Standard

Simulation of the explosive origin of a planetary satellite. / Anisichkin, V. F.; Pruuel, E. R.; Rubtsov, I. A.

In: Journal of Physics: Conference Series, Vol. 1147, No. 1, 012058, 18.01.2019.

Research output: Contribution to journal › Conference article › peer-review

Harvard

Anisichkin, VF, Pruuel, ER & Rubtsov, IA 2019, 'Simulation of the explosive origin of a planetary satellite', Journal of Physics: Conference Series, vol. 1147, no. 1, 012058. https://doi.org/10.1088/1742-6596/1147/1/012058

APA

Anisichkin, V. F., Pruuel, E. R., & Rubtsov, I. A. (2019). Simulation of the explosive origin of a planetary satellite. Journal of Physics: Conference Series, 1147(1), [012058]. https://doi.org/10.1088/1742-6596/1147/1/012058

Vancouver

Anisichkin VF, Pruuel ER, Rubtsov IA. Simulation of the explosive origin of a planetary satellite. Journal of Physics: Conference Series. 2019 Jan 18;1147(1):012058. doi: 10.1088/1742-6596/1147/1/012058

Author

Anisichkin, V. F. ; Pruuel, E. R. ; Rubtsov, I. A. / Simulation of the explosive origin of a planetary satellite. In: Journal of Physics: Conference Series. 2019 ; Vol. 1147, No. 1.

BibTeX

@article{48eafed696cf4b6e8c34b18ba124b499,
title = "Simulation of the explosive origin of a planetary satellite",
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.",
author = "Anisichkin, {V. F.} and Pruuel, {E. R.} and Rubtsov, {I. A.}",
year = "2019",
month = jan,
day = "18",
doi = "10.1088/1742-6596/1147/1/012058",
language = "English",
volume = "1147",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",
number = "1",
note = "33rd International Conference on Equations of State for Matter, ELBRUS 2018 ; Conference date: 01-03-2018 Through 06-03-2018",

}

RIS

TY - JOUR

T1 - Simulation of the explosive origin of a planetary satellite

AU - Anisichkin, V. F.

AU - Pruuel, E. R.

AU - Rubtsov, I. A.

PY - 2019/1/18

Y1 - 2019/1/18

N2 - 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.

AB - 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.

UR - http://www.scopus.com/inward/record.url?scp=85062413789&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/1147/1/012058

DO - 10.1088/1742-6596/1147/1/012058

M3 - Conference article

AN - SCOPUS:85062413789

VL - 1147

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012058

T2 - 33rd International Conference on Equations of State for Matter, ELBRUS 2018

Y2 - 1 March 2018 through 6 March 2018

ER -

ID: 18680505