Juggernaut Drills 1.56 Gpt AuEq over 5 Meters ON Midas and Confirms Extensive Mineralized GOLD Rich Vhms System, Golden Triangle, B.c. 2023 Drilling Highlights:
JUGGERNAUT DRILLS 1.56 GPT AUEQ OVER 5 METERS ON
MIDAS AND CONFIRMS EXTENSIVE MINERALIZED GOLD
RICH VHMS SYSTEM, GOLDEN TRIANGLE, B.C.
2023 DRILLING HIGHLIGHTS:
• Extensive broad copper-zinc-gold rich intervals consisting of considerable chalcopyrite and pyrite
in aggregates, stringers and veinlets have been intersected in multiple drill holes collared from an
area encompassing the VG Zone and Kokomo showing consistent with a Volcanogenic Hosted
Massive Sulphide (VHMS) system. MAP WITH HIGHLIGHTED DRILL HOLES AND TREND
• Drill hole MD-23-34 intersected 1.56 gpt AuEq (0.35 gpt Au, 6.10 gpt Ag, 0.64 % Cu and 0.67 % Zn)
over 5.00 meters, within 0.68 gpt AuEq (0.22 gpt Au, 2.73 gpt Ag, 0.20 % Cu and 0.38 % Zn) over
22.00 meters. Additional intervals in this hole include 0.70 gpt AuEq (0.24 gpt Au, 2.93 gpt Ag, 0.64
% Cu and 0.70 % Zn) over 10 meters and 0.54 gpt AuEq (0.18 gpt Au, 1.70 gpt Ag, 0.09 % Cu and
0.53 % Zn) over 8.00 m. MD-23-34 PHOTO
• Drill hole MD-23-35 intersected 0.53 gpt AuEq (0.18 gpt Au, 1.64 gpt Ag, 0.11 % Cu and 0.47 % Zn)
over 20.00 meters, including 1.41 gpt AuEq (0.38 gpt Au, 3.62 gpt Ag, 0.32 % Cu and 1.40 % Zn) over
3.00 meters and 1.07 gpt AuEq (0.39 gpt Au, 2.48 gpt Ag, 0.28 % Cu and 0.69 % Zn) over 3.00 meters.
MD-23-35 PHOTO
• Drill hole MD -23-36 intersected 1.76 gpt AuEq (0.79 gpt Au, 16.60 gpt Ag, 0.58 % Cu) over 1.00
meter, within 0.45 gpt AuEq (0.19 gpt Au, 4.30 gpt Ag, 0.15 % Cu) over 6.00 meters. An additional
interval in this hole assayed 0.29 gpt AuEq (0.16 gpt Au, 1.69 gpt Ag, 0.14 % Zn) over 32 meters.
MD-23-36 PHOTO
• Drill hole MD-23-46 intersected 2.40 gpt AuEq (1.30 gpt Au, 8.92 gpt Ag, 0.74 % Cu) over 1.00 meter.
• The mineralized horizons consist of aggregates, stringers, and veinlets of chalcopyrite (up to 10 %),
sphalerite (up to 5 %) and pyrite (up to 15 %) in a strongly quartz-sericite altered volcanic host rock
consistent with being in close proximity to an Eskay-style Volcanogenic Hosted Massive Sulphide
(VHMS) deposit.
• Drill holes MD -23-34, MD-23-35 and MD -23-36 were collared from Eskay 1 Pad, located 550 m
south of the gold-silver-copper-zinc rich Kokomo showing (9.343 gpt Au, 117 gpt Ag, 1.58 % Cu and
1.77 % Zn), 250 m northeast of drill hole MD -19-18 (6.22 m of 0.31 gpt Au, 0.95 m of 1.50 gpt Au
with 1.94 % Cu and 3.22 m of 0.36 gpt Au) and 200 m east-northeast of the VG Zone (2.24 gpt Au,
6.83 gpt Ag, 0.18 % Cu and 1.04 % Zn over 4.80 meters).
• The 2023 drill results in combination with results from previous years indicate an extensive north-
south gold-copper-zinc rich mineralized trend that remains open extending for 550 m from Eskay
1 Pad to the Kokomo showing on strike with a large relatively shallow Induced Polarization (IP)
chargeability and resistivity anomaly. The gold and base metals component clearly increases
towards the Kokomo showing, strongly indicating proximity to the heart of a VHMS deposit.
