T227 Porphyry Copper Systems: Advances and Sources of Materials for the Energy Transition
Wednesday, 25 September 2024
8:00 AM - 12:00 PM
213B
METAL ENRICHMENT AND ZONING IN PORPHYRY COPPER DEPOSITS
Paper number: T227-2
Program: Technical Sessions
Time: 8:05 AM – 8:25 AM
Authors
Abstract
Deep deposits (ca. 5-10 km) are formed from single-phase parental intermediate density fluids, and are characterized by sparse quartz veins and chalcopyrite±pyrite or bornite in early halo selvages (bio-Ksp-musc) at ca. 500-600°C. At these relatively high pressures magmatic SO2 gas disproportion or reacts with wall-rock to form H2SO4 and H2S that produce hydrolytic (acid) wall-rock reactions, precipitate anhydrite, and fix sulfides.
In shallow deposits (ca. 2-5 km), parental fluids separate into brine and vapor, and the latter is dominant and enriched in SO2 and HF and ascends into the epithermal environment (<2 km) to form barren quartz-alunite-clay lithocaps. Brine transports most metal and produces abundant A-type quartz veins with chalcopyrite-bornite±magnetite in bio-Ksp alteration zones in the porphyry environment.
In both deep and shallow deposits, late intermediate density fluids are extracted from deep magmas, and produce widespread sericitic (muscovite) rock alteration and pyrite (ca. 350°C) that transport metals from great depth to the epithermal environment.
Metal zonation is dominated by decreasing solubility as temperature declines and acid is neutralized in the order Cu-Mo to Sn-W-Te-Se to As-Sb-Bi to Li-Cs. Additionally, hydrolytic wall-rock alteration removes metals (Pb, Ba, Sr from feldspar; Fe, Zn, Mn, Cr, V from mafic minerals; Cu from sulfides) and transports them upward. Fe released from these reactions is largely fixed as sulfide where H2S is sufficient.
The distribution of base metals and critical minerals is thus both governed both by initial magmatic-hydrothermal alteration, but also by evolving wall-rock reactions and thermal conditions.
Geological Society of America Abstracts with Programs. Vol. 56, No. 5
doi: 10.1130/abs/2024AM-402813
© Copyright 2024 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.