Dome-and-keel formation in Archean granite-greenstone terrains was uniquely favored by high abundances of heat-producing elements (HPEs) in the crust, and the ubiquity of pre-doming "greenstone-over-granite" stratification, which constituted large-scale density inversions and facilitated long-term steepening of the geotherm via burial of felsic basement-hosted HPEs. This contribution investigates the influence of these factors on the thermo-mechanical stability of the crust, with reference to two contrasting Archean granite-greenstone terrains in Western Australia. In the Neoarchean Eastern Goldfields Province, the rapid (2715-2665 Ma) accumulation of a thin (8-km) greenstone succession atop HPEpoor felsic crust (radiogenic heat flow contribution q c = 45 mW m −2 ) raised midcrustal temperatures from 230°C to 370°C prior to 2650 Ma dome-and-keel formation. In such cold, strong crust, the development of broad, granite-cored antiforms and narrow, greenstone-cored synforms with little strike variation is likely to directly reflect far-field, horizontal tectonic forces, oriented perpendicular to the regional structural grain. In contrast, the Mesoarchean East Pilbara Granite-Greenstone Terrane underwent slow (3515-3325 Ma) accumulation of tick (14-km) greenstones atop HPE-rich (q c = 70 mW m −2 ) basement, which raised mid-lower crustal temperatures from 400°C to 750-800°C, prior to 3300 Ma dome-and-keel formation. The effective viscosity of this hot, weak crust was further reduced by partial melting of the felsic basement; the resulting "classical" architecture (featuring granite domes flanked by greenstone keels with a variety of strike orientations) may therefore reflect partial convective overturn and vertical reorganization of the crust during thermo-mechanical stabilization.