For best results when printing this announcement, please click on link below:
https://newsfile.refinitiv.com/getnewsfile/v1/story?guid=urn:newsml:reuters.com:20250317:nRSQ9022Aa&default-theme=true
RNS Number : 9022A Great Southern Copper PLC 17 March 2025
THIS ANNOUNCEMENT CONTAINS INSIDE INFORMATION AS STIPULATED UNDER THE UK
VERSION OF THE MARKET ABUSE REGULATION NO 596/2014 WHICH IS PART OF ENGLISH
LAW BY VIRTUE OF THE EUROPEAN (WITHDRAWAL) ACT 2018, AS AMENDED. ON
PUBLICATION OF THIS ANNOUNCEMENT VIA A REGULATORY INFORMATION SERVICE, THIS
INFORMATION IS CONSIDERED TO BE IN THE PUBLIC DOMAIN.
17 March 2025
Great Southern Copper plc
("GSC" or the "Company")
"Exceptional" High-Grade Cu-Ag Results Confirm Potential of the Mostaza
Deposit, Cerro Negro
Assays demonstrate continuity of grade with mineralisation open laterally and
at depth
Great Southern Copper plc (LSE: GSCU), the company focused on
copper-gold-silver exploration in Chile, is pleased to report further
exceptional assay results from Phase I drilling at the Mostaza Mine, Cerro
Negro.
Highlights:
· Assay results received for holes CNG25 DD002 - DD005 with significant
intervals including;
Ø DD005: 12.0m of 4.24% Cu and 369.5 g/t Ag from 40m, including
§ 7.0m of 5.08% Cu and 449.6 g/t Ag from 45m, within a broader zone of
§ 21.0m of 2.88% Cu and 246.7 g/t Ag from 35m
Ø DD003: 13.0m of 2.48% Cu and 198.1 g/t Ag from 39m, within a broader zone
of
§ 18.6m of 1.85% Cu and 146.6 g/t Ag from 36.6m
Ø DD002: 4.2m of 1.73% Cu and 126.5 g/t Ag from 38.9m
· New results demonstrate continuity of high grades building upon
earlier reported assays for hole CNG25 DD001(1);
Ø DD001: 20.0m of 3.31% Cu and 269.9 g/t Ag from 27m, including
§ 7.0m of 5.72% Cu and 489.6 g/t Ag from 31m
· Assay grades consistently significantly higher than reported results
of historical drill program
· Mineralisation remains open in all directions
· Assay results for remaining Phase I drill holes, CNG25 DD006 - 009,
are pending
· Phase II diamond drilling in progress aiming to expand on
historically reported resources and test exploration targets(2)
· GSC holds option to own 100% of the Mostaza mine and Cerro Negro
project
· Prospect located at low elevation with excellent access to
infrastructure and mining services
Sam Garrett, Chief Executive Officer of Great Southern Copper, said: "These
outstanding results confirm that high grade Cu-Ag mineralisation is continuing
to depth and along strike and demonstrate that the former Mostaza mine has the
potential to be a high-grade high-value Cu-Ag deposit.
"Two diamond drill rigs are now on site - one targeting strike and depth
extensions of the Mostaza pit mineralisation and a second rig is exploring the
structural trend to the south following up earlier drilling of holes
DD006-009.
"We have entered a very exciting phase of exploration at Cerro Negro and have
a lot of work to do as we progress to demonstrate the potential economic
viability of this exciting deposit."
Results of diamond drillholes CNG25 DD002 - DD005
Diamond drillholes CNG25 DD002 - DD005 were designed to target shallow
extensions of the historical Mostaza Lens 2 mineralisation at depth and along
strike of the intercept in CNG25 DD001 (Figure 1). Due to access and safety
limitations in the old mine pit the five holes were drilled in a fan pattern
from a centrally located drill pad and were planned to intersect the
mineralised body on an approximate grid pattern.
All holes intersected the Lens 2 mineralised body over varying widths and
significant assays are summarised in Table 1. The mineralisation is also
weakly anomalous in Sb-As and exhibits pathfinder anomalism for Bi-Cd-Li-Zn
which is consistent with the high-sulphidation style of mineralisation.
