TLM 0.00% 25.5¢ talisman mining limited

Ann: Doolgunna Project - Drilling Update, page-44

  1. 13,811 Posts.
    lightbulb Created with Sketch. 690
    HC, I defer to your wisdom. All trace of the copper at DeG being one body that has faulted is no longer there, as is much older dta.

    HC, from mindat.org.

    'The DeGrussa VHMS (volcanic-hosted massive sulphide) copper–gold deposit is located 900 kilometres north of Perth and 150 kilometres north of Meekatharra in the Peak Hill Mineral Field, on the Peak Hill 1:250 000 map sheet, SG 50-8. It lies on a major drainage divide between the Gascoyne River catchment and the Lake Gregory to Carnegie Lake salinas internal drainage. The deposit lies beneath a mantle of scree and sheet wash deposits on gentle slopes mantling an upland area of exposed bedrock and relic duricrust.

    The DeGrussa copper–gold massive sulphide deposit is hosted within the Bryah Basin, one of a number of separate Palaeo-Proterozoic depositional basins in the eastern part of the Capricorn Orogen, which is a major tectonic unit that lies between the Archaean Pilbara Craton and the Yilgarn Craton. The Bryah Group is a succession of mafic rocks of mid-ocean ridge basalt to oceanic plateau affinity overlain by clastic and chemical sediments.

    The age of the Bryah Group is poorly constrained between 2.0 Ga and 1.8 Ga. It is younger than 2.65 Ga and older than 1785 ±11 Ma (U-Pb zircon age), the age of the uncomformably overlying Mount Leake Formation.

    The Bryah Basin has undergone two episodes of deformation. The 1.96 Ga Glenburgh Orogeny (D1) accreted the Narracoota oceanic plateau onto the Yilgarn Craton. Folding, faulting and shearing attributed to this orogeny have been largely overprinted by the 1.8 Ga Capricorn Orogeny (D2) that was the result of the oblique collision between the Pilbara and Yilgarn cratons. During deformation the volcano-sedimentary succession was metamorphosed to greenschist facies.

    The copper–gold rich-massive sulphide lenses are VHMS-style based on the host rock package, mineralisation style, mineral composition and alteration.

    The host rocks are submarine basalts, mafic volcaniclastic rocks and debris flows with sub-volcanic dolerite/**bro sills of the De Grussa Formation.

    Sulphide mineralisation consists of massive sulphide, semi-massive sulphide and stringer zone mineralisation. The transition from massive sulphide to an underlying stringer zone is not always present because of dolerite intrusion close to or at the base of the massive sulphide. Primary sulphide minerals present are pyrite, chalcopyrite, pyrrhotite, and sphalerite together with magnetite. The base of the massive sulphide is chalcopyrite rich with magnetite, passing upwards into iron sulphides with decreasing copper content and increasing zinc content higher up. Gold is associated with the chalcopyrite-rich zones and occurs as a high-silver electrum.

    The oxide mineralisation is located vertically above Conductor 1 and DeGrussa. The grade and width of the oxide mineralisation is highest proximal to the main lenses and then forms enriched plumes that transgress lithological boundaries as the mineralisation disperses and dissipates. Close to the main lenses there is significant native copper and elevated gold. As the plumes disperse away from the ore zones the grade dissipates and mineralisation transitions through chrysocolla, cuprite, azurite and malachite.

    Alteration associated with the massive sulphide is chlorite + sericite + quartz + pyrite which is typical for VHMS deposits. Stringers in the stringer zone are chalcopyrite rich.
    The massive sulphide lenses are deformed and often exhibit a strong foliation. The harder pyrite and pyrrhotite tends to fracture, while the softer chalcopyrite and sphalerite are easily remobilized and recrystallised.

    Beneath a hardpan cap there is about 80 metres of weathering over the sulphide lenses. Within the weathering profile is an upper, residual, gold-oxide zone overlying an oxide-copper zone. The oxide- copper zone contains the minerals malachite, chrysocolla, native copper and minor cuprite. A secondary supergene chalcocite blanket lies beneath the oxide-copper zone and immediately above fresh primary sulphides.

    Four lenses of copper-rich massive sulphides have been discovered to date. DeGrussa has a strike length of 180m, is some 20m thick on average and dips near vertically to the south. It has a vertical extent of 300m.

