T241 The Cretaceous–Paleogene Boundary: From Impact Cratering Processes to Mass Extinction Mechanisms
Wednesday, 13 October 2021
1:30 PM - 5:30 PM
D139/D140
NEW INSIGHTS INTO THE FORMATION AND EMPLACEMENT OF IMPACT MELT ROCKS WITHIN THE CHICXULUB IMPACT STRUCTURE, FOLLOWING THE 2016 IODP-ICDP EXPEDITION 364
Paper number: T241-4
Program: Technical Sessions
Time: 2:10 PM – 2:25 PM
Authors
-
Christian KoeberlUniversity of Vienna, Vienna
-
Jan SmitVrije Universiteit Amsterdam, Amsterdam
-
Nadine MattielliUniversité Libre de Bruxelles, Brussels
-
Philippe ClaeysVrije Universiteit Brussel, Brussels
-
Pim KaskesVrije Universiteit Brussel, Brussels
-
Pim KaskesUniversité Libre de Bruxelles, Brussels
-
Thomas DehaisUniversité Libre de Bruxelles, Brussels
-
Thomas DehaisVrije Universiteit Brussel, Brussels
-
Steven GoderisVrije Universiteit Brussel, Brussels
-
Vinciane DebailleUniversité Libre de Bruxelles, Brussels
-
Catherine RossJackson School of Geosciences, University of Texas at Austin, Austin, TX
-
Sean P.S. GulickUniversity of Texas at Austin, Austin, TX
-
Sean P.S. GulickJackson School of Geosciences, University of Texas at Austin, Austin, TX
-
Jean-Guillaume FeignonUniversity of Vienna, Vienna
-
Ludovic FerrièreNatural History Museum, Vienna
Abstract
We subdivide the Chicxulub impact melt rocks into two groups: the lower impact melt rock–bearing unit, which intrudes the granitoid peak ring at different intervals, and the upper impact melt rock unit, which overlies the peak ring basement. The geochemical characterization in major and trace element, and isotopic composition of the impact melt rock units and five identified pre-impact lithologies (i.e., granitoid, dolerite, dacite, felsite, and limestone) reveals that the composition of impact melt rock can be explained by the mixing of the primarily felsic and mafic lithologies, but with various degrees of carbonate dilution. The bulk geochemical composition of the pre-impact lithologies constrains the composition of both impact melt rock units. As such, these pre-impact lithologies likely represent the main constituents that were melted to form the impact melt rock and also suggests that these lithologies are likely pervasive throughout the Yucatán subsurface.
Following these observations, we suggest that the two impact melt rock units were initially part of the same impact-produced melt, but discrete processes separated them during crater formation. The lower impact melt rock–bearing unit is interpreted to represent impact melt rock injected into the crystalline basement during the compression/excavation stage of cratering. These impact melt rock layers likely acted as delamination surfaces within the crystalline basement, accommodating its displacement during peak ring formation. The composition of the upper impact melt rock unit was contingent on the entrainment of carbonate components and is interpreted to have lined the transient crater surface during crater development. The upper melt formation was not finalized until the modification stage, when carbonate material would have re-entered the crater.
Geological Society of America Abstracts with Programs. Vol. 53, No. 6
doi: 10.1130/abs/2021AM-369141
© Copyright 2021 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.