Collective Mining Discovers High-Grade Subzones in Apollo and Drills the Best Hole Ever, Intersecting 150.55 Metres at 6.16 g/t AuEq Within 534.40 Metres at 2.70 g/t AuEq
Collective Mining (NYSE: CNL) has announced significant drilling results from its Apollo system at the Guayabales Project in Colombia. The company's drill hole APC104-D1 intercepted 534.40 metres at 2.70 g/t gold equivalent, including a high-grade section of 150.55 metres at 6.16 g/t gold equivalent.
This represents the largest grade accumulation intercepted to date at Apollo at 1,440 g/t gold equivalent, 38% higher than the average of previous significant intercepts. The company has completed two additional holes testing the newly modeled high-grade subzones, with assay results expected in early Q1, 2025.
For 2025, Collective Mining has planned a fully funded 60,000-metre drill program, the largest in company history, focusing on systematically testing the vertical extent of new modeled high-grade subzones covering more than 1,000 vertical metres.
Collective Mining (NYSE: CNL) ha annunciato risultati significativi di perforazione dal suo sistema Apollo presso il progetto Guayabales in Colombia. Il foro di perforazione APC104-D1 ha intercettato 534,40 metri a 2,70 g/t di equivalente oro, inclusa una sezione ad alta legge di 150,55 metri a 6,16 g/t di equivalente oro.
Questo rappresenta il maggior accumulo di grado intercettato fino ad oggi ad Apollo con 1.440 g/t di equivalente oro, superiore del 38% rispetto alla media degli intercetti significativi precedenti. L'azienda ha completato altri due fori testando le nuove subzone ad alta legge modellate, con risultati delle analisi previsti all'inizio del primo trimestre del 2025.
Per il 2025, Collective Mining ha pianificato un programma di perforazione di 60.000 metri completamente finanziato, il più grande nella storia dell'azienda, incentrato sul test sistematico dell'estensione verticale delle nuove subzone ad alta legge modellate che coprono oltre 1.000 metri verticali.
Collective Mining (NYSE: CNL) ha anunciado resultados significativos de perforación de su sistema Apollo en el Proyecto Guayabales en Colombia. El agujero de perforación APC104-D1 interceptó 534,40 metros a 2,70 g/t de equivalente de oro, incluyendo una sección de alta ley de 150,55 metros a 6,16 g/t de equivalente de oro.
Esto representa la mayor acumulación de grado interceptada hasta la fecha en Apollo de 1.440 g/t de equivalente de oro, un 38% más que el promedio de interceptos significativos anteriores. La empresa ha completado dos agujeros adicionales probando las nuevas subzonas de alta ley modeladas, con resultados de ensayo esperados a principios del primer trimestre de 2025.
Para 2025, Collective Mining ha planificado un programa de perforación de 60.000 metros completamente financiado, el más grande en la historia de la empresa, enfocándose en probar sistemáticamente la extensión vertical de nuevas subzonas de alta ley modeladas que cubren más de 1.000 metros verticales.
Collective Mining (NYSE: CNL)는 콜롬비아 Guayabales 프로젝트의 Apollo 시스템에서 중요한 시추 결과를 발표했습니다. 회사의 시추 구멍 APC104-D1은 534.40미터에서 2.70 g/t 금 등가물을 절단했고, 150.55미터에서 6.16 g/t 금 등가물의 고도 금속 구간을 포함했습니다.
이는 현재까지 Apollo에서 절단된 최대 금속 농축량으로, 1,440 g/t 금 등가물이며, 이전의 중요한 절단 평균보다 38% 높습니다. 회사는 새로 모델링된 고등급 하위 구역을 테스트하기 위해 추가로 두 개의 구멍을 완료했으며, 분석 결과는 2025년 1분기 초에 예상됩니다.
2025년을 위해 Collective Mining은 60,000미터의 완전 자금 지원 시추 프로그램을 계획했으며, 이는 회사 역사상 가장 큰 규모로, 1,000미터 이상의 수직 범위를 포괄하는 새로운 모델링된 고등급 하위 구역의 수직 범위를 체계적으로 테스트하는 데 중점을 두고 있습니다.
