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Spin pairs in the Koronis asteroid family

Authors :
Valerio Carruba
A. Lucchini
Alvaro Luiz Fazenda
W. Barletta
P. Furlaneto
B. Martins
Safwan Aljbaae
Universidade Estadual Paulista (Unesp)
Division of Space Mechanics and Control
Universidade de São Paulo (USP)
Source :
Scopus, Repositório Institucional da UNESP, Universidade Estadual Paulista (UNESP), instacron:UNESP
Publication Year :
2020
Publisher :
Elsevier BV, 2020.

Abstract

Made available in DSpace on 2020-12-12T02:49:13Z (GMT). No. of bitstreams: 0 Previous issue date: 2020-11-15 California Institute of Technology Jet Propulsion Laboratory National Aeronautics and Space Administration National Research Council Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) Asteroid groups may either form because of collisions or the rotational failure of a parent body. Collisional asteroid families tend to be more spread in proper element domains, while young spin clusters are usually much more compact. Recently, it has been shown that young spin clusters may form at higher rates in extremely young asteroid families (families younger than ≃3 Myr) than in more evolved groups. Among asteroid families, the Koronis family is a natural laboratory to test this phenomenon. While the family itself is very evolved, with an estimated age of more than 2 Byr, two young sub-families are known to be located among Koronis members: the extremely young family of Karin, with an age of 5.75±0.05 Myr, and the relatively young sub-family of Koronis(2), with an age of 10±5 Myr. This fact allows studying the occurrence of young spin clusters in extremely young, young and evolved asteroid populations, all sharing the same physical properties. Using methods based on backward numerical integrations, we identify one possible pair candidate in the Karin family, and retrieved the pair 1741–258640 recently found in other works. No convincing spin pair candidate was found in the Koronis(2) sub-family. This suggests that the occurrence of young spin clusters in families older than ≃ 3 Myr may be a rarer event than what previously thought. São Paulo State University (UNESP) School of Natural Sciences and Engineering National Space Research Institute (INPE) Division of Space Mechanics and Control, C.P. 515 Federal University of São Paulo (UNIFESP) Science and Technology Institute São Paulo State University (UNESP) School of Natural Sciences and Engineering FAPESP: 16/04476-8 CNPq: 301577/2017-0

Details

ISSN :
00320633
Volume :
193
Database :
OpenAIRE
Journal :
Planetary and Space Science
Accession number :
edsair.doi.dedup.....af58d0494aaefae594f4f7fc24bcc961