On the orbits of the outer satellites of Jupiter
Autor(a) principal: | |
---|---|
Data de Publicação: | 2003 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1051/0004-6361:20030174 http://hdl.handle.net/11449/24808 |
Resumo: | In this work we study the basic aspects concerning the stability of the outer satellites of Jupiter. Including the effects of the four giant planets and the Sun we study a large grid of initial conditions. Some important regions where satellites cannot survive are found. Basically these regions are due to Kozai and other resonances. We give an analytical explanation for the libration of the pericenters (ω) over bar - (ω) over bar (J). Another different center is also found. The period and amplitude of these librations are quite sensitive to initial conditions, so that precise observational data are needed for Pasiphae and Sinope. The effect of Jupiter's mass variation is briefly presented. This effect can be responsible for satellite capture and also for locking (ω) over bar - (ω) over bar (J) in temporary libration. |
id |
UNSP_3f9c3214f89cb2abfa9d877634a3e04f |
---|---|
oai_identifier_str |
oai:repositorio.unesp.br:11449/24808 |
network_acronym_str |
UNSP |
network_name_str |
Repositório Institucional da UNESP |
repository_id_str |
2946 |
spelling |
On the orbits of the outer satellites of Jupiterplanets and satellites : generalsolar system : generalIn this work we study the basic aspects concerning the stability of the outer satellites of Jupiter. Including the effects of the four giant planets and the Sun we study a large grid of initial conditions. Some important regions where satellites cannot survive are found. Basically these regions are due to Kozai and other resonances. We give an analytical explanation for the libration of the pericenters (ω) over bar - (ω) over bar (J). Another different center is also found. The period and amplitude of these librations are quite sensitive to initial conditions, so that precise observational data are needed for Pasiphae and Sinope. The effect of Jupiter's mass variation is briefly presented. This effect can be responsible for satellite capture and also for locking (ω) over bar - (ω) over bar (J) in temporary libration.Univ Estadual Paulista, IGCE, DEMAC, BR-13500970 São Paulo, BrazilUniv Estadual Paulista, FEG, Grp Dinam Orbital & Planetol, BR-12516410 São Paulo, BrazilUniv Estadual Paulista, IGCE, DEMAC, BR-13500970 São Paulo, BrazilUniv Estadual Paulista, FEG, Grp Dinam Orbital & Planetol, BR-12516410 São Paulo, BrazilE D P SciencesUniversidade Estadual Paulista (Unesp)Yokoyama, T.Santos, M. T.Cardin, G.Winter, O. C.2014-02-26T17:15:42Z2014-05-20T14:16:01Z2014-02-26T17:15:42Z2014-05-20T14:16:01Z2003-04-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article763-772application/pdfhttp://dx.doi.org/10.1051/0004-6361:20030174Astronomy & Astrophysics. Les Ulis Cedexa: E D P Sciences, v. 401, n. 2, p. 763-772, 2003.0004-6361http://hdl.handle.net/11449/2480810.1051/0004-6361:20030174WOS:000181708800039WOS000181708800039.pdf5483476857978177Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengAstronomy & Astrophysics2,265info:eu-repo/semantics/openAccess2023-09-30T06:02:58Zoai:repositorio.unesp.br:11449/24808Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T13:33:32.628733Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
On the orbits of the outer satellites of Jupiter |
title |
On the orbits of the outer satellites of Jupiter |
spellingShingle |
On the orbits of the outer satellites of Jupiter Yokoyama, T. planets and satellites : general solar system : general |
title_short |
On the orbits of the outer satellites of Jupiter |
title_full |
On the orbits of the outer satellites of Jupiter |
title_fullStr |
On the orbits of the outer satellites of Jupiter |
title_full_unstemmed |
On the orbits of the outer satellites of Jupiter |
title_sort |
On the orbits of the outer satellites of Jupiter |
author |
Yokoyama, T. |
author_facet |
Yokoyama, T. Santos, M. T. Cardin, G. Winter, O. C. |
author_role |
author |
author2 |
Santos, M. T. Cardin, G. Winter, O. C. |
author2_role |
author author author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) |
dc.contributor.author.fl_str_mv |
Yokoyama, T. Santos, M. T. Cardin, G. Winter, O. C. |
dc.subject.por.fl_str_mv |
planets and satellites : general solar system : general |
topic |
planets and satellites : general solar system : general |
description |
In this work we study the basic aspects concerning the stability of the outer satellites of Jupiter. Including the effects of the four giant planets and the Sun we study a large grid of initial conditions. Some important regions where satellites cannot survive are found. Basically these regions are due to Kozai and other resonances. We give an analytical explanation for the libration of the pericenters (ω) over bar - (ω) over bar (J). Another different center is also found. The period and amplitude of these librations are quite sensitive to initial conditions, so that precise observational data are needed for Pasiphae and Sinope. The effect of Jupiter's mass variation is briefly presented. This effect can be responsible for satellite capture and also for locking (ω) over bar - (ω) over bar (J) in temporary libration. |
publishDate |
2003 |
dc.date.none.fl_str_mv |
2003-04-01 2014-02-26T17:15:42Z 2014-05-20T14:16:01Z 2014-02-26T17:15:42Z 2014-05-20T14:16:01Z |
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/10.1051/0004-6361:20030174 Astronomy & Astrophysics. Les Ulis Cedexa: E D P Sciences, v. 401, n. 2, p. 763-772, 2003. 0004-6361 http://hdl.handle.net/11449/24808 10.1051/0004-6361:20030174 WOS:000181708800039 WOS000181708800039.pdf 5483476857978177 |
url |
http://dx.doi.org/10.1051/0004-6361:20030174 http://hdl.handle.net/11449/24808 |
identifier_str_mv |
Astronomy & Astrophysics. Les Ulis Cedexa: E D P Sciences, v. 401, n. 2, p. 763-772, 2003. 0004-6361 10.1051/0004-6361:20030174 WOS:000181708800039 WOS000181708800039.pdf 5483476857978177 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Astronomy & Astrophysics 2,265 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
763-772 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) |
repository.mail.fl_str_mv |
|
_version_ |
1808128246414311424 |