We study the stability of some model problems in Celestial Mechanics, focusing on the dynamics around synchronous resonances, namely 1:1 commensurabilities among the main characteristic frequencies. In particular, we illustrate the following examples: the Earth's satellites dynamics, co-orbital asteroids, the rotational dynamics. Within such model problems we analyze, respectively, the stability of the Zeipel-Lidov-Kozai integral, the triangular Lagrangian points, the spin-orbit resonance. Stability results are obtained through perturbative methods, precisely the implementation of normal forms, Nekhoroshev-type estimates or KAM theory.

Celletti, A., De Blasi, I., Di Ruzza, S. (2025). Perturbative methods and synchronous resonances in Celestial Mechanics. APPLIED MATHEMATICAL MODELLING, 143 [10.1016/j.apm.2025.116040].

Perturbative methods and synchronous resonances in Celestial Mechanics

Alessandra Celletti
;
Irene De Blasi;
2025-01-01

Abstract

We study the stability of some model problems in Celestial Mechanics, focusing on the dynamics around synchronous resonances, namely 1:1 commensurabilities among the main characteristic frequencies. In particular, we illustrate the following examples: the Earth's satellites dynamics, co-orbital asteroids, the rotational dynamics. Within such model problems we analyze, respectively, the stability of the Zeipel-Lidov-Kozai integral, the triangular Lagrangian points, the spin-orbit resonance. Stability results are obtained through perturbative methods, precisely the implementation of normal forms, Nekhoroshev-type estimates or KAM theory.
2025
Pubblicato
Rilevanza internazionale
Articolo
Esperti anonimi
Settore MATH-04/A - Fisica matematica
English
Con Impact Factor ISI
Celestial Mechanics
Perturbation theory
Resonances
Stability
Celletti, A., De Blasi, I., Di Ruzza, S. (2025). Perturbative methods and synchronous resonances in Celestial Mechanics. APPLIED MATHEMATICAL MODELLING, 143 [10.1016/j.apm.2025.116040].
Celletti, A; De Blasi, I; Di Ruzza, S
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/473405
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