Holocene impact craters on Earth

Author:

Losiak Anna12ORCID

Affiliation:

1. Institute of Geological Sciences, Polish Academy of Sciences , Wrocław , Poland

2. Universities Space Research Association , Houston , United States

Abstract

Abstract Impact craters are formed by collisions of cosmic bodies moving with hypervelocity. The formation of these features is not restricted to the distant geological past; new structures are constantly being created and at least 13 confirmed impact craters and crater fields have formed during the Holocene alone. This short review paper: (1) introduces the basics of the impact cratering process to physical geographers and Quaternary geologists; (2) provides a short description of representative examples of such features (Morasko, Kaali, Kamil, Ilumetsa); and (3) discusses the similarities and differences among very small craters, and contrasts these with larger impact structures. This manuscript may be useful to researchers planning to test whether a small Quaternary depression in the ground may be of impact origin.

Publisher

Walter de Gruyter GmbH

Subject

Earth and Planetary Sciences (miscellaneous)

Reference51 articles.

1. Aaloe, A 1963, ‘New data on the structure of Ilumetsa craters’, Eesti NSV Teaduste Akadeemia Geoloogia Instituudi uurimused, vol. 11, pp. 35–43.

2. Alvarez, LW, Alvarez, W, Asaro, F & Michel, HV 1980, ‘Extraterrestrial cause for the Cretaceous-Tertiary extinction’, Science, vol. 208, pp. 1095–1108.

3. Artemieva, N & Shuvalov, V 2019, ‘Atmospheric shock waves after impacts of cosmic bodies up to 1000 m in diameter’, Meteoritics & Planetary Science, vol. 54, pp. 592–608.

4. Barringer, DM 1909, ‘Meteor Crater (Formerly called Coon Mountain or Coon Butte) in Northern Central Arizona’, A paper read before the National Academy of Sciences, 16 November 1909.

5. Beauford, R 2015, Physical records of impacts in the early and modern solar system. Ph.D. thesis, University of Arkansas. Available from: . [10 April 2023].

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