Great Southrn.Copper - Further "exceptional" assay results from Mostaza

Great Southern Copper

07/04/2025 07:00

RNS Number : 8896D

Great Southern Copper PLC

07 April 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.

 

07 April 2025

 

Great Southern Copper plc

("GSC" or the "Company")

 

Hole DD007 Intersects High-Grade Copper and Silver with Grades up to 16.15% Cu and 646 g/t Ag

 

Exploration holes confirm extension of high-grade  system south of Mostaza, Cerro Negro

 

 

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 diamond drill hole CNG25 DD007 with significant intervals including;

Ø 33m of 1.96% Cu and 60.6 g/t Ag from 87m, including

§ 3.85m of 5.21% Cu and 318.2 g/t Ag from 88m, and

§ 5.0m of 5.90% Cu and 99.2 g/t Ag, from 115m, including

·    2.5m of 9.67% Cu and 175.4 g/t Ag from 116.4m

 

·    New results include highest reported assay grades of 16.15% Cu and 646 g/t Ag with four samples reporting copper assay grades over 8.0% Cu

·    DD007 located 270m to the south of CNG25 DD001 which intersected;

Ø 20m of 3.31% Cu and 269.9g/t Ag from 27m1

·    Mineralisation remains open in all directions including at depth

·    Phase II resource and exploration diamond drilling in progress with a further 10 holes completed for 1,059m

·    GSC holds an option to own 100% of the Cerro Negro project which includes the Mostaza mine

·    Prospect located at low elevation with excellent access to infrastructure and mining services

·    Recent funding round and the ongoing exercising of warrants provide a strong balance sheet for continuing exploration at Mostaza and the greater licence areas

 

Sam Garrett, Chief Executive Officer of Great Southern Copper, said: "The results for hole DD007 confirm that high-grade copper-silver mineralisation is continuing along trend south of the Mostaza mine which greatly enhances the potential value of this significant copper-silver deposit. The 16.15% copper result is the highest assay result received to date for the project.

 

"Phase II diamond drilling is well under-way with two rigs now in the Mostaza pit testing the depth extensions of the high-grade mineralisation identified in Phase I. To date all Phase II holes have intersected the mineralised lens to a vertical depth of 100m below the original hole 1 intercept.

 

"Excitement is building at Cerro Negro, but we have a lot of work ahead of us as we seek to demonstrate the size and economic value of this exciting high-grade deposit."

 

Results of diamond drillholes CNG25 DD006 - DD009

 

Diamond drillholes CNG25 DD006 - DD009 were designed to test extensions of the Mostaza Lens 2 mineralisation along trend to the south where discontinuous outcrops of silicified structurally-controlled mineralisation are mapped as Lenses 3 - 5 (Figure 1). Small-scale artisanal mining of these southern lenses is evident, however, no historical details of tonnages or grades have been previously reported.

 

All drill holes intersected zones of variably mineralised, structurally-controlled silicification over varying widths and significant assays are summarised in Table 1. Holes DD006, 008 and 009 all intersected shallow oxidised zones of lens with anomalous silver (>0.1 g/t Ag) associated with the oxidised silicious breccias indicating surface leaching of sulphides. Geological interpretation of the results are on-going.

 

Drillhole CNG25 DD006 was drilled to test below and along strike to the north of Lens 4. It intercepted several oxidised and reduced grade silicified mineralised zones of "proto-lens" with anomalous Cu and Ag up to 0.16% and 24.9 g/t respectively. (Figure 2)

 

Drillhole CNG25 DD007 was drilled below Lens 3 and intersected 33m of mineralised "lens" rock grading 1.96% Cu and 60.56 g/t Ag over the total intercept from 87m down-hole. The mineralised lens includes two distinct zones of high-grade Cu-Ag mineralisation including 3.9m at 5.21% Cu and 318.21 g/t Ag from 88m and 5.0m of 5.90% Cu and 99.2g/t Ag from 115m. The lower zone of high-grade Cu-Ag includes 2.5m at 9.67% Cu and 175.44 g/t Ag from 116m depth (see Figure 2). This interval includes the highest reported assay grades to date of 16.15% Cu and 646 g/t Ag with 4 samples reporting grades over 8.0% Cu. The mineralised Lens comprises silica-altered breccia clasts within a sulphide-rich matrix containing abundant chalcopyrite, bornite and pyrite (See Figure 3). The highest grades correlate with zones of semi-massive bornite-chalcopyrite mineralisation.

