Geochemistry and textural evolution of As-Tl-Sb-Hg-rich pyrite from a sediment-hosted As-Sb-Tl-Pb ± Hg ± Au mineralization in Janjevo, Kosovo

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Dokumenter

  • Fulltext

    Forlagets udgivne version, 29,6 MB, PDF-dokument

  • Sławomir Mederski
  • Jaroslav Pršek
  • Juraj Majzlan
  • Stefan Kiefer
  • Dimitrina Dimitrova
  • Rastislav Milovský
  • Bender Koch, Christian
  • Dawid Kozień

The sediment-hosted As-Sb-Tl-Pb +/- Hg +/- Au Janjevo occurrence is located in the southern part of the KizhnicaHajvalia-Badovc ore field, in the Trepca (Trepca) Mineral Belt (TMB) in Kosovo. The As-Sb-Tl-Pb +/- Hg +/- Au mineralization is hosted by Upper Triassic marbles and occurs in the form of quartz-stibnite veins and dolomitized irregular pockets associated with jasperoid rocks. The main sulfide most widespread in the mineralization studied is pyrite which is the main carrier of thallium. A wide range of techniques was used to characterize the geochemistry and textural evolution of pyrite/marcasite from Janjevo: polarized reflected-light microscopy, electron microprobe (EPMA), laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS), X-ray powder diffraction (XRPD), MOssbauer spectroscopy, and isotopic studies. The study of 42 thin and polished sections resulted in the identification of 4 generations of pyrite/marcasite. The first generation of pyrite related to the pre-ore stage occurs as framboidal pyrite with different degrees of evolution (Py1a), as well as recrystallized pyrite/marcasite (Py1b). Au-enriched pyrite (Py2) occurs as elongated fibrous aggregates and is genetically associated with the formation of stibnite veins (Sb stage). As-Tl-Sb-Hg pyrite (Py3) forms irregular colloform aggregates which fill the stylolites and also overgrow older generations of pyrite. The youngest generation is represented by marcasite (Py4), which forms euhedral crystals. Co/Ni ratio < 1 in all pyrite/marcasite generations implies a sedimentary fingerprint. On the other hand, delta S-34 isotopic studies confirm a magmatic sulfur source for As-Tl-Sb-Hg pyrite (Py3), as well as co-occurring stibnite and realgar. The most important minor and trace elements in pyrite/marcasite are As (up to 14.1 %), Tl (up to 3.94 %), Sb (up to 3.73 %), and Hg (up to 0.55 %), which are mainly hosted by Py3. In addition to arsenic, thallium, antimony, and mercury, other generations of pyrite show enrichment in Ni, Co, and Cu (framboidal pyrite Py1), Au, and Se (Au-enriched pyrite Py2), and Se (marcasite Py4). The highest gold content of up to 6.08 ppm was recorded at Py2. Studies on Py3 geochemistry confirm the presence of 2Fe(2+) Tl+ + Sb3+ heterovalent substitution in pyrite. As-Tl-Sb-Hg pyrite (Py3) is the main thallium host mineral in the mineralization studied, with significantly less thallium present in the Pb-Sb +/- Tl +/- As sulfosalts. In addition, the high arsenic content of Py3 is due to the presence of arsenic in the form of As1- and As-0 related to amorphous arsenic-rich nanoparticles. The reported Py3 is the best phenomenon of the crystallization of colloform As-Tl-Sb-Hg-rich pyrite under hydrothermal conditions. Pyrite-rich sediment-hosted As-Sb-Tl-Pb +/- Hg +/- Au mineralization from Janjevo is associated with the distal manifestation of a concealed porphyry system.

OriginalsprogEngelsk
Artikelnummer105221
TidsskriftOre Geology Reviews
Vol/bind151
Antal sider26
ISSN0169-1368
DOI
StatusUdgivet - dec. 2022

Bibliografisk note

Funding Information:
The research was funded by the Society of Economic Geologists Foundation (SEGF) Newmont Mining Corporation Student Grant 2020 (number 20-91) to SM. The authors would like to thank B. Hyseni, B. Asllani, and students from AGH-UST for help during fieldwork. Also, we are grateful to A. Włodek from the Laboratory of Critical Elements at AGH-UST for help during EMPA data collection. We are grateful to Associate Editor Reimar Seltmann, and two anonymous reviewers for comments and suggestions that helped significantly improve the manuscript.

Funding Information:
The research was funded by the Society of Economic Geologists Foundation (SEGF) Newmont Mining Corporation Student Grant 2020 (number 20-91) to SM. The authors would like to thank B. Hyseni, B. Asllani, and students from AGH-UST for help during fieldwork. Also, we are grateful to A. Włodek from the Laboratory of Critical Elements at AGH-UST for help during EMPA data collection. We are grateful to Associate Editor Reimar Seltmann, and two anonymous reviewers for comments and suggestions that helped significantly improve the manuscript.

Publisher Copyright:
© 2022 The Authors

ID: 329560500