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.

 

 

 

Gráfico El contenido generado por IA puede ser incorrecto.

 

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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