Silicic Fe-Ti-oxide magmatic series was first recognized in the Sierra Leone axial segment of the MAR near 6o N. The series consists of intrusive rocks harzburgites, lherzolites, bronzitites, norites, gabbronorites, hornblende Fe-Ti-oxide gabbronorites and gabbronorite-diorites, quartz diorites, and trondhjemites and their subvolcanic ilmenite-hornblende dolerites and, possibly, volcanic analogues ilmenite-bearing basalts. The deficit of most incompatible elements in the rocks of the series suggests that the parental melts were derived from a source that had already been melted. Correspondingly, these melts could not be MORB derivatives. The origin of the series is thought to be related to the melting of the hydrated oceanic lithosphere during the emplacement of an asthenospheric plume protuberance on the surface of a large asthenospheric lens beneath MAR. The genesis of different melts was supposedly controlled by the ascent of a chamber of hot mantle magmas thought this lithosphere in compliance with the zone melting mechanism. The melt acquired fluid components from the heated rocks at the peripheries of the plume and became enriched in Fe, Ti, Pb, Cu, Zn, and other components mobile in fluids.
Slow-spreading ridges, Ultramafic cumulates, Fe-Ti-oxides.
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