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      Event- and biostratigraphic evidence for two independent Ries and Steinheim asteroid impacts in the Middle Miocene

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          Abstract

          For decades, the Nördlinger Ries and Steinheim Basin in southern Germany have been regarded as a textbook example of a terrestrial impact crater doublet, although the oldest crater lake deposits in both craters suggest a biostratigraphic age difference of ~ 0.5 to 1 Myr. We previously presented stratigraphic arguments that challenged the double impact scenario and favoured a model of two temporally independent impact events in the Mid-Miocene. We here present, for the first time, four localities within a distance of ~ 50–100 km from the Ries and ~ 50–70 km from the Steinheim crater that expose two independent seismite horizons, together unique within the Upper Freshwater Molasse of the North Alpine Foreland Basin, each one featuring impressive water escape structures. The seismite horizons are separated by ~ 10 to 15 m of undisturbed Molasse deposits and, biostratigraphically, by an entire European Land Mammal Zone, thus providing evidence for two independent major seismic events within a time span of ~ 0.5–1 Myr. Both the lower and the upper seismite horizons can be correlated litho- and biostratigraphically with the basal crater lake sediments at the Ries and Steinheim craters, respectively, deposited immediately after the impacts. From a biostratigraphic point of view, the impact event that formed the Steinheim Basin probably occured around 14 Ma, some 0.8 Myr after the ~ 14.81 Ma Ries impact event.

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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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            The ICS International Chronostratigraphic Chart

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              Earth Impact Effects Program: A Web-based computer program for calculating the regional environmental consequences of a meteoroid impact on Earth

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                Author and article information

                Contributors
                elmar.buchner@hnu.de
                Journal
                Sci Rep
                Sci Rep
                Scientific Reports
                Nature Publishing Group UK (London )
                2045-2322
                3 November 2022
                3 November 2022
                2022
                : 12
                : 18603
                Affiliations
                [1 ]GRID grid.466058.9, HNU - Neu-Ulm University of Applied Sciences, ; Wileystraße 1, 89231 Neu-Ulm, Germany
                [2 ]Meteorkrater-Museum Steinheim, 89555 Steinheim am Albuch, Germany
                [3 ]Fokus Natur, Am Heselsberg 29, 88416 Ochsenhausen, Germany
                Article
                21409
                10.1038/s41598-022-21409-8
                9633785
                36329052
                c62b3fe9-fd06-4892-b1a1-ca45796b1a96
                © The Author(s) 2022

                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 licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence 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 licence, visit http://creativecommons.org/licenses/by/4.0/.

                History
                : 15 June 2022
                : 27 September 2022
                Funding
                Funded by: Stifterverband für die Deutsche Wissenschaft - Dieter Schwarz Stiftung
                Award ID: 11050
                Award Recipient :
                Funded by: Hochschule für angewandte Wissenschaften Neu-Ulm (3366)
                Categories
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                © The Author(s) 2022

                Uncategorized
                palaeontology,sedimentology,seismology,natural hazards,planetary science
                Uncategorized
                palaeontology, sedimentology, seismology, natural hazards, planetary science

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