| 1. Identificação | |
| Tipo de Referência | Artigo em Revista Científica (Journal Article) |
| Site | plutao.sid.inpe.br |
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identificador | 8JMKD3MGP3W/3UGD59U |
| Repositório | sid.inpe.br/plutao/2019/12.03.15.19.20 (acesso restrito) |
| Última Atualização | 2019:12.06.00.06.02 (UTC) lattes |
| Repositório de Metadados | sid.inpe.br/plutao/2019/12.03.15.19.21 |
| Última Atualização dos Metadados | 2021:07.28.22.22.44 (UTC) administrator |
| DOI | 10.1088/1742-6596/1365/1/012007 |
| ISSN | 1742-6588 |
| Rótulo | lattes: 0088337156908774 2 MotaRocc:2019:EqPoSt |
| Chave de Citação | MotaRocc:2019:EqPoSt |
| Título | Equilibrium points stability analysis for the asteroid 21 Lutetia  |
| Ano | 2019 |
| Data de Acesso | 04 maio 2024 |
| Tipo de Trabalho | conference paper |
| Tipo Secundário | PRE PI |
| Número de Arquivos | 1 |
| Tamanho | 1281 KiB |
| 2. Contextualização | |
| Autor | 1 Mota, Marcelo Lisboa 2 Rocco, Evandro Marconi |
| Identificador de Curriculo | 1 2 8JMKD3MGP5W/3C9JH37 |
| Grupo | 1 2 DIDMC-CGETE-INPE-MCTIC-GOV-BR |
| Afiliação | 1 2 Instituto Nacional de Pesquisas Espaciais (INPE) |
| Endereço de e-Mail do Autor | 1 2 evandro.rocco@inpe.br |
| Revista | Journal of Physics: Conference Series |
| Volume | 1365 |
| Páginas | 012007 |
| Nota Secundária | 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 |
| Histórico (UTC) | 2019-12-03 15:19:21 :: lattes -> administrator :: 2019-12-05 23:59:50 :: administrator -> lattes :: 2019 2019-12-06 00:06:02 :: lattes -> administrator :: 2019 2021-07-28 22:22:44 :: administrator -> simone :: 2019 |
| 3. Conteúdo e estrutura | |
| É a matriz ou uma cópia? | é a matriz |
| Estágio do Conteúdo | concluido |
| Transferível | 1 |
| Tipo do Conteúdo | External Contribution |
| Tipo de Versão | publisher |
| Palavras-Chave | Astrodynamics Orbital Motion Small bodies Asteroids Gravitational Potential |
| Resumo | This work investigates the stability of the equilibrium points that occur around the asteroid (21) Lutetia, assuming that this body has a constant velocity of rotation and is immersed in a gravitational field, whose force of attraction presents a perturbation with respect to the central force due to the irregular mass distribution of the asteroid. For the calculation of the potential, as well as of the effective potential, was used the method of the expansion of the potential in series, associated to the asteroid decomposition in tetrahedral elements. The zero velocity curves for a massless particle orbiting the gravitational environment were analyzed. The linearized dynamic equation in the vicinity of the equilibrium points, the associated characteristic equation, and the Jacobi constant were calculated. The validation of the results was ratified by simulations of trajectories around these equilibrium points, considering the gravitational field modelled. It should be emphasized the general nature of the procedures adopted in this work, that is, they can be applied to any other asteroid. |
| Área | ETES |
| Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDMC > Equilibrium points stability... |
| Conteúdo da Pasta doc | acessar |
| Conteúdo da Pasta source | não têm arquivos |
| Conteúdo da Pasta agreement | não têm arquivos |
| 4. Condições de acesso e uso | |
| Idioma | pt |
| Arquivo Alvo | motta_equilibrium.pdf |
| Grupo de Usuários | lattes |
| Grupo de Leitores | administrator lattes |
| Visibilidade | shown |
| Política de Arquivamento | denypublisher denyfinaldraft12 |
| Permissão de Leitura | deny from all and allow from 150.163 |
| Permissão de Atualização | não transferida |
| 5. Fontes relacionadas | |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/446AF4B |
| Lista de Itens Citando | sid.inpe.br/bibdigital/2021/02.11.18.06 2 sid.inpe.br/mtc-m21/2012/07.13.14.45.41 1 |
| Divulgação | WEBSCI; PORTALCAPES; COMPENDEX. |
| Acervo Hospedeiro | dpi.inpe.br/plutao@80/2008/08.19.15.01 |
| 6. Notas | |
| Notas | This work investigates the stability of the equilibrium points that occur around the asteroid (21) Lutetia, assuming that this body has a constant velocity of rotation and is immersed in a gravitational field, whose force of attraction presents a perturbation with respect to the central force due to the irregular mass distribution of the asteroid. For the calculation of the potential, as well as of the effective potential, was used the method of the expansion of the potential in series, associated to the asteroid decomposition in tetrahedral elements. The zero velocity curves for a massless particle orbiting the gravitational environment were analyzed. The linearized dynamic equation in the vicinity of the equilibrium points, the associated characteristic equation, and the Jacobi constant were calculated. The validation of the results was ratified by simulations of trajectories around these equilibrium points, considering the gravitational field modelled. It should be emphasized the general nature of the procedures adopted in this work that is, they can be applied to any other asteroid. |
| Campos Vazios | alternatejournal 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. Controle da descrição | |
| e-Mail (login) | simone |
| atualizar | |