On the stability of high inclined \(\mathbf L_4\) and \(\mathbf L_5\) Trojans

DOI10.1007/S10569-004-1007-2zbMath1147.70308OpenAlexW1995874309MaRDI QIDQ1766251

Markus Gyergyovits, Rudolf Dvorak, Richard I. Schwarz

Publication date: 28 February 2005

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

Full work available at URL: https://doi.org/10.1007/s10569-004-1007-2

zbMATH Keywords

Lagrangian pointsstability limitshigh inclination orbitsrestricted three-body problemsTrojans asteroids

Mathematics Subject Classification ID

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

Related Items (4)

Where are the Uranus Trojans? ⋮ The dynamics of inclined Neptune Trojans ⋮ Special issue: A comparison of the dynamical evolution of planetary systems. Selected papers from the 6th Alexander von Humboldt colloquium on celestial mechanics, Bad Hofgastein, Austria, March 21--27, 2004. ⋮ On the stability regions of the Trojan asteroids

Uses Software

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Cites Work

• The Trojan problem
• 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?

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