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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3RJMH82
Repositorysid.inpe.br/mtc-m21c/2018/08.06.15.18   (restricted access)
Last Update2019:01.10.15.37.45 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2018/08.06.15.18.29
Metadata Last Update2021:02.11.18.10.43 (UTC) administrator
ISSN0065-3438.
Citation KeyMerguizoSanchezPrad:2018:UsMeMo
TitleOn the use of mean motion resonances to explore the Haumea system
Year2018
Access Date2024, May 06
Type of Workconference paper
Secondary TypePRE PI
Number of Files1
Size11287 KiB
2. Context
Author1 Merguizo Sanchez, Diogo
2 Prado, Antonio Fernando Bertachini de Almeida
Resume Identifier1
2 8JMKD3MGP5W/3C9JGJA
Group1 CMC-ETES-SESPG-INPE-MCTIC-GOV-BR
2 DIDMC-CGETE-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 diogo.sanchez@inpe.br
2 antonio.prado@inpe.br
JournalAdvances in the Astronautical Sciences
Volume162
Pages1507-1524
History (UTC)2018-08-07 14:03:25 :: simone -> administrator :: 2018
2018-08-12 06:15:52 :: administrator -> simone :: 2018
2019-01-07 10:10:11 :: simone -> administrator :: 2018
2021-02-11 18:10:43 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractIn this work, Mean Motion Resonances (MMR) are used to create highly eccentric co-orbital orbits with Namaka, the inner moon of the dwarf planet Haumea. We found a region of instability nearby Namaka, caused by the quasi-super position of the critical semi-major axis of Haumea-Namaka (23,576.573 km) and Haumea-Hiiaka (22,422.929 km). These orbits need to be retrograde, since prograde orbits cross the region of instability due to the variation of their semi-major axis. We used the method of the integral of the disturbing acceleration to analyze the region of instability.
AreaETES
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4. Conditions of access and use
Languageen
Target FileStevensonFinal2.pdf
User Groupself-uploading-INPE-MCTI-GOV-BR
simone
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Linking8JMKD3MGP3W34P/3HQHJ72
Next Higher Units8JMKD3MGPCW/3F2UALS
8JMKD3MGPCW/446AF4B
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
NotesAAS/AIAA Astrodynamics Specialist Conference, 2017; Stevenson; United States; 20 August 2017 through 24 August 2017
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