Drillhole CNG25 DD002 was drilled to intersect the lens approximately 25m
north of hole DD001 and returned 4.2m @ 1.73 % Cu, 126.5 g/t Ag, and 0.0824 %
Sb from 38.9m. CNG25 DD003, which was designed to test the lens below hole
DD002, intersected 18.6m @ 1.85% Cu, 146.58 g/t Ag from 36.6m, including 13m @
2.48 % Cu, 198.09 g/t Ag from 39m, with maximum grades of 1m @ 4.64 % Cu,
406.00 g/t Ag, and 0.22% Sb from 50m. These results appear to demonstrate that
both Cu-Ag grade and thickness the lode is increasing with depth.
Hole CNG25 DD005 was drilled below hole DD001 and intersected broad intervals
of high-grade Cu-Ag similar to mineralisation seen in hole DD001(1) including
7m @ 5.08 % Cu, 449.57 g/t Ag from 45m, and 2m @ 6.05 % Cu within a broader
lens-wide zone of 21m @ 2.89 % Cu, 246.71 g/t Ag from 35m.. Maximum grades of
6.2 % Cu, 567 g/t Ag, and 0.23 % Sb are reported over 1m.
Hole CNG DD004 was drilled to the north of DD002 and intersected only weakly
altered and mineralised "proto-lens" in a zone of faults and dykes where the
lens was otherwise expected, suggesting the lode has been structurally
displaced or "pinched out" in this location.
A summary of all Phase I assay results to date are shown in Table 1 below.
Hole_ID From (m) To (m) Interval (m) Cu (%) Ag (g/t) Sb (ppm)
CNG25 DD001 27 47 20.0 3.31 269.9 934
inc 31 38 7.0 5.72 489.6 1085
inc 35 38 3.0 6.62 562.7 407
CNG25 DD002 38.9 43.1 4.2 1.73 126.5 824
CNG25 DD003 36.6 55.2 18.6 1.85 146.6 798
inc 39 52 13.0 2.48 198.1 1049
inc 48 51 3.0 3.31 254.7 1608
inc 50 51 1.0 4.64 406.0 2150
CNG25 DD004 no significant intercepts
CNG25 DD005 35 56 21.0 2.89 246.7 978
inc 37 52 15.0 3.79 328.4 1252
inc 40 52 12.0 4.24 369.5 1279
inc 45 52 7.0 5.08 449.6 1309
inc 45 47 2.0 6.05 547.5 645
Table 1: Summary of significant intercepts for Phase I GSC drill holes.
The Mostaza Cu-Ag deposit, Cerro Negro
The high-grade Cu-Ag mineralisation at Mostaza is confined to a north-south
trending, structurally-controlled lode, or "lens" (specifically Lens 2), of
variable width (<4-20m) that dips moderately steeply to the west (Figure
2). Copper mineralisation comprises abundant disseminations, veinlets, crackle
networks, and breccia matrix fillings of hypogene black to dark metallic grey
chalcocite with lesser bluish bornite and traces of chalcopyrite and pyrite
(Figure 3). Petrographic confirmation is pending, however, the copper
mineralogy may include other silver-rich copper minerals such as stromeyerite
(AgCuS) for example.
Lens 2 host rocks are intensely altered and appear to comprise multiple
generations of breccia, tuffisite, and felsic intrusive altered to texturally
destructive illite ± montmorillonite overprinted by probable alunite ±
dickite ± pyrophyllite (to be confirmed by petrographic studies). The
high-grade Cu-Ag mineralised lens exhibits sharp contacts and is bounded to
the east and west by faults that are typically invaded by narrow (<1-2m)
andesite to rhyolite dykes. Outside of the bounding dykes and faults, the
enclosing wall rocks consist of an east-dipping bedded sequence of fresh,
black volcanic lava flows and red, hematite-rich phreatic and/or
phreatomagmatic breccias that might be part of a large dome-diatreme complex
outcropping to the east.
Insufficient drilling is available to date to allow detailed interpretation of
the architecture of the deposit. The lack of high-grade mineralisation
intersected in hole DD004 indicates late-stage structural dislocation occurs
resulting in variable localised thinning or boudenaging of the lenses. Broad
zones of weakly anomalous silver (>0.1ppm Ag) in hole DD004 might also
suggests the potential for this hole to be adjacent to significant lode
mineralisation. The narrower lode width intersected in hole DD002 suggests
also that mineralisation may be "stoped out" in places by post-mineral dykes
of the same type that intrude the bounding fault structures.
