“…Many of these structures, particularly the lobate scarps, are believed to have formed primarily in response to a decrease in planetary radius (Solomon, 1977;Solomon et al, 2008;Watters et al, 2004Watters et al, , 2009) that accompanied cooling of the interior over the course of the planet's evolution (Solomon, 1977;Hauck et al, 2004;Watters et al, 2004;Zuber et al, 2007). Thermal history models (Solomon, 1976(Solomon, , 1977(Solomon, , 1978(Solomon, , 1979Schubert et al, 1988;Hauck et al, 2004;Dombard and Hauck, 2008) are generally consistent with the inference from the distribution of lobate scarps and their stratigraphic relations with plains units that contraction initiated prior to the end of heavy bombardment, with the oldest lobate scarps predating smooth plains emplacement and the youngest postdating the most recent plains material (Solomon et al, 2008). Contraction occurred primarily in response to interior cooling associated with the decay of heat-producing elements, but the thermal state and contractional history were also influenced by the extraction of melt from the mantle, the possible cessation of mantle convection, and the nucleation and growth of a solid inner core .…”