1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m21b.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34P/3Q592GH |
Repository | sid.inpe.br/mtc-m21b/2017/11.30.17.49 (restricted access) |
Last Update | 2017:11.30.17.49.48 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m21b/2017/11.30.17.49.48 |
Metadata Last Update | 2021:02.11.18.12.57 (UTC) administrator |
DOI | 10.1088/1742-6596/911/1/012019 |
ISSN | 1742-6588 |
Citation Key | RoccoGonç:2017:SiTrDe |
Title | Simulation of the trajectories described by a space vehicle around the asteroid 243 Ida and its natural satellite Dactyl |
Year | 2017 |
Access Date | 2024, May 15 |
Type of Work | journal article |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 812 KiB |
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2. Context | |
Author | 1 Rocco, Evandro Marconi 2 Gonçalves, Liana Dias |
Resume Identifier | 1 8JMKD3MGP5W/3C9JH37 |
Group | 1 DIDMC-CGETE-INPE-MCTIC-GOV-BR 2 CMC-ETES-SESPG-INPE-MCTIC-GOV-BR |
Affiliation | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Instituto Nacional de Pesquisas Espaciais (INPE) |
Author e-Mail Address | 1 evandro.rocco@inpe.br 2 lianadgon@gmail.com |
Journal | Journal of Physics: Conference Series |
Volume | 911 |
Pages | 012019 |
Secondary Mark | B2_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 |
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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 | The 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. |
Area | ETES |
Arrangement 1 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > CMC > Simulation of the... |
Arrangement 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDMC > Simulation of the... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | |
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4. Conditions of access and use | |
Language | en |
Target File | rocco_simulation.pdf |
User Group | simone |
Visibility | shown |
Archiving Policy | denypublisher denyfinaldraft12 |
Read Permission | deny from all and allow from 150.163 |
Update Permission | not transferred |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3F2UALS 8JMKD3MGPCW/446AF4B |
Dissemination | WEBSCI; PORTALCAPES; SCOPUS. |
Host Collection | sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 |
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6. Notes | |
Empty Fields | alternatejournal 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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7. Description control | |
e-Mail (login) | simone |
update | |
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