Simulation of the explosive origin of a planetary satellite Full article
Conference |
XXXIII INTERNATIONAL CONFERENCE ON EQUATIONS OF STATE FOR MATTER 01-06 Mar 2018 , Elbrus |
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Journal |
Journal of Physics: Conference Series
ISSN: 1742-6588 |
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Output data | Year: 2019, Volume: 1147, Pages: 012058 Pages count : 6 DOI: 10.1088/1742-6596/1147/1/012058 | ||||
Tags | Equations of state; Explosives; Molecular dynamics; Moon; Orbits | ||||
Authors |
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Abstract:
Explosion in the planetary interior and the ejection of the part of outer layers of the planet into orbit to form a satellite makes it possible to explain the elemental and isotopic composition of the Moon. Satellite formation has been simulated for a two-dimensional geometry using molecular dynamics methods for up to hundreds of thousands particles. The particles are asteroid-size bodies (diameter of about 100 km) which interact with each other according to Newton's law. The properties of the compact material are described by a short-range potential. A number of calculations with varying initial conditions have shown the scenario of the explosive origin of the Moon to be realistic and preferred over other hypotheses.
Cite:
Anisichkin V.F.
, Pruuel E.R.
, Rubtsov I.A.
Simulation of the explosive origin of a planetary satellite
Journal of Physics: Conference Series. 2019. V.1147. P.012058. DOI: 10.1088/1742-6596/1147/1/012058 Scopus РИНЦ OpenAlex
Simulation of the explosive origin of a planetary satellite
Journal of Physics: Conference Series. 2019. V.1147. P.012058. DOI: 10.1088/1742-6596/1147/1/012058 Scopus РИНЦ OpenAlex
Identifiers:
Scopus: | 2-s2.0-85062413789 |
Elibrary: | 38704097 |
OpenAlex: | W2909327037 |
Citing:
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