Age of the Sääksjärvi impact structure, Finland: reconciling the timing of small impacts in crystalline basement with regional basin development

Author:

Kenny Gavin G.1ORCID,Mänttäri Irmeli2,Schmieder Martin34ORCID,Whitehouse Martin J.1ORCID,Nemchin Alexander A.15,Bellucci Jeremy J.1,Merle Renaud E.1ORCID

Affiliation:

1. Department of Geosciences, Swedish Museum of Natural History, SE-104 05 Stockholm, Sweden

2. Radiation and Nuclear Safety AuthorityLaippatie 4, Box 14, FI-00811 Helsinki, Finland

3. Lunar and Planetary Institute – Universities Space Research Association, Houston, TX 77058, USA

4. Hochschule Neu-Ulm, Neu-Ulm University of Applied Sciences, D-89231 Neu-Ulm, Germany

5. School of Earth and Planetary Sciences, Curtin University, Perth, WA 6845, Australia

Abstract

We report a new age for the Sääksjärvi impact structure, Finland, a 6 km diameter feature that formed in crystalline rocks of the Precambrian Baltic Shield. Two previous studies reported 40Ar/39Ar data for Sääksjärvi and suggested conflicting formation ages of ≤330 Ma or c. 560 Ma. The former age represents a possible complication for models which indicate that the region was covered by sediments of the Caledonian foreland basin throughout much of the Phanerozoic. We conducted a study combining imaging, microstructural analysis and U–Pb dating of shocked zircon from Sääksjärvi. The U–Pb dataset indicates a c. 600 Ma impact into predominantly c. 1850 Ma target rocks. A concordia age of 608 ± 8 Ma (2σ) confirms Sääksjärvi as the first known Ediacaran impact structure in the Baltic Shield and only the second worldwide. Our data indicate that the Sääksjärvi impact structure formed in exposed crystalline basement rocks of the Baltic Shield prior to the development of the Caledonian foreland basin. Given that most impact structures on Earth are relatively small features, radiometric dating of small impact structures in crystalline basement may place boundaries on the timing and spatial extent of palaeobasins that might otherwise be difficult to constrain.Supplementary material: Additional imaging and microstructural analysis of zircon, additional concordia plots, and U–Pb data tables are available at https://doi.org/10.6084/m9.figshare.c.5043462

Funder

H2020 Marie Skłodowska-Curie Actions

Publisher

Geological Society of London

Subject

Geology

Reference71 articles.

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2. Bottomley, R.J. , York, D. and Grieve, R.A.F. 1990. 40Ar–39Ar dating of impact craters. Proceedings of the Lunar and Planetary Science Conference, 20, 421–431.

3. Buchner, E. , Moilanen, J. , Öhman, T. and Schmieder, M. 2009. Shock-molten sandstone clasts in impact melt rocks: age constraints for the Paasselkä impact structure (SE Finland). Abstract No. 2169 presented at the 40th Lunar and Planetary Science Conference, 23–27 March 2009; the Woodlands, TX, US.

4. A terrestrial perspective on usingex situshocked zircons to date lunar impacts

5. Transformations to granular zircon revealed: Twinning, reidite, and ZrO2in shocked zircon from Meteor Crater (Arizona, USA)

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