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COBRE LIMITED Capital/Financing Update 2025

Nov 23, 2025

64610_rns_2025-11-23_d4361e5d-9a63-40db-9a49-327afb47db8b.pdf

Capital/Financing Update

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Cobre Limited A.C.N. 626 241 067 ( ASX: CBE ) Level 10, Kyle House, 27 Macquarie Place SYDNEY NSW 2000 Tel: + 61 407 123 143 www.cobre.com.au

24 November 2025

ASX Limited - Company Announcements Platform

LARGE STEP-OUT HOLE SHOWS STRIKE CONTINUITY OF HIGH-GRADE COPPER

Cosmos Target, Ngami Copper Project, Botswana

______________

Cobre Limited (ASX: CBE , Cobre or Company ) is pleased to announce early results from the Cosmos Target drill programme ( see ASX announcement 23 October 2025 ) on its wholly owned Ngami Copper Project ( NCP ), Botswana.

HIGHLIGHTS:

  • Visual mineralisation estimates, substantiated by pXRF analysis, have defined a promising intersection of vein, cleavage and fracture hosted chalcocite mineralisation in drill hole NCP68 located 400m along strike from NCP55 which includes 10.0m @ 1.32% Cu & 27.7g/t Ag ( see ASX announcement 3 February 2025[1] );

  • Results provide encouragement for a laterally extensive (>400m) higher-grade copper silver zone at Cosmos; and

  • Based on these encouraging preliminary results, two further infill diamond drill holes, located on either side of NCP55, have been added to the drill programme.

The expanded drill programme will corroborate the continuity of higher-grade copper and silver mineralisation at the Cosmos Target. The higher grades at Cosmos may provide opportunity for both In-Situ Copper Recovery ( ISCR ) and conventional underground mining.

Commenting on the early results from the Cosmos Target Drill Programme, Adam Wooldridge, Cobre’s Chief Executive Officer, said:

“This is a great start to the Cosmos drill programme with early results confirming the higher background copper grades at this extensive target. The next two drill holes will provide important indicators of grade continuity and variability which will guide our follow-up programme.”

1 Refer to the “ References ” section at the end of this announcement.

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The Cosmos Target is located approximately 8 km along strike from the Comet Deposit ( 11.5Mt @ 0.52% Cu and 11.6 g/t A g indicated and inferred resource[2] ) and includes approximately 5km of strike length of anomalous copper silver mineralisation defined by 2km wide spaced diamond drilling. Cosmos is part of the greater NCP Exploration Target (estimated at 205 to 308 million tonnes at 0.31 to 0.46 % Cu & 5.5 to 8.3 g/t Ag – refer footnote 2 ), with evidence for higher grade zones which may be economic from an underground mining perspective highlighted by drill hole NCP55 ( see ASX announcement 4 August 2025 ).

Cautionary Statement: The potential quality and grade of the Exploration Target is conceptual in nature. There has been insufficient exploration to estimate a Mineral Resource and there is no certainty that further exploration work will result in the determination of a Mineral Resource.

The ongoing drill programme at Cosmos was originally designed to assess the strike continuity of higher-grade mineralisation intersected in NCP55 on 400m step-outs and consisted of two diamond drill holes totalling 496m. Based on visual estimates supported by pXRF measurements, NCP67, located to the northeast of NCP55 returned relatively average copper grades. However, the intersection in NCP68, located 400m to the southwest of NCP55, appears more significant, comprising notable vein, fracture and cleavage hosted chalcocite mineralisation logged over 6m from 198 to 204m downhole (approximately 4m true width). Based on these results, the drill programme has been extended to include two additional infill holes. Assay results are expected towards the end of January 2026.

Figure 1 illustrates the location of the Cosmos Target with drill collars for the current drill programme overlain. An oblique drill section is provided in Figure 2 for NCP68. A lithological and mineralisation log along with core photos is provided in Figure 3 . Drill hole collar postions for the current programme are provided in Table 1 below.

Table 1 . Location of 2025 Cosmos Drill Holes

Table 1. Location of 2025 Cosmos Drill Holes Table 1. Location of 2025 Cosmos Drill Holes
Hole ID
X
Y
Inclination
Azimuth
Depth
Status
NCP67 609,304
7,689,840
-60
330
239.53
Complete
NCP68 608,577
7,689,512
-60
330
245.65
Complete
NCP69 608,767
7,689,570
-60
330
~250
In progress
NCP70 609,125
7,689,750
-60
330
~250
Planned

2 Refer to the “ ASX Listing Rule Information Relating to the JORC MRE & Exploration Target ” at the end of this announcement.

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ntested stri e
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Figure 1. Locality map illustrating the position of the Cosmos Target relative to NCP drilling with ongoing 2025 drill programme highlighted in the inset (top).

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Figure 2. Oblique 3D section illustrating the location of NCP68 along strike from NCP55. Note this hole has been drilled from footwall (FW) to hangingwall (HW) which has provided better intersection angles on the sub-vertical overturned mineralised contact. The outline of the Exploration Target for NCP is highligh d alo g wi h h low rmo cycl of h r duc d D’Kar Forma io (HW) which ho copp r- silver mineralisation.

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op cu u
op cu
i era isa o t e Cu easure e ts
Es ated cha cocite abu da ce
ein and fracture hosted cha cocite minera isa on
ine rained disseminated cha cocite minera isa on
----- End of picture text -----

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Figure 3. Graphical log with mineralisation and pXRF spot measurement logs (both top-cut @ 2%). Selected core photos illustrating the mineralised contact, (A) vein related and (B) mineralisation are provided.

