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(Referência obtida automaticamente do Web of Science, por meio da informação sobre o financiamento pela FAPESP e o número do processo correspondente, incluída na publicação pelos autores.)

Spin clusters inside four young asteroid groups

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Autor(es):
Carruba, V [1] ; Ramos, L. G. M. [1] ; Spoto, F. [2]
Número total de Autores: 3
Afiliação do(s) autor(es):
[1] Sao Paulo State Univ UNESP, Sch Nat Sci & Engn, BR-12516410 Guaratingueta, SP - Brazil
[2] Univ Cote dAzur, Lab Lagrange, Observ Cate dAzur, CNRS, F-06304 Nice - France
Número total de Afiliações: 2
Tipo de documento: Artigo Científico
Fonte: Monthly Notices of the Royal Astronomical Society; v. 493, n. 2, p. 2556-2567, APR 2020.
Citações Web of Science: 0
Resumo

Asteroid groups may either form because of collisions or because of spin induced fission. Recently it has been shown that young spin clusters tend to form more frequently in young collisional families than in older groups. Here, we study the occurrence of spin clusters inside four very recently identified asteroid groups: the (525) Adelaide, (2258) Viipuri, (6142) Tantawi, and (18429) (1994 AO1) groups. Using combinations of techniques based on backward numerical simulations, we identify four spin pairs among the family members. All groups have fractions of observed spin clusters well above 5 per cent, so confirming an observed trend for other young asteroid groups. The (2258) Viipuri and (18429) (1994 AO1) groups are compatible with an origin as a spin clusters themselves, and could be other occurrences of cascade spin clusters, as recently detected in other asteroid groups. Finally, the separation between collisional asteroid families and spin clusters in domains of dispersion of proper semimajor axis, sigma(a), versus age seems to be more complex than previously thought. While spin clusters tend to be much more compact in proper elements than collisional families, there appears to be a transition region in sigma(a) where both the groups be found. (AU)

Processo FAPESP: 13/15357-1 - Efeito a longo prazo das massas (e sua incertidão) dos asteroides massivos sobre a evolução orbital de planetas terrestres e corpos menores.
Beneficiário:Safwan ALJBAAE
Linha de fomento: Bolsas no Brasil - Pós-Doutorado
Processo FAPESP: 16/04476-8 - Limitações sobre os campos de velocidades de ejeção terminais das famílias de asteroides
Beneficiário:Valerio Carruba
Linha de fomento: Auxílio à Pesquisa - Regular