Future destabilisation of Titan as a result of Saturn’s tilting

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Fig. 16

Maximum spin-axis precession frequency of the planet as a function of its obliquity. The curve is obtained by injecting a = r_F from Eq. (15) in Eq. (42). The extreme values Ω_max and Ω_S are given in Eqs. (44) and (45). For ε = 90°, the value at the maximum is undefined.

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