Talisker Announces the Discovery of High Grade Gold Intercepts in its Maiden Drill Program at the Golden Hornet Project
Talisker Announces the Discovery of High
Grade Gold Intercepts in its Maiden Drill
Program at the Golden Hornet Project
TORONTO
,
Jan. 19, 2022
/CNW/ - Talisker Resources Ltd. ("
Talisker
" or the "
Company
") (TSX:T
SK) (OTCQX: TSKFF) is pleased to announce full assays from the first four holes on its maiden drill
campaign at the Golden Hornet Project near
Rock Creek
, south-central British Columbia. Assay
results for the remaining ten drill holes are expected to be received from the laboratory over the
coming weeks.
Key Points:
Discovery of high-grade fault-controlled quartz-sulphide breccias and veins, highlighted by 8.88
g/t Au, 0.42% Cu and 14.99 g/t Ag over 5.1 metres within a broader zone of 2.59 g/t Au over
21.5 metres in GH-DDH-21-004.
Hole GH-DDH-21-003 intercepted 11.58 g/t Au, 0.37% Cu and 11.1 g/t Ag over 1.05 metres.
Drilling also intersected broader zones of mineralization, including 9.99 g/t Au over 0.5 metres
within 0.82 g/t Au over 10.3 metres (GH-DDH-21-003) and 0.96 g/t Au over 6.67 metres (GH-
DDH-21-001).
A total of 4,853 metres of NQ drilling was completed in 14 holes to a maximum depth of 431
metres.
Ten holes drilled in the central Hornet Zone (3,568 metres) intersected semi-massive sulphide
mineralization in every hole.
Four holes drilled in the Iron Canyon Zone (1,015 metres), a 1,000-metre step-out to the
northwest, intersected semi-massive and breccia-hosted sulphide mineralization in every hole.
Terry Harbort
, President and CEO of Talisker, commented, "Intersecting high-grade gold in our first
four holes of the Golden Hornet Project demonstrates the potential for a large, kilometre scale
mineralized system. The Golden Hornet Project is Talisker's first Greenfields drill program, and we
are thrilled to announce the news of this new Discovery. We eagerly await more results to confirm
gold grades from visual mineralization in the remaining holes."
Table 1: Drill Hole Collar Summary Information
Drill Hole
Total Depth
(m)
Azimuth
Dip
Easting
Northing
Elevation
GH-DDH-21-001
351
060
-45
363436
5478599
1106
GH-DDH-21-002
315
060
-45
363482
5478706
1073
GH-DDH-21-003
360
060
-55
363386
5478686
1114
GH-DDH-21-004
431
060
-60
363278
5478640
1139
GH-DDH-21-001 Hole Description:
Collared in strongly hornfels metasediments in contact with strongly silica-albite-biotite altered
equigranular crowded diorite hosting stockwork pyrite veins and veinlets over the top
100m
.
Semimassive pyrite-pyrrhotite+/-arsenopyrite occurrences, 15-25 cm in width, returned 2.79 g/t
Au over
1.95m
from
90.00m
to
91.95m
and 1.27 g/t Au over
4.5m
from 277.50 to
280.50m
.
Broad zones of pyrite-dominated stockworks returned of 0.25 g/t Au over
42.67m
from
51.00m
to
93.67m
and 0.26 g/t Au over
11.15m
from
201.35m
to
212.50m
.
GH-DDH-21-002 Hole Description:
Collared into silica-albite altered crowded equigranular diorite with the purpose to intersect
semi-massive sulphides hosted in brecciated quartz exposed on the surface in historic trenches.
Intersected semi-massive pyrite-pyrrhotite-arsenopyrite hosted in fractured and weakly
brecciated quartz veins returning 1.98 g/t Au over
0.5m
from
32.65m
to
33.20m
,1.21 g/t Au
over
3.28m
from
78.60m
to
82.42m
, and 1.39 g/t over
0.5m
from
135.32m
to135.82m.
