The New Models of the Central Configurations for the Secondary Planets Systems and Their Stability

Details The New Models of the Central Configurations for the Secondary Planets Systems and Their Stability The New Models of the Central Configurations for the Secondary Planets Systems and Their Stability

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1026p&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

1

Scientific paper

Plane central configurations from 4 to 19 bodies and their stability,
based on the methods of A.M. Lyapunov, are considered. In the frames of
these dynamical models motion of some satellites of the giant planets
are partially explained.

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