Comments on “Using the viscoelastic relaxation of large impact craters to study the thermal history of Mars” (Karimi et al., 2016, Icarus 272, 102-113) and “Studying lower crustal flow beneath Mead basin: Implications for the thermal history and rheology of Venus” (Karimi and Dombard, 2017, Icarus 282, 34-39)

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