Dynamics of the conservative and dissipative spin orbit problem

Details Dynamics of the conservative and dissipative spin orbit problem Dynamics of the conservative and dissipative spin orbit problem

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007p%26ss...55..889c&link_type=abstract

Planetary and Space Science, Volume 55, Issue 7-8, p. 889-899.

Statistics

Computation

6

Scientific paper

We investigate the dynamics of the spin orbit coupling under different settings. First we consider the conservative problem, and then we add a dissipative torque 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.

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