“…The ultimate goal is to develop quantitative models for the properties of multicomponent silicate liquids spanning the P-T range relevant to terrestrial planet evolution consistent with experimental and theoretical constraints. There has already been success in the study of silicate liquids using this approach and even a cursory review of the computational literature applicable to high temperature liquids relevant to geochemical problems (magma end member compositions and molten iron) over the past thirty years reveals a rapid expansion in knowledge with accuracies comparable to experimental studies (e.g., Angell et al, 1982;Dempsey and Kawamura, 1984;Angell et al, 1987;Kubicki and Lasaga, 1990;Rustad et al, 1990;Della Valle and Andersen, 1992;Rustad et al, 1992;Poole et al, 1995;Stein and Spera, 1995;Bryce et al, 1998;Nevins and Spera, 1998;Morgan and Spera, 2001;Alfe et al, 2002;Stixrude and Karki, 2005;Guillot and Sator, 2007a,b;Lacks et al, 2007;Wan et al, 2007;de Koker et al, 2008;Martin et al, 2009;Nevins et al, 2009;Spera et al, 2009;Vuilleumier et al, 2009;de Koker, 2010). Research is accelerating due to the development of increasingly robust algorithms and the wide availability of computational engines.…”