Collective Mining (NYSE: CNL) a annoncé des résultats de forage significatifs de son système Apollo au projet Guayabales en Colombie. Le trou de forage APC104-D1 a intercepté 534,40 mètres à 2,70 g/t d'équivalent or, comprenant une section de haute teneur de 150,55 mètres à 6,16 g/t d'équivalent or.
Ceci représente l'accumulation de grade la plus importante interceptée à ce jour à Apollo avec 1.440 g/t d'équivalent or, soit 38 % de plus que la moyenne des interceptions significatives précédentes. L'entreprise a achevé deux autres trous testant les nouvelles sous-zones à haute teneur modélisées, avec des résultats d'analyse prévus au début du premier trimestre 2025.
Pour 2025, Collective Mining a prévu un programme de forage financé de 60.000 mètres, le plus important de l'histoire de l'entreprise, axé sur le test systématique de l'extension verticale des nouvelles sous-zones à haute teneur modélisées couvrant plus de 1.000 mètres verticaux.
Collective Mining (NYSE: CNL) hat bedeutende Bohrergebnisse aus seinem Apollo-System im Guayabales-Projekt in Kolumbien bekannt gegeben. Das Bohrloch APC104-D1 hat 534,40 Meter mit 2,70 g/t Goldäquivalent abgebohrt, einschließlich eines hochgradigen Abschnitts von 150,55 Metern mit 6,16 g/t Goldäquivalent.
Dies stellt die größte Gradansammlung dar, die bisher im Apollo entdeckt wurde, mit 1.440 g/t Goldäquivalent, was 38% höher ist als der Durchschnitt der vorherigen signifikanten Abfangungen. Das Unternehmen hat zwei zusätzliche Löcher gebohrt, um die neu modellierten hochgradigen Subzonen zu testen, wobei die Analyseergebnisse Anfang des ersten Quartals 2025 erwartet werden.
Für 2025 hat Collective Mining ein vollständig finanziertes Bohrprogramm über 60.000 Meter geplant, das größte in der Unternehmensgeschichte, das sich darauf konzentriert, die vertikale Ausdehnung neuer modellierter hochgradiger Subzonen zu systematisch zu testen, die mehr als 1.000 vertikale Meter abdecken.
- Record-breaking drill results with 150.55m at 6.16 g/t AuEq within 534.40m at 2.70 g/t AuEq
- Largest grade accumulation to date at Apollo (1,440 g/t AuEq)
- Fully funded 60,000-metre drill program planned for 2025
- System remains open in all directions with mineralization from surface to 1,150m depth
- Discovery of new high-grade subzones indicating potential significant upside to grade and size
- Assay results for additional holes delayed until Q1 2025
Insights
The latest drilling results from Collective Mining's Apollo system represent a significant breakthrough in the project's development. The intercept of 150.55 metres at 6.16 g/t AuEq within a broader zone of 534.40 metres at 2.70 g/t AuEq marks the highest grade accumulation to date at
The discovery of high-grade subzones through orthogonal drilling indicates that previous drilling may have underestimated the system's grade potential. With mineralization open in all directions and extending over 1,150 meters below surface, the planned 60,000-metre drill program for 2025 could significantly expand the resource envelope and improve grade profiles.
The newly discovered high-grade subzones and Ramp Zone at Apollo demonstrate exceptional exploration upside. The strategic shift to orthogonal drilling from the northern side has proven highly effective, with hole APC104-D1 revealing multiple high-grade zones including 39.55 metres at 10.60 g/t AuEq. Visual confirmation of similar mineralization in subsequent holes APC104-D2 and APC104-D3 suggests consistency in the high-grade zones.
The proximity to Aris Mining's multi-million-ounce Marmato Deeps deposit, just 1.75 kilometers away and similar geological characteristics enhance the project's potential. The systematic testing planned for 2025 could substantially improve the deposit's economic viability.
- The hole was successfully drilled orthogonally across the Apollo system to test, for the first time, the potential of newly modelled broad high-grade subzones within the system.
- Two additional holes to test the newly modelled high-grade subzones have been completed. Both holes intersected the projection of the newly modelled subzones and cut significant sulphide mineralization over broad intervals with assay results expected in early Q1, 2025.
