Stability of the orbit of a third body in binary asteroid systems

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1 Citation (Scopus)

Abstract

In this work we studied the stable regions around four binary asteroids in the main asteroid belt. The studied systems were (107) Camilla, (22) Kallipe, (45) Eugenia and (762) Pulcova. The stability was characterized with three motion indicators: relative Lyapunov indicator, maximum eccentricity, and maximum difference of eccentricities. The survay covered the P type orbits, where satellite moves around both primaries. On the basis of our work it can be decided, in which system the discovery of a third component can be expected.

Original languageEnglish
Article number012017
JournalJournal of Physics: Conference Series
Volume218
Issue number1
DOIs
Publication statusPublished - Jan 1 2010
Event5th Workshop of Young Researchers in Astronomy and Astrophysics - Budapest, Hungary
Duration: Sep 2 2009Sep 4 2009

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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