“…Possibly due to its expressive volume and depth of emplacement, and consequent slow cooling rates, the CJS preserved important structures of melt segregation in form of subhorizontal lenses and eye-shaped pockets of medium-to coarse-grained mesocratic rocks of gabbroic composition that are injected in the host finegrained diabase, mostly at the upper parts of the sill. Similar segregations have been reported in recent works on thick basaltic flows in the PCFB (Oliveira et al, 2020, Gomes et al, 2022 and fractionated, coarse-grained gabbros and monzogabbros are recognized as more differentiated rocks derived from diabase in intrusive bodies occurring near the CJS (Limeira Sill; Oliveira and Dantas, 2008;Farias, 2012, Lino et al, 2018, Lino and Vlach, 2021. In this scenario, the CJS offers an excellent opportunity to study the mechanisms of melt segregation in large basaltic bodies and their geochemical and morphologic relationships with regional analogous PCFB occurrences.…”