Visual Mineralisation Logging and Disclaimers

Detailed logging of mineralisation including type, setting and abundance has been combined with spot portable XRF measurements taken at 10cm intervals to verify the results. Drill core is currently being cut and sampled and will be sent for assays in the coming week. Assay results are anticipated towards the end of January 2026. A visual mineralisation log is provided in Table 2 below.

Table 2 . Mineralisation abundance from logging, NCP68.

From To Min. #1 Style % Min. #2 Style % Comments
195.25 195.45 Chalcocite Vein 0.2 Chrysocolla Vein 0.1
198.56 199.07 Chalcocite Vein 0.2 Rutile 0.1
199.07 199.58 Chalcocite Vein 1 Specularite Vein 1
199.41 199.58 Chalcocite Vein 3

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199.58 199.75 Chalcocite Foliation 0.4 Specularite Disseminat
ed
1 %.
199.75 199.86 Chalcocite Vein 7
199.86 205.9 Chalcocite Foliation 0.3 Specularite Foliation 0.5 Mineralization is
predominantly along
foliation
205.9 211.7 Specularite Foliation 0.2 Predominantly on
the SLT zones.
231.4 233.04 Chalcocite Vein 0.4 Specularite Vein 0.8 1% at the interval
233.02-233.06m
235.75 235.77 Chalcocite Vein 0.1
241.3 241.42 Chalcopyrite Foliation 0.1 Galena Foliation 0.1
244.03 245.65 Pyrite Disseminated 0.5

Visual estimates of mineral abundance should never be considered a proxy or substitute for laboratory analyses where concentrations or grades are the factor of principal economic interest. Visual estimates also potentially provide no information regarding impurities or deleterious physical properties relevant to valuations.

pXRF analyses are only indicative of mineralisation grade and should not be considered equivalent of laboratory analyses. Laboratory assays are expected in late January 2026.

Geology and Mineralisation

Mineralisation at NCP is sedimentary-hosted, structurally controlled, copper-silver associated with the redox contact between oxidised Ngwako Pan Formation red beds and overlying reduced marine sedimentary roc s of the D’Kar ormation on the imbs of anticlinal structures. Drilling has focussed on the southern anticlinal structure which extends for over 40km across the NCP with evidence for anomalous Cu-Ag mineralisation on both northern and southern limbs. Drilling results to date have returned consistent, wide intersections of anomalous to moderate-grade Cu-Ag values over extensive strike lengths with smaller structurally controlled higher-grade zones. This style of mineralisation is dominated by fine-grained chalcocite which occurs along cleavage planes (S1) and in fractures rather than the vein hosted bornite with chalcopyrite more typical of the KCB style. Importantly, the chalcocite mineralisation is amenable to acid leaching, occurs below the water table and is associated with well-developed fracture zones bounded by more competent hanging and footwall units satisfying key considerations for ISCR.

Target Model

The NCP area is located near the northern margin of the KCB and includes significant strike of subcropping Ngwako Pan / D’Kar ormation contact on which the majority of the nown deposits in the KCB occur.

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Cobre is aimin to prove up a simi ar ISCR process to Tase o Mines Ltd’s (TSX:TKO, NYSE:TG ) orence Copper Deposit (320Mt @ 0.36% Cu) and Copper ox’ an Dy e Deposit[3] (265.6Mt @ 0.29% Cu) in Arizona which both share a similar scale to NCP[4] .

REFERENCES

For further information including full exploration results references, Competent Persons Statement and JORC Tables related to the quoted Mineral Resource Estimate ( MRE ) and assay results from drill hole NCP55 please refer to the following ASX Announcements:

23-Oct-25 Cosmos Exploration Drilling
4-Aug-25 Maiden MRE Comet & Major Increase to NCP Exploration Target
3-Feb-25 Cu-Ag Assay Results Unlock New Discovery- Ngami Project

ASX LISTING RULE INFORMATION RELATING TO THE JORC MRE & EXPLORATION TARGET

JORC MRE

JORC MRE
Mineral Resource
Classification
Tonnage
(Mt)
Cu Grade
(%)
Ag Grade
(g/t)
Cu Metal
(kt)
Ag Metal
(MOz)
Indicated 1.1 0.59 12.8 6.7 0.5
Inferred 10.4 0.52 11.5 53.6 3.8
Total 11.5 0.52 11.6 60.3 4.3

EXPLORATION TARGET

Tonnage (Mt)
High
Tonnage (Mt)
Low
Cu Grade (%)
High
Cu Grade (%)
Low
Ag Grade (g/t)
High
Ag Grade (g/t)
Low
308 205 0.46 0.31 8.3 5.5

No : Fur h r d ail of h ompa y’ JOR MRE and Exploration Target are contained within the ompa y’ ASX a ou c m of 4 August, 2025. Cobre is not aware of any new information or data ha ma rially aff c h i forma io i clud d i h ompa y’ a ou c m a d ha all ma rial assumptions and technical parameters underpinning the estimates referred to therein continue to apply and have not materially changed.

3 Home | Copper Fox Metals Inc.

4 Florence Copper | Taseko Mines Limited

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Basis of the Exploration Target:

  • Mineralisation at NCP is sedimentary-hosted, structurally controlled, copper-silver associated with the redox contact between oxidised NPF red beds and overlying reduced marine sedimentary rocks of the DKF on the limbs of anticlinal structures with smaller structurally controlled higher-grade zones. This style of mineralisation is dominated by fine-grained chalcocite which occurs along cleavage planes (S1) and in fractures. Importantly, the chalcocite mineralisation is associated with well-developed fracture zones bounded by more competent hanging and footwall units.

  • A database of 17 diamond core drill holes (totalling 4,146m) over the NCP, geophysical mapping, downhole orientated core structural data, lithological and regional structural interpretation.

