Advanced search
Start date
Betweenand
(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

An analysis of the region of the Phocaea dynamical family

Full text
Author(s):
Carruba, V. [1, 2]
Total Authors: 1
Affiliation:
[1] UNIVAP, IPD, BR-12244000 Sao Jose Dos Campos, SP - Brazil
[2] UNESP, Dept Math, Guaratingueta, SP - Brazil
Total Affiliations: 2
Document type: Journal article
Source: Monthly Notices of the Royal Astronomical Society; v. 398, n. 3, p. 1512-1526, SEP 21 2009.
Web of Science Citations: 17
Abstract

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)

FAPESP's process: 06/50005-5 - Dynamics and origin of asteroid families
Grantee:Valerio Carruba
Support type: Research Grants - Young Investigators Grants