Fig. 16
Future obliquity of Saturn as a function of Titan’s migration velocity and Saturn’s polar moment of inertia. The axes are the same as in Fig. 8. The 3σ uncertainty ranges of Lainey et al. (2020) yield approximately b∕b0 ∈ [1∕2, 5] for the astrometric measurements and b∕b0 ∈ [1, 3∕2] for the radio-science experiments. Some level curves are shown in red.
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