Depositional Models for the Sediment-Hosted Cu-Zn-Pb Deposits of N. Australia
 
    
    - Organization:
- The Australasian Institute of Mining and Metallurgy
- Pages:
- 4
- File Size:
- 150 KB
- Publication Date:
- Jan 1, 1987
Abstract
The Proterozoic Pb-Zn deposits of the  Gulf of Carpentaria, Australia, include HYC  (McArthur River), Mt. Isa, Dugald River, Lady  Loretta and Hilton. Two seamingly incom- patible depositional models have been proposed  to account for their origin. Finlow-Bates  (1980), Large (1983) and Russell(1983)  classify these-deposits as sediment-hosted  submarine exhalative deposits. This class  includes Rammelsberg, Meggen, Silvermines,  Sullivan and others. In contrast, a lacus- trine, shallow-water origin has been advocated  by Williams and Logan (1981), Logan and  Williams (1984), Muir (1983) and Eugster  (1985). The discrepancies between these two  models can be removed by creating a separate  class, that of continental sediment-hosted  exhalative deposits.. HYC., Mt. Isa and Dugald  belong to this class and their sediments were  deposited in shallow, alkaline lakes. Metal- rich, hot, Na-Ca-Cl brines entered the basins  along boundary faults and interacted with pore  fluids and sediments, depositing-Cu-Zn-Pb sul- fides. Similar brines entered the Lady Loretta  basin after marine flooding, depositing sulfi- des and barite, placing Lady Loretta into the  class of marine Sedex deposits.
Citation
APA: (1987) Depositional Models for the Sediment-Hosted Cu-Zn-Pb Deposits of N. Australia
MLA: Depositional Models for the Sediment-Hosted Cu-Zn-Pb Deposits of N. Australia. The Australasian Institute of Mining and Metallurgy, 1987.