- Drilling in 2025 will systematically test the vertical extent of the new modelled high-grade subzones, which cover more than 1,000 vertical metres, as they have the potential to significantly increase the overall grade profile of the Apollo system.
Ari Sussman, Executive Chairman commented: "This is a remarkable result for which our Colombian technical team deserves much credit. Internal deposit modelling led to the realization that most of the prior drilling from the south was not directly orthogonally across the system and that we should start drilling from the northern side of Apollo in a southerly pattern. As a result, drill Pad17 was constructed, and the hypothesis was tested with hole APC104-D1. 2025 is going to be an exciting year for the Company as we focus drilling on chasing laterally and vertically both the high-grade subzones and Ramp Zone as part of our fully funded, 60,000-metre drill program."
To watch a video of David Reading, Special Advisor to the Company and QP under NI43-101 explain today's results please click on the link here.
Details (see Table 1-2 and Figures 1-5)
- APC104-D1 was drilled southwest from mother hole APC-104D (collared from new Pad17) to intercept, orthogonally, multiple newly modeled high-grade subzones within the Apollo system with assay results as follows:
- 534.40 metres @ 2.70 g/t gold equivalent from 107.10 metres including:
- 150.55 metres @ 6.16 g/t gold equivalent from 107.10 metres which includes,
- 39.55 metres @ 10.60 g/t gold equivalent and,
- 37.75 metres @ 5.04 g/t gold equivalent from 358.20 metres which includes,
- 18.75 metres @ 7.85 g/t gold equivalent
- 18.75 metres @ 7.85 g/t gold equivalent
- 150.55 metres @ 6.16 g/t gold equivalent from 107.10 metres which includes,
- APC104-D1 is the largest grade accumulation intercepted to date at Apollo at 1,440 g/t gold equivalent on a gram x metre basis. For context, the grade accumulation in APC104-D1 at 1,440 g/t gold equivalent is
38% higher than the average of 1,055 g/t gold equivalent for the prior fourteenth grade accumulation intercepts at over 1,000 g/t gold equivalent drilled by the Company.
APC104-D1 is the first hole within a newly designed large drilling program aimed at delineating and extending the high-grade subzones to depth at Apollo. Visual logging of recently completed additional drill holes, APC104-D2 and APC104-D3, indicate that both holes have intersected the same styles of mineralization and sulphide levels as reported in APC104-D1.
- High-grade intercepts within Apollo have now been sparsely drilled from surface down to 1,150 metres below surface with the deepest intercept being the recent discovery of the Ramp Zone which returned an intercept of 57.65 metres @ 8.18 g/t gold equivalent (see press release dated October 22, 2024). The Ramp Zone is located close in elevation to the conceptual underground haulage tunnel for a future mine at the Guayabales Project and shares some geological characteristics with Aris Mining's multi-million-ounce Marmato Deeps deposit located only 1.75 kilometres southeast of Apollo. Drilling at the Ramp Zone is ongoing with assay results anticipated in early Q1, 2025.
- The broad mineralized interval of APC104-D1 has also expanded the Apollo system southwestwards by an additional 30 metres. Additionally, a new zone of mineralization located outside of the breccia body in country rock returned 20.10 metres @ 1.23 g/t gold equivalent and bottomed in mineralization at the end of the hole.
- The discovery of the new high-grade subzones and the recently discovered Ramp Zone highlight that the grade profile of Apollo is poorly understood and that there is potentially significant upside to the grade (and size) of the system. The Company's 2025 drilling program will involve up to five rigs at Apollo and focus on extending and defining both the high-grade subzones and the Ramp Zone, as well as to continue expanding the Apollo system northwards and to depth. Mineralization at Apollo begins directly from surface, remains open in all directions and has current dimensions of 600 metres strike, 400 metres width and extends more than 1,150 metres below surface.