    Operates as underground workings and an open pit by Sandfire Resources. According to the company, it was cash strapped, and on the verge of collapse, when drilling un-covered the deposit. It is one of the few deposits found through exploration over the past 20 years in Western Australia, which has progressed to a major new mine. Sandfire Resources is also one of the few mining companies in Western Australia, who have actively supported the local mineral specimen collecting community. Native copper, chrysocolla, malachite, cuprite and the rare species mcguinnessite have been provided to the public via a shop in central Perth, and donated by the company to the Western Australian Museum, and as fund raising for MINSOCWA. Further, at great expense, it has flown members of the club to inspect the mine. "

    NB the 4 lenses!!

    From Portergeo:

    The DeGrussa copper deposits are located within the Bryah Basin, part of the 2.0 to 1.8 Ga Capricon Orogen that separates the Yilgarn and Pilbara Cratons, approximately 900 km NNE of Perth and 150 km north of Meekatharra in Western Australia.

    Mineralisation is hosted by the Palaeoproterozoic (2.0 Ga) Narracoota Volcanics, occurring as the DeGrussa, Conductor 1, 4 and 5 deposits. The 2 km-thick sequence of volcano-sedimentary rocks that comprise the Narracoota Volcanics are pread over a strike length of 22 km.

    The Narracoota Volcanics comprise basalts, basaltic hyaloclastites, sediments, dolerite and **bro and minor local mineralised quartz carbonate breccias, jasper beds and banded iron formation. This sequence is overlain by the Karalundi Formation, which comprises metamorphosed and locally ferruginous shale and sandstone with metaconglomerate bands and lenses, and chert and siliciclastic metasediments. Together, the Narracoota Volcanics and Karalundi Formation constitute the Bryah Group.

    To the north, the ENE trending belt of Narracoota Volcanics are separated from the Marymia Dome (which comprises two Archaean greenstone belts intruded by granite) by a 1 to 4 km thick band of quartz-mica schist of comparable strike length to the host volcanic belt. The Bryah Basin rocks are underlain by the Palaeoproterozoic, basalt rich Yerrida Group.

    The ores at DeGrussa are classified as volcanic hosted massive sulphide (VHMS)-style deposits, occurring as massive lenses of primary pyrite, chalcopyrite and pyrrhotite with minor magnetite, sphalerite, galena and arsenopyrite in a gangue of siderite, ankerite, stilpnomelane, minnesotaite, quartz and calcite.

    The primary mineralisation has been subjected to oxidation and supergene enrichment near surface to produce a surface zone with native copper and siliceous cap with gold, overlying a layer of oxide/carbonate copper and a blanket of supergene chalcocite with tenorite, cuprite and complex tellurides.

    The main DeGrussa deposit represents a 20 m-thick, steeply dipping to almost vertical body of high grade copper-gold mineralisation with lesser zinc and silver. It is defined over a 180 m lateral strike extent and persists to a known vertical depth of more than 300 m.

    The Conductor 1 deposit occurs as a number of stacked lenses and underlies the main DeGrussa ore zone. It averages 15 m in thickness and extends over a lateral strike length of 350 m, with a steep 75° south-west trending dip, persisting to a known vertical depth of 400 m.

    The smaller Conductor 4 deposit lies 120 m below and 200 m east of Conductor 1 and DeGrussa. A further small deposit, Conductor 5 has also been delineated, ~200 m further to the east.

    All are distributed along the steep, northeast-trending Shiraz Fault zone which offsets the ore bodies and is a significant local structure with varying widths of highly broken material. The Merlot and Pinot faults also have a local, but less pronounced interaction with the massive sulphide lenses.

    In September 2010, the total indicated + inferred resources at DeGrussa, and Conductor 1, 4 and 5 amounts to (Sandfire Resources website):
    10.67 Mt @ 5.6% Cu, 1.9 g/t Au, 15 g/t Ag,
    including a high grade zone of supergene enriched mineralisation of
    0.25 Mt @ 17.6% Cu, 2.6 g/t Au, 21 g/t Ag. "

    All good news to SM.
 
watchlist Created with Sketch. Add TLM (ASX) to my watchlist
(20min delay)
Last
25.5¢
Change
0.000(0.00%)
Mkt cap ! $48.02M
Open High Low Value Volume
25.5¢ 26.0¢ 25.5¢ $30.3K 117.0K

Buyers (Bids)

No. Vol. Price($)
1 38302 25.5¢
 

Sellers (Offers)

Price($) Vol. No.
27.0¢ 78058 1
View Market Depth
Last trade - 15.31pm 25/06/2024 (20 minute delay) ?
TLM (ASX) Chart
arrow-down-2 Created with Sketch. arrow-down-2 Created with Sketch.