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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3Q592GH
Repositorysid.inpe.br/mtc-m21b/2017/11.30.17.49   (restricted access)
Last Update2017:11.30.17.49.48 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21b/2017/11.30.17.49.48
Metadata Last Update2021:02.11.18.12.57 (UTC) administrator
DOI10.1088/1742-6596/911/1/012019
ISSN1742-6588
Citation KeyRoccoGonç:2017:SiTrDe
TitleSimulation of the trajectories described by a space vehicle around the asteroid 243 Ida and its natural satellite Dactyl
Year2017
Access Date2024, May 15
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size812 KiB
2. Context
Author1 Rocco, Evandro Marconi
2 Gonçalves, Liana Dias
Resume Identifier1 8JMKD3MGP5W/3C9JH37
Group1 DIDMC-CGETE-INPE-MCTIC-GOV-BR
2 CMC-ETES-SESPG-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 evandro.rocco@inpe.br
2 lianadgon@gmail.com
JournalJournal of Physics: Conference Series
Volume911
Pages012019
Secondary MarkB2_INTERDISCIPLINAR B2_ENGENHARIAS_III B3_MEDICINA_II B3_GEOCIÊNCIAS B4_MATERIAIS B4_ENGENHARIAS_II B4_BIOTECNOLOGIA C_QUÍMICA C_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA C_ENGENHARIAS_IV C_ECONOMIA C_ASTRONOMIA_/_FÍSICA
History (UTC)2017-11-30 17:49:48 :: simone -> administrator ::
2021-02-11 18:12:57 :: administrator -> simone :: 2017
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractThe asteroid 243 Ida located in the asteroid belt, between Mars and Jupiter, is the fourth largest asteroid of the Koronis asteroid family, with an average diameter of 31.3 km and a mass around 4.2×1016 kg, and a small moon, Dactyl. In order to study the dynamics of this system, orbital trajectories are simulated around Ida considering, besides the gravitational attraction of Dactyl, the non-central gravitational field of the asteroid, defined by a polyhedral model that defines the shape and the non-uniform mass distribution of the body. In this way, the magnitude and the behaviour of such forces, and also their influence on the orbital elements that define the trajectory of the space vehicle, are evaluated and analysed.
AreaETES
Arrangement 1urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > CMC > Simulation of the...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDMC > Simulation of the...
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4. Conditions of access and use
Languageen
Target Filerocco_simulation.pdf
User Groupsimone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3F2UALS
8JMKD3MGPCW/446AF4B
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn keywords label lineage mark mirrorrepository month nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
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