The effect of Jupiter's mass growth on satellite capture - Retrograde case

Detalhes bibliográficos
Autor(a) principal: Neto, E. V.
Data de Publicação: 2004
Outros Autores: Winter, O. C., Yokoyama, T.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1051/0004-6361:20031645
http://hdl.handle.net/11449/24819
Resumo: Gravitational capture can be used to explain the existence of the irregular satellites of giants planets. However, it is only the first step since the gravitational capture is temporary. Therefore, some kind of non-conservative effect is necessary to to turn the temporary capture into a permanent one. In the present work we study the effects of Jupiter mass growth for the permanent capture of retrograde satellites. An analysis of the zero velocity curves at the Lagrangian point L-1 indicates that mass accretion provides an increase of the confinement region ( delimited by the zero velocity curve, where particles cannot escape from the planet) favoring permanent captures. Adopting the restricted three-body problem, Sun-Jupiter-Particle, we performed numerical simulations backward in time considering the decrease of M-4. We considered initial conditions of the particles to be retrograde, at pericenter, in the region 100 R-4 less than or equal to a less than or equal to 400 R-4 and 0 less than or equal to e < 0.5. The results give Jupiter's mass at the moment when the particle escapes from the planet. Such values are an indication of the necessary conditions that could provide capture. An analysis of these results shows that retrograde satellites would be captured as soon as they get inside the Hills' radius and after that they keep migrating toward the planet while it is growing. For the region where the orbits of the four old retrograde satellites of Jupiter ( Ananke, Carme, Pasiphae and Sinope) are located we found that such satellites could have been permanently captured when Jupiter had between 62% and 93% of its present mass.
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spelling The effect of Jupiter's mass growth on satellite capture - Retrograde caseplanets and satellites : generalastrometrycelestial mechanicsGravitational capture can be used to explain the existence of the irregular satellites of giants planets. However, it is only the first step since the gravitational capture is temporary. Therefore, some kind of non-conservative effect is necessary to to turn the temporary capture into a permanent one. In the present work we study the effects of Jupiter mass growth for the permanent capture of retrograde satellites. An analysis of the zero velocity curves at the Lagrangian point L-1 indicates that mass accretion provides an increase of the confinement region ( delimited by the zero velocity curve, where particles cannot escape from the planet) favoring permanent captures. Adopting the restricted three-body problem, Sun-Jupiter-Particle, we performed numerical simulations backward in time considering the decrease of M-4. We considered initial conditions of the particles to be retrograde, at pericenter, in the region 100 R-4 less than or equal to a less than or equal to 400 R-4 and 0 less than or equal to e < 0.5. The results give Jupiter's mass at the moment when the particle escapes from the planet. Such values are an indication of the necessary conditions that could provide capture. An analysis of these results shows that retrograde satellites would be captured as soon as they get inside the Hills' radius and after that they keep migrating toward the planet while it is growing. For the region where the orbits of the four old retrograde satellites of Jupiter ( Ananke, Carme, Pasiphae and Sinope) are located we found that such satellites could have been permanently captured when Jupiter had between 62% and 93% of its present mass.UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, BrazilUniv Estadual Paulista, IGCE, DEMAC, BR-13500970 Rio Claro, SP, BrazilUNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, BrazilUniv Estadual Paulista, IGCE, DEMAC, BR-13500970 Rio Claro, SP, BrazilE D P SciencesUniversidade Estadual Paulista (Unesp)Neto, E. V.Winter, O. C.Yokoyama, T.2014-02-26T17:17:34Z2014-05-20T14:16:03Z2014-02-26T17:17:34Z2014-05-20T14:16:03Z2004-02-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article727-734application/pdfhttp://dx.doi.org/10.1051/0004-6361:20031645Astronomy & Astrophysics. Les Ulis Cedexa: E D P Sciences, v. 414, n. 2, p. 727-734, 2004.0004-6361http://hdl.handle.net/11449/2481910.1051/0004-6361:20031645WOS:000188249200033WOS000188249200033.pdf5483476857978177Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengAstronomy & Astrophysics2,265info:eu-repo/semantics/openAccess2024-01-24T06:34:41Zoai:repositorio.unesp.br:11449/24819Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-01-24T06:34:41Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv The effect of Jupiter's mass growth on satellite capture - Retrograde case
title The effect of Jupiter's mass growth on satellite capture - Retrograde case
spellingShingle The effect of Jupiter's mass growth on satellite capture - Retrograde case
Neto, E. V.
