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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/47KS8TB
Repositorysid.inpe.br/mtc-m21d/2022/09.16.12.51   (restricted access)
Last Update2022:09.16.12.51.36 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/09.16.12.51.36
Metadata Last Update2023:01.03.16.46.15 (UTC) administrator
DOI10.3390/sym14071478
ISSN2073-8994
Citation KeyFerreiraPradWintFerr:2022:MaNaOr
TitleMapping Natural Orbits around Io
Year2022
MonthJuly
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size5562 KiB
2. Context
Author1 Ferreira, Thamis C. F. Carvalho
2 Prado, Antonio Fernando Bertachini de Almeida
3 Winter, Silvia M. Giuliatti
4 Ferreira, Lucas S.
Resume Identifier1
2 8JMKD3MGP5W/3C9JGJA
ORCID1 0000-0002-7281-6805
2 0000-0002-7966-3231
3 0000-0002-3949-6045
4 0000-0002-4506-9971
Group1
2 DIMEC-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Universidade Estadual Paulista (UNESP)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Universidade Estadual Paulista (UNESP)
4 Universidade Estadual Paulista (UNESP)
Author e-Mail Address1 tcf.carvalho@unesp.br
2 antonio.prado@inpe.br
JournalSymmetry
Volume14
Number7
Pagese1478
Secondary MarkB4_CIÊNCIA_DA_COMPUTAÇÃO B5_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA
History (UTC)2022-09-16 12:51:54 :: simone -> administrator :: 2022
2023-01-03 16:46:15 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsastrodynamics
Io
Jupiter
orbits
probe
AbstractAs the most volcanically active celestial body in the Solar System, Io is a natural satellite of Jupiter due to its proximity to the planet and the fact that it is in mean motion resonance, known as the Laplace resonance, with the natural satellites Europa and Ganymede. This natural satellite is a good candidate to be visited by future missions. In this sense, the present work has the goal of studying and mapping the best initial orbital conditions for orbits around Io, considering the symmetrical or asymmetical perturbative effects of a third body (Jupiter) and the (Formula presented.) term from the mass configuration of Io. The initial orbital parameters of the probe were investigated through a set of numerical simulations. The results showed that although most orbits around Io have lifetimes of less than 6 months, some regions were found where the initial conditions of the orbits provided satisfactory times for the accomplishment of future missions around Io.
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4. Conditions of access and use
Languageen
Target Filesymmetry-14-01478.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
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Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.40.20 3
sid.inpe.br/bibdigital/2022/04.03.17.52 2
DisseminationPORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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