Pervasive silica-albite alteration and sulphide veinlets and stockworks decrease with depth
towards the east, with mineralization focused on the near metasediment-intrusive contact zone.
GH-DDH-21-003 Hole Description:
Collared at a greater inclination into strongly hornfels metasediments and is a
50m
step-out to
the NW from hole 001.
Intersected semi-massive pyrite-pyrrhotite-arsenopyrite occurrences, 15-25 cm in width
returning 2.08 g/t Au over
0.5m
from
126.50m
to
127.50m
, 1.66 g/t Au over
0.65m
from
184.50m
to185.15m, 9.99 g/t Au over
0.5m
from 188.00-
188.50m
, 2.05 g/t Au over
0.80m
from
194.00m
to194.80m, 1.12 g/t Au over
1.00m
from 304.50 to
305.50m
, and 11.58 g/t over
1.05m
from
311.95m
to
313.00m
.
A zone of strong pyrite-pyrrhotite stockwork with coincident pervasive silica-albite-biotite
alteration hosting several semi-massive sulphide occurrences returned 0.82 g/t Au over
10.30m
from
184.50m
to
194.80m
within a greater interval of 0.26 g/t Au over
61.5m
from
184.50m
to
218.50m
.
GH-DDH-21-004 Hole Description:
Collared further west into the host metasediments at a greater inclination to test the nature of
the hornfels-metasediment-intrusive contact zone as well as undercut mineralization observed in
GH-DDH-21-003.
Intersected several intrusive fingerlings intruding into the metasediments over the top
80m
with
mineralization coincident or proximal with intrusive contact margins. Values of 1.07g/t Au and
1.01 g/t Au over
1.5m
and
1.12m
respectfully hosted in strong pyrite stockwork intervals and
pervasive silica-albite-biotite alteration.
A significant zone of semi-massive to massive sulphides hosted in and marginal to brecciated
and fractured pre-mineral quartz veins returned values up to
22.73 g/t over
1.10m
within a
greater interval of 8.88 g/t over
5.10m
from
353.90m
to
359.00m
.
Several broad zones of mineralization hosted in stockwork pyrite and lesser pyrrhotite were
intersected returning values of 0.2 g/t Au over
22.5m
from
81.00m
to
102.75m
,
1.38 g/t Au
over
41.10m
from 345.40 to
386.50m
.
Project Overview:
The Hornet Zone represents an intrusion-related gold system (IRGS) where mineralization and
alteration intensity is controlled by localized structures, lithologic contacts, and pre-mineralizing event
veins and breccias, providing permeable conduits for later ore-forming hydrothermal fluids. The
Hornet Zone exhibits a strong alteration zonation decreasing inboard into the host diorite unit from
silica+/-biotite-sericite to sericite-chlorite +/- epidote. Strong continuity of mineralized breccia and
vein zones is observed between drill holes. Mineralized structures are pierced at roughly orthogonal
angles to drill core axis, and therefore true width of intersected intervals are estimated to be 80-90%
of observed widths.
Historic trenching in the Hornet Zone returned channel samples of 22.1 g/t Au over 5.2 metres, 17
g/t Au over 2.0 metres, 4.17 g/t Au over 14 metres.
In addition, broad halos of mineralization surrounding the veins returned intercepts of 1.9 g/t Au
over 21 metres, 1.23 g/t Au over 12.5 metres, 1.32 g/t Au over 17.0 metres and 0.96 g/t gold over
14 metres. The main NW trending high-grade gold veins at the Hornet
Zone outcrop continuously over a 500m x
300m
area. Low-grade mineralization occurs in stockwork
sulphide veinlets between major sheeted vein sets that represent an
additional opportunity for bulk tonnage potential. B-Horizon soil sampling conducted by Talisker in
2020 defined a 2.8km by 1.3km gold soil anomaly (98th percentile) centred on the Hornet Zone.
