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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10.1515-pac-2018-1119.pdf | 150,36 kB | Adobe PDF | View/Open |
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