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      Multiple episodes of extensive marine anoxia linked to global warming and continental weathering following the latest Permian mass extinction

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          Abstract

          Multiple episodes of extensive oceanic anoxia delayed the marine ecosystem recovery from the latest Permian mass extinction.

          Abstract

          Explaining the ~5-million-year delay in marine biotic recovery following the latest Permian mass extinction, the largest biotic crisis of the Phanerozoic, is a fundamental challenge for both geological and biological sciences. Ocean redox perturbations may have played a critical role in this delayed recovery. However, the lack of quantitative constraints on the details of Early Triassic oceanic anoxia (for example, time, duration, and extent) leaves the links between oceanic conditions and the delayed biotic recovery ambiguous. We report high-resolution U-isotope (δ 238U) data from carbonates of the uppermost Permian to lowermost Middle Triassic Zal section (Iran) to characterize the timing and global extent of ocean redox variation during the Early Triassic. Our δ 238U record reveals multiple negative shifts during the Early Triassic. Isotope mass-balance modeling suggests that the global area of anoxic seafloor expanded substantially in the Early Triassic, peaking during the latest Permian to mid-Griesbachian, the late Griesbachian to mid-Dienerian, the Smithian-Spathian transition, and the Early/Middle Triassic transition. Comparisons of the U-, C-, and Sr-isotope records with a modeled seawater PO 4 3− concentration curve for the Early Triassic suggest that elevated marine productivity and enhanced oceanic stratification were likely the immediate causes of expanded oceanic anoxia. The patterns of redox variation documented by the U-isotope record show a good first-order correspondence to peaks in ammonoid extinctions during the Early Triassic. Our results indicate that multiple oscillations in oceanic anoxia modulated the recovery of marine ecosystems following the latest Permian mass extinction.

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          Lethally hot temperatures during the Early Triassic greenhouse.

          Global warming is widely regarded to have played a contributing role in numerous past biotic crises. Here, we show that the end-Permian mass extinction coincided with a rapid temperature rise to exceptionally high values in the Early Triassic that were inimical to life in equatorial latitudes and suppressed ecosystem recovery. This was manifested in the loss of calcareous algae, the near-absence of fish in equatorial Tethys, and the dominance of small taxa of invertebrates during the thermal maxima. High temperatures drove most Early Triassic plants and animals out of equatorial terrestrial ecosystems and probably were a major cause of the end-Smithian crisis.
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            The geochemistry of redox sensitive trace metals in sediments

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              The strontium isotope budget of the modern ocean

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                Author and article information

                Journal
                Sci Adv
                Sci Adv
                SciAdv
                advances
                Science Advances
                American Association for the Advancement of Science
                2375-2548
                April 2018
                11 April 2018
                : 4
                : 4
                : e1602921
                Affiliations
                [1 ]School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287–6004, USA.
                [2 ]Department of Geology, University of Cincinnati, Cincinnati, OH 45221–0013, USA.
                [3 ]State Key Laboratories of Biogeology and Environmental Geology and Geological Processes and Mineral Resources, China University of Geosciences, Wuhan 430074, China.
                [4 ]Deparment of Earth Sciences, University of California, Riverside, Riverside, CA 92521, USA.
                [5 ]Department of Earth and Planetary Sciences, University of California, Santa Cruz, Santa Cruz, CA 95064, USA.
                [6 ]Institute of Earth Sciences, NAWI Graz, University of Graz, Heinrichstraße 26, 8010 Graz, Austria.
                [7 ]Department of Geology, Lund University, Sölvegatan 12, 22362 Lund, Sweden.
                [8 ]Department of Geology and Geophysics, Louisiana State University, Baton Rouge, LA 70803, USA.
                [9 ]Lehr- und Forschungszentrum Francisco-Josephinum, 3250 Wieselburg, Austria.
                [10 ]Department of Lithospheric Research, Vienna University, Althanstr. 14, 1090 Vienna, Austria.
                [11 ]School of Molecular Sciences, Arizona State University, Tempe, AZ, 85287, USA.
                Author notes
                [* ]Corresponding author. Email: fzhang48@ 123456asu.edu
                Author information
                http://orcid.org/0000-0003-3277-445X
                http://orcid.org/0000-0003-1582-6801
                http://orcid.org/0000-0002-3333-7035
                http://orcid.org/0000-0002-2273-8319
                http://orcid.org/0000-0003-4867-7304
                http://orcid.org/0000-0001-5424-3540
                http://orcid.org/0000-0001-8806-9659
                http://orcid.org/0000-0002-2471-1232
                http://orcid.org/0000-0002-6015-7750
                Article
                1602921
                10.1126/sciadv.1602921
                5895439
                30105ea1-a5a8-4454-a850-a93f5c941e81
                Copyright © 2018 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC).

                This is an open-access article distributed under the terms of the Creative Commons Attribution-NonCommercial license, which permits use, distribution, and reproduction in any medium, so long as the resultant use is not for commercial advantage and provided the original work is properly cited.

                History
                : 22 November 2016
                : 26 February 2018
                Funding
                Funded by: NSF Frontiers in Earth System Dynamics program;
                Award ID: EAR-1338810
                Funded by: NASA Exobiology Program;
                Award ID: NNX13AJ71G
                Categories
                Research Article
                Research Articles
                SciAdv r-articles
                Physical Sciences
                Geology
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