Table 1: Assays Results for Drill Hole APC104-D1 (Also see Table 2 below for a complete breakdown of individual assay results that make up the broad subzone of 150.55m @ 6.16 g/t AuEq)
Hole # | From | To | Length | Au | Ag | Cu | Zn | AuEq |
APC104-D1 | 50.30 | 57.10 | 6.80 | 1.32 | 10 | 0.01 | 0.13 | 1.48 |
and | 107.10 | 641.50 | 534.40 | 2.16 | 32 | 0.09 | 0.21 | 2.70 |
Incl | 165.45 | 205.00 | 39.55 | 7.94 | 156 | 0.28 | 1.43 | 10.60 |
Within | 107.10 | 257.65 | 150.55 | 4.71 | 87 | 0.22 | 0.50 | 6.16 |
& incl. | 358.20 | 376.95 | 18.75 | 7.80 | 17 | 0.03 | 0.11 | 7.85 |
Within | 358.20 | 395.95 | 37.75 | 4.88 | 15 | 0.03 | 0.20 | 5.04 |
and | 730.10 | 750.20 | 20.10 | 1.13 | 4 | 0.03 | 0.11 | 1.23 |
*AuEq (g/t) is calculated as follows: (Au (g/t) x 0.97) + (Ag (g/t) x 0.015 x 0.85) + (Cu (%) x 1.44 x 0.95) + (Zn (%) x 0.43 x 0.85) utilizing metal prices of Ag – |
Table 2: Assays Results for the High-Grade Gold Subzone Within APC104-D1 Running 150.55 Metres @ 6.16 g/t AuEq
From (m) | To | Length | Au | Ag | Cu | Zn |
107.10 | 108.25 | 1.15 | 5.44 | 22 | 0.04 | 0.14 |
108.25 | 109.85 | 1.60 | 4.66 | 37 | 0.04 | 0.93 |
109.85 | 110.80 | 0.95 | 10.90 | 54 | 0.11 | 0.53 |
110.80 | 111.65 | 0.85 | 0.96 | 7 | 0.02 | 0.05 |
111.65 | 112.65 | 1.00 | 2.52 | 31 | 0.03 | 0.54 |
112.65 | 113.65 | 1.00 | 3.90 | 93 | 0.14 | 2.94 |
113.65 | 114.50 | 0.85 | 3.10 | 16 | 0.02 | 0.19 |
114.50 | 115.85 | 1.35 | 0.82 | 22 | 0.04 | 0.31 |
115.85 | 117.00 | 1.15 | 2.44 | 47 | 0.08 | 0.81 |
117.00 | 117.90 | 0.90 | 0.10 | 9 | 0.04 | 0.01 |
117.90 | 118.80 | 0.90 | 9.75 | 98 | 0.23 | 0.31 |
118.80 | 119.80 | 1.00 | 4.97 | 33 | 0.07 | 0.27 |
119.80 | 121.40 | 1.60 | 6.02 | 26 | 0.04 | 0.23 |
121.40 | 123.00 | 1.60 | 20.00 | 17 | 0.03 | 0.11 |
123.00 | 124.65 | 1.65 | 8.85 | 13 | 0.03 | 0.08 |
124.65 | 126.50 | 1.85 | 2.43 | 28 | 0.06 | 0.19 |
126.50 | 128.25 | 1.75 | 9.64 | 45 | 0.05 | 0.70 |
128.25 | 129.70 | 1.45 | 3.92 | 37 | 0.03 | 0.09 |
129.70 | 131.20 | 1.50 | 0.28 | 13 | 0.06 | 0.01 |
131.20 | 132.55 | 1.35 | 2.63 | 15 | 0.08 | 0.01 |
132.55 | 134.25 | 1.70 | 0.99 | 10 | 0.05 | 0.01 |
134.25 | 135.15 | 0.90 | 0.04 | 3 | 0.01 | 0.01 |
135.15 | 136.70 | 1.55 | 0.09 | 8 | 0.08 | 0.02 |
136.70 | 137.75 | 1.05 | 1.45 | 175 | 0.61 | 0.05 |