  • Drillholes used to inform the Comet MRE were excluded.

  • Exploration Target modelling was completed in Leapfrog Geo to produce a mineralised solid to determine volume, above 545m RL.

  • A dry bulk density of 2.81 t/m3 was used to determine tonnage from the modelled volume, based on the available density data for the NCP.

  • Copper grades of raw samples were capped to 2%, silver grades were capped to 30 g/t, based on log probability plots and observed break points in the data distributions, before length weighted averages were reported.

  • Unclassified tonnage below and adjacent to the Comet MRE were included in the Exploration Target.

  • The Exploration Target range was calculated by applying ±20% to the tonnes and grade.

  • The focus area for the model is the southern anticline structure extends for approximately 25km along strike with anomalous copper intersections on both fold limbs.

Competent Persons Statement Relating to the JORC MRE & Exploration Target

The information contained herein which relates to the Comet Mineral Resource and NCP Exploration Target is based on, and fairly represents, information compiled by Mr Drew Luck. Mr Luck is a Senior Resource Geologist and full-time employee of WSP Australia Pty Limited, based in Brisbane, QLD and is a member of the Australasian Institute of Mining and Metallurgy.

Mr Luck has sufficient experience which is relevant to the style of mineralisation and type of deposit under consideration, and to the activity which he is undertaking, to qualify as a Competent Person as defined in the 2012 Edition of the ‘ ustra asian Code for Reportin of Exp oration Resu ts, Minera Resources and Ore Reserves’ (the JORC Code 2012). Mr Luc consents to the inclusion in the release of the matters based on the information he has compiled in the form and context in which it appears.

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This ASX release was authorised on behalf of the Cobre Board by: Adam Wooldridge, Chief Executive Officer.

For more information about this announcement, please contact:

Adam Wooldridge

Chief Executive Officer

[email protected]

COMPETENT PERSONS STATEMENT

The information in this announcement that relates to exploration results is based on information compiled by Mr David Catterall, a Competent Person and a member of a Recognised Professional Organisations (ROPO). David Catterall has sufficient experience that is relevant to the style of mineralisation and type of deposit under consideration and to the activity being undertaken to qualify as a Competent Person as defined in the 2012 Edition of the Australasian Code for Reporting of Exploration Results, Mineral Resources and Ore Reserves (JORC 2012). David is the principal geologist at Tulia Blueclay Limited and a consultant to Kalahari Metals Limited. David Catterall is a member of the South African Council for Natural Scientific Professions, a recognised professional organisation.

David Catterall consents to the inclusion in the report of the matters based on his information in the form and context in which it appears.

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Cautionary Statement about Forward-Looking Statements

This announcement contains certain “forward- oo in statements” inc udin statements re ardin our intent, be ief or current expectations with respect to Cobre’s business and operations, mar et conditions, results of operations and financial condition, and risk management practices. The words "likely", "expect", "aim", "should", "could", "may", "anticipate", "predict", "believe", "plan", "forecast" and other similar expressions are intended to identify forward-looking statements. Indications of, and guidance on, future earnings, anticipated production, life of mine and financial position and performance are also forward-looking statements. These forward-looking statements involve known and un nown ris s, uncertainties and other factors that may cause Cobre’s actual results, performance and achievements or industry results to differ materially from any future results, performance or achievements, or industry results, expressed or implied by these forward-looking statements. Relevant factors may include (but are not limited to) changes in commodity prices, foreign exchange fluctuations and general economic conditions, increased costs and demand for production inputs, the speculative nature of exploration and project development, including the risks of obtaining necessary licences and permits and diminishing quantities or grades of reserves, political and social risks, changes to the regulatory framework within which Cobre operates or may in the future operate, environmental conditions including extreme weather conditions, recruitment and retention of personnel, industrial relations issues and litigation.

Forward- oo in statements are based on Cobre’s ood faith assumptions as to the financia , mar et, re u atory and other re evant environments that wi exist and affect Cobre’s business and operations in the future. Cobre does not give any assurance that the assumptions will prove to be correct. There may be other factors that could cause actual results or events not to be as anticipated, and many events are beyond the reasonable control of Cobre. Readers are cautioned not to place undue reliance on forward-looking statements, particularly in the current economic climate with the significant volatility, uncertainty and disruption caused by the COVID-19 pandemic. Forward-looking statements in this document speak only at the date of issue. Except as required by applicable laws or regulations, Cobre does not undertake any obligation to publicly update or revise any of the forward-looking statements or to advise of any change in assumptions on which any such statement is based. Except for statutory liability which cannot be excluded, each of Cobre, its officers, employees and advisors expressly disclaim any responsibility for the accuracy or completeness of the material contained in these forward-looking statements and excludes all liability whatsoever (including in negligence) for any loss or damage which may be suffered by any person as a consequence of any information in forward- looking statements or any error or omission.

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JORC Code, 2012 Edition – Table 1 report template

Section 1 Sampling Techniques and Data

(Criteria in this section apply to all succeeding sections.)

JORC Code, 2012 Edition – Table 1 report template
Section 1 Sampling Techniques and Data
(Criteria in this section apply to all succeeding sections.)
JORC Code, 2012 Edition – Table 1 report template
Section 1 Sampling Techniques and Data
(Criteria in this section apply to all succeeding sections.)
JORC Code, 2012 Edition – Table 1 report template
Section 1 Sampling Techniques and Data
(Criteria in this section apply to all succeeding sections.)
Criteria JORC Code explanation Commentary
Sampling
techniques
Nature and quality of sampling
(e.g. cut channels, random chips,
or specific specialised industry
standard measurement tools
appropriate to the minerals
under investigation, such as
down hole gamma sondes, or
handheld XRF instruments, etc).
These examples should not be
taken as limiting the broad
meaning of sampling.

