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dc.contributor.authorSchmitt, R. T.
dc.contributor.authorWittmann, A.
dc.contributor.authorStöffler, D.
dc.date.accessioned2021-02-12T22:54:17Z
dc.date.available2021-02-12T22:54:17Z
dc.date.issued2004-01-01
dc.identifier.citationSchmitt, R. T., Wittmann, A., & Stöffler, D. (2004). Geochemistry of drill core samples from Yaxcopoil‐1, Chicxulub impact crater, Mexico. Meteoritics & Planetary Science, 39(6), 979-1001.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2004.tb00940.x
dc.identifier.urihttp://hdl.handle.net/10150/656682
dc.description.abstractThe chemical composition of suevites, displaced Cretaceous target rocks, and impactgenerated dikes within these rocks from the Yaxcopoil-1 (Yax-1) drill core, Chicxulub impact crater, Mexico, is reported and compared with the data from the Yucatán 6 (Y6) samples. Within the six suevite subunits of Yax-1, four units with different chemical compositions can be distinguished: a) upper/lower sorted and upper suevite (depth of 795-846 m); b) middle suevite (depth of 846-861 m); degrees C) brecciated impact melt rock (depth of 861-885 m); and d) lower suevite (depth of 885-895 m). The suevite sequence (a), (b), and (d) display an increase of the CaO content and a decrease of the silicate basement component from top to bottom. In contrast, the suevite of Y6 shows an inverse trend. The different distances of the Yax-1 and Y6 drilling sites from the crater center (~60, and ~47 km, respectively) lead to different suevite sequences. Within the Cretaceous rocks of Yax-1, a suevitic dike (depth of ~916 m) does not display chemical differences when compared with the suevite, while an impact melt rock dike (depth of ~1348 m) is significantly enriched in immobile elements. A clastic breccia dike (depth of ~1316 m) is dominated by material derived locally from the host rock, while the silicate-rich component is similar to that found in the suevite. Significant enrichments of the K2O content were observed in the Yax-1 suevite and the impact-generated dikes. All impactites of Yax-1 and Y6 are mixtures of a crystalline basement and a carbonate component from the sedimentary cover. An anhydrite component in the impactites is missing (Yax-1) or negligible (Y6).
dc.language.isoen
dc.publisherThe Meteoritical Society
dc.relation.urlhttps://meteoritical.org/
dc.rightsCopyright © The Meteoritical Society
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectYaxcopoil-1
dc.subjectChicxulub
dc.subjectgeochemistry
dc.subjectsuevite
dc.titleGeochemistry of drill core samples from Yaxcopoil-1, Chicxulub impact crater, Mexico
dc.typeArticle
dc.typetext
dc.identifier.journalMeteoritics & Planetary Science
dc.description.collectioninformationThe Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information.
dc.eprint.versionFinal published version
dc.description.admin-noteMigrated from OJS platform February 2021
dc.source.volume39
dc.source.issue6
dc.source.beginpage979
dc.source.endpage1001
refterms.dateFOA2021-02-12T22:54:17Z


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