“…The gravity-derived profiles suggest the crust beneath the center of SPA has a thickness of $30-55 km, gradually thickening towards $60 km nearer the basin's edge (radial distance of $1200 km). Unlike the majority of gravity-derived crustal profiles for smaller lunar basins, SPA does not appear to possess a thickened annulus of crust around its basin rim (see Wieczorek and Phillips, 1999;Hikida and Wieczorek, 2007;Sasaki et al, 2010Sasaki et al, , 2011. By comparison to the gravity-derived profiles, our steepest LTG (50 K/km) therefore appears to best fit the gravity data, as the other, shallower, LTGs all produced a prominent thickened annulus.…”