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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.)

An analysis of the region of the Phocaea dynamical family

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Autor(es):
Carruba, V. [1, 2]
Número total de Autores: 1
Afiliação do(s) autor(es):
[1] UNIVAP, IPD, BR-12244000 Sao Jose Dos Campos, SP - Brazil
[2] UNESP, Dept Math, Guaratingueta, SP - Brazil
Número total de Afiliações: 2
Tipo de documento: Artigo Científico
Fonte: Monthly Notices of the Royal Astronomical Society; v. 398, n. 3, p. 1512-1526, SEP 21 2009.
Citações Web of Science: 17
Resumo

In this work, I conduct a preliminary analysis of the Phocaea family region. I obtain families and clumps in the space of proper elements and proper frequencies, study the taxonomy of the asteroids for which this information is available, analyse the albedo and absolute magnitude distribution of objects in the area, obtain a preliminary estimate of the possible family age, study the cumulative size distribution and collision probabilities of asteroids in the region, the rotation rate distribution and obtain dynamical map of averaged elements and Lyapunov times for grids of objects in the area. Among my results, I identified the first clump visible only in the frequency domain, the ( 6246) Komurotoru clump, obtained a higher limit for the possible age of the Phocaea family of 2.2 Byr, identified a class of Phocaea members on Mars-crossing orbits characterized by high Lyapunov times and showed that an apparently stable region on time-scales of 20 Myr near the nu(6) secular resonance is chaotic, possibly because of the overlapping of secular resonances in the region. The Phocaea dynamical group seems to be a real S-type collisional family, formed up to 2.2 Byr ago, whose members with a large semimajor axis have been dynamically eroded by the interaction with the local web of mean-motion and secular resonances. Studying the long-term stability of orbits in the chaotic regions and the stability of family and clumps identified in this work remain challenges for future works. (AU)

Processo FAPESP: 06/50005-5 - Dinâmica e origem de famílias de asteroides
Beneficiário:Valerio Carruba
Modalidade de apoio: Auxílio à Pesquisa - Jovens Pesquisadores