S.-P. Zhang, K. A. Innanen
Abstract
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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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.
Key concepts: Physics, Celestial mechanics, Motion (physics), Classical mechanics, Lagrangian point, Astronomy, Astrophysics