“…Many crustal formation models have been proposed based on petrological observations, deformation structures, and geodynamic simulations at various ocean ridge settings and ophiolites (e.g., Nicolas et al, 1988;Phipps Morgan and Chen, 1993;Quick and Denlinger, 1993;Kelemen et al, 1997;Dick et al, 2008). Among these, two end-member models for fast spreading mid-ocean ridges are actively debating whether cumulates of the lower oceanic crust crystalize mainly in a shallow melt lens (e.g., Phipps Morgan and Chen, 1993;Quick and Denlinger, 1993;Coogan et al, 2007;Faak et al, 2015) or in situ solidify largely from magma sills at various depths (e.g., Nicolas et al, 1988;Kelemen et al, 1997;Lissenberg et al, 2004;Maclennan et al, 2005;VanTongeren et al, 2008VanTongeren et al, , 2015Natland and Dick, 2009). The former postulates much slower cooling in the deeper crust (i.e., near-conductive cooling), whereas the latter necessitates efficient heat removal by hydrothermal circulations throughout the entire crust.…”