Laser ablation ICP-MS study of trace elements in scheelite in different types of mineralization from the Bohemian Massif

Authors

  • Jan Pašava Czech Geological Survey, Geologická 6, 15200 Praha 5, Czech Republic https://orcid.org/0000-0002-1457-0165
  • Petr Bohdálek Czech Geological Survey, Geologická 6, 15200 Praha 5, Czech Republic
  • Jan Malec Czech Geological Survey, Geologická 6, 15200 Praha 5, Czech Republic
  • František Veselovský Czech Geological Survey, Geologická 6, 15200 Praha 5, Czech Republic
  • Ana Carolina Miranda Département de Géologie et Génie Géologique, Centre de recherche sur la géologie et l’ingénierie minérale, Université Laval, Québec (QC), Canada https://orcid.org/0000-0002-0223-202X
  • Georges Beaudoin Département de Géologie et Génie Géologique, Centre de recherche sur la géologie et l’ingénierie minérale, Université Laval, Québec (QC), Canada https://orcid.org/0000-0002-4029-2648
  • Bertrand Rottier Département de Géologie et Génie Géologique, Centre de recherche sur la géologie et l’ingénierie minérale, Université Laval, Québec (QC), Canada https://orcid.org/0000-0002-5386-0472

DOI:

https://doi.org/10.7306/gq.1798

Keywords:

scheelite, gold deposits, skarns, greisen-type deposits, Bohemian Massif

Abstract

We describe scheelite in five types of mineral deposit from the Bohemian Massif (greisen, orogenic Au, reduced intrusion-related gold systems (RIRGS), oxidized and reduced skarn) via cathodoluminescence (CL) imaging and laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) analyses. We document variability in the scheelite composition within single grains and/or deposit types that reflects the nature and evolution of the ore-forming fluids. We provide scheelite typical trace element characteristics and chondrite-normalized REE patterns for different deposit types, confirming that scheelite can be used as an indicator mineral for their exploration. For example, scheelite from greisen-related deposits is usually rich in Sn, Sr, Y and HREE with various ranges of median values in individual deposits (0.05–8.0 ppm, 232.4–567.1 ppm, 0.06–465.0 ppm and 0.06–632.5 ppm, respectively) and with typical chondrite-normalized REE patterns showing Eu negative or positive anomaly. Under UV light scheelite from Sn-W deposits displays variable colours from whitish via yellowish to bluish. In contrast to greisen-related deposits, scheelite from Au-orogenic association is usually relative rich in Pb (median range in individual deposits: 6.1–11.2 ppm), and relatively poor in Mg, Mo and Nb. Flat and bell-type chondrite-normalized REE patterns show a pronounced Eu positive anomaly. Under UV light it is predominantly homogenous and bluish. Scheelite from oxidized skarn is enriched in Mo, Nb and ΣLREE (median range in individual deposits: 311.4–7214.1 ppm, 1.3–214.9 ppm, and 1.1–1375.8 ppm, respectively), and scheelite from reduced skarns is characterized by the lowest median ranges of Nb (1.7–107.8 ppm), Y (0.69–41.1 ppm), Mn (0.5–17.0 ppm) and Zn (0.04–0.252 ppm) in individual deposits, when compared to all the groups studied. Scheelite from oxidized and reduced skarn deposits displays several types of chondrite-normalized pattern: (1) LREE-enriched with a positive or negative Eu anomaly, (2) Bell-shaped REE patterns with negative or without Eu anomaly, and (3) Flat REE patterns with a negative Eu anomaly. Scheelite from oxidized and reduced skarn deposits is commonly zoned and mostly bluish under UV light.

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Published

2025-08-29

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Articles