The analysis of restricted circular twice-averaged three body problem in the case of close orbits
From MaRDI portal
Publication:4127435
DOI10.1007/BF01260510zbMath0355.70007MaRDI QIDQ4127435
Publication date: 1974
Published in: Celestial Mechanics (Search for Journal in Brave)
Related Items (9)
Long Term Dynamics for the Restricted $N$-Body Problem with Mean Motion Resonances and Crossing Singularities ⋮ Rotation of a Planet in a Three-Body System: a Non-Resonant Case ⋮ Averaged spatial circular restricted three-body problem: internal case and new results ⋮ The eccentric Kozai-Lidov effect as a resonance phenomenon ⋮ Quasi-satellite orbits in the general context of dynamics in the \(1:1\) mean motion resonance: perturbative treatment ⋮ On the stability of circular ?asteroid? orbits in anN-planetary system ⋮ Lunar close encounters compete with the circumterrestrial Lidov-Kozai effect. The dynamical demise of \textit{Luna 3} ⋮ Circulating, eccentric periodic orbits at the Moon ⋮ Stability analysis of apsidal alignment in double-averaged restricted elliptic three-body problem
Cites Work
This page was built for publication: The analysis of restricted circular twice-averaged three body problem in the case of close orbits
