38 Economic Geology, Igneous and Metamorphic Petrology, Mineralogy (Posters)

Tuesday, 17 April 2018
8:00 AM - 5:30 PM
First Floor Lobby


INQUIRY INTO THE SULFUR ISOTOPE COMPOSITION OF THE VMS DEPOSITS IN THE PENOKEAN VOLCANIC BELT

Paper number: 38-5
Program: Theme Sessions
Time: 8:00 AM – 5:30 PM


Authors


Abstract

The Penokean Volcanic Belt (PVB) of Northern Wisconsin hosts several volcanogenic massive sulfide (VMS) deposits. VMS deposits are significant sources of metallic resources such as Cu, Au, Pb, and Zn in the form of sulfide ores. The sulfide ores can be tested for δ34S values in relation to the Vienna-Canyon Diablo Troilite (VCDT). The δ34S values can indicate possible sources of sulfur for sulfide formation.

For this study 185 sulfide mineral samples were taken from seven VMS deposits within the PVB. The deposits spread over 250 km from east to west in this order; Back Forty, Horseshoe, Bend, Flambeau, Eisenbrey, and Schoolhouse, with Reef being 50 km south of the center of the spread . The sulfide species were identified through petrographic study and prepared for sulfur isotope identification. A Delta V Isotope Ratio Mass Spectrometer was used to process the samples to attain δ34S values.

To date the resulting data shows average δ34S values for each deposit of +2.35 ppm for Back Forty, -0.36 ppm for Bend, -0.95 ppm for Reef, -1.00 ppm for Schoolhouse. Possible sources of the δ34S variance in the Back Forty deposit may indicate a paleo geographic setting near ocean margin. The proximity to land could allow for sulfur contamination from evaporite beds along the shoreline. The more negative values of the other deposits may indicate a deeper ocean setting with little continental contamination of sulfur.


Geological Society of America Abstracts with Programs. Vol. 50, No. 4

doi: 10.1130/abs/2018NC-312688

© Copyright 2018 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.