Fig. 3
From: Sensitivity of elastic thickness to water in the Martian lithosphere
Calculated surface heat flow at Pavonis Mons, Alba Patera, and NE Arabia Terra during the geological history. The grey lines indicate heat fluxes estimated using different chemical and cooling models (Montesi and Zuber 2003). Nimmo and Tanaka (2005) presented a chemical evolution model, resulted in the averaged surface heat flow of 14.3Â mW/m2 for the present day and 63.4Â mW/m2 for 4.1Â Ga