“…This has been interpreted to reflect removal of volatile Mo oxides formed in oxidizing environments (Fegley and Palme, 1985). During planetary differentiation, Mo preferentially partitions into the core and is strongly depleted in the silicate mantle (e.g., Holzheid and Palme, 2007;Newsom and Palme, 1984;Newsom, 1985Newsom, , 1986Righter et al, 1998;Wade et al, 2012;Walter and Thibault, 1995). The magnitude of Mo depletion in the mantle, therefore, can help to assess the pressure, temperature and oxygen fugacity conditions of metal segregation during planetary differentiation (e.g., Wood et al, 2006;Wade et al, 2012).…”