Reconstruction of Phanerozoic climate using carbonate clumped isotopes and implications for the oxygen isotopic composition of seawater

Author:

Thiagarajan Nivedita1,Lepland Aivo234,Ryb Uri5ORCID,Torsvik Trond H.6,Ainsaar Leho3ORCID,Hints Olle4ORCID,Eiler John1

Affiliation:

1. Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125

2. Section for Marine Geology, Geological Survey of Norway, Trondheim 7040, Norway

3. Department of Geology, University of Tartu, Tartu 50411, Estonia

4. Department of Geology, Tallinn University of Technology, Tallinn 19086, Estonia

5. The Fredy & Nadine Herrmann Institute of Earth Sciences, The Hebrew University of Jerusalem, Jerusalem 9190401, Israel

6. Department of Geosciences, University of Oslo, Oslo 0316, Norway

Abstract

The oxygen isotope ratio 18 O/ 16 O (expressed as a δ 18 O VSMOW value) in marine sedimentary rocks has increased by ~8‰ from the early Paleozoic to modern times. Interpretation of this trend is hindered by ambiguities in the temperature of formation of the carbonate, the δ 18 O seawater , and the effects of postdepositional diagenesis. Carbonate clumped isotope measurements, a temperature proxy, offer constraints on this problem. This thermometer is thermodynamically controlled in cases where carbonate achieves an equilibrium internal distribution of isotopes and is independent of the δ 18 O of the water from which the carbonate grew; therefore, it has a relatively rigorous chemical–physics foundation and can be applied to settings where the δ 18 O of the water is not known. We apply this technique to an exceptionally well-preserved Ordovician carbonate record from the Baltic Basin and present a framework for interpreting clumped isotope results and for reconstructing past δ 18 O seawater . We find that the seawater in the Ordovician had lower δ 18 O seawater values than previously estimated, highlighting the need to reassess climate records based on oxygen-isotopes, particularly where interpretations are based on assumptions regarding either the δ 18 O seawater or the temperature of deposition or diagenesis. We argue that an increase in δ 18 O seawater contributed to the long-term rise in the δ 18 O of marine sedimentary rocks since the early Paleozoic. This rise might have been driven by a change in the proportion of high- versus low-temperature water–rock interaction in the earth’s hydrosphere as a whole.

Funder

Research Council ofNorway

Estonian research Council

Publisher

Proceedings of the National Academy of Sciences

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