The high-grade Cu-Ag mineralogy type and associated advanced argillic style
alteration suggests the lodes at Mostaza are part of a high-sulphidation
epithermal system, potentially related to a yet-to-be-discovered porphyry
style deposit occurring at depth.
The Lens 2 mineralisation is interpreted to form one of a number of Cu-Ag rich
bodies mapped at surface which have historically been interpreted as discrete
"lenses" but which collectively have the potential to make up an anastomosing
network of structurally controlled zones of mineralisation continuous over a
strike length of greater than 1-2km.
The results of CNG25 DD001- DD005 targeting mineralisation beneath the
existing Mostaza open pit demonstrate that the deposit continues at depth and
along strike from the historical drilling and is open in all directions
(Figure 4).
Figure 1: Cerro Negro Project, Mostaza Mine: Simplified schematic long section
of Lens 2 with circles showing the approximate location of where Phase 1
drillholes intersect the hanging wall of the mineralised lens. The apparent
thickness of copper mineralisation is indicated below each intersection point.
Note that mineralisation remains open at depth and along strike. Historical
resource blocks are for reference.
Figure 2: Cerro Negro Project, Mostaza Mine: Schematic cross section through
drillholes CNG25 DD001 and DD005 showing Cu-Ag intercepts and the preliminary
geological interpretation and relationship to historical drillholes. Note the
extrapolations from diamond holes DD001 and DD005 to the historical drillholes
EDH25, 23 and 15 are based on assay results only because historical drill core
and logs are unavailable.
Figure 3: Cerro Negro Project, Mostaza Mine. Photograph of core from hole
CNG25 DD002 and DD003, on the left, and DD005 on the right, with grades of Cu
% and Ag g/t. The black disseminations, veinlets and crackle fill are Cu-Ag
bearing sulphides and sulfosalt minerals in association with minor silica and
baryte gangue cutting clay-rich alteration.
Core preparation, sampling and assaying
The Mostaza diamond drill core is collected from site by GSC staff and
transported to the Company's nearby sampling facilities where it is then
processed for geological, geotechnical, petrophysical and geochemical data.
Sampling intervals are selected principally on geologic boundaries and may
vary in length up to 2m. The core is cut into two halves using an electric
diamond brick saw with half-core samples each allocated a unique identifier
code and bagged-tagged separately. Samples for each complete hole are
transported by GSC personnel to ALS laboratories in Santiago, Chile for sample
preparation (drying, weighing, crushing and grinding). A final 200g aliquot of
each sample is forwarded by ALS to their laboratories in Lima, Peru where it
is assayed for Au (by 30g fire assay with ICP-AES finish method) plus a suite
of 48 base metals and trace elements including Cu and Mo (by four acid digest
ICP-MS method).
Sampling and assaying QAQC protocols employed by the company for this drilling
project include routine insertion of standard reference materials including
standards and blanks. Results for each SRM is assessed to monitor the accuracy
and precision of the assay data from ALS for the core samples.
Next steps
Phase II diamond drilling at Mostaza has commenced and is designed to include
resource and exploration drilling. Metallurgical studies of drill core,
stockpiles and tailings are also being planned. Extensions of mineralisation
at depth and along trend under cover may also be targeted with geophysical
surveys.