The information in this release relates to the
ch ical d ail from h ompa y’ xplora io a d
drilling program at the Ngami Copper Project (NCP)
located within the Ngamiland District on the Kalahari
Copper Belt, Republic of Botswana.

Representative diamond half core samples are taken
from zones of interest. Samples were taken
consistently from the same side of the core cutting
line. Core cutting line is positioned to result in two
splits as mirror images with regards to the
mineralisation, and to preserve the orientation line.
Include reference to measures
taken to ensure sample
representivity and the
appropriate calibration of any
measurement tools or systems
used
Diamond core sample representativity was ensured by
bisecting structures of interest, and by the sample
preparation technique in the laboratory.
The diamond drill core samples were selected based
on geological logging and pXRF results, with the ideal
sampling interval being 1m, whilst ensuring that the
sampled interval does not cross any logged significant
feature of interest.
Individual core samples were crushed entirely to 90%
less than 2mm, riffle split off 1kg, pulverise split to
better than 85% passing 75 microns (ALS PREP-31D).
Sample representivity and calibration for ICP AES
analysis is ensured by the insertion of suitable QAQC
samples.
Samples are digested using 4-acid near total digest
and analysed for 34 elements by ICP-AES (ALS ME-
ICP61, and_ME-ICP61a).
• _Over range for Cu and Ag are digested and analysed

with the same method but higher detection limits (ALS
ME-OG62).
Aspects of the determination of
mineralisation that are Material
to the Public Report.

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ca wh r ‘i du ry
a dard’ work ha b do
this would be relatively simple
( .g. ‘r v r circula io drilli g
was used to obtain 1 m samples
from which 3 kg was pulverised
to produce a 30 g charge for fire
a ay’). o h r ca , mor
explanation may be required,
such as where there is coarse
gold that has inherent sampling
problems. Unusual commodities
or mineralisation types (e.g.
submarine nodules) may
warrant disclosure of detailed
information.
pXRF measurements are carried out with appropriate
blanks and reference material analysed routinely to
verify instrument accuracy and repeatability.
Drilling
techniques
Drill type (e.g. core, reverse
circulation, open-hole hammer,
rotary air blast, auger, Bangka,
sonic, etc) and details (e.g. core
diameter, triple or standard
tube, depth of diamond tails,
face-sampling bit or other type,
whether core is oriented and if
so, by what method, etc).
obr ’ Diamo d drilli g i b i g co duc d wi h
Tricone (KF cover sequences), followed by PQ/HQ/NQ
core sizes (standard tube) with HQ and NQ core
oriented using AXIS Champ ORI tool.
For the last phase of drilling PQ3, HQ3 and NQ3 core
sizes were used with HQ3 and NQ3 core oriented using
AXIS Champ ORI tool.
Drill sample
recovery
Method of recording and
assessing core and chip sample
recoveries and results assessed.
Core recovery is measured and recorded for all drilling.
Once bedrock has been intersected, sample recovery
has been >98%.
Measures taken to maximise
sample recovery and ensure
representative nature of the
samples.
pXRF samples are taken along the orientation line at
consistent measured points to avoid sample biases.
Samples were taken consistently from the same side
of the core cutting line to avoid bias.
Geologists frequently check the core cutting
procedures to ensure the core cutter splits the core
correctly in half.
Core samples are selected within logged geological,
structural, mineralisation and alteration constraints.
Samples are collected from distinct geological
domains with sufficient width to avoid overbias.

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Whether a relationship exists
between sample recovery and
grade and whether sample bias
may have occurred due to
preferential loss/gain of
fine/coarse material.
Sample recovery was generally very good and as such
it is not expected that any such bias exists.
Logging Whether core and chip samples
have been geologically and
geotechnically logged to a level
of detail to support appropriate
Mineral Resource estimation,
mining studies and metallurgical
studies.
Cobre Diamond drill core is logged by a team of
qualified geologists using predefined lithological,
mineralogical, physical characteristic (colour,
weathering etc) and logging codes.
The geologists on site followed industry best practice
and standard operating procedure for Diamond core
drilling processes.
Diamond drill core was marked up on site and logged
back at camp where it is securely stored.
Data is recorded digitally using Ocris geological
logging software.
The QAQC compilation data for all logging results are
stored and backed up on the cloud.
Whether logging is qualitative or
quantitative in nature. Core (or
costean, channel, etc)
photography.
All logging used standard published logging charts and
classification for grain size, abundance, colour and
lithologies to maintain a qualitative and semi-
quantitative standard based on visual estimation.
Magnetic susceptibility readings are also taken every
meter and/or half meter using a ZH Instruments SM-
20/SM-30 reader.
The total length and percentage
of the relevant intersections
logged.
100% of all recovered intervals are geologically logged.
Sub-
sampling
techniques
and sample
preparation
If core, whether cut or sawn and
whether quarter, half or all core
taken.
Selected intervals are currently being cut (in half) with
a commercial core cutter, using a 2mm thick blade, for
one half to be sampled for analysis while the other half
is kept for reference.
For selected samples core is quartered and both
quarters being sampled as an original and field
replicate sample.
If non-core, whether riffled, tube
sampled, rotary split, etc and
whether sampled wet or dry

