Fig. 5

LDEI stability diagram for synchronized celestial bodies in the optimal case for the instability, i.e. an optical libration (ϵ = 2e) for a quasi-equilibrium tide. All values are given in Table 5, and the horizontal axis represents the Ekman number Ek based on the thickness of the fluid layer. The label KM98 for Io calls that the point is placed with the values used by Kerswell & Malkus (1998). The zone below the black line, defined by the viscous surfacic damping coefficient α = 2.62, is the stable zone, whereas the black dashed lines represent the extremum values α = 1 and α = 10.
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