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Base Metals Collective Mining Energy Junior Mining Precious Metals

Collective Mining Begins Mobilizing a Fourth Drill Rig to Test Six New High-Grade Porphyry Targets Within a 400 Metre Radius of the Apollo System

  • Exploration fieldwork has identified six well mineralized and outcropping porphyry and related style targets within a 400 metre radius of the Apollo system with assay results for soil and rock samples as follows:
  • Surface mapping at all six targets has outlined the same style of porphyry mineralization as the Apollo system, namely altered porphyry with vein stockwork, inter-mineral breccia with oxide followed by sulphides in the matrix and overprinting late-stage porphyry veins (“CBM Veins”).
  • Although the amount of rock and soil exposure in the sampling radius covering each of the six target areas is limited due to vegetation, historical landslides and volcanic ash cover, the scale of the areas and tenor of the assay results are similar to the original outcrop of the Apollo system. The Company estimates that there is no more than 5% rock exposure anywhere at the Guayabales project.
  • For comparison, the outcrop of the Apollo porphyry system prior to drilling only measured 10 metres in diameter. Subsequent drilling has outlined a porphyry system that to date measures 150 metres by 130 metres at surface, which then expands in dimensions quickly at depth to up to 500 metres wide and remains open.
  • Surface sampling was carried out in oxidized material and if the oxidation zone shares similar characteristics to the Apollo system, the copper and silver grades have been reduced by leaching. Recent drill results from Pad 6 and Pad 7 at Apollo corroborates this assertion.
  • A fourth drill rig is being mobilized to the project and is expected to initiate testing of the six new targets in late Q2, 2023.
  • Six additional holes have been completed at the Apollo system with assay results expected in the near term. APC-41, APC-42 and APC-45 are shorter holes designed to test the contact zones between the inter-mineral breccia and porphyry host rock in search of higher-grade sub zones. APC-44 and APC 46 are longer holes (up to 425 metres in mineralization) drilled from Pad 6 as part of a fan pattern to assess the shallow mineralization in this area and APC-47 is an exploratory hole drilled to the east from Pad 4 to test for mineralization beginning from below surface.

Ari Sussman, Executive Chairman commented: “The discovery of these new mineralized porphyry outcrops around Apollo are both exciting and significant for the Company. The original discovery outcrop of Apollo only covered a 10 metre radius and subsequent drilling has demonstrated that Apollo has the morphology of an inverted carrot with limited surface expression. This fact puts these new targets into perspective and highlights that the Apollo area is highly prospective for further exploration. We only found these new outcrops because of various recently excavated tracks emplaced to service and supply the drilling pads. I am looking forward to new drill rigs turning at these targets in the near term.”

TORONTO, April 18, 2023 /CNW/ – Collective Mining Ltd. (TSXV: CNL) (OTCQX: CNLMF) (“Collective” or the “Company”) is pleased to announce exploration results from six newly generate porphyry and related style targets located within the Apollo target area at the Guayabales project located in Caldas, Colombia. The Apollo porphyry system is a high-grade, bulk tonnage copper-silver-gold system, which owes its excellent metal endowment to an older copper-silver and gold porphyry system being overprinted by younger precious metal rich, carbonate base metal vein systems (intermediate sulphidation porphyry veins) within a magmatic, hydrothermal inter-mineral breccia body currently measuring 395 metres x 385 metres x 915 metres and open for expansion.

Details (See Table 1 and Figures 1-3)

Exploration fieldwork has identified six target areas with outcropping porphyry style mineralization which are located within a 400 metre radius of the Apollo porphyry system. These new targets were generated by geological mapping, soil sampling and most importantly the emplacement of new tracks to enable supplies and equipment to be transported to the current drill pads in the area. Two key characteristics pertinent to understanding the potential impact of the targets and their associated metal values in rock and soil are as follows:

A. Collectively, the targets consist of all the same mineralization styles observed in the Apollo system, namely early-stage porphyry style with various porphyry veinlets, inter-mineral breccia, and late stage CBM veins which host higher values of gold and silver. The copper values range between 31 ppm and 1,410 ppm and reflect leaching of copper and silver due to surface oxidation. The leaching of copper in oxides at Apollo has been observed in all oxidized material drilled from Pad 6 and Pad 7. Copper values near surface in these drill holes display very similar grades to those observed in the six outcrops outlined in this release. Gold values range from 0.18 g/t to 8.29 g/t and silver values from 0.2 g/t to 346 g/t with variation in both cases related to the mineralization styles encountered.
B. Cognizance must be taken of the surface area and 3D morphology of the Apollo porphyry system when assessing these new porphyry outcrops. The original Apollo discovery outcrop was only 10 metres in diameter and was the only exposure identified prior to the drilling of discovery hole APC-1. The discovery outcrop had gold, silver, and copper values in the ranges of 0.07 to 4.1 g/t gold, 1.9 to 29 g/t silver and 377 to 1,023 ppm copper. After the erection of multiple drill pads, another two outcrop areas were located at Apollo following the construction of various tracks which were emplaced to service the various drill rigs with equipment and supplies. There is only approximately 5% outcrop exposure at the Guayabales project due to the dense vegetation and the covering of primary rock surfaces by historic landslide fill and young volcanic ash. Furthermore, drilling at the Apollo deposit has demonstrated that the surface expression is relatively small with a maximum known diameter at present of 150 metres whereas at depth this expands quickly to a known diameter of up to 500 metres. The deposit is still open in all directions.

The following brief descriptions and data are summarized for each outcrop target:

Target 1:

This target is located 200 metres west of the Apollo outcrop area. This outcrop has dimensions of 20 metres by 3 metres and hosts early-stage porphyry mineralization as well as clast supported crackle breccia with an iron oxide matrix cement of 3% to 5% in volume. Drusy quartz veining is superimposed on the breccia. Pervasive and strong sericite alteration overprints the rock exposures. Gold grades range from 1.13 g/t to 0.34 g/t with silver ranging from 0.2 g/t to 6.6 g/t and copper in the range of 90 ppm to 224 ppm.

Target 2:

This target is located 300 metres northeast of the Apollo system, has outcrop dimensions of 120 metres by 60 metres and contains a couple of historical and shallow artisanal mines. Geological mapping has identified altered porphyry hosting angular breccia with quartz diorite clasts. The matrix of the breccia has total sulphides of up to 5% which is predominantly pyrite with some chalcopyrite. CBM veinlets overprint the breccia and trend NW and EW. Alteration is strong and defined by sericite and chlorite. Gold values range from 8.29 g/t to 1.51 g/t, silver from 10 g/t to 346 g/t and copper from 72 ppm to 362 ppm.

Target 3:

Target 3 is located 300 metres east-northeast of the Apollo system and has outcrop dimensions of 15 metres by 3 metres. The outcrop area hosts angular breccia with quartz diorite clasts with an iron oxide cement (1%-2%) after sulphides. Strong Sericite-chlorite alteration is observed. The target has subsequently been expanded to 75 metres by 170 metres by anomalous gold in soil values. Rock samples range from 0.18 g/t to 0.63 g/t gold, silver ranges from 2 g/t to 68 g/t and copper from 43 ppm to 277 ppm.

Target 4:

This target is located 250 metres east of the Apollo system with dimensions measuring 20 metres x 4 metres and host crackle breccia of diorite composition and altered porphyry rocks. Breccia cement hosts 2%-3% iron oxide after sulphide while both the porphyry and breccia units are overprinted by CBM veinlets. Strong sericite alteration is observed in the outcrop. The target has been expanded to 150 metres by 100 metres by anomalous gold in soil values. Rock samples range from 0.90 to 4.31 g/t gold, 1 g/t to 56 g/t silver and copper ranges from 125 ppm to 323 ppm. 

Target 5:

This target area is located 100 metres due east of the Apollo system and has dimensions measuring 15 metres by 10 metres. Geology observed includes altered porphyry, angular breccia and late stage CBM veinlets. The breccia matrix hosts 3%-5% iron oxides after sulphide with strong sericitic alteration. Anomalous soil sample results for gold have expanded the target area to 200 metres by 100 metres. Rock samples range from 0.56 g/t to 5.59 g/t gold, 6 g/t to 70 g/t silver and copper ranges from 477 ppm to 833 ppm.

Target 6:

This target area is located 400 metres due southeast of the Apollo system and outcrops over a 30 metre diameter area. The outcrop hosts angular, polymictic, clast supported breccia (diorite and quartz diorite) and altered porphyry with quartz veinlets. The matrix cement hosts visible sulphides of 3%-5% and consists of chalcopyrite, sphalerite, galena and pyrite. Rock samples range from 0.39 g/t to 1.07 g/t gold, 6 g/t to 20 g/t silver and copper ranges from 32 ppm to 1,410 ppm.

Update on Apollo Drilling Progress

The Phase II drilling program of 2023 is advancing on schedule with thirteen holes completed and a further six holes in the lab awaiting assay results. Since the discovery of the Apollo porphyry system was announced in June 2022, a total of 44 drill holes (approximately 18,978 metres) have been completed and assayed.

Six additional holes have been completed from the three current drill pads with assay results expected in the near term. APC-44 and APC-46 are long holes drilled in westerly direction with continuous visual mineralization of up to 425 metres. APC-41, APC-42 and APC-45 are shorter holes designed to test the contact zones between breccia and porphyry in potentially higher-grade areas. APC-47 is an exploratory hole drilled to the east from Pad 4. Assay results are expected in the near term.

The Company presently has three diamond drill rigs operating at the Apollo project and additional assay results are expected in the near term.

The Apollo target area, as defined to date by surface mapping, rock sampling and copper and molybdenum soil geochemistry, covers a 1,000 metres X 1,200 metres area, and represents a large and unusually high-grade Cu-Ag-Au porphyry system. Mineralization styles include early-stage porphyry veins, inter-mineral breccia mineralization and multiple zones of porphyry related late stage, sheeted, carbonate-base metal veins with high gold and silver grades. The Apollo target area is still expanding as the Company’s geologists have found multiple additional outcrop areas with porphyry veining, breccia, and late stage, sheeted, carbonate base metal veins.

Table 1: Assay Results for Sampling Undertaken on Targets 1 to 6 in the Apollo Target Area

Target #Sample
Type
Au (g/t)Ag (g/t)Cu (ppm)
Target 1Rock0.430.290.1
Target 1Rock0.340.2104.8
Target 1Rock0.881.8154.0
Target 1Rock0.910.6121.1
Target 1Rock1.136.6224.3
Target 2Rock1.5110.371.8
Target 2Rock7.0646.6146.0
Target 2Rock4.1078.0254.0
Target 2Rock4.5519.8309.0
Target 2Rock8.29345.6424.5
Target 2Rock6.55217.2362.0
Target 3Rock0.183.4155.9
Target 3Soil0.4367.743.0
Target 3Soil0.632.2277.0
Target 4Rock2.9735.6322.9
Target 4Soil0.901.3131.1
Target 4Soil2.8856.0198.2
Target 4Soil4.311.2124.6
Target 4Rock1.2827.9186.5
Target 5Rock5.5957.5833.1
Target 5Rock2.7069.7539.6
Target 5Rock2.4132.7507.7
Target 5Soil0.565.6477.0
Target 6Rock0.6019.81410.0
Target 6Rock0.3915.8217.3
Target 6Rock0.9516.441.9
Target 6Rock0.656.031.5
Target 6Rock1.0713.1132.3
Note: The values on the table correspond to rock chip and soil samples and should not be relied upon as being representative of average grades anticipated in any future resource estimate or mining scenario. Sample grades are uncapped and do not represent true width of the mineralization.
Rock and Soil samples have been prepared and analyzed at SGS laboratory facilities in Medellin, Colombia and Lima, Peru. Blanks, duplicates, and certified reference standards are inserted into the sample stream to monitor laboratory performance. Crush rejects and pulps are kept and stored in a secured storage facility for future assay verification. No capping has been applied to sample composites. The Company utilizes a rigorous, industry-standard QA/QC program.
Figure 1: Location and Assay Results of Rock and Soil Samples Taken From the Six Newly Generated Porphyry and Related Style Targets Surrounding the Apollo System (CNW Group/Collective Mining Ltd.)
Figure 1: Location and Assay Results of Rock and Soil Samples Taken From the Six Newly Generated Porphyry and Related Style Targets Surrounding the Apollo System (CNW Group/Collective Mining Ltd.)
Figure 2: Plan View of the Guayabales Project Highlighting the Apollo Target Area (CNW Group/Collective Mining Ltd.)
Figure 2: Plan View of the Guayabales Project Highlighting the Apollo Target Area (CNW Group/Collective Mining Ltd.)
Figure 3: Angular and Crackle Breccia in Target 6 (CNW Group/Collective Mining Ltd.)
Figure 3: Angular and Crackle Breccia in Target 6 (CNW Group/Collective Mining Ltd.)

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 $2 billion in enterprise value, Collective Mining is a copper, silver, and gold exploration company with projects in Caldas, Colombia. The Company has options to acquire 100% interests in two projects located directly within an established mining camp with ten fully permitted and operating mines.

The Company’s flagship project, Guayabales, is anchored by the Apollo target, which hosts the large-scale, bulk-tonnage and high-grade copper-silver-gold Apollo porphyry system. The Company’s near-term objective is to drill the shallow portion of the porphyry system while continuing to expansion the overall dimensions of the system, which remains open in all directions.

Management, insiders and close family and friends own nearly 45% of the outstanding shares of the Company and as a result, are fully aligned with shareholders. The Company is listed on the TSXV under the trading symbol “CNL” and on the OTCQX under the trading symbol “CNLMF”.

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 SGS laboratory facilities in Medellin, Colombia and Lima, Peru. Blanks, duplicates, and certified reference standards are inserted into the sample stream to monitor laboratory performance. Crush rejects and pulps are kept and stored in a secured storage facility for future assay verification. No capping has been applied to sample composites. The Company utilizes a rigorous, industry-standard QA/QC program.

Information Contact:

Follow Executive Chairman Ari Sussman (@Ariski) and Collective Mining (@CollectiveMini1) on Twitter.

