We investigate the dynamics of the spin-orbit coupling under different settings. First we consider the conservative problem, and then we add a dissipative torqije as provided by MacDonald's or Darwin's models. By means of frequency analysis and of the computation Of the maximum Lyapunov indicator we explore the different dynamical behaviors associated to the main resonances. In particular, we focus on the 1:1 and 3:2 resonances in which the Moon and Mercury are actually trapped. (c) 2007 Elsevier Ltd. All rights reserved.

Celletti, A., Froeschle, C., Lega, E. (2007). Dynamics of the conservative and dissipative spin-orbit problem. PLANETARY AND SPACE SCIENCE, 55, 889-899 [10.1016/j.pss.2006.11.023].

Dynamics of the conservative and dissipative spin-orbit problem

CELLETTI, ALESSANDRA;
2007-01-01

Abstract

We investigate the dynamics of the spin-orbit coupling under different settings. First we consider the conservative problem, and then we add a dissipative torqije as provided by MacDonald's or Darwin's models. By means of frequency analysis and of the computation Of the maximum Lyapunov indicator we explore the different dynamical behaviors associated to the main resonances. In particular, we focus on the 1:1 and 3:2 resonances in which the Moon and Mercury are actually trapped. (c) 2007 Elsevier Ltd. All rights reserved.
2007
Pubblicato
Rilevanza internazionale
Articolo
Sì, ma tipo non specificato
Settore MAT/07 - FISICA MATEMATICA
English
Con Impact Factor ISI
Dissipative forces; Resonances; Spin-orbit coupling
Celletti, A., Froeschle, C., Lega, E. (2007). Dynamics of the conservative and dissipative spin-orbit problem. PLANETARY AND SPACE SCIENCE, 55, 889-899 [10.1016/j.pss.2006.11.023].
Celletti, A; Froeschle, C; Lega, E
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/27096
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