Nekhoroshev stability at L4 or L5 in the elliptic-restricted three-body problem - Application to Trojan asteroids

Monthly Notices of the Royal Astronomical Society

Volumn 384, Issue 3, 2008, Pages 1165-1177

  Lhotka, Ch ^a   Efthymiopoulos, C ^b   Dvorak, R ^a  

^a UNIVERSITY OF VIENNA   (Austria)

^b BIOMEDICAL RESEARCH FOUNDATION   (Greece)

Author keywords

Celestial mechanics; Methods: analytical; Minor planets, asteroids

Indexed keywords

ASTROPHYSICS; DYNAMICAL SYSTEMS; HAMILTONIANS; MAPPING; SOLAR SYSTEM; SYSTEM STABILITY;

ANALYTICAL DETERMINATION; CELESTIAL MECHANICS; FIXED POINTS; METHODS:ANALYTICAL; MINOR PLANET, ASTEROID; MINOR PLANETS; NORMAL FORM; RESTRICTED THREE-BODY PROBLEM; SYMPLECTIC; TROJAN ASTEROIDS;

ASTEROIDS;

EID: 43049111365     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12794.x     Document Type: Article

References (35)