• 2024 drilling will be designed to unlock the full mineral potential of the 550 m by 300 m high-grade
mineralization trend between Eskay 1 Pad and the Kokomo showing, focusing on the not yet drill-
tested Kokomo showing close to the heart of the system. 2024 DRILL PLAN MAP
HIGHLIGHTS FROM THE MIDAS PROPERTY:
• Historic drill results from the Midas property include hole MD-18-16 which intersected the peripheral
zone of the IP anomaly and returned 0.56 g/t AuEq over 35.35 meters; hole MD-18-08, which assayed
6.85 gpt Au over 9 meters and narrowly missed a strong IP chargeability anomaly core; and hole MD-
18-01 which intersected 3.27 gpt AuEq over 4.80 meters and ended before it reached the core of a
strong IP chargeability anomaly.
• Channel samples highlights from the VG Zone include 10.28 gpt Au over 4.34 meters; 15.37 gpt Au
over 2 meters; and 5.43 gpt Au over 3.11 meters.
• Multiple high-grade gold grab, chips and channel samples including Kokomo showing where a 1 m
chip sample assayed 9.343 gpt Au, 117 gpt Ag, 1.58 % Cu and 1.77 % Zn.
• Relatively shallow Induced Polarization (IP) chargeability and resistivity anomaly extends under the
Kokomo showing for at least 550 meters on trend to the south conducive for semi-massive to massive
sulphides.
• Alteration zones extracted from Worldview 3 satellite spectral data show a strong silica, iron and
phyllic alteration (quartz -sericite-pyrite) signature overlapping the Kokomo showing and the 550
meter trend immediately to the south coinciding with the IP anomaly in the subsurface , further
indicating the presence of a mineralized VHMS system at depth. 2023 Midas Alteration MAP
• Regional and local geology is highly prospective for VHMS deposits including the presence of a
rhyolitic tuff with strong phyllic alteration (quartz-sericite-pyrite) from the Mt Attree volcanics which
are Mississippian in age. Mississippian age rocks are known to host the majority of significant VHMS
deposits.
• Widespread Zn signature with secondary Au, Ag, Pb, Cu and trace element signature (elevated Au,
Te, As, Sb, Bi, Cd, Hg, Ba).
• Midas is within a world class geologic setting with strong potential for Eskay -style VHMS
mineralization. Midas Summary
ESKAY-STYLE KOKOMO VHMS TARGET HIGHLIGHTS:
• The 3D inversion of the 2018 Induced Polarization (IP) data performed by an independent geophysical
company highlighted a 120 m by 150 m chargeability anomaly and a 350 m by 200 m resistivity
anomaly from surface to 200 m depth that remains open to the South and East conducive for semi -
massive to massive sulphides like those confirmed on surface at Kokomo. 3D IP inversion map
• Kokomo is an Eskay-style VHMS showing with a 1 m chip sample assaying 9.343 gpt Au, 117 gpt Ag,
1.58 % Cu and 1.77 % Zn. The outcrop remains open in all directions where outcrops of the same or
similar lithology extend over several hundred meters. Photo VHMS Y606015
• A BLEG sample collected 700 m down-slope in the drainage of the Kokomo showing assayed 29 ppb
Au, 613 ppb Ag, 137 ppm Cu, 54.4 ppm Pb and 462 ppm Zn, by far the highest BLEG sample recorded
on the property and is coincident with a similar geochemical signature as the Kokomo showing.
• Two outcrop grab samples collected within 50 m of the Kokomo showing in 2017 and 2018 assayed
1.835 gpt Au (with 34.4 gpt Ag, 0.84 % Cu, 0.03 % Pb and 0.79 % Zn) and 2.29 gpt Au (with 21.3 gpt
Ag, 0.01 gpt Cu, 0.00 % Pb and 0.02 % Zn). Photo - B066625 labelled
• The host rock to the Kokomo showing has been mapped by Juggernaut former senior geologist S.
Roach as well as the British Columbia Geological Survey (BCGS; M. McKeown, J. Nelson and R.
Friedman, 2007) as a rhyolitic tuff with strong phyllic alteration (quartz-sericite-pyrite) from the Mt
Attree volcanics, a unit highly prospective for VHMS deposits.
