VHMS Deposit
    
    - Organization:
 - The Australasian Institute of Mining and Metallurgy
 - Pages:
 - 4
 - File Size:
 - 269 KB
 - Publication Date:
 - Jan 1, 1993
 
Abstract
The potential for major new lenses of Volcanic Hosted Massive  Sulphide (VHMS) beneath the existing Rosebery Deposit is  extremely high. Recent deep drill hole intersections of massive  sulphides, including 22 in true thickness at 24 per cent Zn, may  significantly extend the life of the Rosebery Mine. The Rosebery Ore Deposit is located within Australia's most  prospective VHMS mining district, the Mount Read Volcanic  (MRV) arc of western Tasmania (Figure 1). The MRVs are a 10 - 15 krn wide arcuate belt of lavas, related intrusives and  volcaniclastics. Rosebery is a major Cambrian volcanic hosted  Zn-Pb-Cu-Ag-Au rich deposit which has been over-printed by  Devonian deformation and granitoid alteration resulting in local  rcmobilisation of the ore. The Rosebery Mine Sequence is  composed of an east dipping and east facing, predominately felsic  sequence of rhyo-dacitic volcaniclastics, epiclastics, sediments  and shale lenses more than 500 in thick. This sequence is  bounded by two, low angle (35 - 40¦), east dipping thrust faults,  the Rosebery Fault to the west and the Mount Black Fault to the  cast. The Rosebery Mine lithologies are summarised in the  following table: Hangingwall (HW) Polymictic, quartz, feldspar-phyric  epiclastics.  Black Slates Graphitic, pyritic mudstones. Host Rocks Turbiditic mudstones and sandstones.  Footwall (FW) Feldspar-phyric, pumiceous, mass-flow  breccias. Cambrian, quartz-feldspar, porphyritic sills intrude this  sequence at all levels. Thin, Jurassic, dolerite dykes also occur  throughout the mine. Widespread quartz, sericite and chlorite alteration occurs in the  FW. This alteration is manifested as quartz-augen schists beneath  the orebody. The Host Rocks are pervasively altered with silica,  sericite, chlorite and pyrite. Intense carbonate alteration occurs  within the orebody, whereas chlorite and pyrite alteration is  commonly concentrated directly beneath it. Cambrian  volcanogenic alteration is over-printed by three major Devonian,  granite-derived, assemblages. These are massive to quartz veined  tourmaline, pyrrhotite-pyrite and magnetite-chalcopyrite.  Though the Devonian granite has not been intersected in deep  drill holes or in mine workings, there is good evidence that it  exists within a kilometre of the deposit. The Rosebery orebody is structurally complex when compared  to many other VHMS deposits. Evidence for Cambrian growth  faulting has been found at the North End of the mine (B lens)  where displacement of ore lenses occurs without corresponding  displacement of the overlying Black Slates. A well defined  cleavage exists throughout the mine, dipping at 28 to 50¦E. East  dipping shear zones are also obvious in all parts of the mine  workings and reverse movement is evident on many of these.
Citation
APA: (1993) VHMS Deposit
MLA: VHMS Deposit. The Australasian Institute of Mining and Metallurgy, 1993.