Table 2: Golden Hornet Project - Drill Holes GH-DDH-21-001-004
Diamond Drill
Hole Name
From
(m)
To
(m)
Interval
(m)
Au
(g/t)
Ag
(g/t)
Cu
(ppm)
Method Reported
GH-DDH-21-001
87.00
88.50
1.50
0.14
2.18
388
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-001
88.50
90.00
1.50
0.22
2.02
366
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-001
90.00
90.95
0.95
2.09
5.96
1973
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-001
90.95
91.95
1.00
3.47
3.65
1409
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-001
91.95
93.00
1.05
0.15
1.72
463
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-001
93.00
93.67
0.67
0.42
2.47
942
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-001
276.00
277.50
1.50
1.11
0.30
127
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-001
277.50
279.00
1.50
1.96
1.05
141
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-001
279.00
280.50
1.50
0.76
0.63
196
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-002
32.65
33.20
0.55
1.98
1.90
708
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-002
78.60
79.10
0.50
3.05
4.41
1160
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-002
79.10
80.40
1.30
0.26
0.44
131
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-002
80.40
81.00
0.60
0.79
0.62
286
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-002
81.00
81.95
0.95
0.09
0.30
96.7
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-002
81.95
82.42
0.47
4.70
31.27
8259
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-002
135.32
135.82
0.50
1.39
2.10
490
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
126.50
127.00
0.50
2.08
2.43
329
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
184.50
185.15
0.65
1.66
1.71
419
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
185.15
186.00
0.85
0.03
0.44
76.8
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
186.00
187.50
1.50
0.03
0.35
57.1
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
187.50
188.00
0.50
0.02
0.13
21.3
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
188.00
188.50
0.50
9.99
3.75
318
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
188.50
190.00
1.50
0.06
0.34
56.8
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
190.00
191.50
1.50
0.33
0.53
107
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
191.50
192.90
1.40
0.02
0.15
29
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
192.90
193.40
0.50
0.02
0.40
88.7
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
193.40
194.00
0.60
0.06
0.59
105
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
194.00
194.80
0.80
2.05
1.70
169
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
206.00
207.00
1.00
0.90
0.84
238
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
210.50
211.00
0.50
0.75
1.05
297
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
218.00
218.50
0.50
1.16
0.78
251
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
233.00
234.00
1.00
0.52
1.00
210
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
304.00
305.00
1.00
1.12
0.70
205
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-003
311.95
313.00
1.05
11.58
11.10
3747
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
81.00
82.50
1.50
1.07
0.49
125
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
101.63
102.75
1.12
1.01
0.61
275
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
216.5
217
0.5
2.17
2.54
598
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
345.40
346.50
1.10
3.37
2.08
616
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
346.50
348.00
1.50
0.06
0.21
77.1
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
348.00
349.50
1.50
0.90
0.37
113
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
349.50
351.00
1.50
0.02
0.23
69.8
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
351.00
352.50
1.50
0.02
0.17
56.8
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
352.50
353.40
0.90
0.01
0.18
65.8
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
353.40
353.90
0.50
0.07
0.53
94.6
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
353.90
355.00
1.10
22.73
16.04
4607
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
355.00
356.00
1.00
5.45
8.68
1650
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
356.00
357.00
1.00
12.81
35.98
10000
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
357.00
357.50
0.50
2.06
16.10
4304
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
357.50
358.00
0.50
1.12
1.38
223
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
358.00
359.00
1.00
0.46
5.44
492
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
359.00
360.50
1.50
0.06
1.86
57.6
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
360.50
362.00
1.50
0.12
0.22
42.9
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
362.00
363.00
1.00
0.03
0.12
33.5
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
363.00
364.00
1.00
3.00
1.43
304
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
364.00
365.50
1.50
1.25
2.18
434
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
365.50
367.00
1.50
0.02
0.26
70.6
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
367.00
368.50
1.50
0.04
0.24
51.2
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
368.50
370.00
1.50
0.01
0.10
20.9
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
370.00
371.50
1.50
0.01
0.38
216
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
371.50
373.00
1.50
0.14
0.50
95.8
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
373.00
374.50
1.50
0.01
0.19
63.2
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
374.50
376.00
1.50
0.01
0.12
38.2
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
376.00
377.50
1.50
0.01
0.17
60.8
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
377.50
379.00
1.50
0.03
0.54
216
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
379.00
380.50
1.50
0.03
0.26
61.1
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
380.50
382.00
1.50
0.02
0.11
38
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
382.00
383.50
1.50
0.02
0.32
135
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
383.50
384.50
1.00
0.15
0.39
105
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
384.50
385.50
1.00
0.16
0.82
158
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
385.50
386.00
0.50
0.02
0.18
79.3
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
GH-DDH-21-004
386.00
386.50
0.50
0.94
3.86
716
GO-FAA50V10, GE-ICP21B20, GE-IMS21B20
Notes: True widths are estimated at 70 - 90% of intercept lengths and are based on oriented core measurements where available.
