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Dust torus formed by particles ejected from a celestial body at an arbitrary point of its elliptic orbit. / Orlov, S.A.; Kholshevnikov, K.V.

In: Celestial Mechanics and Dynamical Astronomy, Vol. 116, No. 1, 2013, p. 35-52.

Research output: Contribution to journal › Article

Harvard

Orlov, SA & Kholshevnikov, KV 2013, 'Dust torus formed by particles ejected from a celestial body at an arbitrary point of its elliptic orbit', Celestial Mechanics and Dynamical Astronomy, vol. 116, no. 1, pp. 35-52. https://doi.org/10.1007/s10569-013-9473-z

APA

Orlov, S. A., & Kholshevnikov, K. V. (2013). Dust torus formed by particles ejected from a celestial body at an arbitrary point of its elliptic orbit. Celestial Mechanics and Dynamical Astronomy, 116(1), 35-52. https://doi.org/10.1007/s10569-013-9473-z

Vancouver

Orlov SA, Kholshevnikov KV. Dust torus formed by particles ejected from a celestial body at an arbitrary point of its elliptic orbit. Celestial Mechanics and Dynamical Astronomy. 2013;116(1):35-52. https://doi.org/10.1007/s10569-013-9473-z

Author

Orlov, S.A. ; Kholshevnikov, K.V. / Dust torus formed by particles ejected from a celestial body at an arbitrary point of its elliptic orbit. In: Celestial Mechanics and Dynamical Astronomy. 2013 ; Vol. 116, No. 1. pp. 35-52.

BibTeX

@article{0cd63617e93c47bc8c010e04cd6e5f0e,
title = "Dust torus formed by particles ejected from a celestial body at an arbitrary point of its elliptic orbit",
abstract = "Dust complexes form one of the Solar System components. The surface shape of a typical dust complex filled up by particles ejected from a celestial body is found within an analytical approach using reasonable assumptions (the main one is the smallness of perturbations). The parametric equations of the surface are obtained. The main properties of the surface are established and studied. Singular points are found and the topological type of the surface as a whole and in the vicinity of the conic point and the constriction is examined.",
keywords = "dust complex, family of Keplerian ellipses, filled up by trajectories domain, enveloping surface",
author = "S.A. Orlov and K.V. Kholshevnikov",
year = "2013",
doi = "10.1007/s10569-013-9473-z",
language = "English",
volume = "116",
pages = "35--52",
journal = "Celestial Mechanics and Dynamical Astronomy",
issn = "0923-2958",
publisher = "Springer Nature",
number = "1",

}

RIS

TY - JOUR

T1 - Dust torus formed by particles ejected from a celestial body at an arbitrary point of its elliptic orbit

AU - Orlov, S.A.

AU - Kholshevnikov, K.V.

PY - 2013

Y1 - 2013

N2 - Dust complexes form one of the Solar System components. The surface shape of a typical dust complex filled up by particles ejected from a celestial body is found within an analytical approach using reasonable assumptions (the main one is the smallness of perturbations). The parametric equations of the surface are obtained. The main properties of the surface are established and studied. Singular points are found and the topological type of the surface as a whole and in the vicinity of the conic point and the constriction is examined.

AB - Dust complexes form one of the Solar System components. The surface shape of a typical dust complex filled up by particles ejected from a celestial body is found within an analytical approach using reasonable assumptions (the main one is the smallness of perturbations). The parametric equations of the surface are obtained. The main properties of the surface are established and studied. Singular points are found and the topological type of the surface as a whole and in the vicinity of the conic point and the constriction is examined.

KW - dust complex

KW - family of Keplerian ellipses

KW - filled up by trajectories domain

KW - enveloping surface

U2 - 10.1007/s10569-013-9473-z

DO - 10.1007/s10569-013-9473-z

M3 - Article

VL - 116

SP - 35

EP - 52

JO - Celestial Mechanics and Dynamical Astronomy

JF - Celestial Mechanics and Dynamical Astronomy

SN - 0923-2958

IS - 1

ER -

ID: 7375844