The nature and genesis of gold-silver-tellurium mineralization in the Metaliferi Mountains of western Romania

Citation
Dhm. Alderton et Ae. Fallick, The nature and genesis of gold-silver-tellurium mineralization in the Metaliferi Mountains of western Romania, ECON GEOL B, 95(3), 2000, pp. 495-515
Citations number
88
Categorie Soggetti
Earth Sciences
Journal title
ECONOMIC GEOLOGY AND THE BULLETIN OF THE SOCIETY OF ECONOMIC GEOLOGISTS
ISSN journal
03610128 → ACNP
Volume
95
Issue
3
Year of publication
2000
Pages
495 - 515
Database
ISI
SICI code
0361-0128(200005)95:3<495:TNAGOG>2.0.ZU;2-C
Abstract
Precious metal (Au, Ag) and base metal (Pb, Zn) deposits in the Metaliferi Mountains of western Romania occur in steeply clipping quartz-Ca/Mn carbona te veins, which are hosted by Miocene andesitic stocks and lava flows, and surrounding sedimentary rocks. The deposits consist predominantly of sulfid es (pyrite, chalcopyrite, sphalerite, galena), sulfosalts of As and Sb, and a diverse range of Au-Ag tellurides. The igneous host rocks have undergone mild, pervasive propylitic alteration, whereas immediately adjacent to the veins the wall-rock alteration assemblages consist of quartz, sericite, K feldspar, calcite, and pyrite. Fluid inclusion, stable isotope, and thermod ynamic data suggest that the majority of the mineralization and hydrotherma l alteration in these deposits was caused by loci-salinity (0-5 wt % NaCl e quiv), medium-temperature (200 degrees-300 degrees C), near-neutral (pH = 5 -6) fluids, which underwent occasional boiling. The fluid inclusion and stable isotope data support a model in which a meta l-bearing, magmatic fluid was exsolved from a crystallizing calc-alkaline m elt and ascended to higher levels in the crust, undergoing some isotopic ex change with surrounding sedimentary rocks but limited mixing with ground wa ters, Although the deposits in this part of the Romanian Carpathians exhibi t many of the geologic characteristics of classic low-sulfidation, volcanic -hosted, Au-Ag, epithermal deposits, they seem to have formed from essentia lly magmatic waters, and there is little evidence for the incorporation of meteoric fluids into the hydrothermal system.