Abstract
The Cerro Áspero Mining District (CAMD) is located at the Sierras Pampeanas of central Argentina and hosts significant intrusion-related wolframite mineralization. The ore deposits are associated to hydrothermal quartz veins and breccias, hosted by granitoids and metamorphic rocks at the northern contact zone of the Devonian post-orogenic Cerro Áspero Batholith (CAB). The physico-chemical conditions of the different mineralization styles are yet not totally understood, and aiming to deliver a metallogenetic model, the petrography and composition of the main ore and gangue minerals were investigated, and fluid inclusion and stable isotope studies were performed in quartz, muscovite, wolframite, apatite, pyrite, molybdenite, chalcopyrite, and galena. The integrated results revealed that the CAMD ore deposits were generated within the cooling period of the Cerro Áspero Batholith, throughout three late to post-magmatic hydrothermal mineralizing stages. Based on fluid inclusion studies and stable isotope processed data, it was found that the fluids of the first two stages were probably derived from a magmatic source, whereas the third stage solutions would have been originated from meteoric waters. The temperature of the system at the beginning of the hydrothermal phase, was estimated at 384°C; thereafter, the calculated values suggest a decreasing thermal path. Chemical analyses of wolframite showed that the CAMD ore deposit’s evolution was signed by initial formation of ferberite, and subsequently evolved with an increasing H/F ratio that conduced to hübnerite precipitation in the final stage.
Highlights
The south-eastern Sierras Pampeanas, considered as a metallogenic province, concentrate most tungsten deposits of the Argentine Republic
Some scientific studies have focused on the petrology (Pinotti et al, 2002) and structural geology of the district (Mutti et al, 2003), and only some specific aspects related to the W hydrothermal deposits have been treated individually (González Chiozza & Mutti, 2002; Mutti & González Chiozza, 2005)
Mineral compositions were determined on 23 samples through electron-probe microanalyses at the Universidad del País Vasco, Spain, using a Cameca microbeam CMX equipped with TAP, LIF, PET and PC1 analyzing crystals
Summary
The south-eastern Sierras Pampeanas, considered as a metallogenic province, concentrate most tungsten deposits of the Argentine Republic. Two types of intrusionrelated W deposits are common in this province: scheelite skarns (Espeche & Lira, 2019), and magmatic-hydrothermal quartz-wolframite vein systems (Mutti et al, 2005). Since the first documented record of wolframite at the CAMD in the late nineteenth century, its geology has been resumed in different reviews and compilation works (Brodtkorb, 1999; Mutti et al, 2007). Some scientific studies have focused on the petrology (Pinotti et al, 2002) and structural geology of the district (Mutti et al, 2003), and only some specific aspects related to the W hydrothermal deposits have been treated individually (González Chiozza & Mutti, 2002; Mutti & González Chiozza, 2005). The purpose of this paper is to contribute to fulfill this hiatus by presenting mineral chemistry data and temperature estimations based on fluid inclusions and stable isotopes, in order to develop a consistent metallogenic model for the CAMD
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