Quick
Search: 
 
advanced search
 GSW Home    GeoRef Home    My GSW Alerts    Contact GSW    About GSW    Journals List    Help 
Economic Geology Don't get GSW? Talk to your librarian.
JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS

Economic Geology; June 2004; v. 99; no. 4; p. 807-817; DOI: 10.2113/99.4.807
© 2004 Society of Economic Geologists
This Article
Right arrow Figures Only
Right arrow Full Text
Right arrow Full Text (PDF)
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Right arrow Citation Map
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Similar articles in ISI Web of Science
Right arrow Alert me to new issues of the journal
Right arrow Download to citation manager
Right arrow reprints & permissions
Citing Articles
Right arrow Citing Articles via Google Scholar
Google Scholar
Right arrow Articles by Paradis, S.
Right arrow Articles by Lavoie, D.
Right arrow Search for Related Content
GeoRef
Right arrow GeoRef Citation

Scientific Communications

FLUID INCLUSION AND ISOTOPE EVIDENCE FOR THE ORIGIN OF THE UPTON Ba-Zn-Pb DEPOSIT, QUEBEC APPALACHIANS, CANADA*

Suzanne Paradis{dagger}

Mineral Resources Division, Geological Survey of Canada, 9860 West Saanich Road, Sidney, British Columbia, Canada V8L 4B2

Guoxiang Chi

Department of Geology, University of Regina, 3737 Wascana Parkway, Regina, Saskatchewan, Canada S4S 0A2

Denis Lavoie

Geological Survey of Canada, Centre Géoscientifique de Québec, 880 Chemin Ste-Foy, P.O. Box 7500, Québec, Canada G1V 4C7

{dagger} Corresponding author: e-mail, suparadi{at}nrcan.gc.ca

The Upton Ba-Zn-Pb deposit is hosted by the Early Ordovician crinoidal limestone of the Upton Group in the southern Quebec Appalachians. Mineralization consists of barite and minor amounts of sphalerite, pyrite, galena, and chalcopyrite. The paragenesis includes (1) development of secondary porosity and precipitation of subhedral barite, bladed barite, and barite rosettes; (2) precipitation of fracture-filling barite; (3) filling of fractures and remaining voids in the limestone by a sparry calcite; and (4) precipitation of sulfides, quartz, organic matter, and bitumen in the fractures and along the stylolites. Fluid inclusions were studied in pre-barite syntaxial calcite overgrowths, in subhedral and bladed barite, and in post-barite calcite, sphalerite, and quartz. The homogenization temperatures and salinities of the fluid inclusions are greater than 50°C (single-phase liquid inclusions) and 3.9 to 6.9 wt percent NaCl equiv for syntaxial calcite cement, 42.1° to 96.9°C and 4.7 to 8.1 wt percent NaCl equiv for subhedral and bladed barite, 101.4° to 142°C and 5.1 to 7.5 wt percent NaCl equiv for fracture-filling barite, 82.4° to 132.2°C and 18.3 to 19.7 wt percent NaCl equiv for sphalerite, and 121.8° to 164.2°C and 1.7 to 4.2 wt percent NaCl equiv for quartz. Bitumen is present throughout the paragenesis, but primary CH4 inclusions only occur in quartz. H2S- and CH4-enriched gases were detected in barite and calcite by quadrupole mass spectrometry (QMS) analysis, occurring as secondary fluid inclusions. The 87Sr/86Sr ratios of the barite range from 0.70654 to 0.70781, lower than Early Ordovician seawater. Based on these results and previous C-O-S isotope data, we propose that the Upton Ba-Zn-Pb deposit was formed by mixing of two fluids, a marine water-dominated, SO2–4-rich fluid, and an 18O-enriched and 87Sr-depleted basinal brine, which carried Ba, Zn, and Pb. The reduced sulfur required for the precipitation of sulfides was derived from the thermochemical reduction of sulfate by hydrocarbons. The late precipitation of sulfides after barite may be related to the sluggishness of the sulfate reduction. The mineralization occurred during the Middle to Late Ordovician Taconian orogeny, and tectonic burial and compression is thought to have initiated the circulation of fluids, which would have been channeled through the sedimentary pile along thrust faults and vertical fractures and migrated into the confined crinoidal limestone.







JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS
Copyright © 2008 by Society of Economic Geologists