SECONDARY ENRICHMENT OF COPPER AT THE MADISON GOLD SKARN DEPOSIT, SILVER STAR DISTRICT, MONTANA
2CaFeSi2O6 + 2CO2 + ½O2 → Fe2O3 + 4SiO2 + 2CaCO3
Thus, the jasperoid formed from siliceous fluids liberated from the breakdown of the primary hedenbergite skarn. To explain the abundance of hematite, these fluids must have been oxidized, and therefore would have been incapable of mobilizing gold. Instead, the distribution of gold within the jasperoid most likely reflects the grades and distribution of gold within the skarn protore. In contrast, copper-bearing sulfide minerals were destroyed during jasperoid development, resulting in liberation of Cu2+. Cu-rich fluids replaced pyrite and other sulfide minerals outside the main jasperoid body, forming high-grade chalcocite pods. In other locations where no sulfide minerals were present, Cu2+ precipitated as native copper at an advancing reduction front. Some of this native copper occurs as pods and nuggets, up to 21 kg in size. Elsewhere, copper forms impressive stockworks with a geometry similar to the calcite veins within jasperoid. Overall, the secondary copper mineralization at Madison Gold appears to have formed during a low-temperature, oxidized geothermal event, which differs from conventional supergene models for formation of chalcocite and native copper.