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An Early Jurassic age for the Puchezh-Katunki impact structure (Russia) based on 40Ar/39Ar data and palynology

Holm-Alwmark, S. LU ; Alwmark, C. LU ; Ferrière, L. ; Lindström, S. LU ; Meier, M. M.M. LU ; Scherstén, A. LU ; Herrmann, M. LU ; Masaitis, V. L. ; Mashchak, M. S. and Naumov, M. V. , et al. (2019) In Meteoritics and Planetary Science 54(8). p.1764-1780
Abstract

The Puchezh-Katunki impact structure, 40–80 km in diameter, located ~400 km northeast of Moscow (Russia), has a poorly constrained age between ~164 and 203 Ma (most commonly quoted as 167 ± 3 Ma). Due to its relatively large size, the Puchezh-Katunki structure has been a prime candidate for discussions on the link between hypervelocity impacts and extinction events. Here, we present new 40Ar/39Ar data from step-heating analysis of five impact melt rock samples that allow us to significantly improve the age range for the formation of the Puchezh-Katunki impact structure to 192–196 Ma. Our results also show that there is not necessarily a simple relationship between the observed petrographic features of an impact... (More)

The Puchezh-Katunki impact structure, 40–80 km in diameter, located ~400 km northeast of Moscow (Russia), has a poorly constrained age between ~164 and 203 Ma (most commonly quoted as 167 ± 3 Ma). Due to its relatively large size, the Puchezh-Katunki structure has been a prime candidate for discussions on the link between hypervelocity impacts and extinction events. Here, we present new 40Ar/39Ar data from step-heating analysis of five impact melt rock samples that allow us to significantly improve the age range for the formation of the Puchezh-Katunki impact structure to 192–196 Ma. Our results also show that there is not necessarily a simple relationship between the observed petrographic features of an impact melt rock sample and the obtained 40Ar/39Ar age spectra and inverse isochrons. Furthermore, a new palynological investigation of the postimpact crater lake sediments supports an age significantly older than quoted in the literature, i.e., in the interval late Sinemurian to early Pliensbachian, in accordance with the new radioisotopic age estimate presented here. The new age range of the structure is currently the most reliable age estimate of the Puchezh-Katunki impact event.

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organization
publishing date
type
Contribution to journal
publication status
published
subject
in
Meteoritics and Planetary Science
volume
54
issue
8
pages
1764 - 1780
publisher
Wiley-Blackwell
external identifiers
  • scopus:85066464285
ISSN
1086-9379
DOI
10.1111/maps.13309
project
Geochronology of impact structures - constraining syn- and post-impact processes using the 40Ar/39Ar and U-Pb techniques
language
English
LU publication?
yes
id
ffaa5194-8e70-4cef-807f-ab039695e35e
date added to LUP
2019-06-25 14:37:30
date last changed
2023-04-09 18:09:21
@article{ffaa5194-8e70-4cef-807f-ab039695e35e,
  abstract     = {{<p>The Puchezh-Katunki impact structure, 40–80 km in diameter, located ~400 km northeast of Moscow (Russia), has a poorly constrained age between ~164 and 203 Ma (most commonly quoted as 167 ± 3 Ma). Due to its relatively large size, the Puchezh-Katunki structure has been a prime candidate for discussions on the link between hypervelocity impacts and extinction events. Here, we present new <sup>40</sup>Ar/<sup>39</sup>Ar data from step-heating analysis of five impact melt rock samples that allow us to significantly improve the age range for the formation of the Puchezh-Katunki impact structure to 192–196 Ma. Our results also show that there is not necessarily a simple relationship between the observed petrographic features of an impact melt rock sample and the obtained <sup>40</sup>Ar/<sup>39</sup>Ar age spectra and inverse isochrons. Furthermore, a new palynological investigation of the postimpact crater lake sediments supports an age significantly older than quoted in the literature, i.e., in the interval late Sinemurian to early Pliensbachian, in accordance with the new radioisotopic age estimate presented here. The new age range of the structure is currently the most reliable age estimate of the Puchezh-Katunki impact event.</p>}},
  author       = {{Holm-Alwmark, S. and Alwmark, C. and Ferrière, L. and Lindström, S. and Meier, M. M.M. and Scherstén, A. and Herrmann, M. and Masaitis, V. L. and Mashchak, M. S. and Naumov, M. V. and Jourdan, F.}},
  issn         = {{1086-9379}},
  language     = {{eng}},
  month        = {{05}},
  number       = {{8}},
  pages        = {{1764--1780}},
  publisher    = {{Wiley-Blackwell}},
  series       = {{Meteoritics and Planetary Science}},
  title        = {{An Early Jurassic age for the Puchezh-Katunki impact structure (Russia) based on <sup>40</sup>Ar/<sup>39</sup>Ar data and palynology}},
  url          = {{http://dx.doi.org/10.1111/maps.13309}},
  doi          = {{10.1111/maps.13309}},
  volume       = {{54}},
  year         = {{2019}},
}