HOLE_ID SAMPLE FROM TO LONG LITHOLOGY Cu % Ag g/t Sb ppm
ID (m) (m) (m)
CN25-DDH001 994564 0 2 2 Saprock 0.017 0.43 13.45
CN25-DDH001 994565 2 4 2 Black Breccia 0.057 3.96 30.60
CN25-DDH001 994566 4 6 2 0.007 0.62 2.91
CN25-DDH001 994567 6 8 2 0.008 0.41 4.66
CN25-DDH001 994568 8 10 2 Red Breccia 0.001 0.05 1.84
CN25-DDH001 994569 10 12 2 0.002 0.07 2.01
CN25-DDH001 994571 12 14 2 0.001 0.06 2.10
CN25-DDH001 994572 14 16 2 0.003 0.19 3.62
CN25-DDH001 994573 16 18 2 0.002 0.10 3.68
CN25-DDH001 994574 18 20 2 0.004 0.22 5.38
CN25-DDH001 994575 20 22.9 2.9 0.002 0.10 3.60
CN25-DDH001 994576 22.9 24.6 1.7 0.032 1.01 6.89
CN25-DDH001 994578 24.6 26 1.4 Dyke 0.010 0.12 3.21
CN25-DDH001 994579 26 27 1 0.012 0.70 93.20
CN25-DDH001 994580 27 28 1 Lens 2 2.670 193.00 666.00
CN25-DDH001 994581 28 29 1 1.850 169.00 464.00
CN25-DDH001 994582 29 30 1 1.530 138.00 328.00
CN25-DDH001 994583 30 31 1 1.650 129.00 491.00
CN25-DDH001 994585 31 32 1 4.910 455.00 377.00
CN25-DDH001 994586 32 33 1 5.600 451.00 1215.00
CN25-DDH001 994587 33 34 1 6.050 528.00 3460.00
CN25-DDH001 994588 34 35 1 3.650 305.00 1320.00
CN25-DDH001 994589 35 36 1 6.600 530.00 868.00
CN25-DDH001 994590 36 37 1 6.790 575.00 206.00
CN25-DDH001 994591 37 38 1 6.460 583.00 146.00
CN25-DDH001 994592 38 39 1 2.380 182.00 352.00
CN25-DDH001 994594 39 40 1 0.515 23.90 109.50
CN25-DDH001 994595 40 41 1 1.550 74.90 1130.00
CN25-DDH001 994596 41 42 1 1.145 78.10 2080.00
CN25-DDH001 994598 42 43 1 2.460 158.00 2480.00
CN25-DDH001 994599 43 44 1 1.905 139.00 758.00
CN25-DDH001 994600 44 45 1 1.995 152.00 490.00
CN25-DDH001 994601 45 46 1 4.750 395.00 1055.00
CN25-DDH001 994602 46 47 1 1.750 139.00 687.00
CN25-DDH001 994603 47 48 1 0.393 24.70 85.80
CN25-DDH001 994605 48 49 1 Dyke 0.013 0.93 39.30
CN25-DDH001 994606 49 50 1 0.005 0.44 26.40
CN25-DDH001 994607 50 51 1 Red Breccia 0.006 0.41 27.80
CN25-DDH001 994608 61 62 1 0.002 0.15 6.26
CN25-DDH001 994609 71 72 1 0.001 0.08 10.35
CN25-DDH001 994610 81 82 1 0.003 0.09 17.45
CN25-DDH001 994612 91 92 1 0.002 0.12 13.65
CN25-DDH001 994613 101 102 1 0.001 0.06 8.60
CN25-DDH002 994614 0 2 2 Saprock 0.010 0.18 10.20
CN25-DDH002 994615 2 4 2 0.005 0.20 2.56
CN25-DDH002 994616 4 6 2 Black Breccia 0.007 0.40 3.17
CN25-DDH002 994617 6 8.29 2.29 0.024 0.43 8.11
CN25-DDH002 994618 8.29 10 1.71 Red Breccia 0.001 0.02 1.54
CN25-DDH002 994619 10 12 2 0.001 0.03 1.72
CN25-DDH002 994620 12 14 2 0.002 0.04 2.12
CN25-DDH002 994621 14 16 2 0.001 0.03 2.28
CN25-DDH002 994622 16 18 2 0.001 0.01 3.21
CN25-DDH002 994623 18 20 2 0.002 0.03 4.20
CN25-DDH002 994624 20 22 2 0.003 0.12 6.26
CN25-DDH002 994625 22 24 2 0.011 0.15 5.55
CN25-DDH002 994626 24 26 2 0.005 0.09 6.60
CN25-DDH002 994627 26 26.77 0.77 0.045 0.87 5.29
CN25-DDH002 994628 26.77 28 1.23 0.089 2.11 80.70
