EXTENSION AND MAGMATISM IN THE MIRDITA OPHIOLITE, ALBANIA: IMPLICATIONS FOR THE MUNELLA MASSIVE SULFIDES DEPOSIT
The Munella Cu-massive sulfides deposit formed in the crustal sequence overlying the Eastern-type massif, a few km to the East (in the hanging-wall) of the main detachment fault. Sulfides mainly occur at the base of the basaltic sequence, may be associated with rhyolitic (keratophyric) layers, and are everywhere concordant with the hosting volcanic sequence. A thin horizon of red chert commonly directly overlies the massive sulfides. We mapped a 10 km-long section through the crust along the access road to the Munella mine. There, isotropic gabbro with abundant plagiogranite injections/bodies occur just above the detachment fault, followed by sheeted dykes, and two volcanic sequences, a lower MORB/IAT and an upper boninitic series. Stockwerks of albite-epidote veins/veinlets are abundant in the gabbro-sheeted dyke sequence and lower lavas, indicating intense sub-seafloor hydrothermal circulation during seafloor-spreading. The upper lavas, which host the Munella VMS, are almost devoid of hydrothermal alteration, however. The MORB/IAT-to-boninite sequence of the Munella road section suggests an early stage of suprasubduction seafloor-spreading, followed by an amagmatic hiatus, with late boninitic magmatism, possibly during pre-obduction extensional tectonism that led to the exhumation of the Western-type ultramafic massifs.