 

Drillhole CNG25 DD008 was drilled above and 20m to the north of DD007 to intersect the Lens 3 at a shallower depth. The hole intercepted a 21.4m zone of oxidised silicified breccia from surface with strong oxidised sulphides and anomalous Cu and Ag up to 0.51% Cu and 31.3 g/t Ag respectively. These results suggest that near-surface leaching has resulted in lower grades (Figure 3). 

 

Drillhole CNG25 DD009 was drilled 100m to the south of the Mostaza Mine to test the southern extension of Lens 2 and intersected several zones of weakly altered and mineralised "proto-lens", suggesting the Lens has been structurally displaced in this location.

 

A summary of all Phase I significant 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
3.31
269.9
934
inc
31
38
7
5.72
489.6
1085
inc
35
38
3
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
2.48
198.1
1049
inc
48
51
3
3.31
254.7
1608
inc
50
51
1
4.64
406
2150
CNG25 DD004
no significant intercepts
CNG25 DD005
35
56
21
2.9
246.7
978
inc
37
52
15
3.79
328.4
1252
inc
40
52
12
4.24
369.5
1279
inc
45
52
7
5.08
449.6
1309
inc
45
47
2
6.05
547.5
645
CNG25 DD006
132.54
132.91
0.46
0.08
24.9
5.48
CNG25 DD007
87
120
33
1.96
60.6
inc
88
91.85
3.85
5.21
318
and
115
120
5
5.59
99.2
inc
116.4
118.9
2.5
9.67
175.4
CNG25 DD008
0
1.2
1.2
0.512
31.3
28
0
31
31
7.1
inc
8
22
14
9.6
CNG25 DD009
no significant intercept


 

Table 1: Summary of significant intercepts for Phase I GSC drill holes DD001 - DD009.

 

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. Copper-silver 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

 

Host rocks to mineralisation comprise multiple generations of intensely altered breccia, tuffisite, and felsic intrusive. The mineralised lens 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 brecciated dacite that might be part of a large dome-diatreme complex outcropping to the east.

 

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.

 

 

 

 

Figure 1: Cerro Negro Project, Mostaza Mine: Simplified schematic plan map showing the location of GSC drillholes with respect to known mineralised lenses and historical drillholes. Holes reported in this press release are highlighted in yellow.

 

 

 

Figure 2: Cerro Negro Project: Schematic cross section through drillholes CNG25 DD006 and DD007 showing Cu-Ag intercepts and the preliminary geological interpretation and relationship to

historical drillholes. Note the extrapolations to the historical drillholes 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 DD007 on the left and CNG25 DD008 on the right, with grades of Cu % and Ag g/t. The black, brown and bronze minerals filling the cracks and veins in hole DD007 are Cu-Ag bearing sulphides and sulfosalt minerals cutting intensely silicified rock. The core from hole DD008 is texturally similar but has been subject to near-surface oxidation and leaching leaving only Fe-oxides and clays with low grades of Cu and Ag.

 

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 Molybdenum (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  are 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 commenced on 11 March 2025 employing two rigs and is designed to include resource and exploration drilling. To date a further 10 holes have been drilled for the Phase II programme for a total of 1,059 metres. Within the Mostaza pit the Phase II drilling continues to intersect the high-grade Lens 2 mineralisation down to 100m below the DD001 intercept with mineralisation remaining open in all directions.

 

Metallurgical studies of drill core, stockpiles and tailings are also in planning stage. Extensions of mineralisation at depth and along trend under cover may also be targeted with geophysical surveys.

 

