The three-dimensional motion of Trojan asteroids

DOI10.1007/BF01228712zbMath0386.70014OpenAlexW2102365063MaRDI QIDQ4167638

Bálint Érdi

Publication date: 1978

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

Full work available at URL: https://doi.org/10.1007/bf01228712

Mathematics Subject Classification ID

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

Related Items (8)

On the non-linear stability of motions around L5 in the elliptic restricted problem of the three bodies ⋮ New Hamiltonian expansions adapted to the Trojan problem ⋮ Three-dimensional periodic orbits about the triangular equilibrium points of the restricted problem of three bodies ⋮ The Trojan problem ⋮ Influence of the coorbital resonance on the rotation of the trojan satellites of saturn ⋮ The motion of the perihelion of Trojan asteroids ⋮ A new perturbative solution to the motion around triangular Lagrangian points in the elliptic restricted three-body problem ⋮ The perturbations of the orbital elements of Trojan asteriods

Cites Work

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• An asymptotic solution for the Trojan case of the plane elliptic restricted problem of three bodies

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