbon-rich shale sequences represent unique archives of often exceptionally preserved fossil biota. Besides providing high-fidelity preservation, their geochemical signatures can provide insight into the physical and chemical processes during early and later-stage concretion growth. Here, two fossiliferous carbonate concretions of the late Early Cretaceous Santana Formation (Araripe Basin, north-east Brazil) are analysed with an integrative geochemical approach including μ-XRF scanning, δ13C, δ18O, 87Sr/86Sr and Δ47 (clumped isotope thermometry). Individual concretions show a concentric internal zonation with the outermost layer being composed of millimetre thick cone-in-cone calcite. A strong covariance of δ13C and δ18O values of the fine-crystalline concretion body indicates mixing of two different carbonate phases and supports a scenario of temporally separated pervasive growth stages. Microbially-mediated formation of an early porous calcite framework was controlled by the combined processes of fermentation and methanogenesis around the decaying carcass, forming localized environments within a zone of sulphate reduction. Microbial sulphate reduction is indicated by the concentric enrichment of pyrite in the outer part of the concretion body and by high pyrite abundance in the surrounding shale. Information on the later-stage diagenetic processes affecting the Santana concretions can be derived from the outermost fringing cone-in-cone calcite. The carbonate precipitating fluid was characterized by a more or less marine δ18O composition (calculated δ18Oporewater = −1·0 to −1·8‰) and by radiogenic Sr-isotope ratios (up to 0·713331 ± 7·0*10−6), the latter probably reflecting modification due to interaction with the surrounding shale or, alternatively, with underlying evaporitic sulphate deposits influenced by strong continental inflow or with crystalline basement rocks. The Δ47-derived temperature estimates range between 37°C and 42°C ± 5, indicating precipitation of the cone-in-cone calcite at a depth of 650 to 850 m, which is only half as much as the maximum burial depth derived from existing fission-track data. Overall, the study of fossiliferous carbonate concretions in organic carbon-rich sedimentary sequences can reveal a complex growth history spanning incipient microbially-influenced precipitates as well as later-stage burial diagenetic phases.

Keywords

    Carbonate concretion, clumped isotopes, cone-in-cone, inorganic geochemistry, pervasive growth, Santana Formation

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Isotope and elemental geochemistry of black shale-hosted fossiliferous concretions from the Cretaceous Santana Formation fossil Lagerstätte (Brazil). / Heimhofer, Ulrich; Meister, Patrick; Bernasconi, Stefano M. et al.
In: Sedimentology, Vol. 64, No. 1, 01.01.2017, p. 150-167.

Research output: Contribution to journalArticleResearchpeer review

Heimhofer U, Meister P, Bernasconi SM, Ariztegui D, Martill DM, Rios-Netto AM et al. Isotope and elemental geochemistry of black shale-hosted fossiliferous concretions from the Cretaceous Santana Formation fossil Lagerstätte (Brazil). Sedimentology. 2017 Jan 1;64(1):150-167. Epub 2016 Oct 21. doi: 10.1111/sed.12337
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title = "Isotope and elemental geochemistry of black shale-hosted fossiliferous concretions from the Cretaceous Santana Formation fossil Lagerst{\"a}tte (Brazil)",
abstract = "Carbonate concretions hosted within organic carbon-rich shale sequences represent unique archives of often exceptionally preserved fossil biota. Besides providing high-fidelity preservation, their geochemical signatures can provide insight into the physical and chemical processes during early and later-stage concretion growth. Here, two fossiliferous carbonate concretions of the late Early Cretaceous Santana Formation (Araripe Basin, north-east Brazil) are analysed with an integrative geochemical approach including μ-XRF scanning, δ13C, δ18O, 87Sr/86Sr and Δ47 (clumped isotope thermometry). Individual concretions show a concentric internal zonation with the outermost layer being composed of millimetre thick cone-in-cone calcite. A strong covariance of δ13C and δ18O values of the fine-crystalline concretion body indicates mixing of two different carbonate phases and supports a scenario of temporally separated pervasive growth stages. Microbially-mediated formation of an early porous calcite framework was controlled by the combined processes of fermentation and methanogenesis around the decaying carcass, forming localized environments within a zone of sulphate reduction. Microbial sulphate reduction is indicated by the concentric enrichment of pyrite in the outer part of the concretion body and by high pyrite abundance in the surrounding shale. Information on the later-stage diagenetic processes affecting the Santana concretions can be derived from the outermost fringing cone-in-cone calcite. The carbonate precipitating fluid was characterized by a more or less marine δ18O composition (calculated δ18Oporewater = −1·0 to −1·8‰) and by radiogenic Sr-isotope ratios (up to 0·713331 ± 7·0*10−6), the latter probably reflecting modification due to interaction with the surrounding shale or, alternatively, with underlying evaporitic sulphate deposits influenced by strong continental inflow or with crystalline basement rocks. The Δ47-derived temperature estimates range between 37°C and 42°C ± 5, indicating precipitation of the cone-in-cone calcite at a depth of 650 to 850 m, which is only half as much as the maximum burial depth derived from existing fission-track data. Overall, the study of fossiliferous carbonate concretions in organic carbon-rich sedimentary sequences can reveal a complex growth history spanning incipient microbially-influenced precipitates as well as later-stage burial diagenetic phases.",
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Download

TY - JOUR

T1 - Isotope and elemental geochemistry of black shale-hosted fossiliferous concretions from the Cretaceous Santana Formation fossil Lagerstätte (Brazil)

AU - Heimhofer, Ulrich

AU - Meister, Patrick

AU - Bernasconi, Stefano M.