FORWARD-LOOKING STATEMENTS

This news release contains certain forward-looking statements, including, but not limited to, statements about the drill programs, including timing of results, and Collective’s future and intentions. Wherever possible, words such as “may”, “will”, “should”, “could”, “expect”, “plan”, “intend”, “anticipate”, “believe”, “estimate”, “predict” or “potential” or the negative or other variations of these words, or similar words or phrases, have been used to identify these forward-looking statements. These statements reflect management’s current beliefs and are based on information currently available to management as at the date hereof.

Forward-looking statements involve significant risk, uncertainties, and assumptions. Many factors could cause actual results, performance, or achievements to differ materially from the results discussed or implied in the forward-looking statements. These factors should be considered carefully, and readers should not place undue reliance on the forward-looking statements. Although the forward-looking statements contained in this news release are based upon what management believes to be reasonable assumptions, Collective cannot assure readers that actual results will be consistent with these forward-looking statements. These forward-looking statements are made as of the date of this news release, and Collective assumes no obligation to update or revise them to reflect new events or circumstances, except as required by law.

Neither the TSXV nor its Regulation Services Provider (as that term is defined in the policies of the TSXV) accepts responsibility for the adequacy or accuracy of this news release.

Collective Mining Logo (CNW Group/Collective Mining Ltd.)
Collective Mining Logo (CNW Group/Collective Mining Ltd.)

SOURCE Collective Mining Ltd.

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Categories
Base Metals Collective Mining Energy Junior Mining

Collective Mining Drills 271.30 Metres at 3.35 g/t Gold Equivalent from Surface and Expands the Dimensions of the High-Grade Shallow Zone of the Apollo Porphyry System to the West

  • Hole APC-43, cut the longest continuous interval drilled to date of high-grade copper-silver-gold mineralization beginning at surface from Pad 7 at the Apollo system with results as follows:
  • Step out drill hole APC-40 also intercepted high-grade copper-silver-gold mineralization beginning from surface as follows:
  • APC-40 successfully extended the strike length of the shallow mineralization to the west of the previously known mineralization envelope and as a result has expanded the maximum known area of shallow mineralization to 150 metres X 130 metres (previously 130m X 130m).
  • The grade tenor and continuity of the intersections in APC-40 and APC-43 reflect an increased understanding of the dip and geometry of the southernmost, high-grade portion of the Apollo system. The surface dimensions of the shallow mineralization remain open for further expansion with drill holes from newly completed Pad 9 and Pad 10 now underway.
  • Five additional holes have been completed from Pad 6 and Pad 7 with assay results expected in the near term. APC-44 is the longest hole drilled to date as part of the shallow drilling program and cut more than 425 metres of continuous visual mineralization beginning at surface. APC-41 and APC-42 were shorter holes designed to test the contact between the breccia and the quartz diorite porphyry with very intense late-stage porphyry veining observed in APC-42. Assay results are expected in the near term.
  • The Company has commenced a long step out drill hole of up to 1,000 metres to the northwest from Pad 6. Presently, the hole (APC-49) is cutting mineralization, which began at surface, to its current depth of 783 metres.

Ari Sussman, Executive Chairman commented: “The latest assay results continue to demonstrate that the Apollo system has world-class grades for an outcropping bulk tonnage porphyry system. With a strong treasury now in hand due to the recently closed financing, the Company will aggressively look to expand the Apollo system with step out deep drill holes like APC-49 currently underway and by testing satellite targets within the Apollo area. More details on the revised and expanded drilling plan for the remainder of 2023 will be provided shortly.”

TORONTO, April 11, 2023 /CNW/ – Collective Mining Ltd. (TSXV: CNL) (OTCQX: CNLMF) (“Collective” or the “Company”) is pleased to announce assay results from an additional two drill holes completed from Pad 7. Drilling at Apollo in 2023 has been focused on discovering and defining shallow, high-grade mineralization below surface outcrops. With additional financing in place, the Company has expanded the aim of the program to include long step out holes. The Apollo porphyry deposit is a high-grade, bulk tonnage copper-silver-gold system, which owes its excellent metal endowment to an older copper-silver and gold porphyry system being overprinted by younger precious metal rich, carbonate base metal vein systems (intermediate sulphidation porphyry veins) within a magmatic, hydrothermal inter-mineral breccia body currently measuring 395 metres x 385 metres x 915 metres and open for expansion.

Details (See Table 1 and Figures 1-5)

The Phase II drilling program of 2023 is advancing on schedule with eleven holes completed and a further five holes in the lab awaiting assay results. Since the discovery of the Apollo porphyry system was announced in June 2022, a total of 42 drill holes (approximately 18,000 metres) have been completed and assayed. Assay results and geological observations for APC-40 and APC-43 are summarized below.

APC-40 was drilled to the southwest from Pad 7 to a maximum downhole depth of 214.55 metres and was targeted to intersect the contact zone between the mineralized breccia and the adjacent porphyry mineralization to the southwest. The hole intersected continuous and strong copper, silver and gold mineralization from surface bedrock to a depth of 169.25 metres (188 metres vertical due to topography) with the following assay results highlighted below:

  • 169.25 metres @ 2.81 g/t gold equivalent (consisting of 1.93 g/t gold, 19 g/t silver and 0.38% copper) including:

The mineralized interval starts from 1.5 metres depth with saprolite material followed by saprock and then continues with iron oxides and sulphides until a downhole depth of 18.25 metres. Below the oxide transition zone, the intercept passes into fresh rock consisting of quartz diorite breccia with a matrix of chalcopyrite (0.5% to 1.2%), pyrite (up to 1.5%) and 1% pyrrhotite. Higher-grade zones encountered from 18.25 metres and 87.85 metres downhole reflect zones with a higher percentage of sulphides plus quartz and carbonate in the matrix and reflect areas of higher permeability within the porphyry system.

APC-43 was drilled to the northwest from Pad 7 to a maximum downhole depth of 293 metres. The hole targeted the steeply dipping, southern high-grade zone as outlined by previous drilling from Pad 7 (Holes APC-36 and APC-38). The hole intersected continuous mineralization from surface outcrop to a downhole depth of 271.30 metres (282 metres vertical due to topography) with assay results as follows:

  • 271.30 metres @ 3.35 g/t gold equivalent (consisting of 2.37 g/t gold, 23 g/t silver and 0.42% copper) including:

The mineralized interval starts from surface to 3.9 metres depth within saprolite material followed by an additional 8.1 metres of saprock with iron oxides to 12 metres before transitioning into a zone with an oxidized sulphide matrix. From 19.30 metres the intercept passes into fresh rock with a sulphide composition of 0.5% to 1.3% chalcopyrite, 1.8% pyrite and pyrrhotite (up to 1.3%). The higher-grade zones commencing at 19.30 metres and 214.70 metres downhole relate to zones with a higher percentage of sulphides plus quartz and carbonate in the matrix and reflect areas of higher permeability within the porphyry system.

The grade tenor and continuity of the intersections in APC-40 and APC-43 reflect an increased understanding of the dip and geometry of the southern, high grade portion of the Apollo porphyry as gained from previous initial drilling in this area (holes APC-36 and APC-38, see press release dated March 30, 2023 for further details). Outcropping mineralization in the south dips steeply to the northwest and APC-43 has extended the mineralization another 100 metres vertically in this direction. APC-40 has extended the known area of shallow mineralization laterally and now measures 150 metres X 130 metres (previously 130 metres X 130 metres).

Outcrop mapping and sampling in the south and central portions of the system has outlined a 150 metre-by-130 metre area of known surface mineralization, which is open in all directions.  Pads 6 and 7 have been designed with the objective of understanding the styles and tenor of the shallow, high-grade mineralization from surface down to depths of up to 400 metres and Pad 6 is ideally situated for further step out holes to understand grade continuity at depth. In particular, short holes from Pad 6 (APC-41 and APC-42) have been targeted to intersect high grades at the contact zone between breccia and porphyry as previously announced in APC-29 which intersected 32 metres @ 10.48 g/t gold equivalent from a downhole depth of 112.10 metres below surface. (see press release dated January 31, 2023)

Deep drilling (APC-49) has recently commenced from Pad 6 with visuals highlighting continuous porphyry and breccia style mineralization from surface to its current depth of 783 metres. Drilling of APC-49 continues as of publication of this release and represents the longest mineralized intercept drilled to date into the Apollo system.

Five additional shallow drill holes have been completed from drill Pads 6 and 7 with fan drilling in various directions extending the outcropping mineralization to the west and northeast. Visual observations indicate continuous mineralization from surface over core lengths ranging from more than 80 metres to more than 425 metres. The Company presently has three diamond drill rigs operating at the Apollo project and additional assay results are expected in the near term.

Two new pads have recently been completed (Pad 9 and Pad 10) with drilling underway from both pads. The pad locations were chosen in order to provide more drilling options to test the potential for westerly and easterly extensions of the shallow portion of the Apollo system.

The Apollo target area, as defined to date by surface mapping, rock sampling and copper and molybdenum soil geochemistry, covers a 1,000 metres X 1,200 metres area and represents a large and unusually high-grade Cu-Ag-Au porphyry system. Mineralization styles include early-stage porphyry veins, inter-mineral breccia mineralization and multiple zones of porphyry related late stage, sheeted, carbonate-base metal veins with high gold and silver grades. The Apollo target area is still expanding as the Company’s geologists have found multiple additional outcrop areas with porphyry veining, breccia, and late stage, sheeted, carbonate base metal veins.

Table 1: Assays Results for APC-40 and APC-43

Hole #From
 (m)
To
(m)
Intercept
Interval
(m)
Au
(g/t)
Ag
(g/t)
Cu
%
Mo
%
AuEq
(g/t)*
CuEq
(%)*
APC-401.50170.75169.251.93190.380.0032.811.50
Incl**1.5018.2516.752.90160.180.0023.37
18.2530.2011.959.4580.160.0029.57
87.85132.7044.852.58300.610.0053.99
APC-43271.30271.302.37230.420.0023.351.79
Incl**19.3019.304.0260.160.0024.28
19.3051.6032.304.3990.140.0044.65
127.80144.7016.904.02170.320.0024.71
214.70256.7542.055.07120.110.0025.29
*AuEq (g/t) is calculated as follows: (Au (g/t) x 0.97) + (Ag g/t x 0.016 x 0.88) + (Cu (%) x 1.87 x 0.90)+ (Mo (%)*11.43 x 0.85) and CuEq (%) is calculated as follows: (Cu (%) x 0.90) + (Au (g/t) x 0.51 x 0.97) + (Ag (g/t) x 0.009 x 0.88)+ (Mo(%)x 6.10 x 0.85) utilizing metal prices of Cu – US$4.10/lb, Ag – $24/oz Mo – US$25.00/lb and Au – US$1,500/oz and recovery rates of 97% for Au, 88% for Ag, 85% for Mo, and 90% for Cu. Recovery rate assumptions are speculative as limited metallurgical work has been completed to date. A 0.2 g/t AuEq cut-off grade was employed with no more than 15% internal dilution. True widths are unknown, and grades are uncut.
 (**) Zone of Oxidation
Figure 1: Plan View of the Apollo Porphyry System Highlighting Drill Holes APC-40 & APC-43 (CNW Group/Collective Mining Ltd.)
Figure 1: Plan View of the Apollo Porphyry System Highlighting Drill Holes APC-40 & APC-43 (CNW Group/Collective Mining Ltd.)
Figure 2: NW – SE Cross Section Highlighting APC-43 and APC-36 (CNW Group/Collective Mining Ltd.)
Figure 2: NW – SE Cross Section Highlighting APC-43 and APC-36 (CNW Group/Collective Mining Ltd.)
Figure 3: Plan View of the Guayabales Project Highlighting the Apollo Target Area (CNW Group/Collective Mining Ltd.)
Figure 3: Plan View of the Guayabales Project Highlighting the Apollo Target Area (CNW Group/Collective Mining Ltd.)
Figure 4: Core Photo Highlights from Drill Hole APC-40 (CNW Group/Collective Mining Ltd.)
Figure 4: Core Photo Highlights from Drill Hole APC-40 (CNW Group/Collective Mining Ltd.)
Figure 5: Core Photo Highlights from Drill Hole APC-43 (CNW Group/Collective Mining Ltd.)
Figure 5: Core Photo Highlights from Drill Hole APC-43 (CNW Group/Collective Mining Ltd.)

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 $2 billion in enterprise value, Collective Mining is a copper, silver, and gold exploration company with projects in Caldas, Colombia. The Company has options to acquire 100% interests in two projects located directly within an established mining camp with ten fully permitted and operating mines.

The Company’s flagship project, Guayabales, is anchored by the Apollo target, which hosts the large-scale, bulk-tonnage and high-grade copper-silver-gold Apollo porphyry system. The Company’s near-term objective is to drill the shallow portion of the porphyry system while continuing to expansion the overall dimensions of the system, which remains open in all directions.

Management, insiders and close family and friends own nearly 45% of the outstanding shares of the Company and as a result, are fully aligned with shareholders. The Company is listed on the TSXV under the trading symbol “CNL” and on the OTCQX under the trading symbol “CNLMF”.

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 and core samples have been prepared and analyzed at SGS laboratory facilities in Medellin, Colombia and Lima, Peru. Blanks, duplicates, and certified reference standards are inserted into the sample stream to monitor laboratory performance. Crush rejects and pulps are kept and stored in a secured storage facility for future assay verification. No capping has been applied to sample composites. The Company utilizes a rigorous, industry-standard QA/QC program.

Information Contact:

Follow Executive Chairman Ari Sussman (@Ariski) and Collective Mining (@CollectiveMini1) on Twitter

FORWARD-LOOKING STATEMENTS

This news release contains certain forward-looking statements, including, but not limited to, statements about the drill programs, including timing of results, and Collective’s future and intentions. Wherever possible, words such as “may”, “will”, “should”, “could”, “expect”, “plan”, “intend”, “anticipate”, “believe”, “estimate”, “predict” or “potential” or the negative or other variations of these words, or similar words or phrases, have been used to identify these forward-looking statements. These statements reflect management’s current beliefs and are based on information currently available to management as at the date hereof.