CN25-DDH002 994630 28 28.75 0.75 Hydrothermal Breccia 0.359 5.00 357.00
CN25-DDH002 994631 28.75 30 1.25 Dyke 0.026 0.89 86.10
CN25-DDH002 994632 30 32 2 0.011 0.80 82.50
CN25-DDH002 994633 32 34 2 0.012 0.25 6.77
CN25-DDH002 994634 34 36 2 0.009 0.14 2.54
CN25-DDH002 994635 36 38 2 0.007 0.26 35.90
CN25-DDH002 994636 38 38.9 0.9 0.003 0.19 3.74
CN25-DDH002 994638 38.9 40 1.1 Lens 2 1.870 107.00 500.00
CN25-DDH002 994639 40 41 1 1.725 126.00 333.00
CN25-DDH002 994640 41 42 1 2.130 160.00 1465.00
CN25-DDH002 994641 42 43.1 1.1 1.220 116.00 1010.00
CN25-DDH002 994643 43.1 45 1.9 Red Breccia 0.004 0.29 25.50
CN25-DDH002 994644 55 57 2 0.002 0.17 20.70
CN25-DDH003 994645 0 1 1 0.016 0.33 6.22
CN25-DDH003 994646 1 2 1 0.015 0.09 5.56
CN25-DDH003 994647 2 3 1 Black Breccia 0.014 0.84 7.63
CN25-DDH003 994648 3 4 1 0.005 0.48 2.17
CN25-DDH003 994649 4 5 1 0.007 0.72 1.71
CN25-DDH003 994650 5 6 1 0.006 0.48 1.63
CN25-DDH003 994651 6 7.5 1.5 0.011 0.61 3.48
CN25-DDH003 994652 7.5 9 1.5 Red Breccia 0.001 0.03 1.51
CN25-DDH003 994653 9 11 2 0.001 0.01 1.51
CN25-DDH003 994654 11 13 2 0.001 0.03 1.96
CN25-DDH003 994655 13 15 2 0.001 0.01 2.26
CN25-DDH003 994656 15 17 2 0.003 0.12 3.07
CN25-DDH003 994657 17 19 2 0.002 0.03 3.78
CN25-DDH003 994658 19 21 2 0.003 0.02 6.01
CN25-DDH003 994659 21 23 2 0.003 0.04 5.43
CN25-DDH003 994660 23 25 2 0.002 0.01 4.79
CN25-DDH003 994661 25 27 2 0.002 0.02 5.59
CN25-DDH003 994662 27 29 2 0.008 0.15 7.27
CN25-DDH003 994663 29 31 2 0.031 0.71 8.74
CN25-DDH003 994666 31 32.27 1.27 0.064 8.04 56.90
CN25-DDH003 994667 32.27 33.27 1 0.044 1.82 32.00
CN25-DDH003 994668 33.27 35 1.73 Dyke 0.011 0.16 13.25
CN25-DDH003 994669 35 36.6 1.6 0.013 0.30 86.40
CN25-DDH003 994670 36.6 37.1 0.5 Lens 2 0.182 13.20 20.60
CN25-DDH003 994671 37.1 38 0.9 1.055 79.90 178.50
CN25-DDH003 994672 38 39 1 0.153 12.70 25.90
CN25-DDH003 994673 39 40 1 1.020 101.00 161.50
CN25-DDH003 994676 40 41 1 2.510 230.00 299.00
CN25-DDH003 994677 41 42 1 2.350 218.00 320.00
CN25-DDH003 994678 42 43 1 2.590 254.00 325.00
CN25-DDH003 994679 43 44 1 2.430 169.00 830.00
CN25-DDH003 994680 44 45 1 3.220 213.00 1510.00
CN25-DDH003 994681 45 46 1 2.440 170.00 1730.00
CN25-DDH003 994682 46 47 1 2.360 184.00 1635.00
CN25-DDH003 994683 47 48 1 1.400 95.20 793.00
CN25-DDH003 994684 48 49 1 2.390 122.00 1595.00
CN25-DDH003 994685 49 50 1 2.890 236.00 1080.00
CN25-DDH003 994686 50 51 1 4.640 406.00 2150.00
CN25-DDH003 994687 51 52 1 1.975 177.00 1205.00
CN25-DDH003 994688 52 53 1 0.666 34.90 133.50
CN25-DDH003 994689 53 54 1 0.152 13.80 295.00
CN25-DDH003 994690 54 55.2 1.2 0.115 9.40 491.00
CN25-DDH003 994692 55.2 57 1.8 Dyke 0.008 0.39 6.04
CN25-DDH003 994693 57 59 2 0.007 0.37 19.75
CN25-DDH003 994694 59 60 1 Red Breccia 0.017 0.88 38.40
CN25-DDH003 994695 60 61 1 0.002 0.12 24.80
CN25-DDH003 994696 71 73 2 0.001 0.12 6.06
