Tracking the influence of a very close secondary star on planetary growth and evolution

Registro completo de metadados
MetadadosDescriçãoIdioma
Autor(es): dc.contributorUniversidade Estadual Paulista (UNESP)-
Autor(es): dc.contributorUniversidade Federal do Rio de Janeiro (UFRJ)-
Autor(es): dc.contributorScience and Technology-
Autor(es): dc.contributorUniversidade Federal do Paraná (UFPR)-
Autor(es): dc.creatorCamargo, B. C.B.-
Autor(es): dc.creatorMoraes, R. A.-
Autor(es): dc.creatorWinter, O. C.-
Autor(es): dc.creatorForyta, D. W.-
Data de aceite: dc.date.accessioned2025-08-21T17:34:47Z-
Data de disponibilização: dc.date.available2025-08-21T17:34:47Z-
Data de envio: dc.date.issued2025-04-29-
Data de envio: dc.date.issued2024-11-30-
Fonte completa do material: dc.identifierhttp://dx.doi.org/10.1093/mnras/stae2540-
Fonte completa do material: dc.identifierhttps://hdl.handle.net/11449/309909-
Fonte: dc.identifier.urihttp://educapes.capes.gov.br/handle/11449/309909-
Descrição: dc.descriptionThis work investigated the dynamics of planets in binary systems and provided insights into the stability and evolution of these systems. We explored the influence of a nearby secondary star on planetary growth and evolution, focusing on S-type configurations. We tracked the orbits of the planets and analysed their stability over long time-scales, considering various parameters such as mass, eccentricity, and inclination. Our results show that the presence of a secondary star can significantly impact the growth and evolution of planets, leading to changes in their orbits and potential ejection from the system, however, it was possible to identify stable planets even in systems experiencing multiple disturbances. One of the most significant results of the work was the analysis of the increased material in the disc near the primary star, which contributes to planet growth, driven by the density spirals influenced by the binary star. These findings have important implications for the search for habitable exoplanets and emphasize the need for further studies of planetary systems in binary star environments.-
Descrição: dc.descriptionCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)-
Descrição: dc.descriptionConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
Descrição: dc.descriptionGrupo de Dinâmica Orbital e Planetologia São Paulo State University (UNESP), São Paulo-
Descrição: dc.descriptionValongo Observatory Federal University of Rio de Janeiro (UFRJ)-
Descrição: dc.descriptionFederal Institute of Education Science and Technology-
Descrição: dc.descriptionDepartment of Physics Federal University of Parana (UFPR)-
Descrição: dc.descriptionGrupo de Dinâmica Orbital e Planetologia São Paulo State University (UNESP), São Paulo-
Descrição: dc.descriptionCNPq: 316991/2023-6-
Formato: dc.format3020-3034-
Idioma: dc.languageen-
Relação: dc.relationMonthly Notices of the Royal Astronomical Society-
???dc.source???: dc.sourceScopus-
Palavras-chave: dc.subjectbinaries: close-
Palavras-chave: dc.subjectexoplanets-
Palavras-chave: dc.subjecthydrodynamics-
Palavras-chave: dc.subjectplanets and satellites: dynamical evolution and stability-
Palavras-chave: dc.subjectprotoplanetary discs-
Título: dc.titleTracking the influence of a very close secondary star on planetary growth and evolution-
Tipo de arquivo: dc.typelivro digital-
Aparece nas coleções:Repositório Institucional - Unesp

Não existem arquivos associados a este item.