137.75 | 138.60 | 0.85 | 0.17 | 210 | 0.88 | 0.05 |
138.60 | 139.25 | 0.65 | 0.25 | 407 | 1.70 | 0.09 |
139.25 | 140.10 | 0.85 | 0.42 | 499 | 2.28 | 0.12 |
140.10 | 141.00 | 0.90 | 0.89 | 175 | 0.59 | 0.05 |
141.00 | 141.80 | 0.80 | 2.60 | 551 | 1.72 | 0.18 |
141.80 | 142.75 | 0.95 | 3.61 | 216 | 0.67 | 0.08 |
142.75 | 143.55 | 0.80 | 0.62 | 162 | 0.58 | 0.08 |
143.55 | 144.40 | 0.85 | 0.29 | 349 | 1.42 | 0.10 |
144.40 | 145.50 | 1.10 | 0.96 | 336 | 1.43 | 0.14 |
145.50 | 146.80 | 1.30 | 0.53 | 139 | 0.61 | 0.06 |
146.80 | 147.90 | 1.10 | 0.82 | 323 | 1.25 | 0.09 |
147.90 | 149.15 | 1.25 | 1.49 | 161 | 0.63 | 0.06 |
149.15 | 150.45 | 1.30 | 0.17 | 44 | 0.19 | 0.02 |
150.45 | 151.30 | 0.85 | 0.42 | 78 | 0.26 | 0.03 |
151.30 | 152.45 | 1.15 | 0.71 | 55 | 0.15 | 0.25 |
152.45 | 153.40 | 0.95 | 1.64 | 71 | 0.23 | 0.10 |
153.40 | 154.20 | 0.80 | 7.08 | 89 | 0.27 | 0.11 |
154.20 | 155.65 | 1.45 | 6.55 | 61 | 0.19 | 0.09 |
155.65 | 156.45 | 0.80 | 4.32 | 110 | 0.34 | 0.71 |
156.45 | 157.25 | 0.80 | 6.21 | 35 | 0.09 | 0.24 |
157.25 | 158.05 | 0.80 | 6.52 | 142 | 0.44 | 0.06 |
158.05 | 158.85 | 0.80 | 1.11 | 35 | 0.12 | 0.20 |
158.85 | 159.70 | 0.85 | 3.76 | 152 | 0.58 | 0.23 |
159.70 | 160.65 | 0.95 | 0.98 | 72 | 0.26 | 0.06 |
160.65 | 161.40 | 0.75 | 6.10 | 64 | 0.12 | 0.33 |
161.40 | 162.20 | 0.80 | 0.73 | 26 | 0.09 | 0.05 |
162.20 | 163.05 | 0.85 | 0.39 | 23 | 0.06 | 0.07 |
163.05 | 163.85 | 0.80 | 4.70 | 17 | 0.05 | 0.22 |
163.85 | 164.65 | 0.80 | 0.40 | 20 | 0.05 | 0.31 |
164.65 | 165.45 | 0.80 | 0.92 | 46 | 0.14 | 0.08 |
165.45 | 166.25 | 0.80 | 3.91 | 224 | 0.65 | 0.47 |
166.25 | 167.55 | 1.30 | 5.68 | 186 | 0.61 | 0.08 |
167.55 | 168.45 | 0.90 | 5.41 | 152 | 0.34 | 3.86 |
168.45 | 169.35 | 0.90 | 29.30 | 687 | 1.34 | 7.04 |
169.35 | 170.60 | 1.25 | 12.20 | 414 | 0.68 | 8.16 |
170.60 | 171.65 | 1.05 | 17.75 | 1235 | 1.24 | 4.21 |
171.65 | 172.45 | 0.80 | 16.95 | 552 | 0.84 | 5.46 |
172.45 | 173.20 | 0.75 | 12.60 | 435 | 0.28 | 6.42 |
173.20 | 174.30 | 1.10 | 17.15 | 599 | 0.97 | 5.78 |
174.30 | 175.10 | 0.80 | 2.93 | 129 | 0.10 | 3.41 |
175.10 | 175.90 | 0.80 | 8.10 | 388 | 0.67 | 5.86 |
175.90 | 176.70 | 0.80 | 3.83 | 58 | 0.15 | 0.18 |
176.70 | 177.60 | 0.90 | 3.04 | 61 | 0.17 | 0.12 |
