Central Configurations of N Bodies as Models of Secondary Coorbital Planets and Planetary Rings

Details Central Configurations of N Bodies as Models of Secondary Coorbital Planets and Planetary Rings Central Configurations of N Bodies as Models of Secondary Coorbital Planets and Planetary Rings

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1029p&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

Models of motion of planetary coorbital satellites, planetary rings in
the solar system, and planets in the exosolar systems based on N-body
central configurations are considered. The regions of localization of
undiscovered planets in double star systems are presented.

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