An early diagenetic deglacial origin for basal Ediacaran “cap dolostones”

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An early diagenetic deglacial origin for basal Ediacaran “cap dolostones”. / Ahm, Anne Sofie C.; Maloof, Adam C.; Macdonald, Francis A.; Hoffman, Paul F.; Bjerrum, Christian J.; Bold, Uyanga; Rose, Catherine V.; Strauss, Justin V.; Higgins, John A.

I: Earth and Planetary Science Letters, Bind 506, 2019, s. 292-307.

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Harvard

Ahm, ASC, Maloof, AC, Macdonald, FA, Hoffman, PF, Bjerrum, CJ, Bold, U, Rose, CV, Strauss, JV & Higgins, JA 2019, 'An early diagenetic deglacial origin for basal Ediacaran “cap dolostones”', Earth and Planetary Science Letters, bind 506, s. 292-307. https://doi.org/10.1016/j.epsl.2018.10.046

APA

Ahm, A. S. C., Maloof, A. C., Macdonald, F. A., Hoffman, P. F., Bjerrum, C. J., Bold, U., Rose, C. V., Strauss, J. V., & Higgins, J. A. (2019). An early diagenetic deglacial origin for basal Ediacaran “cap dolostones”. Earth and Planetary Science Letters, 506, 292-307. https://doi.org/10.1016/j.epsl.2018.10.046

Vancouver

Ahm ASC, Maloof AC, Macdonald FA, Hoffman PF, Bjerrum CJ, Bold U o.a. An early diagenetic deglacial origin for basal Ediacaran “cap dolostones”. Earth and Planetary Science Letters. 2019;506:292-307. https://doi.org/10.1016/j.epsl.2018.10.046

Author

Ahm, Anne Sofie C. ; Maloof, Adam C. ; Macdonald, Francis A. ; Hoffman, Paul F. ; Bjerrum, Christian J. ; Bold, Uyanga ; Rose, Catherine V. ; Strauss, Justin V. ; Higgins, John A. / An early diagenetic deglacial origin for basal Ediacaran “cap dolostones”. I: Earth and Planetary Science Letters. 2019 ; Bind 506. s. 292-307.

Bibtex

@article{7b9d00e65168432b8862b72e0b522834,
title = "An early diagenetic deglacial origin for basal Ediacaran “cap dolostones”",
abstract = "The beginning of the Ediacaran Period (∼635 Ma) is marked by conspicuous dolostone units that cap Marinoan glacial deposits worldwide. The extent and sedimentary characteristics of the cap dolostones indicate that anomalous carbonate over-saturation coincided with deglacial sea-level rise and ocean warming. However, the geochemical variability within cap dolostones, both between continents, across single continental margins, and within individual stratigraphic sections has been difficult to reconcile with depositional models. Using a compilation of new calcium and magnesium isotope measurements in Marinoan cap dolostone successions worldwide, we show that the geochemical variability can be explained by early diagenetic dolomitization of aragonite along a spectrum of fluid- and sediment-buffered conditions. Dolostones from the outer platform formed under fluid-buffered conditions, whereas dolostones on the inner platform and foreslope environment formed under sediment-buffered conditions. This spatial pattern of dolomitizing conditions is consistent with buoyant recirculation of glacial seawater within carbonate platforms driven by the deglacial sea-level rise and development of a meltwater surface ocean. Using a numerical diagenetic model to evaluate the geochemical differences between sediment- and fluid-buffered cap dolostone units, we constrain the chemical and isotopic composition of both the dolomitizing fluid (glacial seawater [δ13C ∼ 0–2‰]), the meltwater lens (δ13C ∼−11‰), and the primary aragonite sediment (δ13C ∼−6 to −3‰). These model end-members do not imply that primary geochemical variability did not exist but demonstrates that it is not necessary to change the chemistry of seawater to explain the global stratigraphic variability in the geochemistry of basal Ediacaran cap dolostones. Our results provide a novel framework for understanding the geochemical variability of cap dolostone units, including large excursions in carbon isotopes, and how this variability is the product of local diagenetic processes expressed globally in continental margin environments following the last Snowball Earth.",
keywords = "Ca isotopes, cap carbonate, diagenesis, Mg isotopes, Snowball Earth",
author = "Ahm, {Anne Sofie C.} and Maloof, {Adam C.} and Macdonald, {Francis A.} and Hoffman, {Paul F.} and Bjerrum, {Christian J.} and Uyanga Bold and Rose, {Catherine V.} and Strauss, {Justin V.} and Higgins, {John A.}",
year = "2019",
doi = "10.1016/j.epsl.2018.10.046",
language = "English",
volume = "506",
pages = "292--307",
journal = "Earth and Planetary Science Letters",
issn = "0012-821X",
publisher = "Elsevier",

}

RIS

TY - JOUR

T1 - An early diagenetic deglacial origin for basal Ediacaran “cap dolostones”

AU - Ahm, Anne Sofie C.

