Publications
Small impact cratering processes produce distinctive charcoal assemblages
- Author(s)
- A. Losiak, C. M. Belcher, J. Plado, A. Jõeleht, C. D. K. Herd, R. S. Kofman, M. Szokaluk, W. Szczucinski, A. Muszynski, E. M. Wild, S. J. Baker
- Abstract
The frequency of crater-producing asteroid impacts on Earth is not known. Of the predicted Holocene asteroid impact craters of <200 m diameter, only ~30% have been located. Until now there has been no way to distinguish them from “normal” terrestrial structures unless pieces of iron meteorites were found nearby. We show that the reflective properties of charcoal found in the proximal ejecta of small impact craters are distinct from those produced by wildfires. Impact-produced charcoals and wildfire charcoals must derive from different heating regimes. We suggest that charcoal with specific reflective properties may help to recognize the meteoritic origin of small craters.
- Organisation(s)
- Isotope Physics
- External organisation(s)
- Polish Academy of Sciences (PAS), University of Exeter, University of Tartu, University of Alberta, Adam Mickiewicz University
- Journal
- Geology
- Volume
- 50
- Pages
- 1276-1280
- No. of pages
- 5
- ISSN
- 0091-7613
- DOI
- https://doi.org/10.1130/G50056.1
- Publication date
- 11-2022
- Peer reviewed
- Yes
- Austrian Fields of Science 2012
- 103014 Nuclear physics, 105102 General geophysics
- Keywords
- ASJC Scopus subject areas
- Geology
- Portal url
- https://ucris.univie.ac.at/portal/en/publications/small-impact-cratering-processes-produce-distinctive-charcoal-assemblages(cde97772-c229-4ba3-a358-566e7351165f).html