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The \(2/1\) and \(3/2\) resonant asteroid motion: A symplectic mapping approach - MaRDI portal

The \(2/1\) and \(3/2\) resonant asteroid motion: A symplectic mapping approach

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Publication:5945026

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DOI10.1023/A:1011176630525zbMath1015.70013MaRDI QIDQ5945026

John D. Hadjidemetriou, George Voyatzis

Publication date: 5 August 2003

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

zbMATH Keywords

gap perturbations eccentricity group 2/1 resonance 3/2 resonance asteroid belt Jacobi's energy Jupiter resonant asteroid motion secondary resonance symplectic mapping model

Mathematics Subject Classification ID

Celestial mechanics (70F15) Dynamical systems in classical and celestial mechanics (37N05)

Related Items (3)

Formal solution of the asteroid motion near the 2:1 commensurability ⋮ Origin and continuation of \(3/2, 5/2, 3/1, 4/1\) and \(5/1\) resonant periodic orbits in the circular and elliptic restricted three-body problem ⋮ Symmetric and asymmetric librations in planetary and satellite systems at the 2/1 resonance

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