Trojan resonant dynamics, stability, and chaotic diffusion, for parameters relevant to exoplanetary systems

DOI10.1007/s10569-014-9591-2zbMath1314.70013arXiv1410.1407OpenAlexW2061362287MaRDI QIDQ2348890

Christos Efthymiopoulos, Rocío Isabel Páez

Publication date: 16 June 2015

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

Full work available at URL: https://arxiv.org/abs/1410.1407

zbMATH Keywords

resonancestability mapschaotic diffusionFLI mapsescaping timesTrojan exoplanets dynamics

Mathematics Subject Classification ID

Transition to stochasticity (chaotic behavior) for nonlinear problems in mechanics (70K55) Celestial mechanics (70F15) Orbital mechanics (70M20) (n)-body problems (70F10) Stability problems for problems in Hamiltonian and Lagrangian mechanics (70H14)

Related Items (8)

New Hamiltonian expansions adapted to the Trojan problem ⋮ On the coplanar eccentric non-restricted co-orbital dynamics ⋮ Secondary resonances and the boundary of effective stability of Trojan motions ⋮ Bifurcations of families of 1D-tori in 4D symplectic maps ⋮ The rectilinear three-body problem as a basis for studying highly eccentric systems ⋮ Symbolic dynamics in a binary asteroid system ⋮ Moser's quadratic, symplectic map ⋮ Explicit solution and resonance dynamics around triangular libration points of the planar elliptic restricted three-body problem

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