Forward-looking statements involve significant risk, uncertainties, and assumptions. Many factors could cause actual results, performance, or achievements to differ materially from the results discussed or implied in the forward-looking statements. These factors should be considered carefully, and readers should not place undue reliance on the forward-looking statements. Although the forward-looking statements contained in this news release are based upon what management believes to be reasonable assumptions, Collective cannot assure readers that actual results will be consistent with these forward-looking statements. These forward-looking statements are made as of the date of this news release, and Collective assumes no obligation to update or revise them to reflect new events or circumstances, except as required by law.

Neither the TSXV nor its Regulation Services Provider (as that term is defined in the policies of the TSXV) accepts responsibility for the adequacy or accuracy of this news release.

Collective Mining Logo (CNW Group/Collective Mining Ltd.)
Collective Mining Logo (CNW Group/Collective Mining Ltd.)

SOURCE Collective Mining Ltd.

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Categories
Base Metals Collective Mining Energy Junior Mining

Collective Mining Drills 276.3 Metres at 2.95 g/t Gold Equivalent from Surface and Increases the Volume of the High-Grade Portion of the Apollo Porphyry System

  • Assay results for APC-39, which continued to step out to the east from Pad 6 as part of a fan pattern of drilling at the Apollo porphyry system, intersected continuous high-grade copper-silver-gold mineralization from surface as follows:
  • 276.30 metres @ 2.95 g/t gold equivalent (consisting of 2.12 g/t gold, 36 g/t silver and 0.22% copper) in drill hole APC-39 including:
  • The intersection in drill hole APC-39 was terminated short of target depth due to a technical issue while in high-grade copper and silver mineralization, with the final 7.6 metres returning 0.73% copper, 152 g/t silver and 0.46 g/t gold. APC-39 is the easternmost completed hole with assay results from Pad 6 to date and has extended the strike length of the high-grade mineralization at depth from previously announced APC-35 to 125 metres. This subzone of high-grade remains open to the east and west along strike at depth and subsequent completed holes awaiting assay results (APC-41, APC-42 and APC-44) have visually further extended the mineralization.
  • APC-36 and APC-38 are the initial drill holes completed from Pad 7 and confirm for the first time that the mineralization begins directly at surface in this area of the Apollo system. Both holes added new volume of shallow mineralization to the block model and demonstrated excellent continuity of mineralization with higher grade oxide mineralization encountered in the shallowest portions of the holes. Additionally, the holes were beneficial in working out the geometry of the system in this location confirming a steeper dip than modelled with assay results as follows:
  • 169.95 metres @ 2.15 g/t gold equivalent (consisting of 1.36 g/t gold, 19 g/t silver and 0.32% copper) in drill hole APC-38 including:
  • 110.40 metres @ 2.08 g/t gold equivalent (consisting of 1.73 g/t gold, 9 g/t silver and 0.14% copper) in drill hole APC-36 including:
  • Five additional drill holes have been completed from drill Pads 6 and 7 and all appear to have extended the area of outcropping mineralization from bedrock to downhole lengths of up to 400 metres. Assay results are pending.
  • Deep drilling has recently commenced from Pad 6 with a northwesterly hole designed to test for mineralization from surface down to a vertical depth of over 1,000 metres.

Ari Sussman, Executive Chairman commented: “The discovery of the Apollo system within the Guayabales project continues to deliver broad intervals of high-grade copper-silver-gold mineralization. Assay results from fan drilling completed to date from Pads 6 and 7 have added important tonnes of high-grade mineralization to the block model beginning directly from surface. With the fan pattern of shallow drilling from Pad 6 now complete, we are excited to have initiated our first deep hole to test the potential of the system over 1,000 metres vertical. I recently returned from visiting the Guayabales project and came away impressed by both the sheer quantity and quality of mineralization observed in outstanding holes awaiting assaying and the strong support for the Company by our stakeholders. Our team is excited to advance the project swiftly and responsibly and is confident that the Company will be an important contributor to Colombia’s bold decarbonization plans.”

TORONTO, March 30, 2023 /CNW/ – Collective Mining Ltd. (TSXV: CNL) (OTCQX: CNLMF) (“Collective” or the “Company”) is pleased to announce assay results from an additional three drill holes completed from Pad 6 and 7 which form part of the Phase II Apollo program within the Guayabales project located in Caldas, Colombia. The aim of the Phase II program is to test and define through drilling the shallow portion of the Apollo porphyry system as well as continue expanding the system through step-out and deep drilling. The Apollo porphyry deposit is a high-grade, bulk tonnage copper-silver-gold system, which owes its excellent metal endowment to an older copper-silver and gold porphyry system being overprinted by younger precious metal rich, carbonate base metal vein systems (intermediate sulphidation porphyry veins) within a magmatic, hydrothermal inter-mineral breccia body currently measuring 395 metres x 385 metres x 915 metres and open for expansion.

Details (See Table 1 and Figures 1-6)

The Phase II drilling program of 2023 is advancing on schedule with nine holes completed and a further five awaiting assay results from the lab. The aim of this program is to define the high-grade mineralization and dimensions of the Apollo porphyry system near surface while continuing to expand the size of the system through step-out drilling.  To date, a total of 40 drill holes (approximately 17,540 metres) have been completed and assayed at the Apollo target with most of the holes testing the Apollo porphyry system.

Assay results for the first three drill holes (APC-31, APC-33 and APC-35) from the 2023 Phase II program were previously announced on February 23, 2023 and March 15, 2023, respectively. Highlights include 384.7 Metres at 2.46 g/t gold equivalent in APC-31 and 359.15 metres @ 3.32 g/t gold equivalent in APC-35, with mineralization in both holes commencing from surface. Both holes intercepted high-grade oxide mineralization from surface with APC-31 cutting 42.35 metres @ 5.08 g/t gold equivalent and APC-35 cutting 35.30 metres @ 8.06 g/t gold equivalent. (see February 23, 2023 and March 15, 2023 for gold equivalent calculations)

A further three holes, APC-36, APC-38 and APC-39 have now been completed from Pads 6 and 7 with assay results and geological observations summarized below.

APC-36 was drilled steeply in an easterly direction from Pad 7 to a maximum depth of 154.1 metres (90 metres vertical). The hole was designed to test the potential for shallow mineralization located on the eastern side of the southern outcrop area and to better define the geometry of the system in this area. The hole intersected continuous mineralization from surface down to 110.4 metres with assay results as follows:

  • 110.40 metres @ 2.08 g/t gold equivalent (consisting of 1.73 g/t gold, 9 g/t silver and 0.14% copper) in drill hole APC-36 including:

The mineralized interval starts directly below overburden at 2.8 metres in saprolite and saprock material with oxidized sulphides until 19.55 metres before transitioning into fresh mineralized angular breccia rock consisting of chalcopyrite (0.2% to 0.8%), pyrite (up to 2.5%) and pyrrhotite (~1%). As expected, gold grades are significantly higher in the oxidized portion of the intercept.

APC-38 was drilled northwards from Pad 7 to a maximum depth of 183.7 metres (165 metres vertical) and was designed to test the potential for shallow, high-grade mineralization located on the northern side of the southern outcrop area. The hole intersected continuous mineralization from surface down to 169.95 metres before expectingly passing into a post mineral dyke with assay results as follows:

  • 169.95 metres @ 2.15 g/t gold equivalent (consisting of 1.36 g/t gold, 19 g/t silver and 0.32% copper) in drill hole APC-38 including:

The mineralized interval starts from surface within saprolite material followed by an additional 15.25 metres of saprock with iron oxides and sulphides to 20.95 metres before transitioning into fresh rock with a sulphide composition of 0.5% to 1.5% chalcopyrite, 1.5% pyrite and lesser pyrrhotite. Magnetite is also present in the matrix enveloped by chalcopyrite.

APC-39 was drilled steeply to the northeast from Pad 6 to a maximum depth of 284.3 metres (285 metres vertical). The hole was designed to expand upon the continuity of high-grade mineralization from surface in a northeast direction within the main Apollo porphyry system. The hole intersected continuous mineralization from surface down to its final depth of 284.3 metres with assay results as follows:

  • 276.3 metres @ 2.95 g/t gold equivalent (consisting of 2.12 g/t gold, 36 g/t silver and 0.22% copper) in drill hole APC-39 including:

The mineralized interval starts directly below overburden at 8 metres depth with saprolite material followed by oxidized saprock for an additional 33.5 metres to a depth of 41 metres. The intercept then passes into fresh rock with a sulphide composition of chalcopyrite that ranges between 0.5% and 1.5%, pyrite values up to 2.5% and lesser pyrrhotite. Overprinting carbonate base metal vein material is also present with sphalerite and galena specifically from 75.8 metres down hole and again at 185.8 metres down hole. The downhole intersection stopped in high grade copper and silver mineralization, due to technical issues with the rig, with the final 7.6 metres returning 0.73% copper, 152 g/t silver and 0.46 g/t gold. Further drilling will be undertaken in this area.

Drill hole APC-37, which was the first hole of 2023 from Pad 4, was unfortunately lost short of target depth due to a complicated fault. A new hole from Pad 4 is advancing well and is expected to be completed in the coming days.

Outcrop mapping and sampling in the south and central portions of the system has outlined a 130 metre-by-100 metre area of known surface mineralization, which is open in all directions.  Pads 6 and 7 have been designed with the objective of understanding the styles and tenor of the shallow, high-grade mineralization from surface down to depths of up to 400 metres and Pad 6 is ideally situated for further step out holes to understand grade continuity at depth. Deep drilling has recently commenced from Pad 6 with a northwesterly hole designed to test mineralization from surface down to a vertical depth of over 1,000 metres.

Visual observations from another five completed holes indicate continuous mineralization from surface over core lengths ranging from more than 80 metres to more than 400 metres. The Company presently has three diamond drill rigs operating at the Apollo project and additional assay results are expected in the near term.

Two new drill pads, numbered 9 and 10, will be completed shortly and once operational will provide more drilling options to test this expanding area of surface and shallow mineralization down to 400 metres vertical.

The Apollo target area, as defined to date by surface mapping, rock sampling and copper and molybdenum soil geochemistry, covers a 1,000 metres X 1,200 metres area and represents a large and unusually high-grade Cu-Ag-Au porphyry system. Mineralization styles include early-stage porphyry veins, inter-mineral breccia mineralization and multiple zones of porphyry related late stage, sheeted, carbonate-base metal veins with high gold and silver grades. The Apollo target area is still expanding as the Company’s geologists have found multiple additional outcrop areas with porphyry veining, breccia, and late stage, sheeted, carbonate base metal veins.

Table 1: Assays Results for APC-36, APC-38, and APC-39

Hole #From
 (m)
To
(m)
Intercept
Interval (m)
Au
(g/t)
Ag
(g/t)
Cu
%
Mo
%
AuEq
(g/t)*
CuEq
(%)*
APC-362.80113.20110.401.7390.140.0042.081.11
Incl**2.8022.3519.552.57110.110.0022.86
102.05113.2011.156.84140.280.0067.36
APC-38169.95169.951.36190.320.0022.151.15
Incl**20.9520.953.1220.100.0023.24
156.60169.9513.352.28320.630.0023.74
APC-398.00284.30276.302.12360.220.0012.951.57
Incl**8.0041.0033.004.44260.110.0014.87
75.8093.5517.752.84360.400.0013.94
185.80196.9511.153.55180.040.0013.78
*AuEq (g/t) is calculated as follows: (Au (g/t) x 0.97) + (Ag g/t x 0.016 x 0.88) + (Cu (%) x 1.87 x 0.90)+ (Mo (%)*11.43 x 0.85) and CuEq (%) is calculated as follows: (Cu (%) x 0.90) + (Au (g/t) x 0.51 x 0.97) + (Ag (g/t) x 0.009 x 0.88)+ (Mo(%)x 6.10 x 0.85) utilizing metal prices of Cu – US$4.10/lb, Ag – $24/oz Mo – US$25.00/lb and Au – US$1,500/oz and recovery rates of 97% for Au, 88% for Ag, 85% for Mo, and 90% for Cu. Recovery rate assumptions are speculative as limited metallurgical work has been completed to date. A 0.2 g/t AuEq cut-off grade was employed with no more than 15% internal dilution. True widths are unknown, and grades are uncut.
 (**) Zone of Oxidation
Figure 1: Plan View of the Apollo Porphyry System Highlighting Drill Holes APC-36, APC-38 and APC-39 (CNW Group/Collective Mining Ltd.)
Figure 1: Plan View of the Apollo Porphyry System Highlighting Drill Holes APC-36, APC-38 and APC-39 (CNW Group/Collective Mining Ltd.)
Figure 2: Plan View of the Guayabales Project Highlighting the Apollo Target Area (CNW Group/Collective Mining Ltd.)
Figure 2: Plan View of the Guayabales Project Highlighting the Apollo Target Area (CNW Group/Collective Mining Ltd.)
Figure 3: Core Photo Highlights from Drill Hole APC-36 (CNW Group/Collective Mining Ltd.)
Figure 3: Core Photo Highlights from Drill Hole APC-36 (CNW Group/Collective Mining Ltd.)
Figure 4: Core Photo Highlights from Drill Hole APC-38 (CNW Group/Collective Mining Ltd.)
Figure 4: Core Photo Highlights from Drill Hole APC-38 (CNW Group/Collective Mining Ltd.)
Figure 5: Core Photo Highlights from Drill Hole APC-39 (CNW Group/Collective Mining Ltd.)
Figure 5: Core Photo Highlights from Drill Hole APC-39 (CNW Group/Collective Mining Ltd.)
Figure 6: Brecciated porphyry mineralization. Note the mineralized quartz porphyry B veins being overprinted by mineralized angular breccia. (CNW Group/Collective Mining Ltd.)
Figure 6: Brecciated porphyry mineralization. Note the mineralized quartz porphyry B veins being overprinted by mineralized angular breccia. (CNW Group/Collective Mining Ltd.)