Method
Reported includes the most up
to
date information as of the date of this press release.
Talisker is providing an opportunity for shareholders and other interested parties to participate in a
Webinar to be held at
4:15 pm ET on Tuesday
, January 25
th
. To register, please click on the
following link –
https://bit.ly/33IKH9w
.
Qualified Person
The technical information contained in this news release relating to the drill results at the Golden
Hornet Project has been approved by
Leonardo de Souza
(BSc, AusIMM (CP) Membership
224827), Talisker's Vice President, Exploration and Resource Development, who is a "qualified
person" within the meaning of National Instrument 43-101, Standards of Disclosure for Mineral
Projects.
About Talisker Resources Ltd.
Talisker (
taliskerresources.com
)
is a junior resource company involved in the exploration of gold
projects in
British Columbia, Canada
. Talisker's projects include two advanced-stage projects, the
Bralorne Gold Complex and the Ladner Gold Project, both advanced-stage projects with significant
exploration potential from historical high-grade producing gold mines, as well as its Spences Bridge
Project where the Company holds ~85% of the emerging Spences Bridge Gold Belt and several
other early-stage Greenfields projects. With its properties comprising 296,983 hectares over
346 claims, three leases and 198 crown grant claims, Talisker is a dominant exploration player in
south-central
British Columbia
. The Company is well funded to advance its aggressive systematic
exploration program at its projects.
Sample Preparation and QAQC
Drill core at the Golden Hornet project is drilled in NQ size(47.6mm). Drill core samples are minimum
50 cm and maximum 160 cm long along the core axis. Samples are focused on an interval of interest
such as a vein or zone of mineralization. Shoulder samples bracket the interval of interest such that a
total sampled core length of not less than
3m
both above and below the interval of interest must be
assigned. Sample QAQC measures of unmarked certified reference materials (CRMs), blanks, and
duplicates are inserted into the sample sequence and make up 9% of the samples submitted to the
lab for holes reported in this release. Sample preparation and analyses is carried out by SGS
Canada in
Burnaby, British Columbia
, Canada. Drill core sample preparation includes drying in an
oven at a maximum temperature of 60°C, fine crushing of the sample to at least 70% passing less
than 2 mm, sample splitting using a riffle splitter, and pulverizing a 250 g split to at least 85%
passing 75 microns (SGS code PRP89). Gold in diamond drill core is analysed by fire assay and
atomic absorption spectroscopy (AAS) of a 50g sample (SGS code GO_FAA50V10), while multi-
element chemistry is analysed by aqua regia digestion of a 0.25 g sample split with detection by
inductively coupled plasma mass spectrometer (ICP-MS) for 18 elements (Al, Ba, Ca, Cr, Cu, Fe, K,
Li, Mg, Mn, Na, P, S, Sr, Ti, Zn, Zr) (SGS code GE_ICP21B20) as well as detection by atomic
emission spectroscopy (AES) for an additional 33 elements (Ag, As, Be, Bi, Cd, Ce, Co, Cs, Ga,
Ge, Hf, Hg, In, La, Lu, Mo, Nb, Ni, Pb, Rb, Sb, Sc, Se, Sn, Ta, Tb, Te, Th, Tl, U, W, Y, Yb) (SGS
code GE_IMS21B20). Gold assay technique (SGS code FAA50V10) has an upper detection limit of
100 ppm. Any sample that produces an over-limit gold value via the gold assay technique is sent for
gravimetric finish (SGS method GO_FAG50V) which has an upper detection limit of 1,000 ppm Au.