177.60 | 178.70 | 1.10 | 1.88 | 39 | 0.14 | 0.46 |
178.70 | 179.50 | 0.80 | 0.28 | 25 | 0.09 | 0.08 |
179.50 | 180.40 | 0.90 | 1.81 | 36 | 0.11 | 0.08 |
180.40 | 181.35 | 0.95 | 5.50 | 153 | 0.45 | 0.30 |
181.35 | 182.40 | 1.05 | 2.92 | 123 | 0.45 | 0.04 |
182.40 | 183.25 | 0.85 | 1.90 | 47 | 0.14 | 0.32 |
183.25 | 184.15 | 0.90 | 4.51 | 81 | 0.19 | 1.96 |
184.15 | 185.00 | 0.85 | 1.51 | 31 | 0.08 | 0.47 |
185.00 | 185.85 | 0.85 | 2.46 | 59 | 0.12 | 0.62 |
185.85 | 186.70 | 0.85 | 16.90 | 62 | 0.14 | 0.64 |
186.70 | 187.60 | 0.90 | 6.04 | 43 | 0.14 | 0.03 |
187.60 | 188.45 | 0.85 | 19.90 | 46 | 0.08 | 0.08 |
188.45 | 189.30 | 0.85 | 4.56 | 24 | 0.05 | 0.04 |
189.30 | 190.05 | 0.75 | 2.43 | 23 | 0.05 | 0.07 |
190.05 | 190.65 | 0.60 | 0.42 | 9 | 0.03 | 0.07 |
190.65 | 191.55 | 0.90 | 1.57 | 23 | 0.04 | 0.04 |
191.55 | 192.35 | 0.80 | 7.72 | 43 | 0.06 | 0.54 |
192.35 | 193.35 | 1.00 | 26.60 | 57 | 0.09 | 0.62 |
193.35 | 194.15 | 0.80 | 3.24 | 25 | 0.06 | 0.14 |
194.15 | 195.15 | 1.00 | 9.12 | 28 | 0.07 | 0.34 |
195.15 | 196.15 | 1.00 | 5.82 | 30 | 0.07 | 0.18 |
196.15 | 197.05 | 0.90 | 4.34 | 57 | 0.09 | 0.37 |
197.05 | 198.00 | 0.95 | 12.35 | 70 | 0.09 | 0.33 |
198.00 | 198.80 | 0.80 | 6.67 | 44 | 0.07 | 0.99 |
198.80 | 199.80 | 1.00 | 6.33 | 50 | 0.07 | 0.16 |
199.80 | 200.60 | 0.80 | 8.41 | 25 | 0.07 | 0.21 |
200.60 | 201.40 | 0.80 | 2.81 | 23 | 0.06 | 0.08 |
201.40 | 202.20 | 0.80 | 21.30 | 33 | 0.07 | 0.35 |
202.20 | 203.00 | 0.80 | 3.12 | 27 | 0.09 | 0.07 |
203.00 | 204.00 | 1.00 | 2.38 | 14 | 0.05 | 0.03 |
204.00 | 205.00 | 1.00 | 8.00 | 28 | 0.09 | 0.02 |
205.00 | 205.95 | 0.95 | 2.46 | 21 | 0.07 | 0.02 |
205.95 | 206.80 | 0.85 | 1.99 | 14 | 0.05 | 0.02 |
206.80 | 207.80 | 1.00 | 0.17 | 9 | 0.04 | 0.01 |
207.80 | 208.60 | 0.80 | 0.71 | 23 | 0.06 | 0.24 |
208.60 | 209.55 | 0.95 | 0.56 | 12 | 0.04 | 0.04 |
209.55 | 210.60 | 1.05 | 1.11 | 13 | 0.03 | 0.15 |
210.60 | 211.40 | 0.80 | 0.34 | 10 | 0.03 | 0.02 |
211.40 | 212.25 | 0.85 | 0.47 | 8 | 0.02 | 0.03 |
212.25 | 213.25 | 1.00 | 1.32 | 13 | 0.04 | 0.05 |
213.25 | 214.25 | 1.00 | 0.02 | 1 | 0.01 | 0.01 |
214.25 | 215.25 | 1.00 | 0.47 | 30 | 0.09 | 0.05 |
215.25 | 216.05 | 0.80 | 6.47 | 50 | 0.13 | 0.14 |
216.05 | 217.10 | 1.05 | 9.74 | 94 | 0.26 | 0.11 |
217.10 | 218.20 | 1.10 | 5.98 | 29 | 0.08 | 0.03 |
