Invariant manifolds near \(L_1\) and \(L_2\) in the Sun-Jupiter elliptic restricted three-body problem. II: The dynamics of comet Oterma
From MaRDI portal
Publication:6643699
DOI10.1007/S10569-024-10218-YMaRDI QIDQ6643699
Publication date: 26 November 2024
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Lagrangian pointsplanar elliptic restricted three-body problemcomet 39P/Otermarapid transition mechanism
Cites Work
- Title not available (Why is that?)
- Title not available (Why is that?)
- On the persistence of lower dimensional invariant tori under quasi-periodic perturbations
- Geometric chaos indicators and computations of the spherical hypertube manifolds of the spatial circular restricted three-body problem
- Isolating blocks as computational tools in the circular restricted three-body problem
- Using normal forms to study Oterma's transition in the planar RTBP
- Transport and invariant manifolds near \(L_3\) in the Earth-Moon bicircular model
- Numerical computation of the normal behaviour of invariant curves of \(n\)-dimensional maps
- A Software Package for the Numerical Integration of ODEs by Means of High-Order Taylor Methods
- On the normal behaviour of partially elliptic lower-dimensional tori of Hamiltonian systems
- Dynamics and Mission Design Near Libration Points
- Introduction to Hamiltonian dynamical systems and the \(N\)-body problem
- Resonance and capture of Jupiter comets
- Invariant manifolds near \(L_1\) and \(L_2\) in the Sun-Jupiter elliptic restricted three-body problem. I.
This page was built for publication: Invariant manifolds near \(L_1\) and \(L_2\) in the Sun-Jupiter elliptic restricted three-body problem. II: The dynamics of comet Oterma
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q6643699)