Fig. 2: Present-day average interior structure of the northern regions (poleward of 60° N). | Nature

Fig. 2: Present-day average interior structure of the northern regions (poleward of 60° N).

From: Glacial isostatic adjustment reveals Mars’s interior viscosity structure

Fig. 2

a,b, Coloured lines show the viscosity (a) and temperature (b) structure of the interior models that match InSight constraints. Line colour reflects the average mantle temperature, which is related to the thickness of the crust and its enrichment in heat producing elements (HPE). Detailed model description is shown in Extended Data Fig. 1 and Extended Data Table 1.

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