Unraveling the origin of the Andean IOCG clan: A Re-Os isotope approach

Abstract

The Andean IOCG clan in the Coastal Cordillera of northern Chile, comprises the iron oxide-Cu-Au sensu stricto, the iron oxide-apatite (IOA), and the stratabound Cu(-Ag) deposits, also known as Manto-type Cu(-Ag) deposits. IOCGs and Manto-type deposits constitute the second source of copper in Chile, after porphyry Cu-Mo systems, whereas IOAs are an important source of iron. Regardless of their economic importance, little is known about their formation and contrasting genetic models have been proposed i.e., an origin from magmatic-hydrothermal fluids exsolved froma cooling intrusion, or formation fromnon-magmatic basinal brines heated by plutonic bodies. Herewe report Re-Os data for five IOCG deposits: Candelaria,Mantoverde, Casualidad, Diego de Almagro, and Barreal Seco, three IOAs: Los Colorados, El Romeral, and Carmen, and two Manto-type deposits: Altamira and Franke. Calculated Re-Os ages for some of these deposits are consistentwith previously published geochronological data, and indicate an Early to Late Cretaceous age. The calculated ages for the Altamira Manto-type Cu deposit yield a ~90 Ma age, indicating that the Cretaceous Manto-type Cu belt of central Chile extends further north than previously thought. Additionally, the calculated initial Os ratios using reported ages showthat IOCGs have a more radiogenic signature (2.0–2.4) than IOAs (1.0–1.2) and Manto-type Cu deposits (~1.1). A comparison with previously published Os initial ratios for the Mantoverde (0.2) and Candelaria (~0.4) IOCGs suggests that the mineralization in Chilean IOCGs is the result of different events with metals derived from diverse sources i.e., the magmatic-hydrothermal system and basement/host rocks. Rhenium and Os concentrations for the various studied deposits vary over a wide range of values at the ppb and ppt levels, respectively, with many sulfides and magnetite bearing appreciable no common Os. The Re and Os contents in sulfides (pyrite, chalcopyrite) from IOCGs are low, ranging from 2 to 149 ppb Re and up to 49 ppt Os. Pyrite from IOA deposits shows Re and Os concentrations ranging from 10.8 to 214 ppb Re, and Os b156 ppt, whereas magnetite has lower Re and Os contents (0.7–129 ppb Re, 0.2–3.6 ppt Os). However, rhenium and Os concentrations in magnetite might be attributed to small sulfide inclusions. Chalcocite from Manto-type Cu deposits shows the widest range and highest Re and Os concentrations; 15 to 253 ppb and 34 to 639 ppt, respectively. The Os present in all these deposits is dominated by radiogenic 187Os. A comparison of Re and Os data fromdifferent deposit types, shows that Andean IOCG and IOAdeposits have similar characteristics to Chilean porphyry Cu-Mosystemswith lowto moderate Re content (b250 ppb), lowOs concentration (b300 ppt total Os) dominated by radiogenic Os (N90%Osr), and variable initial Os ratios. Our data supports the idea that Andean IOCG and IOA deposits formed by magmatic-hydrothermal processes with little involvement of basinal brines. In contrast, published Re-Os information fromIOCGs in China and Australia argues for the involvement of a much more radiogenic crustal source possibly related to non-magmatic oxidized saline brines that leached basement rocks. We conclude that Andean IOCG (and IOA) deposits in northern Chile were formed mainly by magmatic-hydrothermal processes related to the formation and emplacement of plutonic rocks with moderate contribution from leaching of basement and/or volcanic host rocks. Surface or basin-derived brines as well as sediments appear to play only a minor role in the formation of the Chilean IOCG clan.