N/A

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For all sample types, the nature,
quality and appropriateness of
the sample preparation
techniques
Field sample preparation is suitable for the core
samples.
The laboratory sample preparation technique (ALS
PREP-31D) is considered appropriate and suitable for
the core samples and expected grades.
Metallurgical intermittent bottle roll test work was
carried out on a relatively fine reserve sample crush
with ongoing in-situ copper recovery vessel testing
which is deemed to be more representative of the in-
situ environment.
Quality control procedures
adopted for all sub-sampling
stages to maximise
representivity of samples.
Metallurgical samples were composited, homogenised
and split into test charges.
Measures taken to ensure that
the sampling is representative of
the in-situ material collected,
including for instance results for
field duplicate/second-half
sampling.
Sampling is deemed appropriate for the type of survey
and equipment used.
The duplicate sample data (field duplicate and lab
duplicates) indicates that the results are representative
and repeatable.
Metallurgical samples were taken from several sites on
both anticline limbs deemed to be representative of
mineralisation across the target.
Whether sample sizes are
appropriate to the grain size of
the material being sampled.
Initial metallurgical results quoted have been carried
out on a fine crush sample. Future studies will utilise a
coarser crush or fractured core.
Quality of
assay data
and
laboratory
tests
The nature, quality and
appropriateness of the assaying
and laboratory procedures used
and whether the technique is
considered partial or total.
pXRF measurements undertaken on NCP67 and NCP68
are deemed appropriate for a first pass estimate of
copper abundance and thickness. No grade-thickness
results are provided or implied given the uncertainties
in the analysis.
obr ’ cor ampl ar b i g for 4-acid digest
for “ ar o al” dig a d P-AES analysis (34
elements) at ALS laboratories in Johannesburg, South
Africa.
The analytical techniques (ALS ME-ICP61 and ME-
OG62) are considered appropriate.
Intermittent Bottle Roll Leach test work has been
carried out on 6m composite samples from both high-

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and low- grade intersections in different portions of the
Comet Target. Results provide an indication of the
copper leach performance.
Comprehensive head assay was carried out on
metallurgical samples to determine Cu speciation (acid
soluble Cu, cyanide soluble Cu, residual Cu).
For geophysical tools,
spectrometers, handheld XRF
instruments, etc, the parameters
used in determining the analysis
including instrument make and
model, reading times,
calibrations factors applied and
their derivation, etc.
Cobre use ZH Instruments SM20 and SM30 magnetic
susceptibility meters for measuring magnetic
susceptibilities and readings are randomly repeated to
ensure reproducibility and consistency of the data.
An Olympus Vanta pXRF instrument is used with
reading times on Soil Mode of 120seconds in total.
For the pXRF analyses, well established in-house SOPs
were strictly followed and data subject to QAQC before
acceptance into the database.
A test study of 5 times repeat analyses on selected soil
samples is conducted to establish the reliability and
repeatability of the pXRF at low Cu-Pb-Zn values.
For the pXRF Results, no user factor was applied, and
as per SOP the units calibrated daily with their
respective calibration disks.
All QAQC samples were reviewed for consistency and
accuracy. Results were deemed repeatable and
representative:

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Nature of quality control
procedures adopted (e.g.
standards, blanks,
duplicates, external
laboratory checks) and
whether acceptable levels of
accuracy (i.e. lack of bias)
and precision have been
established.
Appropriate certified reference material was inserted
on a ratio of 1:20 samples.
Laboratory coarse crush and pulp duplicate samples
were alternately requested for every 20 samples.
Blanks were inserted on a ratio of 1:20.
ALS Laboratories insert their own standards,
duplicates and blanks and follow their own SOP for
quality control.
Both internal and laboratory QAQC samples are
reviewed for consistency.
Th i r d RM’ hav highligh d acc p abl
laboratory accuracy and precision for Cu. The inserted
CRM (OREAS96) highlighted acceptable accuracy and
precision for results above 10ppm Ag. There is a rather
poor precision for Ag at concentration levels of less
ha 0x h a aly ical m hod’ d c io limi ( .g. <
10ppm Ag.
The coarse Blank and lab internal pulp Blank results
suggest a low risk of contamination during the sample
preparation and analytical stages respectively.
The duplicate sample data indicates that the results
are representative and repeatable for Cu and Ag.
External laboratory checks were carried out by
Scientific Services Laboratories showing an excellent
correlation and a high degree of repeatability of the
results. The laboratory comparative sample data
indicates that the analytical results from ALS
Laboratories for Cu and Ag are representative and
repeatable
Verification
of sampling
and assaying
The verification of
significant intersections by
either independent or
alternative company
personnel.
All drill core intersections were verified by peer
review.
The use of twinned holes. No twinned holes have been drilled to date.
All data is electronically stored with peer review of
data processing and modelling.
Data entry procedures standardized in SOP, data
checking and verification routine.
Data storage on partitioned drives and backed up on
Documentation of primary
data, data entry procedures,
data verification, data
storage (physical and
electronic) protocols.

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server and on the cloud.
Discuss any adjustment to
assay data.
No adjustments were made to assay data.
Location of
data points
Accuracy and quality of surveys
used to locate drill holes (collar
and down-hole surveys),
trenches, mine workings and
other locations used in Mineral
Resource estimation.
obr ’ drill collar coordi a ar cap ur d u i g
Catalyst differential GPS with 1cm accuracy
During earlier drill programmes, drill holes were
initially surveyed using handheld GPS and then re-
surveyed with differential DGPS at regular intervals to
ensure sub-meter accuracy.
Downhole surveys of drill holes are being undertaken
using an AXIS ChampMag tool or AXIS gyro with
downhole survey spacing generally less than 30m.
Specification of the grid system
used.
The grid system used is WGS84 UTM Zone 34S. All
reported coordinates are referenced to this grid.
Quality and adequacy of
topographic control.
Topographic control is based on satellite survey data
collected at 30m resolution. Quality is considered
acceptable.
Data spacing
and
distribution
Data spacing for reporting of
Exploration Results.
Whether the data spacing, and
distribution is sufficient to
establish the degree of
geological and grade continuity
appropriate for the Mineral
Resource and Ore Reserve
estimation procedure(s) and
classifications applied.