• In 2019, hole MD -19-24 collared 300 m Southwest of the Kokomo showing with an azimuth of 090
and a dip of 50 intersected the fringes of the chargeability and resistivity anomalies highlighted by
the recent 3D inversion modeling of the IP data containing disseminated sulphide mineralization
(mainly pyrite and minor sphalerite) in the bottom half of the hole assaying up to 0.293 gpt Au and
2.8 % Zn closest to the Kokomo discovery outcrop. (See news release September 30, 2019)
• The geology, geochemistry, alteration, and extensive underlying geophysical anomaly coupled with
the high-grade polymetallic Au, Ag, Cu and Zn mineralization in semi -massive to massive sulphides
seen in outcrop at Kokomo strongly indicates the potential of a new Eskay-style VHMS discovery.
Vancouver, British Columbia – December 19, 2023 – Juggernaut Exploration Ltd (JUGR.V) (OTCQB: JUGRF)
(FSE: 4JE) (the “Company” or “Juggernaut”) is pleased to report the assay results from the 2024 drill
program on its 100 % controlled Midas property (the “Property”), Golden Triangle, British Columbia. Drill
hole MD-23-34 collared from Eskay 1 Pad intersected 1.56 gpt AuEq (0.35 gpt Au, 6.10 gpt Ag, 0.64 % Cu
and 0.67 % Zn) over 5.00 meters, within 0.68 gpt AuEq (0.22 gpt Au, 2.73 gpt Ag, 0.20 % Cu and 0.38 % Zn)
over 22.00 meters. All three holes collared from Eskay 1 Pad located at the transition from the VG Zone to
the Kokomo Zone have intersected considerable gold-copper-zinc mineralization and are characterized by
copious amounts of chalcopyrite and pyrite in aggregates, stringers, and veinlets within a strongly altered
volcanic host rock indicating close proximity to an Eskay-style Volcanogenic Hosted Massive Sulphide (VHMS)
deposit. The 2023 drill results in combination with results from previous years indicate an extensive north -
south gold-copper-zinc rich mineralized trend that remains open extending for 550 m by 300 m from Eskay 1
Pad to the Kokomo showing on strike with a large relatively shallow Induced Polarization (IP) chargeability
and resistivity anomaly. The gold and base metals component clearly increased towards the Kokomo
showing, strongly indicating proximity to the heart of a VHMS deposit.
MAP WITH HIGHLIGHTED DRILL HOLES AND TREND
Drill hole MD-23-34 intersected 1.56 gpt AuEq (0.35 gpt Au, 6.10 gpt Ag, 0.64 % Cu and 0.67 % Zn) over 5.00
meters, within 0.68 gpt AuEq (0.22 gpt Au, 2.73 gpt Ag, 0.20 % Cu and 0.38 % Zn) over 22.00 meters.
Additional intervals in this hole include 0.70 gpt AuEq (0.24 gpt Au, 2.93 gpt Ag, 0.64 % Cu and 0.70 % Zn)
over 10 meters and 0.54 gpt AuEq (0.18 gpt Au, 1.70 gpt Ag, 0.09 % Cu and 0.53 % Zn) over 8.00 m. MD-23-
34 PHOTO. Drill hole MD-23-35 intersected 0.53 gpt AuEq (0.18 gpt Au, 1.64 gpt Ag, 0.11 % Cu and 0.47 %
Zn) over 20.00 meters, including 1.41 gpt AuEq (0.38 gpt Au, 3.62 gpt Ag, 0.32 % Cu and 1.40 % Zn) over
3.00 meters and 1.07 gpt AuEq (0.39 gpt Au, 2.48 gpt Ag, 0.28 % Cu and 0.69 % Zn) over 3.00 meters. MD-
23-35 PHOTO Drill hole MD-23-36 intersected 1.76 gpt AuEq (0.79 gpt Au, 16.60 gpt Ag, 0.58 % Cu) over
1.00 meter, within 0.45 gpt AuEq (0.19 gpt Au, 4.30 gpt Ag, 0.15 % Cu) over 6.00 meters. An additional
interval in this hole assayed 0.29 gpt AuEq (0.16 gpt Au, 1.69 gpt Ag, 0.14 % Zn) over 32 meters. MD-23-36
PHOTO In all three holes, the mineralization is cut off by a north-northeast trending, steeply dipping fault.
The mineralized horizon consists of aggregates, stringers, and veinlets of chalcopyrite (up to 10 %) and
pyrite (up to 15 %) in a strongly quartz-sericite altered volcanic host rock with occasional foliated portions
that align with the north-northeast direction of major faults in the area. A series of meter-size mafic dykes
intrude into the mineralized rock.
Table 1: Selected 2023 Midas drill hole assay results reported in this news release.
