Modelling the high-eccentricity planetary three-body problem. Application to the GJ876 planetary system

Monthly Notices of the Royal Astronomical Society

Volumn 341, Issue 3, 2003, Pages 760-770

  Beauge C ^a,c   Michtchenko, T A ^b  

^a UNIVERSIDAD NACIONAL DE CÓRDOBA   (Argentina)

^b UNIVERSITY OF SÃO PAULO   (Brazil)

^c INSTITUTO NACIONAL DE PESQUISAS ESPACIAIS   (Brazil)

Author keywords

Celestial mechanics; Methods: analytical; Planetary systems; Planets and satellites: general

Indexed keywords

EXTRASOLAR PLANETS; HAMILTONIANS; ORBITS; PHASE SPACE METHODS; SATELLITES;

CELESTIAL MECHANICS; DYNAMICAL EVOLUTION; ECCENTRIC ORBITS; LONG TERM STABILITY; MEAN MOTION; METHODS:ANALYTICAL; PLANETARY SYSTEM; PLANETS AND SATELLITES: GENERAL; RESONANCE CAPTURE; THREE-BODY PROBLEM;

ASTROPHYSICS;

EID: 0043118584     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06345.x     Document Type: Article

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