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Published June 26, 2018 | Published + Supplemental Material
Journal Article Open

Oxygen isotope composition of the Phanerozoic ocean and a possible solution to the dolomite problem

Abstract

The ^(18)O/^(16)O of calcite fossils increased by ∼8‰ between the Cambrian and present. It has long been controversial whether this change reflects evolution in the δ^(18)O of seawater, or a decrease in ocean temperatures, or greater extents of diagenesis of older strata. Here, we present measurements of the oxygen and "clumped" isotope compositions of Phanerozoic dolomites and compare these data with published oxygen isotope studies of carbonate rocks. We show that the δ^(18)O values of dolomites and calcite fossils of similar age overlap one another, suggesting they are controlled by similar processes. Clumped isotope measurements of Cambrian to Pleistocene dolomites imply crystallization temperatures of 15–158 °C and parent waters having δ^(18)O_(VSMOW) values from −2 to +12‰. These data are consistent with dolomitization through sediment/rock reaction with seawater and diagenetically modified seawater, over timescales of 100 My, and suggest that, like dolomite, temporal variations of the calcite fossil δ^(18)O record are largely driven by diagenetic alteration. We find no evidence that Phanerozoic seawater was significantly lower in δ^(18)O than preglacial Cenozoic seawater. Thus, the fluxes of oxygen–isotope exchange associated with weathering and hydrothermal alteration reactions have remained stable throughout the Phanerozoic, despite major tectonic, climatic and biologic perturbations. This stability implies that a long-term feedback exists between the global rates of seafloor spreading and weathering. We note that massive dolomites have crystallized in pre-Cenozoic units at temperatures >40 °C. Since Cenozoic platforms generally have not reached such conditions, their thermal immaturity could explain their paucity of dolomites.

Additional Information

© 2018 National Academy of Sciences. Published under the PNAS license. Edited by Donald E. Canfield, University of Southern Denmark, Odense, Denmark, and approved May 16, 2018 (received for review November 10, 2017). Published ahead of print June 11, 2018. We thank Yael Kiro, Max K. Lloyd, and Alex Lipp for assisting in the field and with sample preparation procedures; two anonymous reviewers for their detailed and constructive comments; and the Grand Canyon National Park and the US Geological Survey Core Research Center for facilitating sample collection. This work was supported by NSF Grant EAR-1624827 (to J.M.E.). U.R. was supported by an O. K. Earl fellowship during this study. Author contributions: U.R. and J.M.E. designed research, performed research, analyzed data, and wrote the paper. The authors declare no conflict of interest. This article is a PNAS Direct Submission. This article contains supporting information online at www.pnas.org/lookup/suppl/doi:10.1073/pnas.1719681115/-/DCSupplemental.

Attached Files

Published - 6602.full.pdf

Supplemental Material - pnas.1719681115.sapp.pdf

Supplemental Material - pnas.1719681115.sd01.xlsx

Supplemental Material - pnas.1719681115.sd02.xlsx

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Additional details

Created:
August 22, 2023
Modified:
October 18, 2023