Data spacing and distribution of all survey types is
deemed appropriate for the type of survey and
equipment used.

Drill hole spacing for the Comet MRE is
approximately 130 m along strike and 45 m across
strike.

Drill hole spacing for the Exploration Target varies
between 500m to greater than 5000m, as might be
expected for this stage of exploration.
Whether sample compositing
has been applied.
N/A

==> picture [451 x 90] intentionally omitted <==

Orientation
of data in
relation to
geological
structure
Whether the orientation of
sampling achieves unbiased
sampling of possible structures
and the extent to which this is
known, considering the deposit
type.

Drilling was typically completed perpendicular to the
strike of the mineralisation, approximately 150o
azimuth, at a dip of -60o. For the current phase of
drilling, holes are oriented approximately 330
azimuth and an inclination of -60 to obtain better
intersection angles of the overturned units.

Drillhole intersection angles with the mineralisation
contact were sub-optimal (approximately 25o from
the core axis) and may have affected sample
selection at mineralisation boundaries. This phase
drillholes drilled towards the north west have better
intersection angles with the mineralisation
(approximately 40)
If the relationship between the
drilling orientation and the
orientation of key mineralised
structures is considered to have
introduced a sampling bias, this
should be assessed and reported
if material.

Current available data indicates mineralisation
occurs within steep, sub-vertical structures, sub-
parallel to foliation.
Sample
security
The measures taken to ensure
sample security.
Sample bags are logged, tagged, double bagged and
sealed in plastic bags, stored at the field office.
Diamond core is stored in a secure facility at the field
office and then moved to a secure warehouse.
Sample security includes a chain-of-custody procedure
that consists of filling out sample submittal forms that
are sent to the laboratory with sample shipments to
make certain that all samples are received by the
laboratory. Prepared samples were transported to the
analytical laboratory in sealed gravel bags that are
accompanied by appropriate paperwork, including the
original sample preparation request numbers and
chain-of-custody forms
Audits or
reviews
The results of any audits or
reviews of sampling techniques
and data.
obr ’ drill hol ampli g proc dur i do
according to industry best practice.
Hydrogeological results are reviewed by WSP
Australia Pty Ltd
Metallurgical test work was conducted by and
reviewed by Independent Metallurgical Operations
Pty Ltd.
Metallurgical work was reviewed by METS.
Geological modelling was reviewed by WSP Australia

==> picture [451 x 90] intentionally omitted <==

  • Pty Ltd.

  • Gap Analysis undertaken by METSISCR methodology was reviewed by ERM

==> picture [451 x 90] intentionally omitted <==

JORC Section 2 Reporting of Exploration Results

(Criteria listed in the preceding section also apply to this section.)

Criteria JORC Code explanation Commentary
Mineral
tenement and
land tenure
status
Type, reference name/number,
location and ownership including
agreements or material issues
with third parties such as joint
ventures, partnerships, overriding
royalties, native title interests,
historical sites, wilderness or
national park and environmental
settings.
The security of the tenure held at
the time of reporting along with
any known impediments to
obtaining a licence to operate in
the area.

Cobre Ltd holds 100% of Kalahari Metals
Ltd.

Kalahari Metals in turn owns 100% of
Triprop Holdings Ltd and Kitlanya (Pty) Ltd
both of which are locally registered
companies.

Triprop Holdings holds the NCP licenses
PL035/2017 (306.76km2) and PL036/2017
(49.8km2), which, following a recent renewal,
are due for their next extension on
30/09/2026

Triprop Holdings holds the additional infill
licenses PL252/2022 to 255/2022 which are
due for their next renewal on 31/12/2027.
Exploration
done by other
parties
Acknowledgment and appraisal
of exploration by other parties.
Previous exploration on portions of the NCP
was conducted by BHP.
BHP collected approximately 113 soil samples
over the NCP project in 1998.
BHP collected Geotem airborne
electromagnetic data over a small portion of
PL036/2012.
Geology Deposit type, geological setting
and style of mineralisation.

The regional geological setting underlying
all the Licences is interpreted as
Neoproterozoic meta sediments, deformed
during the Pan African Damara Orogen into
a series of ENE trending structural domes cut
by local structures.

The style of mineralisation comprises strata-
bound and structurally controlled
disseminated, cleavage and vein hosted Cu-
Ag mineralisation.

==> picture [451 x 90] intentionally omitted <==

Drill hole A summary of all information Information material to the understanding of the exploration results including a tabulation of the following information for all Material drill holes:

easting and northing of the drill hole collar

elevation or RL (Reduced Level – elevation above sea level in metres) of the drill hole collar

Summary table of all completed core drill holes on the NCP licenses is presented below. All coordinates are presented in UTM Zone 34S, WGS84 datum. All the holes have been re-surveyed with differentially corrected GPS. Drill holes designated TRDH are original holes drilled by Triprop in 2014, MW are monitoring wells and PW injection/pumping wells.

Summary results of intersections are provided using a cut-off of 0.2% Cu ranked according to intersection width and grade. Summary results for of > 1% Cu over 1m are provided in the following table.

dip and azimuth of the hole

down hole length and interception depth hole length.

