DataVXJournal of Laser ApplicationsPaper
journal article·2011-02-01Open access

Behavior of basalt under laser-induced shock-wave application to the planetary hypervelocity impact effect

Laurent Berthe, Natalia S. Bezaeva, Jerôme Gattaceca, Michel Boustie, Thibaut de Rességuier, Pierre Rochette

Journal of Laser Applications· Volume 23· Issue 1
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Source abstract

Abstract

This paper presents the results of an investigation of the impact of laser-induced shock on basalt samples in a water confinement regime. In order to observe the effect of laser shock-wave propagation, in this material, the rear free surface velocity is measured by a velocimetry interferometer system for any reflector under various specified conditions. Parameters for an elastoplastic constitutive law and the Kanel’s damage model are provided and have been set up in such a way to ensure good correlation between numerical simulations and laboratory experiments. These resultant material properties, identified for the basalt sample studied here, could be used in future investigations looking to further correlating residual effects in material with pressure levels induced by water confined laser-matter interaction. This is of particular importance in meteoritics and planetary science due to the fact that hypervelocity impacts represent a major event taking place in the solar system, and shock waves generated during hypervelocity impacts can significantly affect physical properties of extraterrestrial materials and solid solar system bodies such as Mars, the Moon, asteroids, and others.
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Research context

OpenAlex topics: Surface Treatment and Residual Stress · High-Velocity Impact and Material Behavior · Planetary Science and Exploration

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

UPR CNRS 8006/ARTS et METIERS PARIS TECH Laboratoire PIMM, , 151 Boulevard de l’Hôpital, 75013 Paris, France

UMR CNRS/Aix-Marseille Université CEREGE, , BP 80, 13545 Aix-en-Provence Cedex 4, France; Department of Earth Science and Engineering, , South Kensington Campus, London SW7 2AZ, United Kingdom; and Earth Physics Department, Faculty of Physics, , Leninskie gory, 119991 Moscow, Russia

Imperial College London CEREGE, , BP 80, 13545 Aix-en-Provence Cedex 4, France; Department of Earth Science and Engineering, , South Kensington Campus, London SW7 2AZ, United Kingdom; and Earth Physics Department, Faculty of Physics, , Leninskie gory, 119991 Moscow, Russia

M.V. Lomonosov Moscow State University CEREGE, , BP 80, 13545 Aix-en-Provence Cedex 4, France; Department of Earth Science and Engineering, , South Kensington Campus, London SW7 2AZ, United Kingdom; and Earth Physics Department, Faculty of Physics, , Leninskie gory, 119991 Moscow, Russia

UMR CNRS/Aix-Marseille Université CEREGE, , BP 80, 13545 Aix-en-Provence Cedex 4, France

ENSMA Laboratoire de Combustion et de Détonique, UPR CNRS 9028, , 1 Avenue C. Ader, B.P. 40109, 86961 Futuroscope Cedex, France

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