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dc.contributor.authorCarruba, V. [UNESP]
dc.contributor.authorSpoto, F.
dc.contributor.authorBarletta, W. [UNESP]
dc.contributor.authorAljbaae, S.
dc.contributor.authorFazenda, L.
dc.contributor.authorMartins, B. [UNESP]
dc.date.accessioned2020-12-12T02:28:17Z
dc.date.available2020-12-12T02:28:17Z
dc.date.issued2020-01-01
dc.identifierhttp://dx.doi.org/10.1038/s41550-019-0887-8
dc.identifier.citationNature Astronomy, v. 4, n. 1, p. 83-88, 2020.
dc.identifier.issn2397-3366
dc.identifier.urihttp://hdl.handle.net/11449/201268
dc.description.abstractAsteroid families are groups of objects sharing similar orbits. They are mostly the results of past collisions between two asteroids. Recent studies have shown that some asteroid families can also be the outcome of the spin-up-induced fission of a critically rotating parent body (fission clusters). In at least four young fission clusters, more than 5% of their members belong to subfamilies, secondary clusters of objects mostly formed after the main fission event. However, asteroidal subfamilies are still not well characterized. In this work, using family recognition methods based on time-reversal dynamical simulations, machine-learning clustering algorithms and the exceptional orbit accuracy obtained from Gaia observations of Solar System objects, we identify several subclusters within four extremely young collisional families. We find that collisional asteroid families younger than 100 Myr have a higher fraction of young detectable fission subclusters with respect to older groups. The collisional events that form asteroid families may trigger a subsequent cascade of spin-induced formations of fission clusters by producing fragments in highly rotating states.en
dc.format.extent83-88
dc.language.isoeng
dc.relation.ispartofNature Astronomy
dc.sourceScopus
dc.titleThe population of rotational fission clusters inside asteroid collisional familiesen
dc.typeArtigo
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionLaboratoire Lagrange
dc.contributor.institutionDivision of Space Mechanics and Control
dc.contributor.institutionUniversidade de São Paulo (USP)
dc.description.affiliationSão Paulo State University (UNESP) School of Natural Sciences and Engineering
dc.description.affiliationUniversité de la Côte d’Azur Observatoire de la Côte d’Azur (CNRS) Laboratoire Lagrange
dc.description.affiliationNational Space Research Institute (INPE) Division of Space Mechanics and Control
dc.description.affiliationFederal University of São Paulo (UNIFESP) Science and Technology Institute
dc.description.affiliationUnespSão Paulo State University (UNESP) School of Natural Sciences and Engineering
dc.identifier.doi10.1038/s41550-019-0887-8
dc.identifier.scopus2-s2.0-85073939909
unesp.author.orcid0000-0003-2786-0740[1]
unesp.author.orcid0000-0001-7319-5847[2]
unesp.author.orcid0000-0002-4052-1113[5]
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