TY - JOUR
T1 - Ar-Ar and U-Pb ages of Chelyabinsk and a re-evaluation of its impact chronology
AU - Beard, Sky P.
AU - Swindle, Timothy D.
AU - Lapen, Thomas J.
AU - Kring, David A.
N1 - Publisher Copyright:
© 2022 The Meteoritical Society.
PY - 2022/12
Y1 - 2022/12
N2 - 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).
AB - 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).
UR - https://www.scopus.com/pages/publications/85143287027
UR - https://www.scopus.com/inward/citedby.url?scp=85143287027&partnerID=8YFLogxK
U2 - 10.1111/maps.13927
DO - 10.1111/maps.13927
M3 - Article
AN - SCOPUS:85143287027
SN - 1086-9379
VL - 57
SP - 2276
EP - 2288
JO - Meteoritics and Planetary Science
JF - Meteoritics and Planetary Science
IS - 12
ER -