1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m21c.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34R/3RJMH82 |
Repository | sid.inpe.br/mtc-m21c/2018/08.06.15.18 (restricted access) |
Last Update | 2019:01.10.15.37.45 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m21c/2018/08.06.15.18.29 |
Metadata Last Update | 2021:02.11.18.10.43 (UTC) administrator |
ISSN | 0065-3438. |
Citation Key | MerguizoSanchezPrad:2018:UsMeMo |
Title | On the use of mean motion resonances to explore the Haumea system |
Year | 2018 |
Access Date | 2024, May 26 |
Type of Work | conference paper |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 11287 KiB |
|
2. Context | |
Author | 1 Merguizo Sanchez, Diogo 2 Prado, Antonio Fernando Bertachini de Almeida |
Resume Identifier | 1 2 8JMKD3MGP5W/3C9JGJA |
Group | 1 CMC-ETES-SESPG-INPE-MCTIC-GOV-BR 2 DIDMC-CGETE-INPE-MCTIC-GOV-BR |
Affiliation | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Instituto Nacional de Pesquisas Espaciais (INPE) |
Author e-Mail Address | 1 diogo.sanchez@inpe.br 2 antonio.prado@inpe.br |
Journal | Advances in the Astronautical Sciences |
Volume | 162 |
Pages | 1507-1524 |
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 Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Version Type | publisher |
Abstract | In 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. |
Area | ETES |
Arrangement 1 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > CMC > On the use... |
Arrangement 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDMC > On the use... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | |
|
4. Conditions of access and use | |
Language | en |
Target File | StevensonFinal2.pdf |
User Group | self-uploading-INPE-MCTI-GOV-BR simone |
Visibility | shown |
Read Permission | deny from all and allow from 150.163 |
Update Permission | not transferred |
|
5. Allied materials | |
Linking | 8JMKD3MGP3W34P/3HQHJ72 |
Next Higher Units | 8JMKD3MGPCW/3F2UALS 8JMKD3MGPCW/446AF4B |
Dissemination | WEBSCI; PORTALCAPES; MGA; COMPENDEX. |
Host Collection | urlib.net/www/2017/11.22.19.04 |
|
6. Notes | |
Notes | AAS/AIAA Astrodynamics Specialist Conference, 2017; Stevenson; United States; 20 August 2017 through 24 August 2017 |
Empty Fields | alternatejournal archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress format isbn keywords label lineage mark mirrorrepository month nextedition number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarytype url |
|
7. Description control | |
e-Mail (login) | simone |
update | |
|