AU - Ariztegui, Daniel

AU - Martill, David M.

AU - Rios-Netto, Aristoteles M.

AU - Schwark, Lorenz

N1 - Funding information: We thank D. Buhl and U. Schulte (Ruhr-University Bochum) and M. Jaggi and S. Bishop (ETH Zürich) for laboratory assistance. Financial support from DFG project HE 4467/5-1 and by the Nordrhein-Westfälische Akademie der Wissenschaften und Künste to UH is gratefully acknowledged. Dr. A. Andrade (DNPM Crato) assisted our field work in Brazil. We thankfully acknowledge M. Gutjahr and an anonymous reviewer for critical comments that improved an earlier draft of the manuscript.

PY - 2017/1/1

Y1 - 2017/1/1

N2 - Carbonate concretions hosted within organic carbon-rich shale sequences represent unique archives of often exceptionally preserved fossil biota. Besides providing high-fidelity preservation, their geochemical signatures can provide insight into the physical and chemical processes during early and later-stage concretion growth. Here, two fossiliferous carbonate concretions of the late Early Cretaceous Santana Formation (Araripe Basin, north-east Brazil) are analysed with an integrative geochemical approach including μ-XRF scanning, δ13C, δ18O, 87Sr/86Sr and Δ47 (clumped isotope thermometry). Individual concretions show a concentric internal zonation with the outermost layer being composed of millimetre thick cone-in-cone calcite. A strong covariance of δ13C and δ18O values of the fine-crystalline concretion body indicates mixing of two different carbonate phases and supports a scenario of temporally separated pervasive growth stages. Microbially-mediated formation of an early porous calcite framework was controlled by the combined processes of fermentation and methanogenesis around the decaying carcass, forming localized environments within a zone of sulphate reduction. Microbial sulphate reduction is indicated by the concentric enrichment of pyrite in the outer part of the concretion body and by high pyrite abundance in the surrounding shale. Information on the later-stage diagenetic processes affecting the Santana concretions can be derived from the outermost fringing cone-in-cone calcite. The carbonate precipitating fluid was characterized by a more or less marine δ18O composition (calculated δ18Oporewater = −1·0 to −1·8‰) and by radiogenic Sr-isotope ratios (up to 0·713331 ± 7·0*10−6), the latter probably reflecting modification due to interaction with the surrounding shale or, alternatively, with underlying evaporitic sulphate deposits influenced by strong continental inflow or with crystalline basement rocks. The Δ47-derived temperature estimates range between 37°C and 42°C ± 5, indicating precipitation of the cone-in-cone calcite at a depth of 650 to 850 m, which is only half as much as the maximum burial depth derived from existing fission-track data. Overall, the study of fossiliferous carbonate concretions in organic carbon-rich sedimentary sequences can reveal a complex growth history spanning incipient microbially-influenced precipitates as well as later-stage burial diagenetic phases.

AB - Carbonate concretions hosted within organic carbon-rich shale sequences represent unique archives of often exceptionally preserved fossil biota. Besides providing high-fidelity preservation, their geochemical signatures can provide insight into the physical and chemical processes during early and later-stage concretion growth. Here, two fossiliferous carbonate concretions of the late Early Cretaceous Santana Formation (Araripe Basin, north-east Brazil) are analysed with an integrative geochemical approach including μ-XRF scanning, δ13C, δ18O, 87Sr/86Sr and Δ47 (clumped isotope thermometry). Individual concretions show a concentric internal zonation with the outermost layer being composed of millimetre thick cone-in-cone calcite. A strong covariance of δ13C and δ18O values of the fine-crystalline concretion body indicates mixing of two different carbonate phases and supports a scenario of temporally separated pervasive growth stages. Microbially-mediated formation of an early porous calcite framework was controlled by the combined processes of fermentation and methanogenesis around the decaying carcass, forming localized environments within a zone of sulphate reduction. Microbial sulphate reduction is indicated by the concentric enrichment of pyrite in the outer part of the concretion body and by high pyrite abundance in the surrounding shale. Information on the later-stage diagenetic processes affecting the Santana concretions can be derived from the outermost fringing cone-in-cone calcite. The carbonate precipitating fluid was characterized by a more or less marine δ18O composition (calculated δ18Oporewater = −1·0 to −1·8‰) and by radiogenic Sr-isotope ratios (up to 0·713331 ± 7·0*10−6), the latter probably reflecting modification due to interaction with the surrounding shale or, alternatively, with underlying evaporitic sulphate deposits influenced by strong continental inflow or with crystalline basement rocks. The Δ47-derived temperature estimates range between 37°C and 42°C ± 5, indicating precipitation of the cone-in-cone calcite at a depth of 650 to 850 m, which is only half as much as the maximum burial depth derived from existing fission-track data. Overall, the study of fossiliferous carbonate concretions in organic carbon-rich sedimentary sequences can reveal a complex growth history spanning incipient microbially-influenced precipitates as well as later-stage burial diagenetic phases.

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