Chaotic diffusion and effective stability of Jupiter Trojans
DOI10.1007/S10569-004-3975-7zbMath1083.70515OpenAlexW4238915699WikidataQ56067292 ScholiaQ56067292MaRDI QIDQ815684
Kleomenis Tsiganis, Harry Varvoglis, Rudolf Dvorak
Publication date: 20 February 2006
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10569-004-3975-7
Stability for nonlinear problems in mechanics (70K20) Computational methods for problems pertaining to mechanics of particles and systems (70-08) Transition to stochasticity (chaotic behavior) for nonlinear problems in mechanics (70K55) Celestial mechanics (70F15)
Related Items (10)
Uses Software
Cites Work
- On the stability of the Lagrangian points in the spatial restricted problem of three bodies
- The observed Trojans and the global dynamics around the Lagrangian points of the Sun-Jupiter system
- The Trojan problem
- The effect of eccentricity and inclination on the motion near the Lagrangian points \(L_4\) and \(L_5\)
- A perturbative treatment of the co-orbital motion
- Hamiltonian formulation of the secular theory for Trojan-type motion
- Why do Trojan ASCS (not) escape?
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