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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/47A6MGL
Repositorysid.inpe.br/mtc-m21d/2022/07.18.17.27
Last Update2022:07.18.17.27.49 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/07.18.17.27.49
Metadata Last Update2023:01.03.16.46.10 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyWinterZaviPradAmar:2022:MaLoNa
TitleMapping long-term natural orbits around Titania, a satellite of Uranus
FormatOn-line
Year2022
Access Date2024, May 14
Secondary TypePRE CI
Number of Files1
Size63 KiB
2. Context
Author1 Winter, Silvia giuliatti
2 Zavier, Jadilene
3 Prado, Antonio Fernando Bertachini de Almeida
4 Amarante, André
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JGJA
Group1
2
3 DIMEC-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Universidade Estadual Paulista (UNESP)
2 Universidade Estadual Paulista (UNESP)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Universidade Estadual Paulista (UNESP)
Author e-Mail Address1 giuliatti.winter@unesp.br
2 jadilene.rodrigues@unesp.br
3 antonio.prado@inpe.br
4 andrezinho@msn.com
Conference NameCOSPAR Scientific Assembly, 44
Conference LocationAthens, Greece
Date16-24 July 2022
History (UTC)2022-07-18 17:27:49 :: simone -> administrator ::
2023-01-03 16:46:10 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractNear polar and circular orbits are of great interest to explore natural satellites, such as Titania, Uranus largest natural satellite. The reason is the fact that, from a near-polar and circular orbit, the whole surface of the satellite can be observed while the satellite rotates. In this work, we present several maps showing the lifetime of the orbits that can be used by a probe around Titania. The system analysed consists of Titania, as a central body, a probe in its orbit around Titania, and Uranus, as a disturbing body. Regarding the gravity fields involved, we considered the J2 and C22 gravitational coefficients of Titania, as well as Uranus J2 and J4 gravitational coefficients. We built a set of lifetime maps for five different values of the eccentricity of the orbit around Titania. Besides, we also present lifetime maps to compare the effects caused by the presence of the third-body and the gravity coefficients of Titania on the probes orbit. Our results show that low-altitude almost circular orbits have longer lifetimes. The reason is the equilibrium between the third-body perturbation from Uranus and the J2 and C22 gravitational coefficients of the gravity field of Titania. We also see that the gravity coefficients of Titania affect much more the probes lifetime compared to the effect due to Uranus gravity coefficients. The results also show that the values of $ and are essential in increasing of the orbits lifetime.
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data URLhttp://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/47A6MGL
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/47A6MGL
Languageen
Target FilePSD.1-0027-22-nopref.pdf
User Groupsimone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.40.20 1
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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