If the exclusion of this information is justified on the basis that the information is not Material and this exclusion does not detract from the understanding of the report, the Competent Person should clearly explain why this is the case.

the case.
Hole ID Easting Northing RL EOH Dip Azimuth
NCP01 594786.0
7694068.0

1052.0
76.4 -90.0 0.0
NCP01A 594786.0
7694070.0

1052.0
95.5 -90.0 0.0
NCP02 617226.0
7692104.0

999.0
344.7 -90.0 0.0
NCP03 594746.0
7693874.0

1034.0
294.0 -80.0 155.0
NCP04 590768.0
7691124.0

1054.0
107.0 -80.0 155.0
NCP05 590566.0
7691488.0

1053.0
177.0 -75.0 155.0
NCP06 590610.0
7691398.0

1050.0
283.1 -70.0 155.0
NCP07 599889.5
7685403.0

1099.2
387.3 -55.8 150.8
NCP08 598985.5
7684909.0

1101.9
171.3 -61.0 149.8
NCP09 598092.8
7684452.0

1102.5
246.3 -60.4 147.9
NCP10 601620.3
7686327.4

1092.4
351.5 -62.4 152.5

==> picture [451 x 90] intentionally omitted <==

NCP11
NCP11-A
NCP11-B
NCP12
NCP13
NCP14
NCP15
NCP16
NCP17
NCP18
NCP18A
NCP19
NCP20
NCP20A
NCP21
NCP22
NCP23
NCP24
NCP25
NCP26
NCP27
NCP28
NCP29
NCP30
NCP31
NCP31A
NCP32
NCP33
NCP34
NCP35
NCP36
598960.0
7684952.0
1068.0
45.4
-60
150
598963.0
7684949.0
1083.0
81.3
-60
150
598958.5
7684956.8
1101.9
384.4
-62.8
144.6
599431.6
7685158.1
1100.5
252.3
-58.2
153.0
598533.8
7684688.8
1102.8
210.2
-57.4
150
600311.2
7685611.5
1097.5
276.3
-58.7
151.8
601192.3
7686073.9
1095.5
243.3
-57.9
152.0
602078.3
7686537.5
1092.0
225.3
-57.3
149.9
599185.6
7685059.8
1100.6
261.3
-53.7
150.2
598730.0
7684840.0
1098.0
64.0
-60
150
598727.0
7684848.1
1102.1
317.7
-57.7
159.9
599212.0
7685019.7
1100.3
186.3
-59.7
152.0
598762.0
7684798.0
1115.0
68.6
-60
150
598758.7
7684796.7
1102.2
227.7
-63.1
150.6
589690.1
7679006.7
1120.7
243.4
-58.7
147.3
587386.0
7677006.9
1121.2
180.4
-59.4
150.9
599161.4
7685097.5
1100.9
458.7
-59.5
152.7
605248.0
7688073.3
1085.4
228.3
-57.7
146.0
598876.3
7684850.8
1101.4
164.7
-61.0
145.6
598643.5
7684747.6
1102.8
233.7
-62.4
147.8
605504.4
7683638.7
1087.0
183.5
-62.5
328.2
598622.2
7684786.0
1102.7
317.5
-57.9
147.7
600752.0
7679852.5
1109.8
252.4
-59.2
328.2
598851.9
7684887.0
1101.7
263.7
-57.7
148.9
599441.0
7678120.0
1104.0
63.6
-60
325
599443.3
7678119.6
1114.0
378.5
-60.7
326.5
610526.0
7686924.7
1066.0
104.7
-60.7
329.1
610574.1
7686840.8
1063.7
278.9
-60.6
329.5
590272.0
7679998.6
1121.1
450.4
-59.2
152.1
610139.8
7686588.1
1059.1
290.6
-58.8
334.5
601040.3
7679346.7
1107.4
537.3
-52.6
325.2

==> picture [451 x 90] intentionally omitted <==

NCP37
NCP38
NCP39
NCP40
NCP41
NCP42
NCP43
NCP44
NCP45
NCP46
NCP47
NCP48
NCP49
NCP50
NCP51
NCP52
NCP53P
NCP54RC
NCP55
NCP56
NCP57
NCP58
NCP59
NCP60
NCP61
NCP62
NCP63
NCP64
NCP65
NCP66
612295.1
7687854.7
1062.3
227.6
-62.4
341.2
612745.8
7688087.8
1062.7
305.6
-61.7
331.0
600936.9
7679533.6
1108.4
363.5
-57.2
326.5
611020.3
7687066.1
1066.4
320.8
-61.1
330.5
592795.4
7681630.5
1108.5
468.5
-61.2
152.0
607049.7
7688941.3
1076.2
194.6
-57.6
153.8
599097.1
7684968.9
1101.3
197.6
-61.3
150.1
586591.5
7676382.2
1123.7
318.5
-57.5
154.6
600106.8
7685494.0
1099.4
236.6
-58.2
153.0
600529.7
7685715.5
1096.7
202.0
-56.4
151.4
595337.9
7670959.5
1133.1
520.0
-56.1
149.4
601417.1
7686190.8
1093.7
206.6
-58.7
150.4
600005.8
7685434.3
1100.4
116.6
-58.7
149.3
599790.2
7685325.2
1097.3
215.6
-59.2
151.6
597630.8
7684254.0
1101.2
254.6
-59.9
149.4
598764.0
7684788.0
1101.0
146.6
-60.9
148.6
615131
7691128
1036
49
90
0.0
615133
7691112
1028
116
90
0.0
608861
7689805
1052.0
210.8
-60.0
150
610659.0
7690689.0
1064.9
230.8
-60.0
150
599077.0
7685009.0
1101.0
303.0
60.0
155.0
599320.0
7685093.0
1101.0
219.0
60.0
155.0
599454.0
7685235.0
1100.0
509.0
60.0
155.0
598193.0
7684565.0
1102.0
312.0
60.0
155.0
598367
7684597
1101
174
60
155
598423
7684721
1102
451
60
155
599609
7685245
1099
294
60
155
599683
7685354
1096
447
60
155
599992
7685485
1097
390
60
155
600183
7685564
1098
324
60
155

