“…MMEs resulting from different origins could coexist in a single granitoid pluton (e.g., Grout, 1937;Didier, 1987;Fornelli, 1994;Stimac et al, 1995;Elburg, 1996b;Schödlbauer et al, 1997;Kadioğlu and Güleç, 1999;Waight et al, 2001b;Yang et al, 2004;Barbarin, 2005;Ilbeyli and Pearce, 2005;Esna-Ashari et al, 2011;Clemens and Elburg, 2013). Among the two popular models proposed for the origin of the MMEs in granitic rocks, the magma mixing and mingling model of mantle-and crust-derived magmas accounts for the igneous textural features, finer grain size, and chilled margins of the enclaves and isotopic differences between enclaves and their host granitoids (e.g., Holden et al, 1987Holden et al, , 1991Elburg and Nicholls, 1995;Metcalf et al, 1995;Maas et al, 1997;Altherr et al, 1999;Yang et al, 2004Yang et al, , 2007Chen et al, 2009a;Shaw and Flood, 2009;Shin et al, 2009;Rajaieh et al, 2010;Qin et al, 2010;Zhao et al, 2010;Cheng et al, 2012;Jiang et al, 2013;Liu et al, 2013). The cognate origin model for crystallization of the MMEs from a coeval magma that gave rise to the host granitoids accounts for similar mineral assemblage and similarities in chemical and isotopic compo- sitions between enclaves and their hosts (e.g., Borodina, 1977, 1991;Dodge and Kistler, 1990;Pin et al, 1990;Dorais et al, 1997;…”