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 $2 billion in enterprise value, Collective Mining is a copper, silver, and gold exploration company with projects in Caldas, Colombia. The Company has options to acquire 100% interests in two projects located directly within an established mining camp with ten fully permitted and operating mines.

The Company’s flagship project, Guayabales, is anchored by the Apollo target, which hosts the large-scale, bulk-tonnage and high-grade copper-silver-gold Apollo porphyry system. The Company’s near-term objective is to drill the shallow portion of the porphyry system while continuing to expansion the overall dimensions of the system, which remains open in all directions.

Management, insiders and close family and friends own nearly 45% of the outstanding shares of the Company and as a result, are fully aligned with shareholders. The Company is listed on the TSXV under the trading symbol “CNL” and on the OTCQX under the trading symbol “CNLMF”.

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 and core samples have been prepared and analyzed at SGS laboratory facilities in Medellin, Colombia and Lima, Peru. Blanks, duplicates, and certified reference standards are inserted into the sample stream to monitor laboratory performance. Crush rejects and pulps are kept and stored in a secured storage facility for future assay verification. No capping has been applied to sample composites. The Company utilizes a rigorous, industry-standard QA/QC program.

Information Contact:

Follow Executive Chairman Ari Sussman (@Ariski) and Collective Mining (@CollectiveMini1) on Twitter

FORWARD-LOOKING STATEMENTS

This news release contains certain forward-looking statements, including, but not limited to, statements about the drill programs, including timing of results, and Collective’s future and intentions. Wherever possible, words such as “may”, “will”, “should”, “could”, “expect”, “plan”, “intend”, “anticipate”, “believe”, “estimate”, “predict” or “potential” or the negative or other variations of these words, or similar words or phrases, have been used to identify these forward-looking statements. These statements reflect management’s current beliefs and are based on information currently available to management as at the date hereof.

Forward-looking statements involve significant risk, uncertainties, and assumptions. Many factors could cause actual results, performance, or achievements to differ materially from the results discussed or implied in the forward-looking statements. These factors should be considered carefully, and readers should not place undue reliance on the forward-looking statements. Although the forward-looking statements contained in this news release are based upon what management believes to be reasonable assumptions, Collective cannot assure readers that actual results will be consistent with these forward-looking statements. These forward-looking statements are made as of the date of this news release, and Collective assumes no obligation to update or revise them to reflect new events or circumstances, except as required by law.

Neither the TSXV nor its Regulation Services Provider (as that term is defined in the policies of the TSXV) accepts responsibility for the adequacy or accuracy of this news release.

SOURCE Collective Mining Ltd.

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View original content to download multimedia: http://www.newswire.ca/en/releases/archive/March2023/30/c6791.html

Categories
Base Metals Collective Mining Energy Junior Mining Precious Metals

Collective Mining Drills 359.15 Metres at 3.32 g/t Gold Equivalent from Surface, Including 35.30 Metres at 8.06 g/t Gold Equivalent in Oxides at the Apollo Porphyry System

  • Assay results for two holes APC-33 and APC-35, intended to test the mineralized outcrop of the Apollo porphyry system, intersected significant continuous high-grade copper-silver-gold mineralization from surface as follows:
  • The intersection in drill hole APC-35 is the highest grade (grams X metres) hole drilled to date at the Apollo porphyry system.
  • Both holes terminated while still in strong mineralization at over 350 metres vertical depth. Deeper drilling is planned as part of the 2023 Phase II program.
  • Significant and continuous copper mineralization was intersected in both drill holes beginning directly below the oxide zone of mineralization and continuing to the end of the holes.
  • Four additional drill holes have been completed from drill Pads 6 and 7 with all four holes appearing to have intersected continuous mineralization from bedrock to downhole lengths of up to 275 metres. Assay results are pending.
  • Outcrop mapping and sampling in the south and central portions of the Apollo porphyry system has outlined a 130 metres X 130 metres area of known surface mineralization which is open in all directions. Two new pads (9 and 10) are under construction and once operational will provide more drilling options to test this expanding area of surface and shallow mineralization.

Ari Sussman, Executive Chairman commented: “The Apollo deposit continues to demonstrate that it is in a rare class of discoveries combining both high-grades of copper, silver and gold hosted within a bulk tonnage porphyry system. Surprises through drilling continue to be positive with APC-35 being the highest grade intercept at the project to date. Importantly, the hole began and ended in two separate high-grade subzones of mineralization. Once the shallow portion of the drill program is completed in the coming weeks, we will immediately begin drilling significantly longer holes to test the full potential of the system from surface to depth. Assay turnaround continues to be quick and more results are expected in the near term.”

TORONTO, March 15, 2023 /CNW/ – Collective Mining Ltd. (TSXV: CNL) (OTCQX: CNLMF) (“Collective” or the “Company”) is pleased to announce assay results from an additional two drill holes completed from Pad 6 as part of the Phase II program at the Guayabales project located in Caldas, Colombia. The aim of the Phase II program is to test and define through drilling the shallow portion of the Apollo porphyry system as well as continue expanding the system through step-out drilling. The Apollo porphyry deposit is a high-grade, bulk tonnage copper-silver-gold system, which owes its excellent metal endowment to an older copper-silver and gold porphyry system being overprinted by younger precious metal rich, carbonate base metal vein systems (low and intermediate sulphidation porphyry veins) within a magmatic, hydrothermal intermineral breccia body currently measuring 395 metres x 385 metres x 915 metres and open for expansion.

To watch a short video of David Reading, Special Advisor to Collective Mining, speak about the assay results announced today, please click here.

Details (See Table 1 and Figures 1-3)

The Phase II drilling program of 2023 is advancing on schedule with seven holes completed and a further three in progress. The aim of this program is to define the high-grade mineralization and dimensions of the Apollo porphyry system near surface while continuing to expand the size of the system through step-out drilling.  To date, a total of 34 drill holes (approximately 16,000 metres) have been completed and assayed at the Apollo target with the majority of the holes testing the Apollo porphyry system.

Assay results for the first drill hole (APC-31) from the 2023 Phase II program was announced on February 23, 2023 and intersected 384.7 Metres at 2.46 g/t Gold Equivalent from surface which included high-grade oxide mineralization of 42.35 metres averaging 5.08 g/t gold equivalent.

A further two holes, APC-33 and APC-35 have now been completed from Pad 6 with assay results and geological observations summarized below.

APC-35 was drilled steeply to the northwest from Pad 6 to a maximum depth of 366.15 metres (350 metres vertical). The hole was designed to test the potential for shallow, high-grade mineralization located 50 metres west of APC-31. The hole intersected continuous mineralization from surface down to its final depth where it was terminated while still in strong mineralization (final 3.45m averaging 1.11 g/t gold equivalent). APC-35 is the highest-grade mineralization (grams X metres) reported from drilling to date as follows:

  • 359.15 metres @ 3.32 g/t gold equivalent (consisting of 1.84 g/t gold, 48 g/t silver and 0.48% copper) including:

The mineralized interval starts directly below overburden at 7 metres and into saprolite and oxide material until 42.30 metres before transitioning into fresh mineralized angular breccia rock consisting of chalcopyrite (0.2% to 1.5%), pyrite (1% to 2%) and some pyrrhotite (~1%). The mineralization is overprinted by carbonate-base metal veins containing sphalerite and galena and high grades of gold particularly from 318.30 metres downhole. Gold grades are significantly higher in the oxidized portion of the intercept while copper and silver grades are consistently high throughout the whole intercept below the oxidized zone.

APC-33 was drilled steeply to the north from Pad 6 to a maximum depth of 381.35 metres (360 metres vertical). The hole was also designed to test the potential for shallow, high grade mineralization located 50 metres east of APC-31. The hole intersected continuous mineralization from surface down to its final depth where it was terminated while still in strong mineralization (last 4.44 metres grade 1.7 g/t gold equivalent) and averaged:

  • 374.70 metres @ 2.22 g/t gold equivalent (consisting of 0.85 g/t gold, 53 g/t silver and 0.34% copper) including:

The mineralized interval starts directly below overburden at 6.65 metres and into saprolite and oxide material until 49.50 metres before transitioning into fresh mineralized angular breccia rock consisting of chalcopyrite (0.2% to 1.2%), pyrite (1% to 2.5%) and some pyrrhotite (~1%). The sulphides fill the breccia matrix and are surrounded by clasts of quartz diorite and diorite. The mineralization is overprinted by carbonate-base metal veins containing sphalerite and galena. Gold grades are significantly higher in the oxidized portion of the intercept where copper grades are depleted.

Outcrop mapping and sampling in the south and central portions of the system has outlined a 130 metre-by-130 metre area of known surface mineralization, which is open in all directions.  Pads 6 and 7 have been designed with the objective of understanding the styles and tenor of the shallow, high-grade mineralization from surface down to depths of up to 400 metres. Visual observations from another four completed holes indicate continuous intercepts from surface over core lengths ranging from more than 100 metres to more than 275 metres. The Company presently has three diamond drill rigs operating at the Apollo project and additional assay results are expected in the near term.

Two new drill pads, numbered 9 and 10, are under construction to provide further drilling options to test and expand upon the area which the Apollo porphyry system outcrops at surface.

The Apollo target area, as defined to date by surface mapping, rock sampling and copper and molybdenum soil geochemistry, covers a 1,000 metres X 1,200 metres area, and represents a large and unusually high-grade Cu-Ag-Au porphyry system. Mineralization styles include early-stage porphyry veins, inter-mineral breccia mineralization and multiple zones of porphyry related late stage, sheeted, carbonate-base metal veins with high gold and silver grades. The Apollo target area is still expanding as the Company’s geologists find more outcrop areas with porphyry veining, breccia, and late stage, sheeted, carbonate base metal veins.

Table 1: Assays Results for APC-33 and APC-35

HoleIDFrom
 (m)
To
(m)
Intercept
Interval
(m)
Au
(g/t)
Ag
(g/t)
Cu
%
Mo
%
AuEq
(g/t)*
CuEq(%)**
APC-336.65381.35374.700.85530.340.0022.221.21
Inlc**6.6549.5042.853.87400.120.0014.50
APC-357.00366.15359.151.84480.480.0023.321.82
Incl**7.0042.3035.307.96220.090.0018.06
318.30366.1547.855.47190.050.0025.58
*AuEq (g/t) is calculated as follows: (Au (g/t) x 0.95) + (Ag g/t x 0.016 x 0.95) + (Cu (%) x 1.83 x 0.95)+ (Mo (%)*9.14 x 0.95) and CuEq (%) i:  (Cu (%) x 0.95) + (Au (g/t) x 0.51 x 0.95) + (Ag (g/t) x 0.01 x 0.95)+ (Mo(%)x 3.75 x 0.95) CuEq (%) is calculated as follows:  (Cu (%) x 0.95) + (Au (g/t) x 0.51 x 0.95) + (Ag (g/t) x 0.01 x 0.95)+ (Mo(%)x 5.0 x 0.95). utilizing metal prices of Cu – US$4.00/lb, Ag – $24/oz Mo US$20.00/lb and Au – US$1,500/oz and recovery rates of 95% for Au, Ag, Mo and Cu. Recovery rate assumptions are speculative as no metallurgical work has been completed to date
** A 0.2 g/t AuEq cut-off grade was employed with no more than 15% internal dilution. True widths are unknown, and grades are uncut
Oxidation zone**
Figure 1: Plan View of the Apollo Porphyry System Highlighting Drill Holes APC-33 & APC-35 (CNW Group/Collective Mining Ltd.)
Figure 1: Plan View of the Apollo Porphyry System Highlighting Drill Holes APC-33 & APC-35 (CNW Group/Collective Mining Ltd.)
Figure 2: Core Photo Highlights and Cross Section for Drill Holes APC-33 and APC-35 (CNW Group/Collective Mining Ltd.)
Figure 2: Core Photo Highlights and Cross Section for Drill Holes APC-33 and APC-35 (CNW Group/Collective Mining Ltd.)
Figure 3: Plan View of the Guayabales Project Highlighting the Apollo Target Area (CNW Group/Collective Mining Ltd.)
Figure 3: Plan View of the Guayabales Project Highlighting the Apollo Target Area (CNW Group/Collective Mining Ltd.)

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 $2 billion in enterprise value, Collective Mining is a copper, silver and gold exploration company with projects in Caldas, Colombia. The Company has options to acquire 100% interests in two projects located directly within an established mining camp with ten fully permitted and operating mines.

The Company’s flagship project, Guayabales, is anchored by the Apollo target, which hosts the large-scale, bulk-tonnage and high-grade copper-silver-gold Apollo porphyry system. The Company’s near-term objective is to drill the shallow portion of the porphyry system while continuing to expansion the overall dimensions of the system, which remains open in all directions.

Management, insiders and close family and friends own nearly 52% of the outstanding shares of the Company and as a result, are fully aligned with shareholders. The Company is listed on the TSXV under the trading symbol “CNL” and on the OTCQX under the trading symbol “CNLMF”.

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 and core samples have been prepared and analyzed at SGS laboratory facilities in Medellin, Colombia and Lima, Peru. Blanks, duplicates, and certified reference standards are inserted into the sample stream to monitor laboratory performance. Crush rejects and pulps are kept and stored in a secured storage facility for future assay verification. No capping has been applied to sample composites. The Company utilizes a rigorous, industry-standard QA/QC program.

Information Contact:

Follow Executive Chairman Ari Sussman (@Ariski) and Collective Mining (@CollectiveMini1) on Twitter

FORWARD-LOOKING STATEMENTS

This news release contains certain forward-looking statements, including, but not limited to, statements about the drill programs, including timing of results, and Collective’s future and intentions. Wherever possible, words such as “may”, “will”, “should”, “could”, “expect”, “plan”, “intend”, “anticipate”, “believe”, “estimate”, “predict” or “potential” or the negative or other variations of these words, or similar words or phrases, have been used to identify these forward-looking statements. These statements reflect management’s current beliefs and are based on information currently available to management as at the date hereof.

