“…Numerous experimental studies have focused on the formation of melts under cratonic pressure-temperature-composition conditions, with the emerging consensus that both CO 2 and H 2 O are necessary for melting to occur in cratons (Foley, 1989;Foley et al, 2009;Brey et al, 2008Brey et al, , 2009Girnis et al, 2011;Novella and Frost, 2014;Sokol and Kruk, 2015;Sokol et al, 2013Sokol et al, , 2014Sokol et al, , 2015Sharygin et al, 2015). In most cases, experimental melts are low to very low in silica, spanning the compositional range from carbonatites to kimberlites.…”