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VERA Seminar

Dating small impact craters on Earth

Anna Losiak, Planetary Geology Lab, Institute of Geological Sciences, Polish Academy of Sciences, Wrocław, Poland

Precise and accurate dating of impact craters 1) enables correlation of an impact structure formation with other geological events (e.g. the Chicxulub crater associated with the Cretaceous-Paleogene mass extinction) and with events in human history, 2) is crucial to determine the rate of the impact flux on Earth, and 3) helps us to better understand the overall geological history of the Earth.

Dating small (≲120 m in diameter) impact craters is a complex task. Dating methods based on radioisotopic systems such as 40Ar/39Ar, K/Ar, Rb/Sr or U/Pb are used for larger impact structures, but are not applicable or practical in case of smaller ones (due to lack of rocks with fully re-set isotopic clocks). Ages of craters younger than a couple of million years can be measured with 10Be and 26Al exposure dating methods on boulders, but it does not work for craters developed in unconsolidated target material. The most precise and accurate age of small (≲120 m) and young (<50 ka) craters can be obtained by means of 14C dating of organic material associated with an impact structure. Depending on the geological setting of the organics, only the minimum or the maximum age of the crater can be determined. Unless of course we find an organism that was killed by the impact event. Which we (most probably) did, a few times, in a few craters.

 

Donnerstag, 27.04.2017    16:30 Uhr

Victor-Franz-Hess-Hörsaal
Währinger Str. 17 (Kavalierstrakt, Zugang durch den Hof)
1090 Wien

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