CN25-DDH003 994697 81 83 2 0.002 0.07 10.20
CN25-DDH003 994698 91 93 2 0.002 0.09 7.36
CN25-DDH004 994699 0 1 1 Saprock 0.005 0.24 3.60
CN25-DDH004 994700 1 2 1 0.008 0.05 1.50
CN25-DDH004 994701 2 3 1 Red Breccia 0.007 0.41 3.31
CN25-DDH004 994702 3 4 1 0.005 0.69 1.68
CN25-DDH004 994703 4 5 1 0.006 0.23 1.53
CN25-DDH004 994704 5 6 1 0.064 0.15 5.67
CN25-DDH004 994705 6 7 1 0.020 0.25 5.16
CN25-DDH004 994706 7 9 2 0.010 0.06 2.14
CN25-DDH004 994707 9 11 2 0.001 0.02 1.48
CN25-DDH004 994708 11 13 2 0.001 0.01 1.53
CN25-DDH004 994709 13 15 2 0.001 0.02 1.79
CN25-DDH004 994710 15 17 2 0.002 0.03 2.67
CN25-DDH004 994711 17 19 2 0.003 0.02 2.11
CN25-DDH004 994712 19 21 2 0.003 0.01 3.23
CN25-DDH004 994713 21 23 2 0.002 0.02 4.16
CN25-DDH004 994714 23 25 2 0.001 0.01 3.75
CN25-DDH004 994715 25 26.7 1.7 0.004 0.03 4.95
CN25-DDH004 994718 26.7 27.7 1 0.043 0.25 4.53
CN25-DDH004 994719 27.7 28.7 1 0.077 0.62 3.15
CN25-DDH004 994720 28.7 29.8 1.1 0.031 3.21 8.66
CN25-DDH004 994721 29.8 30.8 1 0.010 0.12 3.40
CN25-DDH004 994722 30.8 31.7 0.9 0.026 0.79 3.65
CN25-DDH004 994723 31.7 33 1.3 0.008 0.22 4.55
CN25-DDH004 994724 33 34 1 0.001 0.01 4.29
CN25-DDH004 994725 34 36 2 0.002 0.05 6.23
CN25-DDH004 994726 36 37.4 1.4 0.062 1.38 8.11
CN25-DDH004 994727 37.4 38.4 1 0.041 2.04 26.00
CN25-DDH004 994728 38.4 39.4 1 0.010 0.16 4.69
CN25-DDH004 994729 39.4 40.4 1 Proto-Lens 2 0.008 0.33 7.51
CN25-DDH004 994732 40.4 41.5 1.1 0.042 1.22 31.80
CN25-DDH004 994733 41.5 42.2 0.7 Red Breccia 0.034 1.42 11.15
CN25-DDH004 994734 42.2 44 1.8 Fine Dyke 0.009 0.27 8.54
CN25-DDH004 994735 48 49 1 Red Breccia 0.021 0.88 23.50
CN25-DDH004 994736 59 61 2 0.008 0.46 5.02
CN25-DDH004 994737 69 71 2 0.006 0.13 7.30
CN25-DDH004 994738 79 81 2 0.002 0.02 4.23
CN25-DDH004 994739 83 84 1 0.001 0.07 1.41
CN25-DDH004 994741 89 91 2 0.002 0.02 4.94
CN25-DDH004 994742 99 101 2 0.001 0.02 4.22
CN25-DDH005 994743 0 1 1 Saprock 0.004 0.12 3.09
CN25-DDH005 994744 1 2 1 0.031 0.23 1.35
CN25-DDH005 994745 2 3 1 Black Breccia 0.011 0.09 5.50
CN25-DDH005 994746 3 4 1 0.006 0.41 3.43
CN25-DDH005 994747 4 5 1 0.005 0.46 1.53
CN25-DDH005 994748 5 6 1 0.004 0.40 1.92
CN25-DDH005 994749 6 7.2 1.2 0.020 0.44 12.00
CN25-DDH005 994750 7.2 9 1.8 0.037 0.30 4.21
CN25-DDH005 994751 9 11 2 Red Breccia 0.001 0.02 1.64
CN25-DDH005 994752 11 13 2 0.001 0.02 1.66
CN25-DDH005 994753 13 15 2 0.001 0.02 2.01
CN25-DDH005 994754 15 17 2 0.002 0.03 2.73
CN25-DDH005 994755 17 19 2 0.002 0.03 3.90
CN25-DDH005 994756 19 21 2 0.002 0.03 5.25
CN25-DDH005 994757 21 23 2 0.003 0.04 5.13
CN25-DDH005 994758 23 25 2 0.002 0.02 4.98
CN25-DDH005 992609 25 26.6 1.6 0.003 0.06 5.17
CN25-DDH005 992612 26.6 27.6 1 0.002 0.02 5.08
CN25-DDH005 992613 27.6 28.6 1 0.021 0.61 6.92
CN25-DDH005 992614 28.6 29.7 1.1 Proto-Lens 2 0.066 4.56 30.70