218.20 | 219.15 | 0.95 | 8.82 | 26 | 0.09 | 0.02 |
219.15 | 220.15 | 1.00 | 23.70 | 23 | 0.07 | 0.03 |
220.15 | 221.15 | 1.00 | 0.86 | 12 | 0.04 | 0.04 |
221.15 | 222.05 | 0.90 | 0.60 | 22 | 0.06 | 0.10 |
222.05 | 223.05 | 1.00 | 1.96 | 25 | 0.08 | 0.05 |
223.05 | 223.90 | 0.85 | 7.00 | 21 | 0.08 | 0.02 |
223.90 | 224.85 | 0.95 | 1.57 | 24 | 0.07 | 0.02 |
224.85 | 225.80 | 0.95 | 0.48 | 20 | 0.07 | 0.01 |
225.80 | 226.80 | 1.00 | 1.31 | 30 | 0.08 | 0.05 |
226.80 | 227.80 | 1.00 | 3.51 | 33 | 0.10 | 0.14 |
227.80 | 228.60 | 0.80 | 8.77 | 61 | 0.18 | 0.04 |
228.60 | 229.55 | 0.95 | 26.20 | 41 | 0.09 | 0.03 |
229.55 | 230.55 | 1.00 | 2.76 | 21 | 0.07 | 0.02 |
230.55 | 231.50 | 0.95 | 0.78 | 14 | 0.04 | 0.03 |
231.50 | 232.30 | 0.80 | 0.05 | 5 | 0.02 | 0.02 |
232.30 | 233.40 | 1.10 | 0.31 | 29 | 0.09 | 0.11 |
233.40 | 234.30 | 0.90 | 2.45 | 18 | 0.06 | 0.02 |
234.30 | 235.10 | 0.80 | 9.47 | 49 | 0.13 | 0.08 |
235.10 | 236.00 | 0.90 | 5.37 | 58 | 0.16 | 0.06 |
236.00 | 236.90 | 0.90 | 14.65 | 60 | 0.16 | 0.15 |
236.90 | 238.00 | 1.10 | 0.17 | 8 | 0.03 | 0.03 |
238.00 | 238.95 | 0.95 | 1.10 | 22 | 0.05 | 0.13 |
238.95 | 239.95 | 1.00 | 10.00 | 100 | 0.24 | 0.18 |
239.95 | 241.10 | 1.15 | 1.08 | 21 | 0.06 | 0.07 |
241.10 | 242.10 | 1.00 | 8.58 | 24 | 0.07 | 0.09 |
242.10 | 242.90 | 0.80 | 6.45 | 74 | 0.25 | 0.04 |
242.90 | 243.70 | 0.80 | 1.33 | 18 | 0.04 | 0.05 |
243.70 | 244.65 | 0.95 | 0.44 | 17 | 0.05 | 0.06 |
244.65 | 245.40 | 0.75 | 6.78 | 73 | 0.18 | 0.59 |
245.40 | 246.20 | 0.80 | 1.41 | 35 | 0.10 | 0.41 |
246.20 | 247.10 | 0.90 | 1.80 | 118 | 0.43 | 0.10 |
247.10 | 248.10 | 1.00 | 0.84 | 32 | 0.09 | 0.07 |
248.10 | 249.15 | 1.05 | 1.55 | 22 | 0.07 | 0.02 |
249.15 | 250.15 | 1.00 | 1.56 | 24 | 0.05 | 0.38 |
250.15 | 251.00 | 0.85 | 3.83 | 27 | 0.08 | 0.14 |
251.00 | 252.00 | 1.00 | 0.14 | 18 | 0.07 | 0.02 |
252.00 | 253.00 | 1.00 | 0.07 | 10 | 0.03 | 0.01 |
253.00 | 253.85 | 0.85 | 0.78 | 32 | 0.11 | 0.03 |
253.85 | 254.75 | 0.90 | 1.20 | 26 | 0.09 | 0.02 |
254.75 | 255.65 | 0.90 | 0.72 | 33 | 0.09 | 0.02 |
255.65 | 256.65 | 1.00 | 1.02 | 32 | 0.11 | 0.12 |
256.65 | 257.65 | 1.00 | 4.91 | 37 | 0.10 | 0.03 |
Weighted Average | 150.55 | 4.71 | 87 | 0.22 | 0.50 |
About Collective Mining Ltd.
