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dc.rights.license© 2021 The Authors. Published by Elsevier B.V.-
dc.contributor.authorOrmö, J.-
dc.contributor.authorGulick, S. P. S.-
dc.contributor.authorWhalen, M. T.-
dc.contributor.authorKing, D. T.-
dc.contributor.authorSturkell, E.-
dc.contributor.authorMorgan, Joanna-
dc.date.accessioned2022-02-15T14:12:15Z-
dc.date.available2022-02-15T14:12:15Z-
dc.date.issued2021-06-15-
dc.identifier.citationEarth and Planetary Science Letters 564: 116915(2021)es
dc.identifier.issn0004-6361-
dc.identifier.otherhttps://www.sciencedirect.com/science/article/pii/S0012821X21001746-
dc.identifier.urihttp://hdl.handle.net/20.500.12666/570-
dc.descriptionHighlights Debris-laden ocean resurge crested Chicxulub's peak ring and was at least 450 m deep. Dominant sediment deposition occurred after a rapid drop in resurge transport energy. Relative distribution of melt and target clasts hints at provenance and flow dynamics. A method to estimate impactor (thus indirectly, crater) size and/or paleobathymetry is proposed. Records of resurge depend on depositional setting within the marine-target crater.es
dc.description.abstractThe rim wall of water formed from even a modestly-sized marine impact may be kilometers in height. Although modeling has shown that this wave swiftly breaks and relatively rapidly loses energy during outwards travel from the impact site, the portion of the rim wall that collapses inwards may generate a resurge flow with tremendous transport energy. Here we compare the deposits generated by this ocean resurge inside one of the largest marine-target craters on Earth, the 200-km wide Chicxulub crater, Yucatán Peninsula, México, with resurge deposits (breccias) in eight drill cores from five other marine-target craters in Sweden and the United States. Examination of the wide range of cored locations within the craters, and target water depths (H) relative to modeled projectile diameters (d) reveal a high correlation between location, average clast frequency (), and from which any of the four variables can be obtained. The relationship shown here may provide an important tool for diagnosing marine impact cratering processes where there is limited understanding of crater size and/or paleobathymetry.es
dc.description.sponsorshipWe thank the HET and IAC resident astronomers and telescope operators for their support. A.N. was supported by the Polish National Science Centre grant no. 2015/19/B/ST9/02937. E.V. acknowledges support from the Spanish Ministerio de Ciencia Inovacion y Universidades under grant PGC2018-101950-B-100. K.K. was funded in part by the Gordon and Betty Moore Foundation's Data-Driven Discovery Initiative through Grant GBMF4561. This research was supported in part by PL-Grid Infrastructure. The HET is a joint project of the University of Texas at Austin, the Pennsylvania State University, Stanford University, Ludwig-Maximilians-Universitat Munchen, and Georg-August-Universitat Gottingen. The HET is named in honor of its principal benefactors, William P. Hobby and Robert E. Eberly. The Center for Exoplanets and Habitable Worlds is supported by the Pennsylvania State University, the Eberly College of Science, and the Pennsylvania Space Grant Consortium. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. This research has made use of NASA's Astrophysics Data System. The acknowledgements were compiled using the Astronomy Acknowledgement Generator. This research made use of SciPy (Jones et al. 2001). This research made use of the yt-project, a toolkit for analyzing and visualizing quantitative data (Turk et al. 2011). This research made use of matplotlib, a Python library for publication quality graphics (Hunter 2007). This research made use of Astropy, a community-developed core Python package for Astronomy (Astropy Collaboration 2013). IRAF is distributed by the National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under cooperative agreement with the National Science Foundation (Tody 1993). This research made use of NumPy (Walt et al. 2011). We thank the referee for comments that have significantly contributed to improving this paper.es
dc.language.isoenges
dc.publisherElsevier BVes
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-101950-B-I00/ES/ON THE ROCKS II/-
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internationales
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/-
dc.subjectMarine Target Crateres
dc.subjectResurge Depositses
dc.subjectChicxulub Crateres
dc.subjectSite M0077es
dc.subjectSuevitees
dc.subjectMelt Water Interactiones
dc.titleAssessing event magnitude and target water depth for marine-target impacts: Ocean resurge deposits in the Chicxulub M0077A drill core comparedes
dc.typeinfo:eu-repo/semantics/articlees
dc.identifier.doi10.1016/j.epsl.2021.116915-
dc.identifier.e-issn1432-0746-
dc.contributor.funderPolish National Science Centre-
dc.contributor.funderGordon and Betty Moore Foundation (GBMF)-
dc.description.peerreviewedPeerreviewes
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501-
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