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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentificadorJ8LNKAN8RW/3D537A2
Repositóriodpi.inpe.br/plutao/2012/11.28.14.05.33
Última Atualização2013:01.28.13.09.35 (UTC) administrator
Repositório de Metadadosdpi.inpe.br/plutao/2012/11.28.14.05.34
Última Atualização dos Metadados2021:02.11.18.11.14 (UTC) administrator
Chave SecundáriaINPE--PRE/
DOI10.1111/j.1365-2966.2012.21101.x
ISSN1365-2966
Rótulolattes: 7340081273816424 3 AraujoWintPradSukh:2012:StReAr
Chave de CitaçãoAraujoWintPradSukh:2012:StReAr
TítuloStability regions around the components of the triple system 2001 SN263
Ano2012
MêsJuly
Data de Acesso29 abr. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho4455 KiB
2. Contextualização
Autor1 Araujo, R. A. N.
2 Winter, Othon Cabo
3 Prado, Antonio Fernando Bertachini de Almeida
4 Sukhanov, A.
Identificador de Curriculo1
2
3 8JMKD3MGP5W/3C9JGJA
Grupo1
2
3 DMC-ETE-INPE-MCTI-GOV-BR
Afiliação1 UNESP - São Paulo State University, CEP 12516-410 Guaratinguetá, SP, Brazil
2 UNESP - São Paulo State University, CEP 12516-410 Guaratinguetá, SP, Brazil
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1
2
3 prado@dem.inpe.br
Endereço de e-Mailprado@dem.inpe.br
RevistaMonthly Notices of the Royal Astronomical Society
Volume423
Número4
Páginas3058-3073
Nota SecundáriaA2_ASTRONOMIA_/_FÍSICA A1_ENGENHARIAS_III C_ENSINO_DE_CIÊNCIAS_E_MATEMATICA A1_INTERDISCIPLINAR A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A1_QUÍMICA
Histórico (UTC)2012-11-28 23:06:21 :: lattes -> administrator :: 2012
2012-11-30 13:52:23 :: administrator -> marciana :: 2012
2012-12-13 18:30:13 :: marciana -> administrator :: 2012
2013-01-20 15:54:19 :: administrator -> marciana :: 2012
2013-01-28 13:09:35 :: marciana -> administrator :: 2012
2021-02-11 18:11:14 :: administrator -> marciana :: 2012
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-Chavecelestial mechanics
N-body simulations
minor planets
asteroids
astrodinâmica
manobras orbitais
trajetórias espaciais
ResumoSpace missions are an excellent way to increase our knowledge of asteroids. Near-Earth asteroids (NEAs) are good targets for such missions, as they periodically approach the orbit of the Earth. Thus, an increasing number of missions to NEAs are being planned worldwide. Recently, NEA (153591) 2001 SN263 was chosen as the target of the ASTER MISSION - the First Brazilian Deep Space Mission, with launch planned for 2015. NEA (153591) 2001 SN263 was discovered in 2001. In 2008 February, radio astronomers from Arecibo-Puerto Rico concluded that (153591) 2001 SN263 is actually a triple system. The announcement of ASTER MISSION has motivated the development of the present work, whose goal is to characterize regions of stability and instability of the triple system (153591) 2001 SN263. Understanding and characterizing the stability of such a system is an important component in the design of the mission aiming to explore it. The method adopted consisted of dividing the region around the system into four distinct regions (three of them internal to the system and one external). We performed numerical integrations of systems composed of seven bodies, namely the Sun, Earth, Mars, Jupiter and the three components of the asteroid system (Alpha, the most massive body; Beta the second most massive body; and Gamma, the least massive body), and of thousands of particles randomly distributed within the demarcated regions, for the planar and inclined prograde cases. The results are displayed as diagrams of semi-major axis versus eccentricity that show the percentage of particles that survive for each set of initial conditions. The regions where 100per cent of the particles survive are defined as stable regions. We found that the stable regions are in the neighbourhood of Alpha and Beta, and in the external region. Resonant motion of the particles with Beta and Gamma was identified in the internal regions, leading to instability. For particles with I > 45° in the internal region, where I is the inclination with respect to Alpha's equator, there is no stable region, except for particles placed very close to Alpha. The stability in the external region is not affected by the variation of inclination. We also present a discussion of the long-term stability in the internal region, for the planar and circular case, with comparisons with the short-term stability.
ÁreaETES
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Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/J8LNKAN8RW/3D537A2
URL dos dados zipadoshttp://urlib.net/zip/J8LNKAN8RW/3D537A2
Idiomaen
Arquivo AlvoStability regions around the components.pdf
Grupo de Usuáriosadministrator
lattes
marciana
Visibilidadeshown
Política de Arquivamentoallowpublisher allowfinaldraft
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/446AF4B
Lista de Itens Citandosid.inpe.br/mtc-m21/2012/07.13.14.40.20 1
sid.inpe.br/bibdigital/2021/02.11.18.06 1
DivulgaçãoWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup readpermission rightsholder schedulinginformation secondarydate session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Controle da descrição
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