Simulation of the explosive origin of a planetary satellite | Sciact

Simulation of the explosive origin of a planetary satellite Научная публикация

Конференция

XXXIII INTERNATIONAL CONFERENCE ON EQUATIONS OF STATE FOR MATTER
01-06 мар. 2018 , Elbrus

Журнал

Journal of Physics: Conference Series
ISSN: 1742-6588

Вых. Данные

Год: 2019, Том: 1147, Страницы: 012058 Страниц : 6 DOI: 10.1088/1742-6596/1147/1/012058

Ключевые слова

Equations of state; Explosives; Molecular dynamics; Moon; Orbits

Авторы

Anisichkin V F ^1,2 , Pruuel E R ^1,2 , Rubtsov I A ^1,2

Организации

1	Lavrentyev Institute of Hydrodynamics of the Siberian Branch of the Russian Academy of Sciences,
2	Novosibirsk State University

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.

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

Scopus:	2-s2.0-85062413789
РИНЦ:	38704097
OpenAlex:	W2909327037

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