Optimized Nekhoroshev stability estimates for the Trojan asteroids with a symplectic mapping model of co-orbital motion

Monthly Notices of the Royal Astronomical Society

Volumn 364, Issue 1, 2005, Pages 253-271

  Efthymiopoulos, C ^a   Sandor Z ^b  

^a BIOMEDICAL RESEARCH FOUNDATION   (Greece)

^b EÖTVÖS LORÁND UNIVERSITY   (Hungary)

Author keywords

Celestial mechanics; Minor planets, asteroids; Solar system: General

Indexed keywords

ASTROPHYSICS; HAMILTONIANS; MAPPING; ORBITS; SOLAR SYSTEM; SYSTEM STABILITY;

CELESTIAL MECHANICS; MAPPING MODELING; MINOR PLANET, ASTEROID; MINOR PLANETS; NORMAL FORM; ORBITAL MOTIONS; SOLAR SYSTEM: GENERAL; STABILITY ESTIMATES; SYMPLECTIC; TROJAN ASTEROIDS;

ASTEROIDS;

EID: 27944435270     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09572.x     Document Type: Article

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