E. D. Kuznetsov, M. A. Vasileva, A. S. Perminov, V. S. Safronova
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Abstract
The search for new members of young asteroid families is of interest for studying the history of the formation of these families. The paper considers 17 young families. Young families are characterized by strong clustering of both proper and osculating orbital elements. When searching for candidates for new members of young families, the osculating orbital elements were analyzed. Kholshevnikov metrics were estimated, the behavior of nodes and pericenters was analyzed, and a search for low relative-velocity close encounters was performed. For all selected candidates, synthetic proper orbital elements were calculated using the OrbFit software package, based on which a conclusion was made about the belonging of the asteroid to the family. As a result, new members were found for eight young asteroid families.
期刊介绍：
Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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