Please use this identifier to cite or link to this item: http://elar.urfu.ru/handle/10995/92679
Title: High pressure impacts on meteorites
Authors: Petrova, E. V.
Grokhovsky, V. I.
Issue Date: 2019
Publisher: De Gruyter
Citation: Petrova E. V. High pressure impacts on meteorites / E. V. Petrova, V. I. Grokhovsky. — DOI 10.1515/pac-2018-1119 // Pure and Applied Chemistry. — 2019. — Vol. 11. — Iss. 91. — P. 1857-1867.
Abstract: In the invited article, we review observations on changes in meteorite texture relevant to the early stages of formation of the Solar System based on the experimental shock wave loading of the material at the laboratory. Investigation of the physical and structural properties of high-pressure impacts on meteorites is important for few reasons, such as: Protection of the Earth from the near-Earth objects (NEOs); Study of processes that cannot yet be achieved under laboratory conditions; Understanding of conditions for asteroid mining. © 2019 IUPAC & De Gruyter. This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License. For more information, please visit: http://creativecommons.org/licenses/by-nc-nd/4.0/2019.
Keywords: FORMATION
HTMC-XVI
METEORITES
SHOCK EXPERIMENT
SHOCK FEATURES
STRUCTURE
METEORITES
SHOCK WAVES
STRUCTURE (COMPOSITION)
TEXTURES
FORMATION
HIGH PRESSURE
HTMC-XVI
LABORATORY CONDITIONS
NEAR EARTH OBJECTS
SHOCK FEATURES
SHOCK-WAVE LOADING
METEOR IMPACTS
URI: http://elar.urfu.ru/handle/10995/92679
Access: info:eu-repo/semantics/openAccess
SCOPUS ID: 85075488929
PURE ID: 11331730
ISSN: 0033-4545
DOI: 10.1515/pac-2018-1119
Appears in Collections:Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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