Secular orbit-orbit resonance between two satellites with non-zero masses

DOI10.1007/BF01232190zbMath0566.70007MaRDI QIDQ3681977

Th. Pauwels

Publication date: 1983

Published in: Celestial Mechanics (Search for Journal in Brave)

zbMATH Keywords

libration periodprecession ratesRhea-Titan resonancesecular orbit- orbit resonances

Mathematics Subject Classification ID

Three-body problems (70F07) Orbital mechanics (70M20)

Related Items (4)

The phase-space architecture in extrasolar systems with two planets in orbits of high mutual inclination ⋮ Sweeping through a second order resonance ⋮ Note on the reducing transformation and secular coupling ⋮ Analytical approach to the secular behaviour of exoplanetary systems

Cites Work

• Commensurabilities of Satellites' Apsidal Precession Periods

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