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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3MPQHTP
Repositorysid.inpe.br/mtc-m21b/2016/11.11.18.44   (restricted access)
Last Update2016:11.11.18.44.36 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21b/2016/11.11.18.44.36
Metadata Last Update2021:07.28.22.52.23 (UTC) administrator
DOI10.1007/s40314-015-0264-x
ISSN2238-3603
Labelself-archiving-INPE-MCTI-GOV-BR
Citation KeyGomesOlivPradSanc:2016:ClApCl
TitleClose approach of a cloud of particles around an oblate planet
Year2016
MonthOct.
Access Date2024, Apr. 18
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size4442 KiB
2. Context
Author1 Gomes, Vivian Martins
2 Oliveira, Geraldo M. C.
3 Prado, Antonio Fernando Bertachini de Almeida
4 Sanchez, Diogo Merguizo
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JGJA
Group1
2
3 DMC-ETE-INPE-MCTI-GOV-BR
4 CMC-ETES-SPG-INPE-MCTI-GOV-BR
Affiliation1 Universidade Estadual Paulista (UNESP)
2 Centro Federal para Educação Tecnológica de Minas Gerais (CEFET-MG)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 vivianmartinsgomes@gmail.com
2
3 antonio.prado@inpe.br
4 diogo.sanchez@inpe.br
JournalComputational and Applied Mathematics
Volume35
Number3
Pages663-673
History (UTC)2016-11-11 18:45:48 :: simone -> administrator :: 2016
2021-07-28 22:52:23 :: administrator -> simone :: 2016
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsAstrodynamics
Close approaches
Orbital maneuver
Oblate planet
AbstractThe goal of the present paper is to study close approaches of a cloud of particles with an oblate planet, which means that there is a term in the gravitational potential of the planet. This cloud of particles is assumed to be created during the passage of a spacecraft by the periapsis of its orbit, by an explosion or any other disruptive event. The system is formed by two large bodies (Sun and planet), assumed to be in circular orbits around the center of mass of the system, and the cloud of particles. The particles that belong to the cloud make a close approach to the flat planet and then they are dispersed by the gravitational force of the planet. The motion is governed by the equations of motion given by the planar restricted circular three-body problem plus the effects of the oblateness of the planet. Jupiter is used for numerical simulations. The results show the differences between the behavior of the cloud after the passage, considering or not the effects of the oblateness of the planet. The results show that the oblateness of the planet is equivalent to an increase in the mass of the planet.
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4. Conditions of access and use
Languageen
Target Filegomes_close.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryurlib.net/www/2011/03.29.20.55
Next Higher Units8JMKD3MGPCW/3F2UALS
8JMKD3MGPCW/446AF4B
Citing Item Listsid.inpe.br/bibdigital/2021/02.11.18.06 1
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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