| Literature DB >> 33627429 |
Steven Goderis1, Honami Sato2,3, Ludovic Ferrière4, Birger Schmitz5, David Burney6, Pim Kaskes7,8, Johan Vellekoop7,9, Axel Wittmann10, Toni Schulz11,12, Stepan M Chernonozhkin13, Philippe Claeys7, Sietze J de Graaff7,8, Thomas Déhais7,8, Niels J de Winter7,14, Mikael Elfman5, Jean-Guillaume Feignon11, Akira Ishikawa15,3, Christian Koeberl11, Per Kristiansson5, Clive R Neal6, Jeremy D Owens16, Martin Schmieder17,18, Matthias Sinnesael7,19, Frank Vanhaecke13, Stijn J M Van Malderen13, Timothy J Bralower20, Sean P S Gulick21,22,23, David A Kring18, Christopher M Lowery21, Joanna V Morgan24, Jan Smit25, Michael T Whalen26.
Abstract
The Cretaceous-Paleogene (K-Pg) mass extinction is marked globally by elevated concentrations of iridium, emplaced by a hypervelocity impact event 66 million years ago. Here, we report new data from four independent laboratories that reveal a positive iridium anomaly within the peak-ring sequence of the Chicxulub impact structure, in drill core recovered by IODP-ICDP Expedition 364. The highest concentration of ultrafine meteoritic matter occurs in the post-impact sediments that cover the crater peak ring, just below the lowermost Danian pelagic limestone. Within years to decades after the impact event, this part of the Chicxulub impact basin returned to a relatively low-energy depositional environment, recording in unprecedented detail the recovery of life during the succeeding millennia. The iridium layer provides a key temporal horizon precisely linking Chicxulub to K-Pg boundary sections worldwide.Entities:
Year: 2021 PMID: 33627429 DOI: 10.1126/sciadv.abe3647
Source DB: PubMed Journal: Sci Adv ISSN: 2375-2548 Impact factor: 14.136