Pad ID Hole ID From
(m)
To
(m)
Interval
(m) Au (gpt) Ag (gpt) Cu (%) Pb (%) Zn (%) AuEq
(gpt)
Eskay 1 MD-23-34
Interval 12 20 8 0.18 1.70 0.09 0.01 0.53 0.54
Interval 23 33 10 0.24 2.93 0.13 0.01 0.64 0.70
Interval 35 57 22 0.22 2.73 0.20 0.02 0.38 0.68
Including 47 52 5 0.35 6.10 0.64 0.05 0.67 1.56
Eskay 1 MD-23-35
Interval 6 26 20 0.18 1.46 0.11 0.01 0.47 0.54
Including 6 9 3 0.38 3.62 0.32 0.01 1.40 1.41
Including 20 23 3 0.39 2.48 0.28 0.01 0.69 1.07
Eskay 1 MD-23-36
Interval 1 33 32 0.16 1.69 0.04 0.01 0.14 0.29
Interval 167 173 6 0.19 4.30 0.15 0.001 0.04 0.45
Including 172 173 1 0.79 16.60 0.58 0.001 0.01 1.76
Kokomo 2 MD-23-46 Interval 95 96 1 1.30 8.92 0.74 0.001 0.01 2.40
Drill holes MD-23-34, MD-23-35 and MD-23-36 were collared from Eskay 1 Pad, located 550 m south of the
gold-silver-copper-zinc rich Kokomo showing (9.343 gpt Au, 117 gpt Ag, 1.58 % Cu and 1.77 % Zn), 250 m
northeast of drill hole MD-19-18 (6.22 m of 0.31 gpt Au, 0.95 m of 1.50 gpt Au with 1.94 % Cu and 3.22 m of
0.36 gpt Au) and 200 m east -northeast of the VG Zone (2.24 gpt Au, 6.83 gpt Ag, 0.18 % Cu and 1.04 % Zn
over 4.80 meters). The distribution of the mineralization shows based on results from the 2023 drilling, in
combination with results from previous years, mapping , and geophysical surveys , clearly define a large,
mineralized trend extending for 550 meters by 300 meters between Eskay 1 Pad and the Kokomo showing.
The same trend is seen in the subsurface geophysical IP data and remains open. Geochemical results
confirmed in drill core and outcrop clearly show a significant increase in gold and base metal values near the
Kokomo showing strongly indicating that the heart of the VHMS deposit lies in very close proximity. This
vector to the core of the mineralization is also supported by multiple other lines of evidence including the
large open IP anomaly, structures, and mapping.
2024 Drill Plan
Based on the new results from the 2023 drill program and a thorough compilation of data from previous drill
campaigns and exploration programs on the Property, including geochemistry, geophysics and mapping, that
have allowed to vector-in and strongly point to the heart of the VHMS system, a drill plan designed to outline
the full VHMS potential of the 550 m by 300 m north-south trend between the Eskay 1 Pad and the Kokomo
showing has been prepared. The drilling is designed to specifically target the 550 m by 300 m area between
the Eskay 1 Pad and the Kokomo showing that is strongly indicated to contain the heart of the gold rich VHMS
system. 3D MODEL
Due to a challenging drill environment and an underpowered light drill rig used, the Kokomo target was not
able to be tested. The 2024 drilling is designed to overcome the challenges seen in 2023 by using a larger ,
more powerful drill rig . The Kokomo showing consists of a VHMS style outcrop where a 1 m chip sample
assayed 9.343 gpt Au, 117 gpt Ag, 1.58 % Cu and 1.77 % Zn. The outcrop is 5 m wide and strikes on surface
for 30 m and remains open and is underlain by an extensive strong 550 m long Induced Polarization (IP)
chargeability and resistivity anomaly that remains open, conducive for semi-massive to massive sulphides
like those confirmed on surface on the Kokomo showing.
MIDAS 2024 DRILL PLAN MAP
Table 2: Collar information for the drill holes reported in this news release.
