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The effect of eccentricity and inclination on the motion near the Lagrangian points \(L_4\) and \(L_5\)

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Publication:1582387
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DOI10.1023/A:1008385726569zbMath0965.70022MaRDI QIDQ1582387

R. Smith

Publication date: 3 October 2000

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)


zbMATH Keywords

circular restricted three-body problemeccentricityinclinationcoorbital motioneffective libration centresLagrangian equilibrium pointssmall amplitude librations


Mathematics Subject Classification ID

Three-body problems (70F07) Celestial mechanics (70F15)


Related Items (6)

New Hamiltonian expansions adapted to the Trojan problem ⋮ Photogravitational perturbations in the infinitesimal orbits around the libration points in the oblate RTBP ⋮ Trojan resonant dynamics, stability, and chaotic diffusion, for parameters relevant to exoplanetary systems ⋮ Stability of co-orbital motion in exoplanetary systems ⋮ Chaotic diffusion and effective stability of Jupiter Trojans ⋮ Formal integrals and Nekhoroshev stability in a mapping model for the Trojan asteroids







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