AU - Maloof, Adam C.

AU - Macdonald, Francis A.

AU - Hoffman, Paul F.

AU - Bjerrum, Christian J.

AU - Bold, Uyanga

AU - Rose, Catherine V.

AU - Strauss, Justin V.

AU - Higgins, John A.

PY - 2019

Y1 - 2019

N2 - The beginning of the Ediacaran Period (∼635 Ma) is marked by conspicuous dolostone units that cap Marinoan glacial deposits worldwide. The extent and sedimentary characteristics of the cap dolostones indicate that anomalous carbonate over-saturation coincided with deglacial sea-level rise and ocean warming. However, the geochemical variability within cap dolostones, both between continents, across single continental margins, and within individual stratigraphic sections has been difficult to reconcile with depositional models. Using a compilation of new calcium and magnesium isotope measurements in Marinoan cap dolostone successions worldwide, we show that the geochemical variability can be explained by early diagenetic dolomitization of aragonite along a spectrum of fluid- and sediment-buffered conditions. Dolostones from the outer platform formed under fluid-buffered conditions, whereas dolostones on the inner platform and foreslope environment formed under sediment-buffered conditions. This spatial pattern of dolomitizing conditions is consistent with buoyant recirculation of glacial seawater within carbonate platforms driven by the deglacial sea-level rise and development of a meltwater surface ocean. Using a numerical diagenetic model to evaluate the geochemical differences between sediment- and fluid-buffered cap dolostone units, we constrain the chemical and isotopic composition of both the dolomitizing fluid (glacial seawater [δ13C ∼ 0–2‰]), the meltwater lens (δ13C ∼−11‰), and the primary aragonite sediment (δ13C ∼−6 to −3‰). These model end-members do not imply that primary geochemical variability did not exist but demonstrates that it is not necessary to change the chemistry of seawater to explain the global stratigraphic variability in the geochemistry of basal Ediacaran cap dolostones. Our results provide a novel framework for understanding the geochemical variability of cap dolostone units, including large excursions in carbon isotopes, and how this variability is the product of local diagenetic processes expressed globally in continental margin environments following the last Snowball Earth.

AB - The beginning of the Ediacaran Period (∼635 Ma) is marked by conspicuous dolostone units that cap Marinoan glacial deposits worldwide. The extent and sedimentary characteristics of the cap dolostones indicate that anomalous carbonate over-saturation coincided with deglacial sea-level rise and ocean warming. However, the geochemical variability within cap dolostones, both between continents, across single continental margins, and within individual stratigraphic sections has been difficult to reconcile with depositional models. Using a compilation of new calcium and magnesium isotope measurements in Marinoan cap dolostone successions worldwide, we show that the geochemical variability can be explained by early diagenetic dolomitization of aragonite along a spectrum of fluid- and sediment-buffered conditions. Dolostones from the outer platform formed under fluid-buffered conditions, whereas dolostones on the inner platform and foreslope environment formed under sediment-buffered conditions. This spatial pattern of dolomitizing conditions is consistent with buoyant recirculation of glacial seawater within carbonate platforms driven by the deglacial sea-level rise and development of a meltwater surface ocean. Using a numerical diagenetic model to evaluate the geochemical differences between sediment- and fluid-buffered cap dolostone units, we constrain the chemical and isotopic composition of both the dolomitizing fluid (glacial seawater [δ13C ∼ 0–2‰]), the meltwater lens (δ13C ∼−11‰), and the primary aragonite sediment (δ13C ∼−6 to −3‰). These model end-members do not imply that primary geochemical variability did not exist but demonstrates that it is not necessary to change the chemistry of seawater to explain the global stratigraphic variability in the geochemistry of basal Ediacaran cap dolostones. Our results provide a novel framework for understanding the geochemical variability of cap dolostone units, including large excursions in carbon isotopes, and how this variability is the product of local diagenetic processes expressed globally in continental margin environments following the last Snowball Earth.

KW - Ca isotopes

KW - cap carbonate

KW - diagenesis

KW - Mg isotopes

KW - Snowball Earth

U2 - 10.1016/j.epsl.2018.10.046

DO - 10.1016/j.epsl.2018.10.046

M3 - Journal article

AN - SCOPUS:85056702038

VL - 506

SP - 292

EP - 307

JO - Earth and Planetary Science Letters

JF - Earth and Planetary Science Letters

SN - 0012-821X

ER -

ID: 226912860