Forward-looking statements involve significant risk, uncertainties, and assumptions. Many factors could cause actual results, performance, or achievements to differ materially from the results discussed or implied in the forward-looking statements. These factors should be considered carefully, and readers should not place undue reliance on the forward-looking statements. Although the forward-looking statements contained in this news release are based upon what management believes to be reasonable assumptions, Collective cannot assure readers that actual results will be consistent with these forward-looking statements. These forward-looking statements are made as of the date of this news release, and Collective assumes no obligation to update or revise them to reflect new events or circumstances, except as required by law.

Neither the TSXV nor its Regulation Services Provider (as that term is defined in the policies of the TSXV) accepts responsibility for the adequacy or accuracy of this news release.

SOURCE Collective Mining Ltd.

Cision
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View original content to download multimedia: http://www.newswire.ca/en/releases/archive/March2023/15/c7360.html

Categories
Base Metals Collective Mining Energy Junior Mining Precious Metals

Goldshore Intersects Multiple New Parallel Shears Increasing Width of QES Zone by Over 100 meters – Including 1.33 g/t Au over 54.45m

Vancouver, British Columbia–(Newsfile Corp. – March 14, 2023) – Goldshore Resources Inc. (TSXV: GSHR) (OTCQB: GSHRF) (FSE: 8X00) (“Goldshore” or the “Company“), is pleased to announce assay results from its ongoing 100,000-meter drill program at the Moss Lake Project in Northwest Ontario, Canada (the “Moss Gold Project“).

Highlights:

  • Results from seven holes in-filling the QES Zone have confirmed wide zones of gold mineralization containing multiple, closely spaced high grade shears in previously poorly drilled volumes with best intercepts of:
  • Additionally, these holes intersected parallel mineralized shears at shallow depths south of the main QES zone which are open along strike and expand the cumulative width of the QES Zone by over 100m to 620m. Best intercepts include:

President and CEO Brett Richards stated: As previously illustrated throughout the last 12 months of publishing drill results, these results continue to support our thesis that the size and scale of the Moss Gold Project will be large enough to support a material and meaningful update to the mineral resource estimate, which is expected in April 2023, followed by a preliminary economic assessment on the updated resource. We continue to find additions to the resource on step out holes laterally and along strike from the historic resource profile, and QES continues to widen with continued mineralization to be tested to make it even wider. We look forward to seeing the impact of these additions to the resource model.”

Technical Overview

Figure 1 shows the better intercepts in plan view and Figure 2 is a typical section through hole MQD-22-100 and -104. Table 1 shows the significant intercepts. Table 2 shows the drill hole locations.

Figure 1: Drill plan showing best of several +1 g/t Au intercepts relative to the current Mineral Resource and highlighting the additional shears.

To view an enhanced version of this graphic, please visit:
https://images.newsfilecorp.com/files/8051/158334_fe74b843e49a68d9_002full.jpg

Figure 2: Drill section through MQD-22-100 and -104 relative to the current Mineral Resource and highlighting the additional shears and potential to significantly deepen the open pit shell.

To view an enhanced version of this graphic, please visit:
https://images.newsfilecorp.com/files/8051/158334_fe74b843e49a68d9_003full.jpg

These most recent results continue to build on the successful winter infill and expansion program at the QES Zone. The robust widths and consistent gold grades in all seven holes provide strong confirmation of the geological interpretation, and significantly increase the resolution of data in hitherto poorly defined volumes.

Holes MQD-22-098, -100, -102 and -103 were focused on closing gaps in the existing drill pattern at shallower elevations. All four holes intercepted a tightly spaced set of narrow, high grade shear zones within a broad envelope of strongly altered granodiorite.

Holes MQD-22-099, -101 and -104 were stepped back to the southeast to test the deeper portion of the eastern end of the QES Zone. These holes have defined the true width of the high- and low-grade mineralized domains in an area of widely spaced and partially sampled historical drilling. In addition to these deeper intercepts on the main QES shear zone, all three holes generated significant high-grade intercepts at shallow depths which define a series of parallel mineralized shears in sericite-hematite altered volcanics and narrow diorite intrusive bodies 200m to the south of the main QES Zone.

Figure 3: Drill core from 112-123m (1m @ 22.1g/t Au) in MQD-22-100 highlighting a mineralized quartz-rhodochrosite vein within the sheared, altered intrusion. Note that this photo is not intended to be representative of broader mineralization on the Moss Lake Gold Project.

To view an enhanced version of this graphic, please visit:
https://images.newsfilecorp.com/files/8051/158334_fe74b843e49a68d9_004full.jpg

Pete Flindell, VP Exploration for Goldshore, said “These results confirm our belief that the Moss Gold deposit is wider and deeper than previously thought – now filling a 600-700-meter-wide corridor – and that there are many more shears hosting high-grade gold mineralization. This will assist our goal of expanding the mineral resource and improving its quality in April 2023.”

Table 1: Significant downhole gold intercepts

HOLEIDFROMTOLENGTH
(m)
TRUE WIDTH
(m)
CUT GRADE
(g/tAu)
UNCUT GRADE
(g/tAu)
MQD-22-098122.00124.002.001.40.320.32
245.00279.8034.8026.30.650.65
including254.90258.954.053.02.682.68
and269.00273.004.003.01.681.68
298.00364.0066.0050.90.590.59
including307.00315.008.006.11.031.03
397.00407.0010.007.90.380.38
529.00533.004.003.30.370.37
MQD-22-09918.0020.002.001.30.450.45
183.35205.5522.2015.50.510.51
256.00258.002.001.40.510.51
280.00285.005.003.60.320.32
294.30309.0014.7010.80.510.51
379.00394.0015.0011.30.450.45
including382.00385.003.002.31.231.23
410.00412.002.001.50.320.32
425.00435.5010.508.00.330.33
461.65469.607.956.20.390.39
540.90548.107.205.70.510.51
555.90557.952.051.60.380.38
576.00579.303.302.60.350.35
591.15635.4544.3035.81.061.06
including594.00621.1027.1021.91.551.55
MQD-22-10099.40104.004.602.80.310.31
119.05130.2511.207.02.232.23
168.05189.8521.8014.10.540.54
including187.60189.852.251.52.302.30
208.40393.95185.55128.70.480.48
including287.80290.002.201.51.021.02
and310.05314.003.952.81.071.07
and335.00339.904.903.51.131.13
and346.25359.0012.759.11.671.67
409.00418.009.006.70.360.36
436.00456.2520.2515.20.740.74
including439.00449.0010.007.51.091.09
496.00500.004.003.00.320.32
MQD-22-10191.0093.602.601.75.905.90
179.80196.6016.8011.60.570.57
including192.55194.802.251.62.612.61
215.05272.0056.9540.30.390.39
including231.90234.552.651.91.291.29
325.00357.0032.0023.40.410.41
including345.10347.602.501.81.761.76
375.00379.154.153.10.420.42
425.85447.0021.1515.90.310.31
464.40467.002.602.00.330.33
502.00517.5015.5012.00.370.37
528.00562.2034.2026.70.480.48
including533.10539.306.204.81.041.04
614.65676.0061.3549.50.810.81
including623.35638.0014.6511.81.181.18
and643.00657.7514.7511.91.001.00
and661.80668.006.205.01.501.50
710.90714.954.053.30.340.34
728.05737.159.107.50.300.30
745.80750.004.203.50.480.48
MQD-22-10223.8029.505.704.10.340.34
166.50170.804.303.20.350.35
193.05274.0080.9563.70.740.74
including205.00209.004.003.11.731.73
and246.10266.1020.0016.01.431.43
291.00298.607.606.20.340.34
324.00352.0028.0023.00.690.69
including329.00334.605.604.62.222.22
369.00372.003.002.50.460.46
MQD-22-103114.45134.0019.5513.50.310.31
140.05158.0017.9512.60.410.41
168.40178.9510.557.50.750.75
190.00267.0077.0056.80.710.71
including203.00219.0016.0011.61.431.43
and262.10264.652.551.95.105.10
279.00284.655.654.31.711.71
including280.35282.952.602.03.213.21
435.90449.0013.1010.40.630.63
MQD-22-104112.70121.208.505.82.412.41
220.80236.8516.0511.60.700.70
249.00252.203.202.30.470.47
290.90296.655.754.30.640.64
473.05483.009.957.90.460.46
495.80521.0025.2020.10.310.31
533.80557.0023.2018.70.590.59
including544.00547.003.002.41.521.52
568.00575.507.506.10.940.94
593.00713.65120.65101.20.860.86
including614.00628.2014.2011.81.061.06
and657.00711.4554.4546.11.331.33
726.00731.105.104.40.520.52
755.70760.454.754.10.560.56
771.05778.857.806.70.310.31

Intersections calculated above a 0.3 g/t Au cut off with a top cut of 30 g/t Au and a maximum internal waste interval of 10 metres. Bordered intervals are intersections calculated above a 1.0 g/t Au cut off. Intervals in bold are those with a grade thickness factor exceeding 20 gram x metres / tonne gold. True widths are approximate and assume a subvertical body.

Table 2: Location of drill holes in this press release

HOLEEASTNORTHRLAZIMUTHDIPEOH
MQD-22-098669,8295,379,161431337°-49°651
MQD-22-099670,6645,379,431433336°-50°750
MQD-22-100670,4775,379,624428335°-55°525
MQD-22-101670,6065,379,384441337°-51°750
MQD-22-102670,3985,379,573428336°-45°402
MQD-22-103670,1625,379,469428336°-50°552
MQD-22-104670,5285,379,315441339°-50°801

Analytical and QA/QC Procedures

All samples were sent to ALS Geochemistry in Thunder Bay for preparation and analysis was performed in the ALS Vancouver analytical facility. ALS is accredited by the Standards Council of Canada (SCC) for the Accreditation of Mineral Analysis Testing Laboratories and CAN-P-4E ISO/IEC 17025. Samples were analyzed for gold via fire assay with an AA finish (“Au-AA23”) and 48 pathfinder elements via ICP-MS after four-acid digestion (“ME-MS61”). Samples that assayed over 10 ppm Au were re-run via fire assay with a gravimetric finish (“Au-GRA21”).

In addition to ALS quality assurance / quality control (“QA/QC”) protocols, Goldshore has implemented a quality control program for all samples collected through the drilling program. The quality control program was designed by a qualified and independent third party, with a focus on the quality of analytical results for gold. Analytical results are received, imported to our secure on-line database and evaluated to meet our established guidelines to ensure that all sample batches pass industry best practice for analytical quality control. Certified reference materials are considered acceptable if values returned are within three standard deviations of the certified value reported by the manufacture of the material. In addition to the certified reference material, certified blank material is included in the sample stream to monitor contamination during sample preparation. Blank material results are assessed based on the returned gold result being less than ten times the quoted lower detection limit of the analytical method. The results of the on-going analytical quality control program are evaluated and reported to Goldshore by Orix Geoscience Inc.

About Goldshore

Goldshore is an emerging junior gold development company, and owns 100% of the Moss Gold Project located in Ontario. Wesdome is currently a large shareholder of Goldshore with an approximate 22% equity position in the Company. Well-financed and supported by an industry-leading management group, board of directors and advisory board, Goldshore is positioned to advance the Moss Gold Project through the next stages of exploration and development.

Peter Flindell, P.Geo., MAusIMM, MAIG, Vice President – Exploration of the Company, a qualified person under NI 43-101 has approved the scientific and technical information contained in this news release.

Neither the TSXV nor its Regulation Services Provider (as that term is defined in the policies of the TSXV) accepts responsibility for the adequacy or accuracy of this release.

For More Information – Please Contact:

Brett A. Richards
President, Chief Executive Officer and Director
Goldshore Resources Inc.

P. +1 604 288 4416 M. +1 905 449 1500
E. brichards@goldshoreresources.com
W. www.goldshoreresources.com

Facebook: GoldShoreRes | Twitter: GoldShoreRes | LinkedIn: goldshoreres

Cautionary Note Regarding Forward-Looking Statements

This news release contains statements that constitute “forward-looking statements.” Such forward-looking statements involve known and unknown risks, uncertainties and other factors that may cause the Company’s actual results, performance or achievements, or developments to differ materially from the anticipated results, performance or achievements expressed or implied by such forward-looking statements. Forward-looking statements are statements that are not historical facts and are generally, but not always, identified by the words “expects,” “plans,” “anticipates,” “believes,” “intends,” “estimates,” “projects,” “potential” and similar expressions, or that events or conditions “will,” “would,” “may,” “could” or “should” occur.

Forward-looking statements in this news release include, among others, statements relating to expectations regarding the exploration and development of the Moss Lake Gold Project, the release of an updated mineral resource estimate and preliminary economic assessment, and other statements that are not historical facts. By their nature, forward-looking statements involve known and unknown risks, uncertainties and other factors which may cause our actual results, performance or achievements, or other future events, to be materially different from any future results, performance or achievements expressed or implied by such forward-looking statements. Such factors and risks include, among others: the Company may require additional financing from time to time in order to continue its operations which may not be available when needed or on acceptable terms and conditions acceptable; compliance with extensive government regulation; domestic and foreign laws and regulations could adversely affect the Company’s business and results of operations; the stock markets have experienced volatility that often has been unrelated to the performance of companies and these fluctuations may adversely affect the price of the Company’s securities, regardless of its operating performance; and the impact of COVID-19.

The forward-looking information contained in this news release represents the expectations of the Company as of the date of this news release and, accordingly, is subject to change after such date. Readers should not place undue importance on forward-looking information and should not rely upon this information as of any other date. The Company undertakes no obligation to update these forward-looking statements in the event that management’s beliefs, estimates or opinions, or other factors, should change.