HOLE
SAMPLE ID
FROM (m)
TO
(m)
LONG (m)
LITHOLOGY
Cu %
Ag g/t
Sb ppm
CN25-DDH006
937159
0
2
2
Black Breccia
0.003
0.03
6.33
CN25-DDH006
937160
2
4
2
0.004
0.04
7.47
CN25-DDH006
937161
4
6.2
2.2
0.006
0.11
10.85
CN25-DDH006
937162
6.2
7
0.8
0.024
0.45
2.61
CN25-DDH006
937163
7
8
1
0.007
0.1
3.82
CN25-DDH006
937164
8
10
2
0.011
0.16
3.21
CN25-DDH006
937165
10
12
2
0.012
0.13
3.43
CN25-DDH006
937166
12
14
2
Coarse Feldspar Porphyry
0.009
0.09
3.66
CN25-DDH006
937167
14
16
2
0.013
0.21
4.68
CN25-DDH006
937168
16
18
2
0.014
0.49
5.62
CN25-DDH006
937170
18
20
2
0.015
0.2
5.12
CN25-DDH006
937171
20
22
2
0.010
0.1
5.21
CN25-DDH006
937172
22
24
2
0.012
0.09
3.86
CN25-DDH006
937173
24
26
2
0.010
0.08
5.17
CN25-DDH006
937174
26
28
2
0.012
0.07
4.39
CN25-DDH006
937175
28
30
2
0.014
0.07
4.34
CN25-DDH006
937176
30
32
2
0.013
0.04
4.98
CN25-DDH006
937177
32
34
2
0.026
0.06
4.98
CN25-DDH006
937179
34
35.3
1.3
0.041
0.09
4.7
CN25-DDH006
937180
35.3
36.3
1
0.027
0.04
5.51
CN25-DDH006
937181
36.3
37.3
1
0.068
0.08
47.3
CN25-DDH006
937182
37.3
38.3
1
Proto-Lens 4
0.159
0.16
108
CN25-DDH006
937183
38.3
39
0.7
0.057
0.1
48
CN25-DDH006
937185
39
40
1
0.038
0.18
24
CN25-DDH006
937186
40
41.1
1.1
0.024
0.11
8.89
CN25-DDH006
937187
41.1
42.1
1
Black Breccia
0.010
0.15
8.36
CN25-DDH006
937188
42.1
43.1
1
0.046
1.18
35.4
CN25-DDH006
937189
43.1
44
0.9
0.002
0.03
1.82
CN25-DDH006
937190
44
45
1
0.002
0.03
2.11
CN25-DDH006
937192
45
46
1
0.001
0.02
2.62
CN25-DDH006
937193
46
47
1
0.002
0.06
3.02
CN25-DDH006
937194
47
48
1
0.002
0.07
3.23
CN25-DDH006
937195
48
49
1
0.002
0.13
2.31
CN25-DDH006
937196
49
50
1
Proto-Lens in breccia
0.002
0.1
2.21
CN25-DDH006
937197
50
51
1
0.002
0.05
2.18
CN25-DDH006
937198
51
52
1
0.004
0.08
2.42
CN25-DDH006
937199
52
53
1
0.001
0.03
2.21
CN25-DDH006
937200
53
54
1
0.003
0.05
2.26
CN25-DDH006
937202
54
55
1
Black Breccia
0.007
0.17
2.54
CN25-DDH006
937203
55
56
1
0.001
0.03
3.6
CN25-DDH006
937204
56
57
1
0.001
0.03
5.29
CN25-DDH006
937205
57
58
1
0.001
0.04
7.06
CN25-DDH006
937206
58
59
1
0.001
0.02
5.54
CN25-DDH006
937207
59
60
1
0.001
0.02
7.05
CN25-DDH006
937208
60
61
1
0.000
0.02
4.72
CN25-DDH006
937209
61
62
1
0.001
0.02
9.63
CN25-DDH006
937210
62
63
1
0.001
0.02
10.65
CN25-DDH006
937212
63
64
1
0.000
0.02
4.46
CN25-DDH006
937213
64
65
1
0.001
0.01
6.06
CN25-DDH006
937214
65
66
1
0.001
0.04
6.75
CN25-DDH006
937215
66
67
1
0.012
1.1
6.73
CN25-DDH006
937216
67
68
1
0.005
0.25
5.82
CN25-DDH006
937217
68
69
1
0.000
0.01
6.22
CN25-DDH006
937218
69
69.6
0.6
0.001
0.05
5.62
CN25-DDH006
937219
78
80
2
Pink Breccia
0.001
0.08
16.6
CN25-DDH006
937220
88
90
2
0.001
0.01
12.1
CN25-DDH006
937221
98