Samples where visible gold was observed are sent directly to screen metallics analysis and all
samples that fire assay above 1 ppm Au are re-analysed with method (SGS code - 6 -
GO_FAS50M) which employs a 1kg pulp screened to 100 microns with assay of the entire oversize
fraction and duplicate 50g assays on the undersize fraction. Where possible all samples initially sent
to screen metallics processing will also be re-run through the fire assay with gravimetric finish
provided there is enough material left for further processing.
Caution Regarding Forward-Looking Information
Certain statements contained in this press release constitute forward-looking information. These
statements relate to future events or future performance. The use of any of the words "could",
"intend", "expect", "believe", "will", "projected", "estimated" and similar expressions and statements
relating to matters that are not historical facts are intended to identify forward-looking information
and are based on Talisker's current belief or assumptions as to the outcome and timing of such
future events. Actual future results may differ materially. Those assumptions and factors are based
on information currently available to Talisker. Although such statements are based on reasonable
assumptions of Talisker's management, there can be no assurance that any conclusions or forecasts
will prove to be accurate.
While Talisker considers these statements to be reasonable based on information currently
available, they may prove to be incorrect. Forward-looking information involves known and unknown
risks, uncertainties and other factors which may cause the actual results, performance or
achievements to be materially different from any future results, performance or achievements
expressed or implied by the forward-looking information. Such factors include market risks and the
demand for securities of the Company, risks inherent in the exploration and development of mineral
deposits, including risks relating to changes in project parameters as plans continue to be redefined,
risks relating to variations in grade or recovery rates, risks relating to changes in mineral prices and
the worldwide demand for and supply of minerals, risks related to increased competition and current
global financial conditions and the COVID-19 pandemic, access and supply risks, reliance on key
personnel, operational risks, and regulatory risks, including risks relating to the acquisition of the
necessary licenses and permits, financing, capitalization and liquidity risks.
The forward-looking information contained in this news release is made as of the date hereof, and
Talisker is not obligated to update or revise any forward-looking information, whether as a result of
new information, future events or otherwise, except as required by applicable securities laws.
Because of the risks, uncertainties and assumptions contained herein, investors should not place
undue reliance on forward-looking information. The foregoing statements expressly qualify any
forward-looking information contained herein.
Figure 1: High-grade semi-massive quartz sulphide breccia averaging 8.88 g/t Au, 0.42% Cu and
14.99 g/t Ag over 5.1m Au. (CNW Group/Talisker Resources Ltd)
Figure 2: Section showing holes GH-DDH-21-001-004 with interpreted geology and gold
intersections. (CNW Group/Talisker Resources Ltd)
Figure 3: 2020 Regional Geochemistry with Geology and Drill Collar Locations. (CNW
Group/Talisker Resources Ltd)
Figure 4: Drill Collar locations overlaid on geology and geochemistry within the Main Hornet Zone.
(CNW Group/Talisker Resources Ltd)
Figure 5: All drill hole locations showing strike extent between the Main Hornet Zone and the Iron
Sky Zone. (CNW Group/Talisker Resources Ltd)
SOURCE
Talisker Resources Ltd
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For further information:
Terry Harbort, President and CEO, [email protected],
+1 416 361 2808
CO: Talisker Resources Ltd
CNW 07:00e 19-JAN-22