MAGMAS FROM EL TENIENTE CU-MO DEPOSIT (34ºS, CENTRAL CHILE): THE FINAL STAGES OF AN EVOLVING SOURCE THROUGH CENOZOIC CONSTRUCTION OF THE MODERN ANDEAN OROGEN
The main El Teniente intrusive units (~6.4-4.8 Ma) show a relatively radiogenic and restricted Hf isotopic composition (ƐHfI: +6 to +10), which is also indistinguishable from that defined by preceding Cenozoic barren igneous rocks in central Chile. All these rocks derive from nearly 25 Myr of subduction-related magmatic activity developed under contrasting tectonic regimes (extensive to compressive) and margin configurations. This suggests a primary control of the isotopic signature by a stable long-lived MASH-type reservoir in the deep lithosphere. The long-lasting magmatism that preceded the El Teniente formation was probably responsible for the progressive enrichment of this MASH source.
Tectonic and magmatic evolution of central Chile during construction of the modern Andes supports the hypothesis of dehydration melting reactions in the enriched MASH reservoir, and this is considered fundamental in the origin of El Teniente fertile intrusions. Such reactions probably occurred as a consequence of increasing crustal thickness, and were prompted by a high-temperature thermal regime resulting from a long history of preceding magmatism. Dehydration melting reactions are also expected to occur at a regional scale, and thus can explain the simultaneous generation of porphyry deposits in the Miocene-Pliocene Cu-Mo belt of central Chile. The latter can be considered as an example of how, given the appropriate conditions, dehydration melting processes can enhance magma fertility in a particular metallogenic epoch.