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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/46MLNR2
Repositorysid.inpe.br/mtc-m21d/2022/04.14.12.18   (restricted access)
Last Update2022:04.14.12.18.18 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/04.14.12.18.18
Metadata Last Update2023:01.03.16.46.04 (UTC) administrator
DOI10.3390/sym14040667
ISSN2073-8994
Citation KeyXavierPradWintAmar:2022:MaLoNa
TitleMapping Long-Term Natural Orbits about Titania, a Satellite of Uranus
Year2022
MonthApr.
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3204 KiB
2. Context
Author1 Xavier, Jadilene
2 Prado, Antonio Fernando Bertachini de Almeida
3 Winter, Silvia Giuliatti
4 Amarante, André
Resume Identifier1
2 8JMKD3MGP5W/3C9JGJA
ORCID1 0000-0002-7009-1572
2 0000-0002-7966-3231
3 0000-0002-3949-6045
4 0000-0002-9448-141X
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 jadilene.rodrigues@unesp.br
2 antonio.prado@inpe.br
3 giuliatti.winter@unesp.br
4 andre.amarante@unesp.br
JournalSymmetry
Volume14
Number4
Pagese667
History (UTC)2022-04-14 12:18:39 :: simone -> administrator :: 2022
2023-01-03 16:46:04 :: 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
celestial mechanics
lifetime
numerical simulations
orbits
planetary satellite
AbstractClose polar and circular orbits are of great interest for the exploration of natural satellites. There are still no studies in the literature investigating orbits around Titania, the largest satellite of Uranus. In this work, we present results of a set of numerical simulations carried out to obtain long-duration orbits for a probe around Titania. Through an expansion of the gravitational potential up to second order, the asymmetry of the gravitational field due to Titanias coefficient C22, the zonal coefficient J2, and the gravitational perturbation of Uranus is considered. The analysis of lifetime sensitivity due to possible errors in the values of J2 and C22 is investigated using multiple regression models. Simulations were performed for different eccentricity values, and lifetime maps were constructed. The results show that low-altitude and near-circular orbits have longer lifetimes due to the balance between the disturbance of Uranus and the gravitational coefficients of Titania. The results also show that non-zero values of the longitude of periapsis (ω) and longitude of the ascending node (Ω) are essential to increase the lifetime up to eight times compared to cases where ω = Ω = 0°. We also show that an orbit with eccentricity 10−3 is the most affected by errors in the values of J2 and C22.
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4. Conditions of access and use
Languageen
Target Filesymmetry-14-00667.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.40.20 1
DisseminationPORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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