Categories
Base Metals Collective Mining Energy Junior Mining Precious Metals

Collective Mining Intersects 55.25 Metres at 1.91 g/t Gold Equivalent in Step Out Drilling at the Olympus Target

  • Reconnaissance underground step-out drilling for the three hole Phase II program at the Olympus target has intercepted continuous mineralization with highlight assay results including:
  • Drill hole OLCU-2 has extended the known strike of the Olympus system by 150 metres to the southwest of drill hole OLCC-4 from the Phase I program in H1 2022 with previously announced results including:
  • As a result of OLCU-2, the dimensions of the Olympus system now measure 600 metres by 400 metres and remains open to the east, west, north and to depth for further expansion.
  • Drill hole OLCU-2 is located only 280 metres to the northwest of the currently known northern boundary of the Apollo porphyry system which was intercepted in step out hole APC-17, which returned 547.65 metres at 1.03 g/t gold equivalent (see press release November 29, 2022). Porphyry mineralization observed in drill core at Olympus raise the possibility that the Apollo porphyry system might continue at depth below Olympus. Future deep drilling will test this concept.
  • Multiple zones of NW trending sheeted late-stage porphyry related carbonate base metal veins have now been mapped and/or drilled from Aris Mining’s multi-million-ounce Marmato mine through the ME, Apollo and Olympus targets respectively covering a strike length of approximately three kilometres.
  • Presently, the Company has three diamond drill rigs turning at the Apollo porphyry system focused on testing the southern portion of the system where it daylights at surface. On February 23, 2023, the Company reported initial assay results from its first hole (APC-31) drilled in 2023 and confirmed that high-grade mineralization extends to surface with assay results as follow:
  • An additional seven holes have been completed at Apollo and have all appeared to have cut continuous mineralization from surface down to depths of up to 375 metres. Assay results for holes APC-33 and APC-35 are expected in the near term.

Ari Sussman, Executive Chairman commented: “Inspection of drill core and underground sampling at the Olympus target point to the potential for a mineralized porphyry system at depth. It is entirely conceivable that below Olympus we might find the Apollo porphyry system’s down plunge extension or another porphyry intrusion altogether. This model is directly comparable to the Marmato mine located less than 4 kilometres away and along the same mountain slope. Marmato hosts a CBM vein system similar to Olympus, which lies atop a porphyry at depth. We are truly blessed with remarkable geology. Hydrothermal fluid systems this robust in both nature and scale are exceedingly rare globally.”

TORONTO, March 7, 2023 /CNW/ – Collective Mining Ltd. (TSXV: CNL) (OTCQX: CNLMF) (“Collective” or the “Company”) is pleased to announce assay results from three underground drill holes completed at the Olympus target which forms part of the Company’s Guayabales project located in Caldas, Colombia. Mineralization at Olympus is characterized by zones of sheeted, late-stage carbonate base metal (“CBM”) veins and veinlets impregnating either porphyry diorite host rock or schist host rock. The Olympus target area measures 600 metres north-south by 400 metres east-west. Previously, the Company announced drilling results from drilling in the northern portion of the Olympus target area which included discovery hole OLCC-3 which averaged 301.9 metres @ 1.11 g/t AuEq (see press release dated March 15, 2022).

Details (See Table 1 and Figures 1 and 2)

Assay results for underground drill holes OLCU-1 to OLCU-3 are announced in this press release. All three holes were drilled from an underground chamber constructed within shallow ancestral underground workings located approximately 280 metres to the west and northwest of the current known northern extent of the Apollo porphyry deposit.

Assay results and geological observations are summarized below.

OLCU-2 was drilled northeastwards at a shallow dip below old workings from the underground chamber to a maximum depth of 331.8 metres. The hole was drilled orthogonally to CBM veins mapped in higher levels within the historical workings. The hole intersected two zones of polymetallic CBM veins and veinlets returning the following results:

  • 55.25 metres @ 1.91 g/t gold equivalent from 172.6 metres including 7.45 metres @ 8.69 g/t gold equivalent, and
  • 47.17 metres @ 0.94 g/t gold equivalent from 284.15 metres downhole.

Both mineralized zones consist of multiple polymetallic CBM veins and veinlets hosting pyrite, sphalerite, chalcopyrite, and galena. The sheeted vein systems are associated with intense sericite alteration and overprint older, potassic altered porphyry diorites containing magnetite and quartz-sulphide, porphyry veins.

Drill hole OLCU-3 was drilled in a NNE direction at a shallow dip from the underground chamber to a final depth of 290.2 metres and intersected a CBM vein zone with similar characteristics to those described in OLCU-2 and grading 0.81 g/t gold equivalent over 17.45 metres. The CBM zone is associated with intense sericite alteration and this mineralized system overprints potassically altered, porphyry diorite.

Hole OLCU-1 failed to intersect the targeted CBM zone due to drilling problems related to faulting and a historical mining cavity.

The current underground drilling and previously reported Olympus drill results (all summarized in Figure 1) outline multiple CBM vein zones covering an area of 600 metres north-south by- 400 metres east-west which is open to the NW and SE as the vein systems strike in this direction.

The CBM vein intercepts in OLCU-2 are located only 280 metres to the northwest of the known extent of Apollo porphyry system mineralization intercepted in step out drill hole APC-17. Drill hole APC-17 was an important step out hole which significantly extended the size of the Apollo deposit northwards returning a long intercept of 547.65 metres @ 1.03 g/t gold equivalent (see press release date November 29, 2022). This hole was terminated at 912.8 metres due to rig capacity limitations and bottomed in strong mineralization with the final 2.75 metres averaging 1.56 g/t gold and 9 g/t silver.

Interpretation work undertaken by the Company’s geological team has, to date, identified three zones of sheeted CBM vein systems which overprint both the inter-mineral breccia within the Apollo porphyry system and then continue to the northwest through the Olympus system. Additionally, porphyry style mineralization has been observed throughout Olympus drill core and underground mapping. As a result, it is entirely possible that the inter-mineral breccia making up the Apollo porphyry system (which plunges to depth as the system is traced northwards) or another porphyry intrusion might lie below the Olympus vein system. This model is directly analogous to the Marmato mine located approximately three kilometres along strike to the southeast where a CBM vein system lies above a porphyry system (Marmato Deeps).

Table 1: Assays Results for holes OLCU-1 to OLCU-3

Hole #From (m)To (m)Intercept
(m)
Au (g/t)Ag (g/t)Cu %Mo %AuEq
(g/t)*
OLCU-1NSV*
OLCU-25.906.400.503.42420.130.0047.18
133.55134.250.701.511800.130.0024.41
OLCU-2172.60227.8555.251.75110.020.0031.91
Incl.205.00206.601.603.01200.020.0103.29
207.60208.801.202.89100.010.0062.97
211.05211.600.554.39140.020.0014.44
217.30224.757.458.62280.040.0028.69
OLCU-2264.70265.200.508.05890.050.0029.24
and284.15331.3047.150.61180.030.0040.94
Incl.301.50302.701.202.75550.020.0043.51
329.80331.301.502.87340.050.0033.36
OLCU-358.5559.400.854.53120.010.0044.54
116.85134.3017.450.6490.030.0020.81
Incl.111.55112.250.702.121080.140.0023.92
133.70134.300.608.95100.030.0018.72
and204.80206.101.303.45260.030.0033.76

*AuEq (g/t) is calculated as follows: (Au (g/t) x 0.95) + (Ag g/t x 0.016 x 0.95) + (Cu (%) x 1.83 x 0.95)+ (Mo (%)*9.14 x 0.95) and CuEq (%) is calculated as follows: (Cu (%) x 0.95) + (Au (g/t) x 0.51 x 0.95) + (Ag (g/t) x 0.01 x 0.95)+ (Mo(%)x 3.75 x 0.95) utilizing metal prices of Cu – US$4.00/lb, Ag – $24/oz Mo US$20.00/lb and Au – US$1,500/oz and recovery rates of 95% for Au, Ag, Mo and Cu. Recovery rate assumptions are speculative as no metallurgical work has been completed to date. No top cut has been applied.

Reconnaissance drilling south of the Apollo porphyry system: Two drill holes (APC-32 and APC-34) were completed to test a surface soil anomaly for copper which is located 150 metres south of the southern limit of the currently defined Apollo porphyry system. The holes were collared from a newly constructed Pad 8 and drilled steeply northwards and westwards respectively, below the soil anomaly. Both holes intersected potassically altered porphyry diorites with low density of quartz-molybdenum-pyrite-pyrrhotite-chalcopyrite veins. Neither hole returned significant precious or base metal values. The Exploration team are using the trace element data to understand the location of these holes and their alteration patterns in comparison with the Apollo porphyry system.

Figure 1: Plan View Outlining Drilling at the Olympus Target. Proximity to the Apollo Porphyry System is Highlighted on the Map. (CNW Group/Collective Mining Ltd.)
Figure 1: Plan View Outlining Drilling at the Olympus Target. Proximity to the Apollo Porphyry System is Highlighted on the Map. (CNW Group/Collective Mining Ltd.)
Figure 2: Plan View of the Guayabales Project Highlighting the Olympus Target Area (CNW Group/Collective Mining Ltd.)
Figure 2: Plan View of the Guayabales Project Highlighting the Olympus Target Area (CNW Group/Collective Mining Ltd.)
Figure 3: Core Photo Highlights from Drill Hole OLCU-2 (CNW Group/Collective Mining Ltd.)
Figure 3: Core Photo Highlights from Drill Hole OLCU-2 (CNW Group/Collective Mining Ltd.)

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 $2 billion in enterprise value, Collective Mining is a copper, silver and gold exploration company with projects in Caldas, Colombia. The Company has options to acquire 100% interests in two projects located directly within an established mining camp with ten fully permitted and operating mines.

The Company’s flagship project, Guayabales, is anchored by the Apollo target, which hosts the large-scale, bulk-tonnage and high-grade copper-silver-gold Apollo porphyry system. The Company’s near-term objective is to drill the shallow portion of the porphyry system while continuing to expansion the overall dimensions of the system, which remains open in all directions.

Management and insiders own nearly 52% of the outstanding shares of the Company and as a result, are fully aligned with shareholders. The Company is listed on the TSXV under the trading symbol “CNL” and on the OTCQX under the trading symbol “CNLMF”.

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 and core samples have been prepared and analyzed at SGS laboratory facilities in Medellin, Colombia and Lima, Peru. Blanks, duplicates, and certified reference standards are inserted into the sample stream to monitor laboratory performance. Crush rejects and pulps are kept and stored in a secured storage facility for future assay verification. No capping has been applied to sample composites. The Company utilizes a rigorous, industry-standard QA/QC program.

Information Contact:

Follow Executive Chairman Ari Sussman (@Ariski) and Collective Mining (@CollectiveMini1) on Twitter

FORWARD-LOOKING STATEMENTS

This news release contains certain forward-looking statements, including, but not limited to, statements about the drill programs, including timing of results, and Collective’s future and intentions. Wherever possible, words such as “may”, “will”, “should”, “could”, “expect”, “plan”, “intend”, “anticipate”, “believe”, “estimate”, “predict” or “potential” or the negative or other variations of these words, or similar words or phrases, have been used to identify these forward-looking statements. These statements reflect management’s current beliefs and are based on information currently available to management as at the date hereof.

Forward-looking statements involve significant risk, uncertainties, and assumptions. Many factors could cause actual results, performance, or achievements to differ materially from the results discussed or implied in the forward-looking statements. These factors should be considered carefully, and readers should not place undue reliance on the forward-looking statements. Although the forward-looking statements contained in this news release are based upon what management believes to be reasonable assumptions, Collective cannot assure readers that actual results will be consistent with these forward-looking statements. These forward-looking statements are made as of the date of this news release, and Collective assumes no obligation to update or revise them to reflect new events or circumstances, except as required by law.

Neither the TSXV nor its Regulation Services Provider (as that term is defined in the policies of the TSXV) accepts responsibility for the adequacy or accuracy of this news release.

SOURCE Collective Mining Ltd.

Cision
Cision

View original content to download multimedia: http://www.newswire.ca/en/releases/archive/March2023/07/c3264.html

Categories
Base Metals Collective Mining Energy Junior Mining Precious Metals

Collective Mining Intersects 384.7 Metres at 2.46 g/t Gold Equivalent Including 109.8 Metres grading 4.14 g/t Gold Equivalent from Surface at the Apollo Porphyry System

  • Assay results for drill hole APC-31, which is the first hole to test the mineralized outcrop of the Apollo porphyry system (*formerly known as the Main Breccia discovery), has intersected significant continuous high-grade copper-silver-gold mineralization from surface as follows:
  • High-grade oxide mineralization was encountered over the initial 42.35 metres of the drill hole averaging 5.08 g/t gold equivalent.
  • Five additional drill holes have been completed in 2023 to date from drill Pads 6 and 7. All five holes appear to have cut significant mineralization beginning at bedrock with the three completed holes from Pad 6 intersecting more than 350 metres of continuous mineralization and the two outstanding holes from Pad 7 intersecting more than 100 metres and 170 metres of continuous mineralization, respectively. Assay results for these holes are expected in the near term.
  • Outcrop mapping and sampling in the south and central portions of the Apollo porphyry system has outlined a 130 metres X 130 metres area of known surface mineralization which is open in all directions. Two new pads (9 and 10) are under construction and once operational will provide more drilling options to test this expanding area of surface and shallow mineralization.

Ari Sussman, Executive Chairman commented: “2023 is off to an excellent start to say the least. Not only did drill hole APC-31 confirm for the first time that the high-grade copper-silver-gold mineralization in the Apollo porphyry system comes right to surface, but also that there is a significant zone of high-grade oxide mineralization. We have truly discovered a remarkable porphyry system at Apollo characterized by unusually high-grades of combined gold, silver and copper. We are equally fortunate that our Guayabales project is located in a mining camp contiguous to the multi-million-ounce Marmato mine and are confident that our Apollo porphyry system will play a key role in Colombia’s decarbonization strategy. Our plan in 2023 is to remain aggressive with both drilling and ESG so that our “Collective” model for mining yields dividends for stakeholders and shareholders alike.”

