An interstellar origin for high-inclination Centaurs

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Autor(es): dc.contributorUniv Cote Azur-
Autor(es): dc.contributorUniversidade Estadual Paulista (Unesp)-
Autor(es): dc.creatorNamouni, F.-
Autor(es): dc.creatorMorais, M. H. M. [UNESP]-
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Descrição: dc.descriptionWe investigate the possible origins of real high-inclination Centaurs and trans-neptunian objects using a high-resolution statistical search for stable orbits that simulates their evolution back in time to the epoch when planet formation ended 4.5 billion years in the past. The simulation is a precise orbit determination method that does not involve ad hoc initial conditions or assumptions such as those found in planetesimal disc relaxation models upon which their conclusions depend. It can therefore be used to independently test origin theories based on relaxation models by examining the past orbits of specific real objects. Here, we examined 17 multiple-opposition high-inclination Centaurs and the two polar trans-neptunian objects 2008 KV42 and (471325) 2011 KT19. The statistical distributions show that their orbits were nearly polar 4.5 Gyr in the past, and were located in the scattered disc and inner Oort cloud regions. Early polar inclinations cannot be accounted for by current Solar system formation theory as the early planetesimal system must have been nearly flat in order to explain the low-inclination asteroid and Kuiper belts. Furthermore, the early scattered disc and inner Oort cloud regions are believed to have been devoid of Solar system material as the planetesimal disc could not have extended far beyond Neptune's current orbit in order to halt the planet's outward migration. The nearly polar orbits of high-inclination Centaurs 4.5 Gyr in the past therefore indicate their probable early capture from the interstellar medium.-
Descrição: dc.descriptionFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)-
Descrição: dc.descriptionConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
Descrição: dc.descriptionFunding Authority for Studies and Projects of Brazil (FINEP)-
Descrição: dc.descriptionUniv Cote Azur, Observ Cote Azur, CNRS, CS 34229, F-06304 Nice, France-
Descrição: dc.descriptionUniv Estadual Paulista, Inst Geociencias & Ciencias Exatas, UNESP, Av 24-A,1515, BR-13506900 Rio Claro, SP, Brazil-
Descrição: dc.descriptionUniv Estadual Paulista, Inst Geociencias & Ciencias Exatas, UNESP, Av 24-A,1515, BR-13506900 Rio Claro, SP, Brazil-
Descrição: dc.descriptionFAPESP: FAPESP/2018/08620-1-
Descrição: dc.descriptionCNPq: Pq2/304037/2018-4-
Formato: dc.format2191-2199-
Idioma: dc.languageen-
Publicador: dc.publisherOxford Univ Press-
Relação: dc.relationMonthly Notices Of The Royal Astronomical Society-
???dc.source???: dc.sourceWeb of Science-
Palavras-chave: dc.subjectcelestial mechanics-
Palavras-chave: dc.subjectcomets: general-
Palavras-chave: dc.subjectKuiper belt: general-
Palavras-chave: dc.subjectminor planets, asteroids: general-
Palavras-chave: dc.subjectOort Cloud-
Título: dc.titleAn interstellar origin for high-inclination Centaurs-
Tipo de arquivo: dc.typelivro digital-
Aparece nas coleções:Repositório Institucional - Unesp

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