Pad ID Hole ID Easting Northing Grid Azimuth Dip Length (m)
Kokomo 2 MD-23-46 543495 6023013 NAD83 / UTM zone 9N 310 48 129
Eskay 1 MD-23-36 543336 6022836 NAD83 / UTM zone 9N 160 65 243
Eskay 1 MD-23-35 543337 6022835 NAD83 / UTM zone 9N 35 70 240
Eskay 1 MD-23-34 543338 6022836 NAD83 / UTM zone 9N 90 60 123
Eskay-Style Kokomo VHMS target
The 3D inversion of the 2018 Induced Polarization data performed by an independent geophysical company
highlighted a 120 m by 150 m chargeability anomaly and 350 m by 200 resistivity anomalies from surface to
200 m depth that remain open to the South and E ast conducive for semi-massive to massive sulphides like
those confirmed on surface at Kokomo. Most likely the chargeability (30 -70 mrads) and resistivity (100-500
Ohm-m) signature are due to a combination of relatively large volumes of interconnected metallic sulphides
such as chalcopyrite and pyrite in combination with slightly more resistive material such as sphalerite and
strongly silicified domains.
The Kokomo showing has been mapped by the British Columbia Geological Survey (BCGS; M. McKeown, J.
Nelson and R. Friedman, 2007 ) as a conformable sequence of layered Paleozoic felsic to mafic subaqueous
volcaniclastic rocks including lenses of massive sulphide surrounded by an extensive alteration zone
consistent with VHMS deposits as described at the nearby Sub showing located 400 m NW from the Kokomo
showing. Samples collected by the BCGS from the Sub showing returned 0.275 gpt Au, 18.3 gpt Ag, 0.02 %
Cu, 0.31 % Pb and 0.44 % Zn (Photo – BCGS Nelson Figure8). JoAnne Nelson (BCGS) stated in her report (on
page 112) that the Sub and Gazelle showings demonstrate mineralization indicative of a VHMS deposit, most
likely peripheral VHMS feeder zone below the seafloor, that have been discovered in an intensely altered
body within the Mt Attree volcanics. The stratigraphy in the area includes andesiste, rhyolite and rhyolitic tuff
of the Mt Attree formation which are Mississipian in age known to host the majority of significant VHMS
deposits (Midas Age). Alteration includes quartz-sericite-pyrite (phyllic alteration), silicification and Fe -rich
chlorite (including an intense depletion of Na 2O and CaO) increasing in intensity from west to east. This
alteration pattern is useful in providing a vector to the centre of the system (Midas Alteration) The area is
characterized by a widespread Zn signature with secondary Au, Ag, Pb, Cu and trace element signature
(elevated Au, Te, As, Sb, Bi, Cd, Hg, Ba) indicative of VHMS systems (Midas Geochemistry).
The Kokomo target has strong potential to evolve into a significant new VHMS discovery which is supported
by known mineralization, grade, alteration and textures observed at surface and most recently by the
chargeability and resistivity anomalies highlighted by the 3D inversion of the IP data. The latter is confirmation
of the continuation of the system at depth which remains open to the east and to the south making the
Kokomo showing a strong drill target.
The Midas Property
The Midas property is 100% controlled and covers 20,803 hectares and is located 24 km southeast of Terrace,
British Columbia in close proximity to logging access roads, power, railway and major infrastructure. The
property is located in an area of recent glacial abatement and permanent snowpack recession at the southern
end of the Golden Triangle, British Columbia. Multiple high-grade gold grab, chips and channel samples were
collected from the Kokomo VHMS target where a 1.00 m chip sample assayed 9.343 gpt Au, 117 gpt Ag, 1.58
% Cu and 1.77 % Zn and is drill ready. Relatively shallow Induced Polarization (IP) chargeability and resistivity
anomalies extend under the Kokomo showing on trend to the south for at least 550 m towards the Eskay 1
Pad, conducive for a buried VHMS containing semi-massive to massive sulphides at depth. Channel samples
highlights from the VG Zone include 10.28 gpt Au over 4.34 meters; 15.37 gpt Au over 2 meters; and 5.43 gpt
Au over 3.11 meters. Historic drill results from the Midas property include hole MD-18-16 which intersected
the peripheral zone of the IP anomaly core and returned 0.56 g/t AuEq over 35.35 meters; hole MD -18-08,
which assayed 6.85 gpt Au over 9 meters and narrowly missed a strong IP chargeability anomaly; and hole
MD-18-01 which intersected 3.27 gpt AuEq over 4.80 meters and ended before it reached the core of a strong
IP chargeability anomaly.
Dan Stuart, President and CEO of Juggernaut Exploration states : “It is exciting to see the right type of
mineralization and alteration in drill core from the Midas property. We are confident based on drill results
and multiple other lines of evidence that our 2024 drill plan is targeting the heart of a gold rich VHMS system
that all the data indicates is sitting below the Kokomo showing. Drilling in 2024 will focus on unlocking the
full potential of the 550 m by 300 m high-grade mineralized trend. We are on track for discovery.”
