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.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