TORONTO, Feb. 23, 2023 /CNW/ – Collective Mining Ltd. (TSXV: CNL) (OTCQX: CNLMF) (“Collective” or the “Company”) is pleased to announce assay results from the first drill hole of 2023 as part of the Company’s phase II drill program at the Guayabales project located in Caldas, Colombia. The aim of the phase II program is to test and define through drilling the shallow portion of the Apollo porphyry system (*formerly known as the Main Breccia discovery) as well as continue expanding the system through step-out drilling. The Apollo porphyry deposit is a high-grade, bulk tonnage copper-silver-gold system, which owes its excellent metal endowment to an older porphyry copper-silver and gold mineralization being overprinted by younger precious metal rich, carbonate base metal vein systems (low and intermediate sulphidation) within a magmatic, hydrothermal intermineral breccia body currently measuring 395 metres x 385 metres x 915 metres and open for expansion.

Details (See Table 1 and Figures 1-3)

Assay results for the first drill hole (APC-31) from the 2023 phase II program is announced in this press release. The Phase II drilling program of 2023 is advancing on schedule with six holes completed and a further three in progress. The aim of this program is to define the high-grade mineralization and dimensions of the Apollo porphyry near surface while continuing to expand the size of the system through step-out drilling.

To date, a total of 32 drill holes (approximately 15,400 metres) have been completed and assayed at the Apollo target with the majority of the holes testing the Apollo porphyry system.

Assay results and geological observations of APC-31 are summarized below.

APC-31 was a shallow hole, drilled steeply to the northwest from Pad 6 to a maximum depth of 389.6 metres (370 metres vertical). The hole was designed to exclusively test the upper portion of the porphyry system from a location where the system outcrops at surface. The hole intersected continuous mineralization from surface down to its final depth where it was terminated while still in strong mineralization. APC-31 is the highest-grade accumulation of mineralization reported from drilling to date and averaged:

  • 384.7 metres @ 2.46 g/t gold equivalent (consisting of 1.17 g/t gold, 43 g/t silver and 0.37% copper) and including;

The mineralized interval starts from surface to 30 metres depth within saprolite material followed by an additional 17.5 metres of saprock with iron oxides and sulphides to 47.25 metres before transitioning into fresh rock consisting of chalcopyrite (0.5% to 1.5%), pyrite (1% to 2.5%) and some pyrrhotite (~1%). The mineralization is overprinted by carbonate-base metal veins containing sphalerite and galena and high grades of gold. Gold grades are significantly higher in the oxidized portion of the intercept down to 47.25 metres, while copper and silver grades are reduced within the same interval presumably due to weathering.

Outcrop mapping and sampling in the south and central portions of the system has outlined a 130 metre-by-130 metre area of known surface mineralization, which is open in all directions. 2023 drill Pads 6 and 7 have been designed to achieve the objective of understanding the styles and tenor of the shallow, high-grade mineralization from surface down to depths of up to 400 metres. Visual observations from five completed holes that are awaiting assay results in the near term indicate continuous intercepts from surface over core lengths ranging from more than 100 metres to more than 350 metres. The Company presently has three diamond drill rigs operating at the project.

Two new drill pads, numbered 9 and 10, are under construction to provide further drilling options to test and expand upon the area which the Apollo porphyry system outcrops at surface.

The Apollo target area, as defined to date by surface mapping, rock sampling and copper and molybdenum soil geochemistry, covers a 1,000 metres X 1,200 metres area, and represents a large and unusually high-grade Au-Cu-Ag porphyry system. Mineralization styles include early-stage porphyry veining, inter-mineral breccia mineralization and multiple zones of late stage, sheeted, carbonate-base metal veins with high gold and silver grades. The Apollo target area is still expanding as the Company’s geologists find more outcrop areas with porphyry veining, breccia, and late stage, sheeted, carbonate base metal veins.

Table 1: Assays Results for APC-31

Hole IDFrom
(m)
To
 (m)
Intercept
(m)
Au
(g/t)
Ag
(g/t)
Cu
%
Mo
%
AuEq
(g/t)*
APC-314.90389.60384.701.17430.370.022.46
Including4.90325.70320.801.34490.440.022.84
4.90114.70109.803.15450.250.014.14
**4.9047.2542.354.81230.090.0015.08

*AuEq (g/t) is calculated as follows: (Au (g/t) x 0.95) + (Ag g/t x 0.016 x 0.95) + (Cu (%) x 1.83 x 0.95)+ (Mo (%)*9.14 x 0.95) and CuEq (%) is calculated as follows:  (Cu (%) x 0.95) + (Au (g/t) x 0.51 x 0.95) + (Ag (g/t) x 0.01 x 0.95)+ (Mo(%)x 3.75 x 0.95) utilizing metal prices of Cu – US$4.00/lb, Ag – $24/oz Mo US$20.00/lb and Au – US$1,500/oz and recovery rates of 95% for Au, Ag, Mo and Cu. Recovery rate assumptions are speculative as no metallurgical work has been completed to date. A 0.2 g/t AuEq cut-off grade was employed with no more than 15% internal dilution. True widths are unknown, and grades are uncut
**Zone of Oxidation

Figure 1: Plan View of the Apollo Porphyry System (formerly known as the Main Breccia Discovery) Highlighting Drill Hole APC-31 (CNW Group/Collective Mining Ltd.)
Figure 1: Plan View of the Apollo Porphyry System (formerly known as the Main Breccia Discovery) Highlighting Drill Hole APC-31 (CNW Group/Collective Mining Ltd.)
Figure 2: Plan View of the Guayabales Project Highlighting the Apollo Target Area (CNW Group/Collective Mining Ltd.)
Figure 2: Plan View of the Guayabales Project Highlighting the Apollo Target Area (CNW Group/Collective Mining Ltd.)
Figure 3: Core Photo Highlights from Drill Hole APC-31 (CNW Group/Collective Mining Ltd.)
Figure 3: Core Photo Highlights from Drill Hole APC-31 (CNW Group/Collective Mining Ltd.)

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 $2 billion in enterprise value, Collective Mining is a copper, silver and gold exploration company with projects in Caldas, Colombia. The Company has options to acquire 100% interests in two projects located directly within an established mining camp with ten fully permitted and operating mines.

The Company’s flagship project, Guayabales, is anchored by the Apollo target, which hosts the large-scale, bulk-tonnage and high-grade copper-silver-gold Apollo porphyry system. The Company’s near-term objective is to drill the shallow portion of the porphyry system while continuing to expansion the overall dimensions of the system, which remains open in all directions.

Management, insiders and close family and friends own nearly 52% of the outstanding shares of the Company and as a result, are fully aligned with shareholders. The Company is listed on the TSXV under the trading symbol “CNL” and on the OTCQX under the trading symbol “CNLMF”.

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 and core samples have been prepared and analyzed at SGS laboratory facilities in Medellin, Colombia and Lima, Peru. Blanks, duplicates, and certified reference standards are inserted into the sample stream to monitor laboratory performance. Crush rejects and pulps are kept and stored in a secured storage facility for future assay verification. No capping has been applied to sample composites. The Company utilizes a rigorous, industry-standard QA/QC program.

Information Contact:

Follow Executive Chairman Ari Sussman (@Ariski) and Collective Mining (@CollectiveMini1) on Twitter

FORWARD-LOOKING STATEMENTS

This news release contains certain forward-looking statements, including, but not limited to, statements about the drill programs, including timing of results, and Collective’s future and intentions. Wherever possible, words such as “may”, “will”, “should”, “could”, “expect”, “plan”, “intend”, “anticipate”, “believe”, “estimate”, “predict” or “potential” or the negative or other variations of these words, or similar words or phrases, have been used to identify these forward-looking statements. These statements reflect management’s current beliefs and are based on information currently available to management as at the date hereof.

Forward-looking statements involve significant risk, uncertainties, and assumptions. Many factors could cause actual results, performance, or achievements to differ materially from the results discussed or implied in the forward-looking statements. These factors should be considered carefully, and readers should not place undue reliance on the forward-looking statements. Although the forward-looking statements contained in this news release are based upon what management believes to be reasonable assumptions, Collective cannot assure readers that actual results will be consistent with these forward-looking statements. These forward-looking statements are made as of the date of this news release, and Collective assumes no obligation to update or revise them to reflect new events or circumstances, except as required by law.

Neither the TSXV nor its Regulation Services Provider (as that term is defined in the policies of the TSXV) accepts responsibility for the adequacy or accuracy of this news release.

SOURCE Collective Mining Ltd.

Categories
Base Metals Collective Mining Energy Junior Mining Precious Metals

Collective Mining Step-Out Drilling Intersects 601.65 Metres at 1.40 g/t Gold Equivalent and Extends the Main Breccia System at Apollo to the West and Depth

  • Step-out drill hole APC-28, which was drilled to the west from the eastern side of the Main Breccia system at Apollo cut the longest intercept to date as follows:
  • As a result of APC-28, the maximum width and vertical dimensions of the Main Breccia system have increased to 395 metres (previously 350 metres) and 915 metres (previously 825 metres), respectively.
  • Drill hole APC-28 bottomed while still in mineralization indicating that the Main Breccia system remains open for expansion to the west and at depth (as well as to the east and north based on previously announced assay results).
  • Hole APC-30 was drilled southwards on the western side of the deposit and intercepted the Main Breccia system over a broad interval as follows:
  • Four holes have now been completed into the Main Breccia system as part of the 2023 Phase II drill program at the Guayabales project. All four holes appear to have intercepted the Main Breccia system with mineralization beginning from surface.  Assay results for these holes are expected in the near term.

Ari Sussman, Executive Chairman commented: “The Main Breccia system at Apollo continues to yield positive surprises. The Company drilled three long holes in 2022, APC-17, APC-22 and APC-28, with each hole expanding the size of the deposit and bottoming while still in mineralization. In addition, 2023 drilling is off to an excellent start with the initial four holes testing the Main Breccia system all intersecting mineralization beginning at surface. Our aim for 2023 is to define the newly discovered high-grade and near surface mineralization while continuing to be aggressive with expansion drilling. Without question, we have discovered a large copper-silver-gold deposit in a mining friendly jurisdiction of Colombia which will play a vital role in the country’s aggressive decarbonization goals.”

TORONTO, Feb. 15, 2023 /CNW/ – Collective Mining Ltd. (TSXV: CNL) (OTCQX: CNLMF) (“Collective” or the “Company”) is pleased to announce assay results from a further three holes drilled into the Main Breccia system at the Apollo target (“Apollo”), which is part of the Guayabales project located in Caldas, Colombia. The Main Breccia is a high-grade, bulk tonnage copper-silver-gold porphyry-related system, which owes its excellent metal endowment to multiple phases of mineralization which includes older copper-silver-gold porphyry mineralization and younger, overprinting, low and intermediate sulphidation, precious metal rich sheeted carbonate base metal vein systems.

Details (See Table 1 and Figures 1–5)

Assay results for all thirty-one diamond drill holes from the Phase I drilling program for 2022 have now been announced at Apollo. The Phase II drilling program for 2023 is advancing on schedule with assay results for the first holes expected in the near term. This press release summarizes assay results of the final three diamond drill holes from the Phase I program with results summarized below.

APC-28 was a step-out hole drilled steeply to the west from Pad 2 to a maximum depth of 956.35 metres (915 metres vertical) and was designed to test western and depth extensions to the Main Breccia system. The hole intersected the longest interval drilled to date within the system, commencing at 354.70 metres down hole (335 vertical) and averaging:

  • 601.65 metres @ 1.4 g/t gold equivalent and including internal intervals of:

The mineralized angular breccia of this intercept represents the largest accumulation of metal returned to date within the Main Breccia system and contains a sulphide matrix which includes 0.5% up to 2.5% chalcopyrite and between 1% and 3% pyrite plus some pyrrhotite. The breccia has been overprinted by zones of carbonate and base metal (sphalerite and galena) veins, which yield the higher gold equivalent intervals. APC-28 stopped in mineralized breccia due to rig constraints. This hole has extended the main breccia westwards by 115 metres and is the deepest intercept drilled to date outlining continuity of mineralized breccia to a vertical depth of approximately 915 metres below surface. APC-28 also represents the westernmost hole drilled into the Main Breccia system and demonstrates that the mineralization is thickening with depth and has an inverted funnel morphology as outlined in Figure 2 below. This western area of the deposit remains open for expansion as the hole stopped in strong mineralization.

As a result of drill hole APC-28, the overall volume of rock in which the Main Breccia system is located has grown in width to 395 metres (from 350 metres) and a vertical dimension of 915 metres (from 825 metres). The strike of the system remains the same at 385 metres.

APC-30 was drilled southwards from Pad 4 to a total length of 589 metres downhole and intersected mineralized breccia from 267.60 metres downhole (240 metres vertical), averaging:

  • 318.85 metres @ 1.10 g/t gold equivalent and including internal intervals of:

Gold, silver and copper mineralization relates to sulphides hosted within the angular breccia matrix with average concentrations of pyrite (2%) and chalcopyrite (0.5%). An upper zone of 60.8 metres bearing 2% to 3% chalcopyrite was intercepted at the beginning of the mineralized interval and a sheeted and overprinting sphalerite rich CBM vein zone of 81.4 metres was encountered from 472.3 metres downhole.

Reconnaissance hole APC-27 was drilled due east away from the Main Breccia system to test outcropping mineralization at surface. From 300.40 metres downhole (210 metres vertical depth) the Company intersected a new zone of continuous low-grade mineralization with assay results as follows:

  •  

Core logging of the breccia system at Apollo by the Company’s geologists has identified that the crackle breccia as seen in this newly discovered zone, is typically found both above and on the periphery of the more intensely mineralized angular breccia phase. As a result of this assessment, the Company may have drilled over top of an angular breccia zone with stronger mineralization than was intercepted in APC-27. Further exploratory drilling will be undertaken in this area.

The Company’s Phase II 2023 program is well underway with three rigs focused on drilling near surface, high grade mineralization below mineralized outcrops in the southern and central areas of the Main Breccia system from newly constructed pads 6 and 7. To date, four shallow holes have been completed and confirm continuous mineralized angular breccia from surface. Three of these holes were drilled from Pad 6 and were terminated while still in strong mineralization. The fourth hole from Pad 7 appears to have drilled out the east side of the system indicating a more vertical orientation to the system that was previously modelled. Assay results are expected in the near term.

