The motion of planetary triangular Lagrange particles with high inclinations

Details The motion of planetary triangular Lagrange particles with high inclinations The motion of planetary triangular Lagrange particles with high inclinations

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aj.....96.1995z&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 96, Dec. 1988, p. 1995-2002. Research supported by NSERC.

Statistics

Computation

12

Celestial Mechanics, Lagrangian Equilibrium Points, Many Body Problem, Planetary Orbits, Computational Astrophysics, Equations Of Motion, Orbital Mechanics

Scientific paper

A theory is developed to study the stability of the inclined Trojan
asteroids in idealized circular three-body and elliptic three-body
circumstances. Some numerical checks are made in an idealized planetary
system, including the triangular Lagrange points of planets other than
Jupiter.

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