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      Precise radiometric age establishes Yarrabubba, Western Australia, as Earth’s oldest recognised meteorite impact structure

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          Abstract

          The ~70 km-diameter Yarrabubba impact structure in Western Australia is regarded as among Earth’s oldest, but has hitherto lacked precise age constraints. Here we present U–Pb ages for impact-driven shock-recrystallised accessory minerals. Shock-recrystallised monazite yields a precise impact age of 2229 ± 5 Ma, coeval with shock-reset zircon. This result establishes Yarrabubba as the oldest recognised meteorite impact structure on Earth, extending the terrestrial cratering record back >200 million years. The age of Yarrabubba coincides, within uncertainty, with temporal constraint for the youngest Palaeoproterozoic glacial deposits, the Rietfontein diamictite in South Africa. Numerical impact simulations indicate that a 70 km-diameter crater into a continental glacier could release between 8.7 × 10 13 to 5.0 × 10 15 kg of H 2O vapour instantaneously into the atmosphere. These results provide new estimates of impact-produced H 2O vapour abundances for models investigating termination of the Paleoproterozoic glaciations, and highlight the possible role of impact cratering in modifying Earth’s climate.

          Abstract

          The ~70 km-diameter Yarrabubba impact structure in Western Australia has previously been regarded as among Earth’s oldest meteorite craters, but has hitherto lacked absolute age constraints. Here, the authors determine a precise impact age of 2229 ± 5 Ma, which extends the terrestrial cratering record back in time by > 200 million years and establishes Yarrabubba as the oldest recognised meteorite impact structure on Earth.

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          Subcommission on geochronology: Convention on the use of decay constants in geo- and cosmochronology

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            The Chicxulub asteroid impact and mass extinction at the Cretaceous-Paleogene boundary.

            The Cretaceous-Paleogene boundary approximately 65.5 million years ago marks one of the three largest mass extinctions in the past 500 million years. The extinction event coincided with a large asteroid impact at Chicxulub, Mexico, and occurred within the time of Deccan flood basalt volcanism in India. Here, we synthesize records of the global stratigraphy across this boundary to assess the proposed causes of the mass extinction. Notably, a single ejecta-rich deposit compositionally linked to the Chicxulub impact is globally distributed at the Cretaceous-Paleogene boundary. The temporal match between the ejecta layer and the onset of the extinctions and the agreement of ecological patterns in the fossil record with modeled environmental perturbations (for example, darkness and cooling) lead us to conclude that the Chicxulub impact triggered the mass extinction.
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              U-Pb geochronology of zircons from lunar breccia 73217 using a sensitive high mass-resolution ion microprobe

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                Author and article information

                Contributors
                Timmons.M.Erickson@nasa.gov
                Journal
                Nat Commun
                Nat Commun
                Nature Communications
                Nature Publishing Group UK (London )
                2041-1723
                21 January 2020
                21 January 2020
                2020
                : 11
                : 300
                Affiliations
                [1 ]ISNI 0000 0004 0613 2864, GRID grid.419085.1, Jacobs—JETS, Astromaterials Research and Exploration Science Division, , NASA Johnson Space Center, ; 2101 NASA Parkway, Houston, TX 77058 USA
                [2 ]ISNI 0000 0004 0375 4078, GRID grid.1032.0, The Institute for Geoscience Research (TIGeR), Space Science and Technology Centre, School of Earth and Planetary Sciences, , Curtin University, ; GPO Box 1984, Perth, WA 6845 Australia
                [3 ]ISNI 0000 0000 8634 1877, GRID grid.410493.b, Center for Lunar Science and Exploration, Lunar and Planetary Institute, , Universities Space Research Association, ; 3600 Bay Area Blvd, Houston, TX 77058 USA
                [4 ]ISNI 0000 0004 0375 4078, GRID grid.1032.0, The Institute for Geoscience Research (TIGeR), Centre for Exploration Targeting—Curtin Node, School of Earth and Planetary Sciences, , Curtin University, ; GPO Box 1984, Perth, WA 6845 Australia
                [5 ]ISNI 0000 0001 2113 8111, GRID grid.7445.2, Impacts and Astromaterials Research Centre, Department of Earth Science and Engineering, , Imperial College London, ; London, SW7 2AZ UK
                Author information
                http://orcid.org/0000-0003-4520-7294
                http://orcid.org/0000-0003-3367-8961
                http://orcid.org/0000-0001-8790-873X
                Article
                13985
                10.1038/s41467-019-13985-7
                6974607
                31964860
                9611c4b3-8378-4ce5-b1bd-aaf22d118219
                © This is a U.S. government work and not under copyright protection in the U.S.; foreign copyright protection may apply 2020

                Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

                History
                : 12 March 2019
                : 11 December 2019
                Funding
                Funded by: FundRef https://doi.org/10.13039/501100000923, Department of Education and Training | Australian Research Council (ARC);
                Award ID: LE130100053
                Award Recipient :
                Funded by: Geological Society of Australia, Western Australia Division
                Categories
                Article
                Custom metadata
                © The Author(s) 2020

                Uncategorized
                planetary science,geochemistry,petrology
                Uncategorized
                planetary science, geochemistry, petrology

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