The Apollo target area, as defined to date by surface mapping, rock sampling and copper and molybdenum soil geochemistry, covers a 1,000 metres X 1,200 metres area. The Apollo target area hosts the Company’s Main Breccia system and multiple additional untested breccia, porphyry and vein targets. The overall Apollo target area also remains open for further expansion.

Table 1: Apollo Target Assays Results for Holes APC-27, APC-28, and APC-30

Hole IDFrom
(m)
To
 (m)
Intercept
(m)
Au
(g/t)
Ag
(g/t)
Cu
%
Mo
%
AuEq
(g/t) *
APC-27299.50372.4072.900.3060.020.0020.44
APC-28286.60305.5518.951.11120.040.0011.30
And354.70956.35601.650.89240.100.0011.40
Incl354.70614.65259.951.21430.200.0012.15
713.10772.8059.702.04150.140.042.23
863.15868.805.652.00130.040.0012.17
APC-30267.60586.25318.650.61190.120.0021.10
Incl267.60328.4060.800.17480.400.0021.64
472.30553.7081.401.95180.040.0022.22
*AuEq (g/t) is calculated as follows: (Au (g/t) x 0.95) + (Ag g/t x 0.016 x 0.95) + (Cu (%) x 1.83 x 0.95)+ (Mo (%)*9.14 x 0.95) and CuEq (%) is calculated as follows:  (Cu (%) x 0.95) + (Au (g/t) x 0.51 x 0.95) + (Ag (g/t) x 0.01 x 0.95)+ (Mo(%)x 3.75 x 0.95) utilizing metal prices of Cu – US$4.00/lb, Ag – $24/oz Mo US$20.00/lb and Au – US$1,500/oz and recovery rates of 95% for Au, Ag, Mo and Cu. Recovery rate assumptions are speculative as no metallurgical work has been completed to date.
** A 0.2 g/t AuEq cut-off grade was employed with no more than 15% internal dilution. True widths are unknown, and grades are uncut.
Figure 1: Plan View of the Main Breccia System at Apollo Highlighting Drill Holes APC-27, APC-28, APC-30 and Visual Results for APC-31, APC-33, APC-35 and APC-36 (CNW Group/Collective Mining Ltd.)
Figure 1: Plan View of the Main Breccia System at Apollo Highlighting Drill Holes APC-27, APC-28, APC-30 and Visual Results for APC-31, APC-33, APC-35 and APC-36 (CNW Group/Collective Mining Ltd.)
Figure 2: East-West Cross Section Highlighting APC-28, ACP-30, and Visual Results for
APC-31 (CNW Group/Collective Mining Ltd.)
Figure 2: East-West Cross Section Highlighting APC-28, ACP-30, and Visual Results for APC-31 (CNW Group/Collective Mining Ltd.)
Figure 3: Plan View of the Guayabales Project Highlighting the Apollo Target (CNW Group/Collective Mining Ltd.)
Figure 3: Plan View of the Guayabales Project Highlighting the Apollo Target (CNW Group/Collective Mining Ltd.)
Figure 4: Core Photo Highlights from Drill Hole APC-28 (CNW Group/Collective Mining Ltd.)
Figure 4: Core Photo Highlights from Drill Hole APC-28 (CNW Group/Collective Mining Ltd.)
Figure 5: Core Photo Highlights from Drill Hole APC-30 (CNW Group/Collective Mining Ltd.)
Figure 5: Core Photo Highlights from Drill Hole APC-30 (CNW Group/Collective Mining Ltd.)

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 $2 billion in enterprise value, Collective Mining is a copper, silver and gold exploration company based in Canada, with projects in Caldas, Colombia. The Company has options to acquire 100% interests in two projects located directly within an established mining camp with ten fully permitted and operating mines.

The Company’s flagship project, Guayabales, is anchored by the Apollo target, which hosts the large-scale, bulk-tonnage and high-grade copper, silver, and gold Main Breccia system. The Company’s near-term objective is to continue with expansion drilling of the Main Breccia system while increasing confidence in the highest-grade portions of the system.

Management, insiders and close family and friends own nearly 52% of the outstanding shares of the Company and as a result, are fully aligned with shareholders. The Company is listed on the TSXV under the trading symbol “CNL” and on the OTCQX under the trading symbol “CNLMF”.

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 and core samples have been prepared and analyzed at SGS laboratory facilities in Medellin, Colombia and Lima, Peru. Blanks, duplicates, and certified reference standards are inserted into the sample stream to monitor laboratory performance. Crush rejects and pulps are kept and stored in a secured storage facility for future assay verification. No capping has been applied to sample composites. The Company utilizes a rigorous, industry-standard QA/QC program.

Information Contact:

Follow Executive Chairman Ari Sussman (@Ariski) and Collective Mining (@CollectiveMini1) on Twitter

FORWARD-LOOKING STATEMENTS

This news release contains certain forward-looking statements, including, but not limited to, statements about the drill programs, including timing of results, and Collective’s future and intentions. Wherever possible, words such as “may”, “will”, “should”, “could”, “expect”, “plan”, “intend”, “anticipate”, “believe”, “estimate”, “predict” or “potential” or the negative or other variations of these words, or similar words or phrases, have been used to identify these forward-looking statements. These statements reflect management’s current beliefs and are based on information currently available to management as at the date hereof.

Forward-looking statements involve significant risk, uncertainties, and assumptions. Many factors could cause actual results, performance, or achievements to differ materially from the results discussed or implied in the forward-looking statements. These factors should be considered carefully, and readers should not place undue reliance on the forward-looking statements. Although the forward-looking statements contained in this news release are based upon what management believes to be reasonable assumptions, Collective cannot assure readers that actual results will be consistent with these forward-looking statements. These forward-looking statements are made as of the date of this news release, and Collective assumes no obligation to update or revise them to reflect new events or circumstances, except as required by law.

Neither the TSXV nor its Regulation Services Provider (as that term is defined in the policies of the TSXV) accepts responsibility for the adequacy or accuracy of this news release.

SOURCE Collective Mining Ltd.

Cision
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View original content to download multimedia: http://www.newswire.ca/en/releases/archive/February2023/15/c3425.html

Categories
Base Metals Collective Mining Energy Junior Mining Precious Metals

Ari Sussman from Collective Mining to Present at OTC Markets Group Precious Metals Virtual Investor Conference on February 15th, 2023

TORONTO, Feb. 8, 2023 /CNW/ – Collective Mining Ltd. (TSXV: CNL) (OTCQX: CNLMF) (“Collective” or the “Company”) will be presenting at the OTC Markets Group Precious Metals Virtual Investor Conference on Wednesday, February 15, 2023, at 11:00am ET.

Using the link below, investors can register and listen to the presentation, and take part in a question and answer session at the end. The presentation is expected to last 30 minutes.

DATE: Wednesday, February 15, 2023
TIME: 11:00am ET – 11:30am ET
LINK: https://bit.ly/3JCTs89

Please log in 5-10 minutes early to register. An archived webcast will also be made available after the event.

Ari Sussman, Executive Chairman of Collective Mining will be providing an overview and will discuss the Company’s “Main Breccia” discovery at the Apollo target. The Main Breccia discovery is a high-grade and bulk tonnage, copper-silver-gold porphyry-related breccia system characterized by two main, yet distinct pulses of mineralized fluids flooding the breccia with metals.

The Company’s Guayabales project is located in the mining-friendly department of Caldas, Colombia, in the heart of a long-established mining camp with ten fully permitted and operating mines located within three kilometres of the project. As a result, the Guayabales project is blessed with excellent infrastructure with roads and hydroelectric powerlines traversing the project and an abundant labour force located nearby in the townships of Supia and Marmato.

The phase II drilling program is underway with three rigs currently operating focused on testing near surface mineralization and expanding the dimensions of the Main Breccia system. Assay results are expected in the near term for the final three holes of the 2022 program, including westwards step-out hole APC-28, which cut more than 600 metres of continuous mineralization. Additionally, the first hole of the Phase II program is now complete, and core has been dispatched to the lab for assaying.

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 $2 billion in enterprise value, Collective Mining is a copper, silver and gold exploration company based in Canada, with projects in Caldas, Colombia. The Company has options to acquire 100% interests in two projects located directly within an established mining camp with ten fully permitted and operating mines.

The Company’s flagship project, Guayabales, is anchored by the Apollo target, which hosts the large-scale, bulk-tonnage and high-grade copper, silver and gold Main Breccia discovery. The Company’s near-term objective is to continue with expansion drilling of the Main Breccia discovery while increasing confidence in the highest-grade portions of the system.

Management, insiders and close family and friends own approximately 52% of the outstanding shares of the Company and as a result, are fully aligned with shareholders. The Company is listed on the TSXV under the trading symbol “CNL” and on the OTCQX under the trading symbol “CNLMF”.

Information Contact:

Follow Executive Chairman Ari Sussman (@Ariski) and Collective Mining (@CollectiveMini1) on Twitter

FORWARD-LOOKING STATEMENTS

This news release contains certain forward-looking statements, including, but not limited to, statements about the drill programs, including timing of results, and Collective’s future and intentions. Wherever possible, words such as “may”, “will”, “should”, “could”, “expect”, “plan”, “intend”, “anticipate”, “believe”, “estimate”, “predict” or “potential” or the negative or other variations of these words, or similar words or phrases, have been used to identify these forward-looking statements. These statements reflect management’s current beliefs and are based on information currently available to management as at the date hereof.

Forward-looking statements involve significant risk, uncertainties, and assumptions. Many factors could cause actual results, performance, or achievements to differ materially from the results discussed or implied in the forward-looking statements. These factors should be considered carefully, and readers should not place undue reliance on the forward-looking statements. Although the forward-looking statements contained in this news release are based upon what management believes to be reasonable assumptions, Collective cannot assure readers that actual results will be consistent with these forward-looking statements. These forward-looking statements are made as of the date of this news release, and Collective assumes no obligation to update or revise them to reflect new events or circumstances, except as required by law.

Neither the TSXV nor its Regulation Services Provider (as that term is defined in the policies of the TSXV) accepts responsibility for the adequacy or accuracy of this news release.

SOURCE Collective Mining Ltd.

Categories
Base Metals Collective Mining Junior Mining Precious Metals

Collective Mining Hosts the Vice Minister of Mines of Colombia to its Project Facilities in Supia, Colombia

TORONTO, Feb. 6, 2023 /CNW/ – Collective Mining Ltd. (TSXV: CNL) (OTCQX: CNLMF) (“Collective” or the “Company”) is pleased to announce the Company had a recent opportunity to host the new Vice Minister of Mines of Colombia, Giovanni Franco, at its operation facilities in Supia, Colombia. The Vice Minister was visiting the region as part of the Ministry of Mines and Energy’s Social Mining Forum, which is a communication-based platform to discuss mining between the Ministry and municipalities.

During the visit, the Company had the opportunity to present its “Collective” model to mining, which is based on honesty, transparency, education and open dialogue with its stakeholders. The Company reviewed in detail its business and social approach within the area of influence of the Guayabales and San Antonio projects as it relates to various sustainability initiatives and exploration methodologies.

Upon completion of the visit, the Vice Minister of Mines recorded a short video summarizing his thoughts, which includes the following statement:

“What we see in the advances made by Collective Mining over the past three years is what we would like to have in Colombia. We wish to have 10, 50, 100 companies like Collective Mining all around Colombia to improve the geoscientific knowledge of the country, to improve the understanding of the subsoil resources that we have in Colombia to define public policies to improve the extraction of our subsoil resources.”

Please click on the link below to watch the full two-minute video testimony of the Vice Minister of Mines: https://youtu.be/-Ak3a_HJiPE

Figure 1 - Vice Minister of Mines Engaging with the Collective Mining Team in our Core Shack in Supía, Colombia (CNW Group/Collective Mining Ltd.)
Figure 1 – Vice Minister of Mines Engaging with the Collective Mining Team in our Core Shack in Supía, Colombia (CNW Group/Collective Mining Ltd.)

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 $2 billion in enterprise value, Collective Mining is a copper, silver and gold exploration company based in Canada, with projects in Caldas, Colombia. The Company has options to acquire 100% interests in two projects located directly within an established mining camp with ten fully permitted and operating mines.

The Company’s flagship project, Guayabales, is anchored by the Apollo target, which hosts the large-scale, bulk-tonnage and high-grade copper, silver and gold Main Breccia discovery. The Company’s near-term objective is to continue with expansion drilling of the Main Breccia discovery while increasing confidence in the highest-grade portions of the system.

Management, insiders and close family and friends own nearly 35% of the outstanding shares of the Company and as a result, are fully aligned with shareholders. The Company is listed on the TSXV under the trading symbol “CNL” and on the OTCQX under the trading symbol “CNLMF”.

Information Contact:

Follow Executive Chairman Ari Sussman (@Ariski) and Collective Mining (@CollectiveMini1) on Twitter

FORWARD-LOOKING STATEMENTS

This news release contains certain forward-looking statements, including, but not limited to Collective’s future and intentions. Wherever possible, words such as “may”, “will”, “should”, “could”, “expect”, “plan”, “intend”, “anticipate”, “believe”, “estimate”, “predict” or “potential” or the negative or other variations of these words, or similar words or phrases, have been used to identify these forward-looking statements. These statements reflect management’s current beliefs and are based on information currently available to management as at the date hereof.

Forward-looking statements involve significant risk, uncertainties, and assumptions. Many factors could cause actual results, performance, or achievements to differ materially from the results discussed or implied in the forward-looking statements. These factors should be considered carefully, and readers should not place undue reliance on the forward-looking statements. Although the forward-looking statements contained in this news release are based upon what management believes to be reasonable assumptions, Collective cannot assure readers that actual results will be consistent with these forward-looking statements. These forward-looking statements are made as of the date of this news release, and Collective assumes no obligation to update or revise them to reflect new events or circumstances, except as required by law.

Neither the TSXV nor its Regulation Services Provider (as that term is defined in the policies of the TSXV) accepts responsibility for the adequacy or accuracy of this news release.

SOURCE Collective Mining Ltd.