EMPIRE PROPERTY DRILLING UPDATE
Drilling at the Metallica Zone on the Empire property didn’t return significant assay results. Additional
detailed data compilation, interpretation and modeling is required to determine the extent and distribution
of the gold mineralization on the Empire property and understand its remaining gold potential.
Qualified Person
Rein Turna P . Geo is the qualified person as defined by National Instrument 43-101, for Juggernaut Exploration
projects, and supervised the preparation of, and has reviewed and approved, the technical information in this
release.
Other
Oriented HQ-diameter or NQ-diameter diamond drill core from the drill campaign is placed in core boxes by
the drill crew contracted by the Company. Core boxes are transported by helicopter to the staging area, and
then transported by truck to the core shack. The core is then re -orientated, meterage blocks are checked,
meter marks are labelled, Recovery and RQD measurements taken, and primary bedding and secondary
structural features including veins, dykes, cleavage, and shears are noted and measured. The co re is then
described and transcribed in MX Deposit. Drill holes were planned using Leapfrog Geo and QGIS software and
data from the 2017 -2022 exploration campaigns. Drill core containing quartz breccia, stockwork, veining
and/or sulphide(s), or notable alteration are sampled in lengths of 0.5 to 1.5 meters. Core samples are cut
lengthwise in half, one -half remains in the box and the other half is inserted in a clean plastic bag with a
sample tag. Standards, blanks and duplicates were added in the sample stream at a rate of 10%
Grab, channels, chip and talus samples were collected by foot with helicopter assistance. Prospective areas
included, but were not limited to, proximity to MINFile locations, placer creek occurrences, regional soil
anomalies, and potential gossans based on high-resolution satellite imagery. The rock grab and chip samples
were extracted using a rock hammer, or hammer and chisel to expose fresh surfaces and to liberate a sample
of anywhere between 0.5 to 5.0 kilograms. All sample sites were flagged with biode gradable flagging tape
and marked with the sample number. All sample sites were recorded using hand-held GPS units (accuracy 3-
10 meters) and sample ID, easting, northing, elevation, type of sample (outcrop, subcrop, float, talus, chip,
grab, etc.) and a description of the rock were recorded on all-weather paper. Samples were then inserted in
a clean plastic bag with a sample tag for transport and shipping to the geochemistry lab. QA/QC samples
including blanks, standards, and duplicate samples were inserted regularly into the sample sequence at a rate
of 10%.
All samples, including core, rock grabs, channels, and talus samples, are transported in rice bags sealed with
numbered security tags. A transport company takes them from the core shack to the ALS labs facilities in
North Vancouver. ALS is either certified to ISO 9001:2008 or accredi ted to ISO 17025:2005 in all of its
locations. At ALS samples were processed, dried, crushed, and pulverized before analysis using the ME-MS61
and Au-SCR21 methods. For the ME -MS61 method, a prepared sample is digested with perc hloric, nitric,
hydrofluoric and hydrochloric acids. The residue is topped up with dilute hydrochloric acid and analyzed by
inductively coupled plasma atomic emission spectrometry. Overlimits were re-analyzed using the ME-OG62
and Ag-GRA21 methods (gravimetric finish). For Au -SCR21 a large volume of sample is needed (typically 1 -
3kg). The sample is crushed and screened (usually to -106 micron) to separate coarse gold particles from fine
material. After screening, two aliquots of the fine fraction are analys ed using the traditional fire assay
method. The fine fraction is expected to be reasonably homogenous and well represented by the duplicate
analyses. The entire coarse fraction is assayed to determine the contribution of the coarse gold.
Some of the reported data is historical in nature and is a compilation of third-party data from previous
operators. The reader is cautioned that grab samples are spot samples which are typically, but not exclusively,
constrained to mineralization. Grab samples are selective in nature and collected to determine the presence
or absence of mineralization and are not intended to be representative of the material sampled. In addition,
the reader is cautioned that proximity to known mineralization does not guarantee similar mineralization will
exist on the properties.
For more information, please contact:
Juggernaut Exploration Ltd.
Dan Stuart
President and Chief Executive Officer
Tel: (604)-559-8028
www.juggernautexploration.com
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Certain disclosure in this release may constitute forward -looking statements that are subject to numerous
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