One to one resonance at high inclination

DOI10.1023/B:CELE.0000016810.65114.17zbMath1131.70303OpenAlexW1988192809MaRDI QIDQ1769099

D. C. Heggie, Seppo Mikkola, Ramon Brasser

Publication date: 17 March 2005

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

Full work available at URL: https://doi.org/10.1023/b:cele.0000016810.65114.17

zbMATH Keywords

restricted three-body problemChaos\(1:1\) resonanceCo-orbital motionhigh inclination

Mathematics Subject Classification ID

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

Related Items (5)

The circular restricted three-body problem in curvilinear coordinates ⋮ On the stability of high inclined \(\mathbf L_4\) and \(\mathbf L_5\) Trojans ⋮ Detecting irregular orbits in gravitational N-body simulations ⋮ 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

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