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

S.A. Orlov, K.V. Kholshevnikov

Результат исследований: Научные публикации в периодических изданияхстатья

1 цитирование (Scopus)

Выдержка

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.
Язык оригиналаанглийский
Страницы (с-по)35-52
ЖурналCelestial Mechanics and Dynamical Astronomy
Том116
Номер выпуска1
DOI
СостояниеОпубликовано - 2013

Отпечаток

celestial bodies
Particles (particulate matter)
Dust
Torus
Orbits
dust
Orbit
orbits
Arbitrary
Solar system
Singular Point
solar system
perturbation
Perturbation
particle

Цитировать

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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.",
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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.

В: Celestial Mechanics and Dynamical Astronomy, Том 116, № 1, 2013, стр. 35-52.

Результат исследований: Научные публикации в периодических изданияхстатья

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 -