CN25-DDH005 992615 29.7 32 2.3 Dyke 0.009 0.21 16.45
CN25-DDH005 992616 32 32.9 0.9 0.012 0.24 61.40
CN25-DDH005 992617 32.9 34 1.1 Hydrothermal Breccia 0.209 7.01 21.70
CN25-DDH005 992618 34 35 1 0.004 0.29 12.60
CN25-DDH005 992619 35 36 1 Lens 2 0.399 26.90 218.00
CN25-DDH005 992620 36 37 1 0.707 63.30 325.00
CN25-DDH005 992621 37 38 1 2.170 180.00 1505.00
CN25-DDH005 992622 38 39 1 2.330 195.00 1225.00
CN25-DDH005 992623 39 40 1 1.455 117.00 709.00
CN25-DDH005 992624 40 41 1 3.280 293.00 2310.00
CN25-DDH005 992625 41 42 1 1.550 137.00 863.00
CN25-DDH005 992626 42 43 1 2.590 252.00 930.00
CN25-DDH005 992627 43 44 1 3.700 275.00 1080.00
CN25-DDH005 992630 44 45 1 4.200 330.00 999.00
CN25-DDH005 992631 45 46 1 5.910 567.00 538.00
CN25-DDH005 992632 46 47 1 6.180 528.00 752.00
CN25-DDH005 992633 47 48 1 5.480 473.00 1580.00
CN25-DDH005 992634 48 49 1 3.570 309.00 1095.00
CN25-DDH005 992635 49 50 1 5.130 455.00 1155.00
CN25-DDH005 992636 50 51 1 4.150 383.00 1805.00
CN25-DDH005 992637 51 52 1 5.140 432.00 2240.00
CN25-DDH005 992638 52 53 1 0.636 37.60 354.00
CN25-DDH005 992639 53 54 1 0.485 26.40 322.00
CN25-DDH005 992640 54 55 1 0.155 7.88 46.80
CN25-DDH005 992641 55 56 1 1.360 92.90 488.00
CN25-DDH005 992642 56 56.5 0.5 Red Breccia 0.017 1.28 27.10
CN25-DDH005 992643 56.5 57.5 1 0.014 0.52 24.70
CN25-DDH005 992644 57.5 58.5 1 0.008 0.22 20.90
CN25-DDH005 992646 68 70 2 Dyke 0.013 0.47 4.17
CN25-DDH005 992647 78 80 2 Red Breccia 0.002 0.07 22.10
CN25-DDH005 992648 88 90 2 0.002 0.25 20.40
CN25-DDH005 992649 98 100 2 Dyke 0.002 0.03 9.12
Table 2: Cerro Negro Project, Mostaza Mine; Mostaza drill core assay results
for Cu, Ag and Sb.
Cautionary note:
The Company cautions that all references to "resources", "mineral resources",
or "mineral resource estimates" in this RNS are historical and were prepared
and reported prior to the implementation of the JORC code and therefore are
non-JORC compliant. The Company advises that the resource categories used in
the historical estimates, for example "measured, indicated, demonstrated and
inferred", may not have the same meaning or degree of confidence as current
JORC categories. Historical records indicate that the quoted non-JORC
resources were calculated using the polygonal method based on underground
sampling, 1024m of drilling in 25 holes, and geological cross-sections and
level plans. GSC is presenting this information for historical context only
and is not treating it as a current mineral resource estimate. The Company has
not been able to independently verify the results of historical drilling or
mine channel samples. References to mineralised grade intervals in drill holes
are considered apparent thicknesses as there is not sufficient geological
information to calculate true thickness of mineralised intercepts at this
time.
