On the stability regions of the Trojan asteroids

DOI10.1007/S10569-005-2630-2zbMath1149.70315OpenAlexW4243467552MaRDI QIDQ815693

Rudolf Dvorak, Richard I. Schwarz

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/s10569-005-2630-2

zbMATH Keywords

stability regionsTrojans

Mathematics Subject Classification ID

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 (3)

Long-term evolution of quasi-circular Trojan orbits ⋮ Where are the Uranus Trojans? ⋮ The dynamics of inclined Neptune Trojans

Cites Work

• On the stability of the Lagrangian points in the spatial restricted problem of three bodies
• Formal integrals and Nekhoroshev stability in a mapping model for the Trojan asteroids
• The observed Trojans and the global dynamics around the Lagrangian points of the Sun-Jupiter system
• The Trojan problem
• On the stability of high inclined \(\mathbf L_4\) and \(\mathbf L_5\) Trojans
• One to one resonance at high inclination
• Trojans in stable chaotic motion
• The Lyapunov characteristic exponents-applications to celestial mechanics
• The dynamics of bodies with variable masses
• Why do Trojan ASCS (not) escape?

This page was built for publication: On the stability regions of the Trojan asteroids