100
2
0.002
0.01
15.8
CN25-DDH006
937222
108
110
2
Black Breccia
0.001
0.01
10.1
CN25-DDH006
937223
118
120
2
0.001
0.01
3.12
CN25-DDH006
937225
128
130
2
0.000
0.05
5.01
CN25-DDH006
937226
138
140
2
0.000
0.01
2.49
CN25-DDH006
937227
148
150
2
0.000
0.01
1.34
CN25-DDH006
937228
158
160
2
0.000
0.02
1.59
CN25-DDH006
937229
168
170
2
Dacite Dome
0.000
0.01
5.02
CN25-DDH006
937230
178
180
2
0.000
<0.01
6.3
CN25-DDH006
937231
188
190
2
Altered Dacite Dome
0.000
0.01
6.65
CN25-DDH006
937232
198
200
2
0.000
0.01
5.89
CN25-DDH006
937233
208
210
2
0.000
<0.01
5.96
CN25-DDH006
937234
218
220.3
2.3
0.000
0.02
4.13
CN25-DDH006
937235
132.54
132.91
0.37
Proto-Lens
0.080
24.9
5.48
HOLE
SAMPLE ID
FROM (m)
TO
(m)
LONG (m)
LITHOLOGY
Cu %
Ag g/t
Sb ppm
CN25-DDH007
937236
0
2
2
Black Breccia
0.031
0.23
13.85
CN25-DDH007
937237
2
4
2
0.082
0.07
9.51
CN25-DDH007
937238
4
6
2
0.122
0.14
7.79
CN25-DDH007
937239
8
10
2
0.046
0.07
16.3
CN25-DDH007
937240
21
23
2
0.141
8.42
15.8
CN25-DDH007
937241
32
34
2
0.008
0.48
15.45
CN25-DDH007
937242
36
38
2
Dacite Dyke
0.008
0.2
3.06
CN25-DDH007
937243
56
58
2
0.006
0.15
2.13
CN25-DDH007
937244
68.4
70
1.6
Proto-Lens
0.004
0.16
5.38
CN25-DDH007
937245
82
84
2
Dacite Dyke
0.019
0.41
2.51
CN25-DDH007
937247
85
86
1
0.027
0.65
3.37
CN25-DDH007
937248
86
87
1
Black Breccia
0.153
4.7
27.4
CN25-DDH007
937249
87
88
1
Lens Halo
0.709
37.4
9.62
CN25-DDH007
937250
88
89.2
1.2
8.890
410
6.03
CN25-DDH007
937251
89.2
90.4
1.2
0.259
13.8
26.5
CN25-DDH007
937252
90.4
91
0.6
Lens
8.310
646
8.14
CN25-DDH007
937253
91
91.85
0.85
4.830
387
226
CN25-DDH007
937255
91.85
93
1.15
0.401
14.9
85.1
CN25-DDH007
937256
93
94
1
0.260
5.92
9.39
CN25-DDH007
937257
94
95
1
0.243
4.11
9.4
CN25-DDH007
937258
95
96
1
0.236
3.31
10.1
CN25-DDH007
992659
96
97
1
0.559
4.84
13.65
CN25-DDH007
992660
97
98
1
0.579
5.71
37.8
CN25-DDH007
992661
98
99
1
0.359
6.72
139
CN25-DDH007
992662
99
100
1
0.537
9.41
18.05
CN25-DDH007
992663
100
101.2
1.2
0.236
5.47
10.3
CN25-DDH007
992664
101.2
102
0.8
0.027
1.15
5.67
CN25-DDH007
992666
102
103
1
1.425
23.8
7.82
CN25-DDH007
992667
103
104.9
1.9
0.932
24.7
6.91
CN25-DDH007
992668
104.9
105
0.1
0.222
9.1
7.92
CN25-DDH007
992669
105
106.6
1.6
0.248
5
8.59
CN25-DDH007
992670
106.6
107
0.4
2.210
33.2
12
CN25-DDH007
992671
107
108.1
1.1
1.960
27
10.25
CN25-DDH007
992672
108.1
109
0.9
0.444
3.15
15.7
CN25-DDH007
992673
109
110
1
0.687
5.35
16.15
CN25-DDH007
992674
110
111
1
0.581
5.35
17.6
CN25-DDH007
992675
111
112
1
0.807
6.1
134
CN25-DDH007
992676
112
113
1
1.720
15.1
1445
CN25-DDH007
992677
113
114.1
1.1
0.789
5.94
86.7
CN25-DDH007
992679
114.1
115
0.9
0.741
12.6
9.49
CN25-DDH007
992680