planets and satellites : general
astrometry
celestial mechanics
title_short The effect of Jupiter's mass growth on satellite capture - Retrograde case
title_full The effect of Jupiter's mass growth on satellite capture - Retrograde case
title_fullStr The effect of Jupiter's mass growth on satellite capture - Retrograde case
title_full_unstemmed The effect of Jupiter's mass growth on satellite capture - Retrograde case
title_sort The effect of Jupiter's mass growth on satellite capture - Retrograde case
author Neto, E. V.
author_facet Neto, E. V.
Winter, O. C.
Yokoyama, T.
author_role author
author2 Winter, O. C.
Yokoyama, T.
author2_role author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
dc.contributor.author.fl_str_mv Neto, E. V.
Winter, O. C.
Yokoyama, T.
dc.subject.por.fl_str_mv planets and satellites : general
astrometry
celestial mechanics
topic planets and satellites : general
astrometry
celestial mechanics
description Gravitational capture can be used to explain the existence of the irregular satellites of giants planets. However, it is only the first step since the gravitational capture is temporary. Therefore, some kind of non-conservative effect is necessary to to turn the temporary capture into a permanent one. In the present work we study the effects of Jupiter mass growth for the permanent capture of retrograde satellites. An analysis of the zero velocity curves at the Lagrangian point L-1 indicates that mass accretion provides an increase of the confinement region ( delimited by the zero velocity curve, where particles cannot escape from the planet) favoring permanent captures. Adopting the restricted three-body problem, Sun-Jupiter-Particle, we performed numerical simulations backward in time considering the decrease of M-4. We considered initial conditions of the particles to be retrograde, at pericenter, in the region 100 R-4 less than or equal to a less than or equal to 400 R-4 and 0 less than or equal to e < 0.5. The results give Jupiter's mass at the moment when the particle escapes from the planet. Such values are an indication of the necessary conditions that could provide capture. An analysis of these results shows that retrograde satellites would be captured as soon as they get inside the Hills' radius and after that they keep migrating toward the planet while it is growing. For the region where the orbits of the four old retrograde satellites of Jupiter ( Ananke, Carme, Pasiphae and Sinope) are located we found that such satellites could have been permanently captured when Jupiter had between 62% and 93% of its present mass.
publishDate 2004
dc.date.none.fl_str_mv 2004-02-01
2014-02-26T17:17:34Z
2014-05-20T14:16:03Z
2014-02-26T17:17:34Z
2014-05-20T14:16:03Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1051/0004-6361:20031645
Astronomy & Astrophysics. Les Ulis Cedexa: E D P Sciences, v. 414, n. 2, p. 727-734, 2004.
0004-6361
http://hdl.handle.net/11449/24819
10.1051/0004-6361:20031645
WOS:000188249200033
WOS000188249200033.pdf
5483476857978177
url http://dx.doi.org/10.1051/0004-6361:20031645
http://hdl.handle.net/11449/24819
identifier_str_mv Astronomy & Astrophysics. Les Ulis Cedexa: E D P Sciences, v. 414, n. 2, p. 727-734, 2004.
0004-6361
10.1051/0004-6361:20031645
WOS:000188249200033
WOS000188249200033.pdf
5483476857978177
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Astronomy & Astrophysics
2,265
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eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 727-734
application/pdf
dc.publisher.none.fl_str_mv E D P Sciences
publisher.none.fl_str_mv E D P Sciences
dc.source.none.fl_str_mv Web of Science
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
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