Volcanogenic massive sulfide (VMS) deposits are associated with bimodal volcanism in subaqueous rift-related environments. The felsic - mafic succession of volcanic rocks are hosts to semi-massive and massive sulfides (Cu-Zn-Pb) some of which contain precious metals (Au and Ag). The deposits are sustained by high heat flow (supplied by subvolcanic intrusions and/or upwelling plumes) and by circulating hot fluids within the volcanic pile.
A typical VMS deposit consists of a concordant lens of massive sulfides underlain by a discordant pipe-like stringer zone. The sulfide lenses are formed by hot fluids discharging into the seafloor. The stringer zone and the discharge zone immediately above it, contain much of the chalcopyrite ore. In the more distal parts of the pipe and higher up in the stratigraphy, pyrite, sphalerite and galena dominate. The Cu-Zn-Pb sulfides grade outwards from a Cu-rich core to a Zn-Pb-rich margin. Gangue minerals associated with the ore include barite, quartz, chlorite and carbonate. A siliceous cap rock generally overlies the deposit. PETROGRAPHIC REPORTS will include microscopic examination of thin sections with transmitted and reflected lights, detailed description of mineralogy and texture, classification of rocks where possible, visually estimated modal proportion of minerals, and description of primary and secondary minerals and their paragenetic sequence. In mineralized samples, the genesis of ore will be estimated. All reports will include 2 or more photomicrographs of each thin section taken by a digital Leica cooled camera, a cd with file(s) and 2 hard copies of the report. |
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(x-axis of photos: 1.6mm)
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MAGMATIC SULFIDES The photomicrographs below show some typical ore textures and some host rocks to the ores. |
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Ni-sulfides from Voisey’s Bay Ni-Co-Cu deposit, Labrador
(x-axis of photos: 1.6mm)
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