- 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:
-
- 55.25 metres @ 1.91 g/t gold equivalent (OLCU-2).
- 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:
-
- 301.9 metres @ 1.11 g/t AuEq (OLCC-3) (see release dated
March 15, 2022), and
- 216.7 metres @ 1.08 g/t AuEq (OLCC-4) (see release dated
May 9, 2022).
- 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:
-
- 384.7 metres at 2.46 g/t gold equivalent (consisting of 1.17
g/t gold, 43 g/t silver and 0.37% copper), including 109.8 metres
at 4.14 g/t gold equivalent from surface.
- 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-1
|
NSV*
|
OLCU-2
|
5.90
|
6.40
|
0.50
|
3.4
|
242
|
0.13
|
0.004
|
7.18
|
|
133.55
|
134.25
|
0.70
|
1.51
|
180
|
0.13
|
0.002
|
4.41
|
OLCU-2
|
172.60
|
227.85
|
55.25
|
1.75
|
11
|
0.02
|
0.003
|
1.91
|
Incl.
|
205.00
|
206.60
|
1.60
|
3.01
|
20
|
0.02
|
0.010
|
3.29
|
|
207.60
|
208.80
|
1.20
|
2.89
|
10
|
0.01
|
0.006
|
2.97
|
|
211.05
|
211.60
|
0.55
|
4.39
|
14
|
0.02
|
0.001
|
4.44
|
|
217.30
|
224.75
|
7.45
|
8.62
|
28
|
0.04
|
0.002
|
8.69
|
OLCU-2
|
264.70
|
265.20
|
0.50
|
8.05
|
89
|
0.05
|
0.002
|
9.24
|
and
|
284.15
|
331.30
|
47.15
|
0.61
|
18
|
0.03
|
0.004
|
0.94
|
Incl.
|
301.50
|
302.70
|
1.20
|
2.75
|
55
|
0.02
|
0.004
|
3.51
|
|
329.80
|
331.30
|
1.50
|
2.87
|
34
|
0.05
|
0.003
|
3.36
|
OLCU-3
|
58.55
|
59.40
|
0.85
|
4.53
|
12
|
0.01
|
0.004
|
4.54
|
|
116.85
|
134.30
|
17.45
|
0.64
|
9
|
0.03
|
0.002
|
0.81
|
Incl.
|
111.55
|
112.25
|
0.70
|
2.12
|
108
|
0.14
|
0.002
|
3.92
|
|
133.70
|
134.30
|
0.60
|
8.95
|
10
|
0.03
|
0.001
|
8.72
|
and
|
204.80
|
206.10
|
1.30
|
3.45
|
26
|
0.03
|
0.003
|
3.76
|
*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.
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.