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1. Identity statement
Reference TypeJournal Article
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Siteplutao.sid.inpe.br (namespace prefix: upn:33M4QT8)
Identifier8JMKD3MGP3W/3UGCRGD
Repositorysid.inpe.br/plutao/2019/12.03.13.57.11   (restricted access)
Last Update2019:12.06.00.20.32 (UTC) lattes
Metadata Repositorysid.inpe.br/plutao/2019/12.03.13.57.12
Metadata Last Update2021:07.28.22.22.44 (UTC) administrator
DOI10.1088/1742-6596/1365/1/012011
ISSN1742-6588
Labellattes: 7340081273816424 3 MurciaPGuedPrad:2019:PrTrRe
Citation KeyMurciaPiñerosGuedPrad:2019:PrTrRe
TitlePropagation of the trajectories for reentry spherical debris including rotation, melting fragmentation and voxel method
Year2019
Access Date2026, Oct. 24
Type of Workconference paper
Secondary TypePRE PI
Number of Files1
Size625 KiB
2. Context
Author1 Murcia Piñeros, Jhonathan Orlando
2 Guedes, Ulisses Thadeu Vieira
3 Prado, Antonio Fernando Bertachini de Almeida
Resume Identifier1
2 8JMKD3MGP5W/3C9JJAG
3 8JMKD3MGP5W/3C9JGJA
Group1 DIDSE-CGETE-INPE-MCTIC-GOV-BR
2 DIDSE-CGETE-INPE-MCTIC-GOV-BR
3 DIDMC-CGETE-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3 antonio.prado@inpe.br
JournalJournal of Physics: Conference Series
Volume1365
Pages012011
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
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01 upn:33M4QT8
History (UTC)2019-12-03 13:57:12 :: lattes -> administrator ::
2019-12-06 00:18:08 :: administrator -> lattes :: 2019
2019-12-06 18:20:53 :: lattes -> administrator :: 2019
2021-07-28 22:22:44 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsAstrodinâmica
Astrodynamics
Manobras Orbitais
AbstractIt is estimated that more than 22.000 objects are in orbit around the Earth, with a total mass of 8.400.000 kg. These numbers consider only objects with dimensions above 10 cm and some non-operational, but still orbiting satellites without control (debris). The debris represent a hazard to operational satellites and aerospace operations due to the high probability of collisions. Due to the interaction of the debris with the atmosphere of the Earth and the solar activity, they began to lose energy and finally decay. During the de-orbit process, the debris fall into the Earths atmosphere at hypersonic speeds and these objects can break-up and/or be fragmented due to the aerodynamics, thermal and structural loads. It is important to obtain the trajectory and attitude of any fragment to determine the possible survival mass, impact area, hazard conditions and risks to the population, the air traffic control, and infrastructure. In this case, it is implemented a computational code to integrate the equations of motion to propagate the dynamics and kinematics of spherical debris or propellant tanks. It is also analyzed the results of trajectories with six degrees of freedom, atmospheric winds, and Magnus effect. A voxel method is implemented to analyze the tanks heat transfer, surface temperature and structures stress. To determine and observe the influence of the rotation and the Magnus force in six reentry spherical bodies, three materials are selected; aluminum alloy, due to its application in many aerospace structures; titanium and graphite epoxy I, due to their highest melting point and specific heat. Generally, these materials are used in tanks and rocket motors. More than 62 trajectories were simulated. The mathematical model and computational code were validated in three degrees of freedom. Results are compared with data from other computational tools available in the scientific literature. The results show a good approximation with reported cases of study. New results are generated in the simulations of rotational bodies, due to the influence of aerodynamic forces in the trajectory and the changes in the stagnation regions. Due to the implementation of wind and rotation of the debris, the fragments increased the survivability and the dispersion area.
AreaETES
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDMC > Propagation of the...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDSE > Propagation of the...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languagept
Target Filemurcia_propagation.pdf
User Grouplattes
Reader Groupadministrator
lattes
Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/446AF4B
8JMKD3MGPCW/446AUSL
Citing Item Listsid.inpe.br/bibdigital/2021/02.11.18.06 - 98
sid.inpe.br/bibdigital/2021/02.11.20.54 - 75
sid.inpe.br/mtc-m21/2012/07.13.14.40.20 - 15
sid.inpe.br/mtc-m21/2012/07.13.15.01.08 - 9
DisseminationWEBSCI; PORTALCAPES; COMPENDEX.
6. Notes
NotesXIX Brazilian Colloquium on Orbital Dynamics 2018
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn lineage mark mirrorrepository month nextedition number orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
7. Description control
e-Mail (login)simone
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