Stability of triangular points in the relativistic R3BP when the bigger primary is an oblate spheroid
From MaRDI portal
Publication:5069601
DOI10.1080/1726037X.2016.1177930zbMath1499.70009OpenAlexW2497583158MaRDI QIDQ5069601
Publication date: 19 April 2022
Published in: Journal of Dynamical Systems and Geometric Theories (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1080/1726037x.2016.1177930
Relativistic dynamics for problems in Hamiltonian and Lagrangian mechanics (70H40) Celestial mechanics (70F15)
Cites Work
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Existence and stability of \(L_{4,5}\) in the relativistic restricted three-body problem
- On the stability of equilibrium points in the relativistic restricted three-body problem
- On the equilibrium points of the relativistic restricted three-body problem.
- The Three-Body Problem
- Collinear equilibria and their characteristic exponents in the restricted three-body problem when the primaries are oblate spheroids
- Solar System Dynamics
- ON MOULTON'S ORBITS IN THE RESTRICTED PROBLEM OF THREE BODIES