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Periodic and quasi-periodic attractors for the spin-orbit evolution of Mercury with a realistic tidal torque | | Michele Bartuccelli
; Jonathan Deane
; Guido Gentile
; | | Date: |
3 Mar 2017 | | Abstract: | Mercury is entrapped in a 3:2 resonance: it rotates on its axis three times
for every two revolutions it makes around the Sun. It is generally accepted
that this is due to the large value of the eccentricity of its orbit. However,
the mathematical model originally introduced to study its spin-orbit evolution
proved not to be entirely convincing, because of the expression commonly used
for the tidal torque. Only recently, in a series of papers mainly by Efroimsky
and Makarov, a different model for the tidal torque has been proposed, which
has the advantages of being more realistic, and of providing a higher
probability of capture in the 3:2 resonance with respect to the previous
models. On the other hand, a drawback of the model is that the function
describing the tidal torque is not smooth and consists of a superposition of
kinks, so that both analytical and numerical computations turn out to be rather
delicate: indeed, standard perturbation theory based on power series expansion
cannot be applied and the implementation of a fast algorithm to integrate the
equations of motion numerically requires a high degree of care. In this paper,
we make a detailed study of the spin-orbit dynamics of Mercury, as predicted by
the realistic model: In particular, we present numerical and analytical results
about the nature of the librations of Mercury’s spin in the 3:2 resonance. The
results provide evidence that the librations are quasi-periodic in time. | | Source: | arXiv, 1703.1189 | | Services: | Forum | Review | PDF | Favorites | |
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