Fig. 6From: Cold-based glaciation of Pavonis Mons, Mars: evidence for moraine deposition during glacial advanceModel snapshots illustrating assumptions regarding the timing and location of ice accumulation. Inset plot shows obliquity history at the beginning of the simulations with time and obliquity on x and y axes, respectively. Precipitation occurs at times indicated by the filled blue regions (see Fig. 6). a MOLA hillshade contour (1 km interval) map indicating location of model flowline (white line) and extent of ice in the model (transparent blue lines) at − 25.1 (circle in inset) and − 24.8 Myr (square in inset). Topographic profiles of the ice deposit at − 25.1 and − 24.8 Myr are shown in b and c, respectively with the blue line (and right y-axis) indicating ice accumulation/ablation rate. Ice thickness for these times are shown in d and e with the shaded region in d indicating extent of ice accumulationBack to article page