Abstract
We provide a result of non-analytic integrability of the so-called J 2-problem. Precisely by using the Lerman theorem we are able to prove the existence of a region of the phase space, where the dynamical system exhibits chaotic motions.
Similar content being viewed by others
References
Danby, J. M. A.: 1962, Fundamentals of Celestial Mechanics, Macmillan, New York.
Fédoriouk, M.: 1987, Méthodes Asymptotiques pour les Equations Différentielles Ordinaires Linéaires, MIR, Moscow.
Grotta Ragazzo, G., Koiller, J. and Oliva, W. M., Motion of Massive Vortices in Two Dimensions (preprint).
Kyner, W. T.: 1968, ‘Rigorous and Formal Stability of Orbits around an Oblate Planet’, Mem. AMS 81, 1.
Irigoyen, M. and Simó, C.: 1993, ‘Non Integrability of the J 2 Problem’, Cel. Mech. and Dynam. Astron. 55, 281.
Landau, L. D. and Lifschitz, E. M.: 1982, Quantum Mechanics, MIR, Moscow.
Lerman, L. M.: 1991, ‘Hamiltonian Systems with Loops of a Separatrix of a Saddle-Center’, Selecta Math. Sov. 10, 297.
Mielke, A., Holmes, P. and O'Reilly, O.: 1992, ‘Cascades of Homoclinic Orbits to, and Chaos near, a Hamiltonian Saddle Center’, J. Dyn. Diff. Eqs. 4, 95.
Simó, C.: 1991, ‘Measuring the Lack of Integrability of the J 2 Problem for Earth's Satellites’, in A. E. Roy (ed.), Predictability, Stability, and Chaos in N-Body Dynamical Systems, Plenum Press, New York.
Yoshida, H.: 1987, ‘A Criterion for the Non-Existence of an Additional Integral in Hamiltonian Systems with a Homogeneous Potential’, Physica 29D, 128.
Ziglin, S. L.: 1983, ‘Branching of Solutions and Non-Existence of First Integrals in Hamiltonian Mechanics’, Funct. Anal. Appl. 16, 181 and 17, 6.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Celletti, A., Negrini, P. Non-integrability of the problem of motion around an oblate planet. Celestial Mech Dyn Astr 61, 253–260 (1995). https://doi.org/10.1007/BF00051896
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1007/BF00051896