To see our latest corporate presentation and related information, please visit www.collectivemining.com
Founded by the team that developed and sold Continental Gold Inc. to Zijin Mining for approximately
The Company's flagship project, Guayabales, is anchored by the Apollo system, which hosts the large-scale, bulk-tonnage and high-grade gold-silver-copper-tungsten Apollo system. The Company's objectives are to expand the Apollo system by stepping out along strike and testing the newly discovered high-grade Apollo Ramp Zone, expand the Trap system and drill a series of newly generated targets including Tower and X.
Management, insiders, a strategic investor and close family and friends own
Qualified Person (QP) and NI43-101 Disclosure
David J Reading is the designated Qualified Person for this news release within the meaning of National Instrument 43-101 ("NI 43-101") and has reviewed and verified that the technical information contained herein is accurate and approves of the written disclosure of same. Mr. Reading has an MSc in Economic Geology and is a Fellow of the Institute of Materials, Minerals and Mining and of the Society of Economic Geology (SEG).
Technical Information
Rock, soils and core samples have been prepared and analyzed at ALS laboratory facilities in
Information Contact:
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FORWARD-LOOKING STATEMENTS
This news release contains "forward-looking statements" and "forward-looking information" within the meaning of applicable securities legislation (collectively, "forward-looking statements"). All statements, other than statements of historical fact, are forward-looking statements and are based on expectations, estimates and projections as at the date of this news release. Any statement that involves discussion with respect to predictions, expectations, beliefs, plans, projections, objectives, assumptions, future events or performance (often, but not always using phrases such as "plans", "expects", "is expected", "budget", "scheduled", "estimates", "forecasts", "intends", "anticipates", or "believes" or variations (including negative variations) of such words and phrases, or state that certain actions, events or results "may", "could", "would", "might" or "will" be taken, occur or be achieved) are not statements of historical fact and may be forward-looking statements. In this news release, forward-looking statements relate, among other things, to: the anticipated advancement of mineral properties or programs; future operations; future recovery metal recovery rates; future growth potential of Collective; and future development plans.
These forward-looking statements, and any assumptions upon which they are based, are made in good faith and reflect our current judgment regarding future events including the direction of our business. Management believes that these assumptions are reasonable. Forward-looking statements involve known and unknown risks, uncertainties and other factors which may cause the actual results, performance or achievements of the Company to be materially different from any future results, performance or achievements expressed or implied by the forward-looking statements. Such factors include, among others: risks related to the speculative nature of the Company's business; the Company's formative stage of development; the Company's financial position; possible variations in mineralization, grade or recovery rates; actual results of current exploration activities; conclusions of future economic evaluations; fluctuations in general macroeconomic conditions; fluctuations in securities markets; fluctuations in spot and forward prices of gold, precious and base metals or certain other commodities; fluctuations in currency markets; change in national and local government, legislation, taxation, controls regulations and political or economic developments; risks and hazards associated with the business of mineral exploration, development and mining (including environmental hazards, industrial accidents, unusual or unexpected formation pressures, cave-ins and flooding); inability to obtain adequate insurance to cover risks and hazards; the presence of laws and regulations that may impose restrictions on mining; employee relations; relationships with and claims by local communities and indigenous populations; availability of increasing costs associated with mining inputs and labour; the speculative nature of mineral exploration and development (including the risks of obtaining necessary licenses, permits and approvals from government authorities); and title to properties, as well as those risk factors discussed or referred to in the annual information form of the Company dated March 27, 2024. Forward-looking statements contained herein are made as of the date of this news release and the Company disclaims any obligation to update any forward-looking statements, whether as a result of new information, future events or results, except as may be required by applicable securities laws. There can be no assurance that forward-looking statements will prove to be accurate, as actual results and future events could differ materially from those anticipated in such statements and there may be other factors that cause results not to be anticipated, estimated or intended. Accordingly, readers should not place undue reliance on forward-looking statements.
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