References:
1. RNS 5182Y (26 February 2025): Cerro Negro assays return 20m of3.3%
Cu & 270g_t Ag
2. RNS 2017A (11 March 2025): Phase II Resource Drilling Commences at
the Mostaza Cu-Ag Deposit
Enquiries:
Great Southern Copper plc
Sam Garrett, Chief Executive Officer +44 (0) 20 4582 3500
SI Capital Limited
Nick Emerson +44 (0) 1483 413500
Gracechurch Group
Harry Chathli, Alexis Gore, Henry Gamble +44 (0) 20 4582 3500
Notes for Editors:
About Great Southern Copper
Great Southern Copper PLC is a UK-listed mineral exploration company focused
on the discovery of copper-gold-silver deposits in Chile. The Company has the
option to acquire rights to 100% of two projects in the under-explored coastal
belt of Chile that are prospective for large scale copper-gold deposits. Chile
is a globally significant mining jurisdiction being the world's largest copper
producer and the second-largest producer of lithium.
The two early-stage Cu-Au projects comprise the Especularita and San Lorenzo
Projects, both located in the coastal metallogenic belt of Chile which hosts
significant copper mines and deposits, including Teck's Carmen de Andacollo
copper mine, and boasts excellent access to infrastructure such as roads,
power and ports. Significant historical small-scale and artisanal workings for
both copper and gold are readily evident in both exploration project areas.
Great Southern Copper is strategically positioned to support the global market
for copper - a critical battery metal in the clean energy transition around
the world. The Company is actively engaged in exploration and evaluation work
programmes targeting both large tonnage, low to medium grade Cu-Au deposits as
well as high-grade Cu-Au deposits.
Further information on the Company is available on the Company's website:
https://gscplc.com (https://gscplc.com)
Competent Person Statement
The information in this announcement that relates to exploration results is
based on and fairly represents information reviewed or compiled by Mr Sam
Garrett, a Competent Person who is a Member of the Australian Institute of
Geoscientists and a Fellow of the Society of Economic Geologists. Mr Garrett
is the CEO and a shareholder of Great Southern Copper PLC. Mr Garrett has
sufficient experience that is relevant to the styles of mineralisation and
types of deposit under consideration and to the activity being undertaken to
qualify as a Competent Person as defined in the 2012 Edition of the
"Australasian Code for Reporting of Exploration Results, Mineral Resources and
Ore Reserves". Mr Garrett has provided his prior written consent to the
inclusion in this announcement of the matters based on information in the form
and context in which it appears.
This announcement includes information that relates to Exploration Results
prepared and first disclosed under the JORC Code (2012) and extracted from the
Company's previous LSE announcements as noted, and the Company's Prospectus
dated 20 December 2021. Copies of these announcements are available from the
LSE Announcements page of the Company's website: www.gscplc.com.
The Company confirms that it is not aware of any new information or data that
materially affects the information included within the Prospectus dated 20
December 2021.
Forward Looking and Cautionary Statements
Some statements in this announcement regarding estimates or future events are
forward-looking statements. They include indications of, and guidance on,
future earnings, cash flow, costs and financial performance. Forward-looking
statements include, but are not limited to, statements preceded by words such
as "planned", "expected", "projected", "estimated", "may", "scheduled",
"intends", "anticipates", "believes", "potential", "predict", "foresee",
"proposed", "aim", "target", "opportunity", "could", "nominal", "conceptual"
and similar expressions. Forward-looking statements, opinions and estimates
included in this report are based on assumptions and contingencies which are
subject to change without notice, as are statements about market and industry
trends, which are based on interpretations of current market conditions.
Forward-looking statements are provided as a general guide only and should not
be relied on as a guarantee of future performance. Forward-looking statements
may be affected by a range of variables that could cause actual results to
differ from estimated or anticipated results and may cause the Company's
actual performance and financial results in future periods to materially
differ from any projections of future performance or results expressed or
implied by such forward-looking statements. So, there can be no assurance that
actual outcomes will not materially differ from these forward-looking
statements.
This information is provided by RNS, the news service of the London Stock Exchange. RNS is approved by the Financial Conduct Authority to act as a Primary Information Provider in the United Kingdom. Terms and conditions relating to the use and distribution of this information may apply. For further information, please contact
rns@lseg.com (mailto:rns@lseg.com)
or visit
www.rns.com (http://www.rns.com/)
.
RNS may use your IP address to confirm compliance with the terms and conditions, to analyse how you engage with the information contained in this communication, and to share such analysis on an anonymised basis with others as part of our commercial services. For further information about how RNS and the London Stock Exchange use the personal data you provide us, please see our
Privacy Policy (https://www.lseg.com/privacy-and-cookie-policy)
. END MSCJRMFTMTBBMRA