115
116.4
1.4
1.825
22.2
533
CN25-DDH007
992681
116.4
117
0.6
16.150
287
203
CN25-DDH007
992682
117
118
1
9.690
179
13.15
CN25-DDH007
992683
118
118.9
0.9
5.340
97.1
13.35
CN25-DDH007
992684
118.9
119.3
0.4
1.195
23.4
77
CN25-DDH007
992685
119.3
120
0.7
1.010
24.3
350
CN25-DDH007
992687
120
121
1
Coarse Feldspar Porphyry
0.055
4.14
43.2
CN25-DDH007
992688
131
133
2
Black Breccia
0.008
0.18
4.03
CN25-DDH007
992689
139
139.6
0.6
0.019
1.34
4.38
HOLE
SAMPLE ID
FROM (m)
TO
(m)
LONG (m)
LITHOLOGY
Cu %
Ag g/t
Sb ppm
CN25-DDH008
992690
0
1.2
1.2
Black Breccia
0.512
31.3
28
CN25-DDH008
992691
1.2
2.2
1
0.162
3.74
4.12
CN25-DDH008
992692
2.2
3.2
1
0.157
4.34
5.89
CN25-DDH008
992694
3.2
4.2
1
0.096
2.85
21.9
CN25-DDH008
992695
4.2
5
0.8
Lens 3
0.063
3.45
47.3
CN25-DDH008
992696
5
6
1
0.012
7.23
14.5
CN25-DDH008
992697
6
7
1
0.009
3.57
11.9
CN25-DDH008
992698
7
8
1
0.010
5.12
11.85
CN25-DDH008
992699
8
9
1
0.026
8.13
13.8
CN25-DDH008
992701
9
10
1
0.010
4.48
11.8
CN25-DDH008
992702
10
11
1
0.014
5.81
11.55
CN25-DDH008
992703
11
12
1
0.020
10.15
13.8
CN25-DDH008
992704
12
13
1
0.019
15.35
11.45
CN25-DDH008
992705
13
14
1
0.010
7.1
15.7
CN25-DDH008
992706
14
15
1
0.026
12.35
15.45
CN25-DDH008
992707
15
16
1
0.006
6.08
19.15
CN25-DDH008
992708
16
17
1
0.007
13.25
21.5
CN25-DDH008
992709
17
18
1
0.005
9.97
10.4
CN25-DDH008
992710
18
19
1
0.039
15.5
12.7
CN25-DDH008
992712
19
20
1
0.008
9.4
8.64
CN25-DDH008
992713
20
21
1
0.007
8.48
16.5
CN25-DDH008
992714
21
22
1
0.008
8.67
20.1
CN25-DDH008
992715
22
23
1
0.004
2.62
8.67
CN25-DDH008
992716
23
24
1
0.004
2.62
7.56
CN25-DDH008
992717
24
25.6
1.6
0.022
3.62
7.42
CN25-DDH008
992718
25.6
27
1.4
Lens Halo
0.035
2.12
6.54
CN25-DDH008
992719
27
28
1
0.052
1.14
6.77
CN25-DDH008
992720
28
29
1
0.051
0.95
3.72
CN25-DDH008
992721
29
30
1
0.091
1.1
2.95
CN25-DDH008
992723
30
31
1
0.097
1.1
5.79
CN25-DDH008
992724
31
31.6
0.6
0.193
0.72
5.25
CN25-DDH008
992725
39
40.6
1.6
Black Breccia
0.002
0.1
3.14
HOLE
SAMPLE ID
FROM (m)
TO (m)
LONG (m)
LITHOLOGY
Cu %
Ag g/t
Sb ppm
CN25-DDH009
992726
0
2
2
Black Breccia
0.083
4.15
27.5
CN25-DDH009
992727
2
4
2
0.064
2.11
12.7
CN25-DDH009
992728
4
6
2
0.072
2.07
15.35
CN25-DDH009
992729
6
8
2
0.039
0.78
12.95
CN25-DDH009
992730
8
10
2
0.025
0.82
18.6
CN25-DDH009
992731
10
11.6
1.6
0.022
0.47
8.26
CN25-DDH009
992732
11.6
14
2.4
Proto-Lens?
0.006
0.33
7.09
CN25-DDH009
992733
14
16
2
0.020
1.42
13.05
CN25-DDH009
992734
16
18
2
0.010
2.48
7.5
CN25-DDH009
992735
18
19.2
1.2
0.016
1.38
12.95
CN25-DDH009
992736
19.2
21
1.8
Black Breccia
0.033
0.88
10.45
CN25-DDH009
992738
21
23.4
2.4
0.011
0.54
6.41
CN25-DDH009
992739
23.4
24
0.6
0.004
0.18
