CALL FOR PROPOSALS:

ORGANIZERS

  • Harvey Thorleifson, Chair
    Minnesota Geological Survey
  • Carrie Jennings, Vice Chair
    Minnesota Geological Survey
  • David Bush, Technical Program Chair
    University of West Georgia
  • Jim Miller, Field Trip Chair
    University of Minnesota Duluth
  • Curtis M. Hudak, Sponsorship Chair
    Foth Infrastructure & Environment, LLC

 

Paper No. 9
Presentation Time: 4:00 PM

MAJOR, MINOR, AND TRACE ELEMENT CONTENTS OF GAHNITE (ZINCIAN SPINEL) AS GUIDES IN THE SEARCH FOR BROKEN HILL-TYPE MINERALIZATION NEAR BROKEN HILL, AUSTRALIA: A PRELIMINARY STUDY


O'BRIEN, Joshua J., Geological and Atmospheric Sciences, Iowa State University, 253 Science I, Ames, IA 50011-3212, SPRY, Paul G., Geological and Atmospheric Sciences, Iowa State University, 253 Science I, Ames, IA 50011, TEALE, Graham S., Teale and Associates, P.O. Box 740, North Adelaide, South Australia, 5006, Australia, JACKSON, Simon, Natural Resources Canada, Geological Survey of Canada, 601 Booth Street, Ottawa, ON K1A 0E8, Canada and ROGERS, Dean, Perilya Limited, P.O. Box 5001, Broken Hill, New South Wales, 2880, Australia, jjobrien@iastate.edu

Gahnite (ZnAl2O4) occurs in a wide variety of geological settings, including metamorphosed massive sulfide deposits (MMSD), and has been used as a guide in the exploration for ores of this type. The major element composition of gahnite depends on host rock composition, T, P, fS2, and fO2. Major (Zn, Fe, and Mg) and minor (Mn) element contents of gahnite have been used to fingerprint potential host rock lithologies, effectively defining a distinct compositional range for gahnite spatially associated with MMSD. However, while useful in distinguishing between various geological settings, major element compositions of gahnite fail to discriminate between sulfide-rich rocks and sulfide-poor uneconomic prospects. In an attempt to overcome this deficiency, we combine the major and minor element compositions of gahnite with trace element data. To date, no trace element studies of gahnite have been published.

LA-ICP-MS and electron microprobe studies of gahnite from 12 Broken Hill-type (BHT) deposits, including the supergiant (200 Mt) Broken Hill Pb-Zn-Ag deposit, were undertaken to evaluate whether or not a geochemical fingerprint can be used to distinguish prospective BHT deposits from non-prospective BHT occurrences. LA-ICP-MS analyses (n = 220) of gahnite, show compositions of up to 4000 ppm Mn, 240 ppm Co, 6400 ppm Cr, 880 ppm V, 520 ppm Ti, 140 ppm Ni, 2 ppm Sn, 570 ppm Ga, 26 ppm Cd, 16 ppm Li, 21 ppm Be, and 4 ppm Sc, with rare earth elements being generally below detection limits (< ~1 ppb). Gahnite from the main Broken Hill deposit and smaller BHT deposits north of Broken Hill (Potosi, Globe, Round Hill, Flying Doctor), can generally be distinguished from those south of Broken Hill (Ten Two, Henry George, 11:30, Stirling Hill) in various discrimination diagrams (e.g., V vs Cr, Co vs Cr, Ni vs V, Zn/Fe vs V, Zn/Fe vs Cr), and statistically through a principal component analysis. A dendrogram plot of our data suggests that it can be used to identify gahnite in smaller deposits with compositions similar to gahnite from the main Broken Hill lode. Before a geochemical fingerprint can be established for exploration purposes, further studies will need to consider the dependency of ionic radii, and the partition coefficients for each element between gahnite and coexisting minerals (e.g., garnet, biotite, muscovite, and staurolite).

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