GSA Annual Meeting in Denver, Colorado, USA - 2016

Paper No. 212-8
Presentation Time: 3:35 PM

TRACKING AN EVOLVING ORE FLUID WITH PYRITE IN A CARLIN-TYPE GOLD DEPOSIT AT THE TURQUOISE RIDGE MINE, GETCHELL, NEVADA


LONGO, Anthony A.1, CLINE, Jean S.1 and MUNTEAN, John L.2, (1)Department of Geoscience, University of Nevada Las Vegas, 4505 Maryland Parkway, Las Vegas, NV 89154-4010, (2)Nevada Bureau of Mines and Geology, University of Nevada, Reno, Mail Stop 178, University of Nevada, Reno, NV 89557, longotal@aol.com

Primary Au in Carlin-type deposits of northern Nevada occurs in trace element-rich pyrite in ore-stage rims on earlier-formed pyrite cores. The trace elements in these rims are ionically bound in pyrite and marcasite, and we interpret the trace metal chemistry as a proxy for evolving ore fluid trace element chemistry. By studying the vertical and lateral variations in morphology and chemistry of ore-stage pyrite across the Turquoise Ridge gold deposit, we tracked fluid flow pathways through space and time. Pyrites from six zones in the deposit were analyzed for 22 elements using a JEOL electron probe microanalyzer. Patterns revealed by the ore-stage pyrite show that ore fluids migrated up the Getchell fault and a sub-parallel dacite dike, then upward into high-angle fracture zones that contain the 148, HGB, and BBT ore zones. The most definitive and consistently present ore-stage elements are As, Au, Hg, Sb, Te, and Cu. Tl is present in late-formed rims at HGB and BBT; Au, As, Sb, Cu and Te are anomalous in both ore-stage rims and pre-ore pyrite cores at 148, Getchell Fault, and Dike zones. The Deep East Feeder zone features As-Hg rich rims and Au-W rich cores.

Ore-stage pyrites include fuzzy pyrite, small (1-15 µm dia.) spheroidal pyrites with fuzzy rims that lack distinct cores, and core-rim pyrite, cores of pre-ore pyrite overgrown with 2-45 µm-wide trace element-rich pyrite rims. Multiple ore-stage rims (>10 µm) developed as chemically-zoned overgrowths that recorded changes in the ore fluid chemistry. High-grade gold ore is associated with areas in the deposit where prolonged sulfidation precipitated multiple rims. Pyrites at 148 with high-Au inner rims and low-Au outer rims contribute to high-grade ore reaching 2 oz/t. Pyrites at HGB with high Au-Te inner rims and high Au-Tl outer rims, coexist with late high Au-Tl fuzzy pyrites and contribute to the highest grade gold ore in the deposit ( >5 oz/t). Pyrites along the Getchell fault and in the BBT have single rims with high Au, but contribute to lower Au grades overall (typically <0.5 oz/t). Variations in core-to-rim chemistry are interpreted to reflect temporal and spatial evolution in ore fluid composition. These patterns suggest that high gold grades result from the presence of multiple rims of ore-stage pyrite and reflect extended periods of ore fluid flux and ore deposition.