2015 GSA Annual Meeting in Baltimore, Maryland, USA (1-4 November 2015)

Paper No. 322-13
Presentation Time: 4:30 PM

THE MAJOR- AND TRACE-ELEMENT COMPOSITION OF GAHNITE AS A CHEMICAL DISCRIMINANT FOR GRANITIC PEGMATITES AND BROKEN HILL-TYPE PB-ZN-AG DEPOSITS


HEIMANN, Adriana1, YONTS, Jason A.1, WISE, Michael A.2, SPRY, Paul G.3, O'BRIEN, Joshua J.4, RODRIGUES SOARES, Dwight5 and LEYH, Wolf6, (1)Department of Geological Sciences, East Carolina University, 101 Graham Building, Greenville, NC 27858, (2)Dept. of Mineral Sciences, Smithsonian Institution, P.O. Box 37012, Washington, DC 20013-7012, (3)Geological and Atmospheric Sciences, Iowa State University, 253 Science I, Ames, IA 50011, (4)Geological and Atmospheric Sciences, Iowa State University, 253 Science I, Ames, IA 50011-3212, (5)Instituto Federal de Educação, Ciência e Tecnologia da Paraíba (IFPB), N-PEG (Núcleo de Estudos de Pegmatitos), R. Tranquilino Coelho Lemos 671, Campina Grande-Paraíba, 58100–000, Brazil, (6)Eaglehawk Geological Consulting Pty. Ltd, P.O. Box 965, Broken Hill, New South Wales, 2880, Australia, heimanna@ecu.edu

Gahnite (ZnAl2O4) is an accessory phase in a variety of rocks, including granitic pegmatites and metamorphosed massive sulfide deposits. Although variations in the major element content of gahnite in different geologic environments are known, those of trace-elements are still unknown for several settings. The major- and trace-element composition of gahnite in Broken Hill-type (BHT) deposits was recently investigated to distinguish prospective BHT deposits from non-prospective BHT occurrences. Here we present the first in-situ trace-element compositions of gahnite from various types of LCT (lithium-cesium-tantalum enriched) granitic pegmatites (25) worldwide obtained by LA-ICP-MS and compare them, along with major- and minor- element contents, with those from BHT deposits (12) of the southern Curnamona Province, Australia, to identify compositional differences indicative of each environment.

Major-element contents of gahnite in both environments partly overlap, but those in granitic pegmatites have higher Zn contents. In addition, gahnite in granitic pegmatites has higher Mn (1,300 – 8,800 ppm; avg. 3,850 ppm), Li (6 – 243 ppm; avg. 52 ppm), and Cu (8 – 68 ppm; avg. 25 ppm), and lower Mg (30-5,765 ppm; avg. 1,213 ppm), Fe (0.55 – 8.8 wt.% Fe; avg. 4.8 wt.%), Cr (1-11 ppm; avg. 3.5 ppm), Co (0-40 ppm; avg. 6 ppm), and Ni (1.8 – 18.7 ppm; avg. 6 ppm) contents than gahnite in BHT deposits. Gahnite with Mg < 5,800 ppm, Fe < 8.8 wt.%, Mn > 4,000 ppm, Li > 28 ppm, Cu > 40 ppm, Cr < 10 ppm, Co < 40 ppm, and Ni < 20 ppm is characteristic of granitic pegmatites, some of which contain economic rare-metal (Li, Ta) mineralization. In contrast, gahnite with Mg > ~6,000 ppm, Fe > 8.8 wt.%, Cr > 11 ppm, Ni > 20 ppm, and Co > 40 ppm characterizes BHT deposits. A Cu-Co-Cr ternary diagram clearly separates gahnite from both settings.

High Mg, Fe, Cr, Co, and Ni contents in gahnite from BHT deposits are consistent with a previously recognized genetic relationship with mafic magmatism. High Li and low Fe, Mg, Cr, Co, and Ni contents in gahnite from granitic pegmatites reflect the ultra-felsic composition of these rocks and extreme fractional crystallization. Combined major- and trace-element compositions of gahnite obtained from covered terranes can be used as chemical fingerprints to distinguish granitic pegmatites from BHT deposit sources.