Obliquity of Mercury with a fluid core and a deformable mantle

Open Access

Fig. 3

Mantle’s in-plane obliquity without viscous dissipation at the CMB (τ_ν → ∞). The curve labelled ‘linear’ was computed using the present model and represents a transverse view of the top line in Fig. 2a. The non-linear curve is from Boué (2020).

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