IntroductionVolcanogenic massive sulfides (VMS) and podiform chromitites commonly occur in ophiolite complexes. The VMS bodies are found in or near the contact of the pillow basalts and the overlying sedimentary rocks. A common feature of these deposits, particularly those relatively unaffected by tectonic deformation, is their mound-like morphology and subsurface stockwork-type mineralization, which are reminiscent of the structure of hydrothermal vents and their associated metal accumulations observed in modern mid-oceanic ridges (Hannington et al., 1995;Knott et al., 1998) and backarc basin rifts (Halbach et al., 1989;Binns and Scott, 1993). The podiform chromitites, on the other hand, occur in the transition zone dunites and residual upper mantle sequences of ophiolite complexes (Roberts, RESOURCE GEOLOGY, vol. 51, no. 2, 145-164, 2001 145 (IAB). The residual upper mantle sequence is harzburgitic and generally more depleted than the upper mantle underlying modern mid-oceanic ridges. Calculations using whole-rock and mineral compositions show that they can represent the residue of a fertile mantle source, which have undergone degrees of partial melting ranging from 9-22.5 %. Some of the mantle samples display chondrite-normalized REE and extended multi-element patterns suggesting enrichments in LREE, Rb, Sr and Zr, which are comparable to those found in fore-arc peridotites from the Izu-Bonin-Mariana (IBM) arc system. The Antique ultramafic rocks also record relatively oxidizing mantle conditions (∆log f O 2 (FMQ)=0.9-3.5). As a whole, the ophiolite probably represents an agglomeration of oceanic ridge and fore-arc crust fragments, which were juxtaposed during the Miocene collision of the PMB and the NPB. The intrusion of the serpentinites might be either coeval or subsequent to the accretion of the oceanic crust onto the fore-arc.Volcanogenic massive sulfide (VMS) deposits occur either in or near the contact between the pillow basalts and the overlying sediments or interbedded with the sediments. The morphology of the deposits, type of metals, ore texture and the nature of the host rocks suggest that the formation of the VMS bodies was similar to the accumulation of metals around and in the subsurface of hydrothermal vents observed in modern mid-oceanic ridge and back-arc basin rift settings. The podiform chromitites occur as pods and subordinate layers within totally serpentinized dunite in the residual upper mantle sequence. No large coherent chromitite deposit was found since the host dunitic rocks often occur as blocks within the serpentinites. It is difficult to evaluate the original geodynamic setting of the mineralized bodies since the chemistry of the host rocks were considerably modified by alteration during their tectonic emplacement. A preliminary conclusion for Antique is that the VMS is apparently associated with a primitive tholeiitic intermediate MORB-IAB volcanic suite, the chemistry of which is close to the calculated composition of the liquid that coexisted with the podiform chromitites.