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dc.contributor.authorJunium, Christopher
dc.contributor.authorZerkle, Aubrey Lea
dc.contributor.authorWitts, James
dc.contributor.authorIvany, Linda
dc.contributor.authorYancey, Thomas
dc.contributor.authorLiu, Chengjie
dc.contributor.authorClaire, Mark
dc.date.accessioned2022-03-24T09:40:51Z
dc.date.available2022-03-24T09:40:51Z
dc.date.issued2022-04-05
dc.identifier277631202
dc.identifier92c7d7c2-b240-4f90-9e64-d0caf0b2e099
dc.identifier85126844757
dc.identifier000789363900019
dc.identifier.citationJunium , C , Zerkle , A L , Witts , J , Ivany , L , Yancey , T , Liu , C & Claire , M 2022 , ' Massive perturbations to atmospheric sulfur in the aftermath of the Chicxulub impact ' , Proceedings of the National Academy of Sciences of the United States of America , vol. 119 , no. 14 , e2119194119 . https://doi.org/10.1073/pnas.2119194119en
dc.identifier.issn1091-6490
dc.identifier.otherORCID: /0000-0003-2324-1619/work/110423280
dc.identifier.otherORCID: /0000-0001-9518-089X/work/110423282
dc.identifier.urihttps://hdl.handle.net/10023/25079
dc.descriptionThis project has received funding from the National Science foundation (EAR 1455258 to C.K.J), the European Research Council under the European Union’s Horizon 2020 research and innovation programme (Grant 678812 to M.W.C.) and a University of St Andrews Global Fellowship (to C.K.J.).en
dc.description.abstractSulfate aerosols have long been implicated as a primary forcing agent of climate change and mass extinction in the aftermath of the end-Cretaceous Chicxulub bolide impact. However, uncertainty remains regarding the quantity, residence time, and degree to which impact-derived sulfur transited the stratosphere, where its climatic impact would have been maximized. Here, we present evidence of mass-independent fractionation of sulfur isotopes (S-MIF) preserved in Chicxulub impact ejecta materials deposited in a marine environment in the Gulf Coastal Plain of North America. The mass anomalous sulfur is present in Cretaceous–Paleogene event deposits but also extends into Early Paleogene sediments. These measurements cannot be explained by mass conservation effects or thermochemical sulfate reduction and therefore require sulfur-bearing gases in an atmosphere substantially different from the modern. Our data cannot discriminate between potential source reaction(s) that produced the S-MIF, but stratospheric photolysis of SO2 derived from the target rock or carbonyl sulfide produced by biomass burning are the most parsimonious explanations. Given that the ultimate fate of both of these gases is oxidation to sulfate aerosols, our data provide direct evidence for a long hypothesized primary role for sulfate aerosols in the postimpact winter and global mass extinction.
dc.format.extent871222
dc.language.isoeng
dc.relation.ispartofProceedings of the National Academy of Sciences of the United States of Americaen
dc.subjectK-Pg extinctionen
dc.subjectSulfur isotopesen
dc.subjectMass-independent fractionationen
dc.subjectMass extinctionen
dc.subjectSulfur cycleen
dc.subjectGE Environmental Sciencesen
dc.subjectDASen
dc.subjectSDG 13 - Climate Actionen
dc.subjectSDG 14 - Life Below Wateren
dc.subject.lccGEen
dc.titleMassive perturbations to atmospheric sulfur in the aftermath of the Chicxulub impacten
dc.typeJournal articleen
dc.contributor.sponsorEuropean Research Councilen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.contributor.institutionUniversity of St Andrews. School of Earth & Environmental Sciencesen
dc.contributor.institutionUniversity of St Andrews. St Andrews Isotope Geochemistryen
dc.identifier.doihttps://doi.org/10.1073/pnas.2119194119
dc.description.statusPeer revieweden
dc.identifier.grantnumber678812en


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