5.25
CN25-DDH009
992740
24
26
2
0.007
0.22
8.31
CN25-DDH009
992741
26
28
2
0.001
0.1
4.77
CN25-DDH009
992742
28
30
2
0.001
0.13
4.84
CN25-DDH009
992743
30
32
2
0.002
0.44
5.96
CN25-DDH009
992744
32
34
2
0.002
0.11
7
CN25-DDH009
992745
34
36
2
0.002
0.15
7.2
CN25-DDH009
992746
36
38
2
0.002
0.84
5.9
CN25-DDH009
992747
38
39.1
1.1
0.002
0.08
6.54
CN25-DDH009
992748
39.1
40
0.9
0.001
0.05
5.4
CN25-DDH009
992749
40
42.3
2.3
0.001
0.05
5.5
CN25-DDH009
992750
42.3
43.3
1
0.001
0.02
4.69
CN25-DDH009
992751
43.3
44
0.7
0.002
0.13
6.76
CN25-DDH009
992752
44.3
45
0.7
Proto-Lens 2
0.013
1.39
28
CN25-DDH009
992754
45
46
1
0.010
0.48
13.35
CN25-DDH009
992755
46
47
1
0.011
1.14
12.3
CN25-DDH009
992756
47
48
1
0.011
0.36
13.75
CN25-DDH009
992757
48
49
1
0.008
0.21
11.55
CN25-DDH009
992758
49
50
1
0.005
0.08
7.76
CN25-DDH009
992650
50
51
1
0.017
0.43
20.7
CN25-DDH009
992651
51
52
1
0.005
0.06
8.39
CN25-DDH009
992653
52
52.9
0.9
0.004
0.15
7.86
CN25-DDH009
992654
52.9
53.65
0.75
0.002
0.22
6.88
CN25-DDH009
992655
53.65
54.4
0.75
0.001
0.01
4.19
CN25-DDH009
992656
54.4
55
0.6
0.001
0.01
36.3
CN25-DDH009
992657
55
56
1
0.012
0.7
14.15
CN25-DDH009
992658
56
56.9
0.9
0.070
2.89
15.7
CN25-DDH009
995259
56.9
58
1.1
Red Breccia
0.002
0.03
32.4
CN25-DDH009
995260
58
59
1
0.001
0.02
17.55
CN25-DDH009
995261
67
69
2
0.002
0.05
33.1
CN25-DDH009
995262
77
79
2
0.001
0.03
16.8
CN25-DDH009
995263
87
89
2
0.002
0.01
28.8
CN25-DDH009
995264
97
99
2
0.002
0.02
11.05
CN25-DDH009
995266
107.3
108.3
1
0.003
0.03
16.35
CN25-DDH009
995267
108.3
109.3
1
0.002
0.07
27.6
CN25-DDH009
995268
109.3
110
0.7
Proto-Lens 2
0.001
0.02
90.3
CN25-DDH009
995269
110
110.4
0.4
0.001
0.02
101.5
CN25-DDH009
995271
110.4
111
0.6
0.001
0.04
72.9
CN25-DDH009
995272
111
112
1
0.001
0.03
90.1
CN25-DDH009
995273
112
113
1
0.005
0.05
130.5
CN25-DDH009
995274
113
114
1
0.004
0.05
76.1
CN25-DDH009
995276
114
115
1
Andesite Dyke
0.007
0.08
40.5
CN25-DDH009
995277
115
117
2
Red Breccia
0.000
0.01
6.08
CN25-DDH009
995278
124
124.7
0.7
0.002
0.06
66.4

 

Table 2: Cerro Negro Project, Mostaza Mine; Mostaza drill core assay results for Cu, Ag and Sb, CNG25 DD006 - DD009.

 

 

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 of 3.3% Cu & 270g/t Ag

 

Enquiries:

 

Great Southern Copper plc
Sam Garrett, Chief Executive Officer
+44 (0) 20 4582 3500
SI Capital Limited
Nick Emerson
+44 (0) 1483 413500
BlytheRay
Tim Blythe / Megan Ray
+44 (0) 20 7138 3204
GSC@blytheray.com

 

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

 

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 or visit www.rns.com.

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