On the non-linear stability of motions around L5 in the elliptic restricted problem of the three bodies

DOI10.1007/BF01230741zbMath0579.70008OpenAlexW1662731141MaRDI QIDQ3702546

Judit Györgyey

Publication date: 1985

Published in: Celestial Mechanics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf01230741

zbMATH Keywords

planarstability regionsLagrange pointelliptic restricted problem of three bodiesorbital eccentricity

Mathematics Subject Classification ID

Three-body problems (70F07)

Related Items (5)

A parametric study of stability and resonances around \(L_4\) in the elliptic restricted three-body problem ⋮ Unnamed Item ⋮ Characteristics exponents of the triangular solutions in the elliptical restricted three-body problem under radiating primaries ⋮ Non-linear stability of triangular equilibrium points in ER3BP under radiating primaries in presence of resonance ⋮ Stability of co-orbital motion in exoplanetary systems

Cites Work

• Unnamed Item
• The motion of the perihelion of Trojan asteroids
• The three-dimensional motion of Trojan asteroids
• Periodic collision orbits in the elliptic restricted three-body problem
• Matrix methods in the calculation and analysis of orbits

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