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Fig. 10

image

Computed Q factor for ice-rich planets with masses of 1 (a), 5 (b), and 10 (c) M, and three icecontents (10, 20, and 50%), as a function of viscosity η and tidal frequency χ for theice mantle. The vertical thick black segments indicate the expected values of Q for three planet candidates (Trappist-1 f, Trappist-1 g, and K2-240 c) for a high-pressure ice viscosity of 1016 Pa s. The black arrows indicate the trend if larger ice viscosity values are considered.

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