Collective Mining Expands Apollo's Surface Footprint by Drilling 31.70 Metres @ 17.35 g/t AuEq Within 165.75 Metres @ 5.35 g/t AuEq from 8.85 Metres
-
Step-out drilling from surface at the Apollo system in hole APC-159 has expanded the breccia body to the northeast by approximately 30 metres (where it remains open for further expansion) by intercepting gold grades up to 40% above the grades at the outer edge of the internal model. Highlights from the high-grade section of this hole are as follows:
-
165.75 metres @ 5.35 g/t gold equivalent from 8.85 metres including 31.70 metres @ 17.35 g/t gold equivalent
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165.75 metres @ 5.35 g/t gold equivalent from 8.85 metres including 31.70 metres @ 17.35 g/t gold equivalent
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Four additional holes have infilled the Apollo breccia body near surface by intercepting gold, tungsten, silver and copper grades above the prediction of the internal block model with highlights as follows:
-
60.45 metres @ 4.68 g/t gold equivalent from surface including 22.15 metres @
6.98 g/t gold equivalent (APC-155)
- 131.20 metres @ 2.61 g/t gold equivalent from 6.80 metres including 34.55 metres @ 4.13 g/t gold equivalent from 8.45 metres (APC-158)
-
60.45 metres @ 4.68 g/t gold equivalent from surface including 22.15 metres @
6.98 g/t gold equivalent (APC-155)
To date, Collective has completed 167,500 metres of diamond drilling across the Guayabales and
With
Details (see Table 1 and Figures 1-5)
- Five drill holes collared from Pad 22 intersected high-grade gold, tungsten, silver and copper mineralization starting from at or near surface with results as follows:
- 60.45 metres @ 4.68 g/t AuEq from surface (APC-155) including:
- 22.15 metres @ 6.98 g/t AuEq from 20.50 metres down hole
- 22.15 metres @ 6.98 g/t AuEq from 20.50 metres down hole
- 99.95 metres @ 2.64 g/t AuEq from surface (APC-156) including:
- 26.25 metres @ 4.72 g/t AuEq from surface
- 20.80 metres @ 3.04 g/t AuEq from 50.45 metres down hole
- 60.85 metres @ 3.06 g/t AuEq from surface (APC-157)
- 131.20 metres @ 2.61 g/t gold equivalent from 6.80 metres down hole (APC-158) including:
- 34.55 metres @ 4.13 g/t gold equivalent from 8.45 metres down hole
- 19.90 metres @ 3.50 g/t gold equivalent from 118.10 metres down hole
- 165.75 metres @ 5.35 g/t gold equivalent from 8.85 metres down hole (APC-159) including:
- 31.70 metres @ 17.35 g/t gold equivalent from 59.40 metres down hole
- 8.50 metres @ 27.82 g/t gold equivalent from 81.60 metres down hole
- 60.45 metres @ 4.68 g/t AuEq from surface (APC-155) including:
In APC-159, the Company also intersected 64.00 metres @ 2.00 g/t gold equivalent from 236.00 metres down hole. This mineralization represents newly discovered sheeted veinlets, which are located within the recently discovered
Planning is underway to follow up on the results of hole APC-159 by continuing to drill test for this high-grade mineralization in a northeast direction.
- Results announced today have expanded the Apollo breccia body from surface by up to 30 metres to the northeast and have increased the local gold and tungsten grades by up to 40% as compared to the internal block model. Also, the holes have successfully closed drilling gaps within the internal block model with drill spacing now down to 30 meter centers in this area (from surface down to 150 metres depth).
These results reinforce Apollo's status as a robust exploration discovery with multi-metal upside. The Company remains focused on aggressive expansion and delineation drilling to unlock further value ahead of a planned maiden mineral resource estimate in H1, 2027.
Table 1: Assays Results for Drill Holes APC-155, APC-156, APC-157, APC-158 and APC-159
|
Hole # |
From |
To |
Length |
Au |
WO3 % |
Ag |
Cu |
AuEq |
WO3Eq |
|
APC-155 |
0.00 |
60.45 |
60.45 |
1.28 |
0.66 |
43 |
0.15 |
4.68 |
0.83 |
|
Incl. |
20.50 |
42.65 |
22.15 |
1.12 |
1.33 |
25 |
0.14 |
6.98 |
1.24 |
|
APC-156 |
0.00 |
99.95 |
99.95 |
0.98 |
0.24 |
29 |
0.28 |
2.64 |
|
|
Incl. |
0.00 |
26.25 |
26.25 |
2.70 |
0.38 |
33 |
0.10 |
4.72 |
|
|
& Incl. |
50.45 |
71.25 |
20.80 |
0.36 |
0.53 |
23 |
0.18 |
3.04 |
|
|
APC-157 |
0.00 |
60.85 |
60.85 |
1.20 |
0.25 |
42 |
0.24 |
3.06 |
|
|
APC-158 |
6.80 |
138.00 |
131.20 |
1.21 |
0.22 |
27 |
0.14 |
2.61 |
|
|
Incl. |
8.45 |
43.00 |
34.55 |
1.35 |
0.48 |
50 |
0.16 |
4.13 |
|
|
& Incl. |
118.10 |
138.00 |
19.90 |
3.08 |
0.04 |
19 |
0.08 |
3.50 |
|
|
APC-159 |
8.85 |
174.60 |
165.75 |
4.39 |
0.09 |
42 |
0.13 |
5.35 |
|
|
Incl. |
59.40 |
91.10 |
31.70 |
15.65 |
0.26 |
66 |
0.17 |
17.35 |
|
|
Incl. |
81.60 |
90.10 |
8.50 |
25.18 |
0.24 |
156 |
0.20 |
27.82 |
|
|
and |
236.00 |
300.00 |
64.00 |
1.87 |
- |
10 |
0.02 |
2.00 |
|
*AuEq (g/t) is calculated as follows: (Au (g/t) x 0.97) + (Ag (g/t) x 0.017 x 0.85) + (Cu (%) x 1.14 x 0.95) + (WO3 (%) x 5.64 x 0.72) utilizing metal prices of
Au –
**WO3Eq% is calculated as follows: (WO3 (%) x 0.72) + (Au (g/t) x 0.18 x 0.97) + (Ag (g/t) x 0.003 x 0.85) + (Cu (%) x 0.20 x 0.95) utilizing metal prices of WO3 –
Recovery rate assumptions for metals are based on metallurgical results announced on
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To see our latest corporate presentation and related information, please visit www.collectivemining.com.
Founded by the team that developed and sold
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 at the
Additionally, the Company is drilling its optioned
Management, insiders, a strategic investor and close family and friends own 45.3% of the outstanding shares of the Company and as a result, are fully aligned with shareholders. The Company is listed on both the NYSE American and TSX under the trading symbol "CNL".
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.
Technical Information
Samples were cut by Company personnel at
Core samples have been prepared and analyzed at ALS laboratory facilities in
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