Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/10510
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dc.contributor.authorKale, Vivek S.en_US
dc.contributor.authorUpasani, Devdutten_US
dc.contributor.authorRajput, Madhuen_US
dc.contributor.authorDole, Gaurien_US
dc.contributor.authorPATIL PILLAI, SHILPAen_US
dc.date.accessioned2025-11-07T10:13:09Z
dc.date.available2025-11-07T10:13:09Z
dc.date.issued2025-11en_US
dc.identifier.citationGSA Bulletinen_US
dc.identifier.issn943-2674en_US
dc.identifier.issn0016-7606en_US
dc.identifier.urihttps://doi.org/10.1130/B38412.1en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/10510
dc.description.abstractThe recognition of Deccan flood basalts as a causal mechanism for the Terminal Cretaceous Mass Extinction has been contentious. Our computation of their spatio-temporal distribution reiterates that ∼1.5 million km3 of the Deccan flood basalts erupted in <700 k.y., during Chron C29r (66.31−65.73 Ma) straddling the 66.05 Ma Cretaceous-Paleogene boundary (KPgB). Unlike earlier projections, we demonstrate that ∼70% of these lavas erupted in the terminal Maastrichtian before the KPgB. The toxic degassing of the lavas in the ∼300 k.y. prior to the KPgB set the stage for mass extinction. The early Danian lavas contributed to the delayed biotic recovery.en_US
dc.language.isoenen_US
dc.publisherGeological Society of Americaen_US
dc.subjectDeccan volcanismen_US
dc.subjectDeccan flooden_US
dc.subjectShapeen_US
dc.subjectDivisionen_US
dc.subjectGrowthen_US
dc.subjectCurvatureen_US
dc.subjectDivisomeen_US
dc.subject2025-NOV-WEEK4en_US
dc.subjectTOC-NOV-2025en_US
dc.subject2025en_US
dc.titleSpatio-temporal volume recalibration shows Deccan volcanism caused Terminal Cretaceous Mass Extinctionen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Earth and Climate Scienceen_US
dc.identifier.sourcetitleGSA Bulletinen_US
dc.publication.originofpublisherForeignen_US
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