Source - LSE Regulatory
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 DD0011;

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 targets2

·    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 DD0011 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.

 

Imagen que contiene edificio, ladrillo, piedra, caliente El contenido generado por IA puede ser incorrecto.

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

ID

FROM

(m)

TO

(m)

LONG

(m)

LITHOLOGY

Cu %

Ag g/t

Sb ppm

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

 

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.

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.
 
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