Ar-Ar and U-Pb ages of Chelyabinsk and a re-evaluation of its impact chronology
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Chelyabinsk Manuscript_Resub_F ...
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Final Accepted Manuscript
Affiliation
Lunar and Planetary Laboratory, University of ArizonaIssue Date
2022-12
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WileyCitation
Beard, 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.Journal
Meteoritics & Planetary ScienceRights
© 2022 The Meteoritical Society.Collection Information
This 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.Abstract
The 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).Note
12 month embargo; published 01 Dec 2022.ISSN
1086-9379EISSN
1945-5100Version
Final accepted manuscriptae974a485f413a2113503eed53cd6c53
10.1111/maps.13927