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dc.contributor.authorBeard, Sky P.
dc.contributor.authorSwindle, Timothy D.
dc.contributor.authorLapen, Thomas J.
dc.contributor.authorKring, David A.
dc.date.accessioned2023-02-21T22:57:52Z
dc.date.available2023-02-21T22:57:52Z
dc.date.issued2022-12
dc.identifier.citationBeard, S. P., Swindle, T. D., Lapen, T. J., & Kring, D. A. (2022). A r‐A r and U‐P b ages of Chelyabinsk and a re‐evaluation of its impact chronology.en_US
dc.identifier.issn1086-9379
dc.identifier.doi10.1111/maps.13927
dc.identifier.urihttp://hdl.handle.net/10150/667919
dc.description.abstractThe LL5 chondrite Chelyabinsk has had numerous isotopic studies since its fall in 2013. These data have been used to suggest ~8 impact events recorded from multiple isotopic systems (e.g., Ar-Ar, U–Pb, Sm-Nd, Rb-Sr, among others). We report details of Ar-Ar and U-Pb results and re-evaluate the geochronology of Chelyabinsk. Argon has the youngest Ar-Ar age recorded in meteorites, 25 ± 11 Ma, and an older resetting event at ~2550 Ma. The U-Pb analysis has an upper concordia age of 4456 ± 23 Ma and a lower concordia age of 184 ± 200 Ma. The lower concordia intercept represents a later thermal event (e.g., an impact), the most recent time that lead loss occurred, and could represent resetting by the youngest event recorded by Ar-Ar. Combining our data with literature results, we find strong evidence of at least four impact events (~4450, 2550, 1700, 25 Ma), with some evidence for two additional impacts (~3700, 1000 Ma).en_US
dc.language.isoenen_US
dc.publisherWileyen_US
dc.rights© 2022 The Meteoritical Society.en_US
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/en_US
dc.subjectSpace and Planetary Scienceen_US
dc.subjectGeophysicsen_US
dc.titleAr-Ar and U-Pb ages of Chelyabinsk and a re-evaluation of its impact chronologyen_US
dc.typeArticleen_US
dc.identifier.eissn1945-5100
dc.contributor.departmentLunar and Planetary Laboratory, University of Arizonaen_US
dc.identifier.journalMeteoritics & Planetary Scienceen_US
dc.description.note12 month embargo; published 01 Dec 2022.en_US
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en_US
dc.eprint.versionFinal accepted manuscripten_US
dc.identifier.pii10.1111/maps.13927
dc.source.journaltitleMeteoritics & Planetary Science
dc.source.volume57
dc.source.issue12
dc.source.beginpage2276
dc.source.endpage2288


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