Dust Torus Produced by Particles Ejected in the Apsidal Points

S.A. Orlov, K.V. Kholshevnikov

Результат исследований: Научные публикации в периодических изданияхстатья

2 Цитирования (Scopus)

Выдержка

Dust complexes form one of the Solar System components. There are many ways of their forming: ejection of matter from comets and satellites due to volcanic (geyser) eruptions and meteorites bombardement, explosions and collisions of artificial satellites, etc. Many works are dedicated to describe the distribution of matter in such complexes. In the present paper we find the shape of a typical complex under reasonable assumptions (the main one is the smallness of perturbations) using purely analytical methods.
Язык оригиналаанглийский
Страницы (с-по)208-219
ЖурналSolar System Research
Том46
Номер выпуска3
СостояниеОпубликовано - 2012

Отпечаток

geyser
meteorite
comet
solar system
analytical method
volcanic eruption
collision
dust
perturbation
artificial satellites
meteorites
comets
ejection
volcanic eruptions
collisions
distribution
artificial satellite
particle

Цитировать

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abstract = "Dust complexes form one of the Solar System components. There are many ways of their forming: ejection of matter from comets and satellites due to volcanic (geyser) eruptions and meteorites bombardement, explosions and collisions of artificial satellites, etc. Many works are dedicated to describe the distribution of matter in such complexes. In the present paper we find the shape of a typical complex under reasonable assumptions (the main one is the smallness of perturbations) using purely analytical methods.",
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Dust Torus Produced by Particles Ejected in the Apsidal Points. / Orlov, S.A.; Kholshevnikov, K.V.

В: Solar System Research, Том 46, № 3, 2012, стр. 208-219.

Результат исследований: Научные публикации в периодических изданияхстатья

TY - JOUR

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AU - Orlov, S.A.

AU - Kholshevnikov, K.V.

PY - 2012

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AB - Dust complexes form one of the Solar System components. There are many ways of their forming: ejection of matter from comets and satellites due to volcanic (geyser) eruptions and meteorites bombardement, explosions and collisions of artificial satellites, etc. Many works are dedicated to describe the distribution of matter in such complexes. In the present paper we find the shape of a typical complex under reasonable assumptions (the main one is the smallness of perturbations) using purely analytical methods.

KW - dust complex

KW - family of Keplerian ellipses

KW - filled up by trajectories domain

KW - enveloping surface

M3 - Article

VL - 46

SP - 208

EP - 219

JO - Solar System Research

JF - Solar System Research

SN - 0038-0946

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