==> picture [451 x 90] intentionally omitted <==

NCP67
NCP68
TRDH14-01
TRDH14-02
TRDH14-02A
TRDH14-03
TRDH14-04
TRDH14-05
TRDH14-06
TRDH14-07
TRDH14-08
TRDH14-09
TRDH14-10
TRDH14-11
TRDH14-12
TRDH14-13
TRDH14-14
TRDH14-15
TRDH14-16
TRDH14-16A
TRDH14-17
TRDH14-17A
MW_001
MW_010
MW_002
PW_001
MW_012
PW_002
609,304
7,689,840
1067
239.53
-60
330
608,577
7,689,512
1071.1
245.65
-60
330
612247.8
7687953.7
1062.6
71.7
-90.0
0.0
612339.0
7687802.0
1047.0
58.6
-90.0
0.0
612335.7
7687808.5
1062.4
83.9
-89.4
0.0
612293.6
7687885.6
1062.0
92.8
-89.9
0.0
609703.0
7686345.0
1040.0
149.7
-89.1
0.0
609595.7
7686510.3
1061.0
59.7
-89.9
0.0
609653.0
7686433.0
1038.0
59.7
-89.7
0.0
609663.0
7686414.0
1042.0
111.0
-60.0
331.6
607204.0
7684683.0
1056.0
71.4
-89.7
0.0
607133.0
7684805.0
1055.0
73.0
-89.6
0.0
607061.0
7684936.0
1024.0
68.3
-89.4
0.0
607150.0
7684776.0
1014.0
182.9
-62.6
331.4
600845.0
7685696.0
1080.0
71.2
-89.4
0.0
600924.0
7685567.0
1073.0
80.4
-87.6
0.0
600816.0
7685737.0
1070.0
110.4
-62.0
147.7
600721.0
7685893.0
1042.0
191.7
-60.0
150.0
600758.0
7685834.0
1081.0
49.2
-60.0
150.0
600764.0
7685829.0
1083.0
200.7
-58.3
145.6
608880.0
7685776.0
1027.0
81.2
-60.0
330.0
608862.0
7685805.0
1028.0
179.7
-60.0
330.0
598846.1
7684767.8
1102.2
265.0
-90
0
598817.1
7684772.7
1102.3
265.0
-82
150
598840.0
7684690.7
1102.0
180.0
-90
0
598816.8
7684742.0
1102.3
265.0
-90
0
598791.9
7684712.7
1102.0
211.0
-87
330
598760.7
7684684.3
1100.9
363.0
-83
330

==> picture [451 x 90] intentionally omitted <==

Hole Id FROM TO Length Intersection
78m @ 0.75% Cu & 10 g/t Ag_drilled down-dip_
35m @ 1.3% Cu & 18g/t Ag
40m @ 0.63% Cu & 10 g/t Ag_drilled down dip_
20.05m @ 0.85% Cu & 20g/t Ag
21.9m @ 0.8% Cu & 13g/t Ag
25m @ 0.63% Cu & 10 g/t Ag_drilled down-dip_
26.5m @ 0.55% Cu & 12 g/t Ag
18.5m @ 0.52% & 15 g/t Ag
19m @ 0.5% Cu & 13g/t Ag
18.7m @ 0.53% Cu & 11 g/t Ag
29m @ 0.4% Cu & 3g/t Ag
15.2m @ 0.6% Cu & 13.2 g/t Ag
16.3m @ 0.52% & 14 g/t Ag
15.7m @ 0.5% Cu & 15g/t Ag
25.5m @ 0.4% Cu & 1g/t Ag
15m @ 0.5% Cu & 13g/t Ag
17.8m @ 0.4% Cu & 10g/t Ag
16.7m @ 0.5% Cu & 4g/t Ag
16.7m @ 0.44% Cu & 10 g/t Ag
17.7m @ 0.4% Cu & 12g/t Ag
9.3m @ 6.9% Cu & 17 g/t Ag
19.2m @ 0.3% Cu & 8g/t Ag
14.1m @ 0.5% Cu & 11g/t Ag
17.9m @ 0.4% Cu & 6g/t Ag
12.9m @ 0.5% Cu & 13g/t Ag
12m @ 0.5% Cu & 13g/t Ag
11.6m @ 0.5% Cu & 7g/t Ag
14.6m @ 0.4% Cu & 1g/t Ag
PW_001 187.0 265.0 78.0
NCP20A 124.0 159.0 35.0
MW012 171 211 30.0
NCP55 145.77 165.82 20.05
NCP08 125.0 146.9 21.9
MW_001 97.0 122.0 25.0
NCP56 164.3 191.8 26.3
NCP66 295.98 314.49 18.5
NCP25 122.0 141.0 19.0
NCP63 264.9 283.6 18.7
NCP40 269.0 298.0 29.0
NCP60 283.6 298.7 15.2
NCP64 419.1 436.0 16.3
NCP45 188.9 204.6 15.7
TRDH14-07 62.0 87.5 25.5
NCP42 142.5 157.5 15.0
NCP43 157.0 174.8 17.8
NCP33 228.0 244.7 16.7
NCP65 360.52 377.22 16.7
NCP51 221.2 238.9 17.7
NCP57 277.9 287.2 9.3
NCP29 187.0 206.2 19.2
NCP50 177.9 192.0 14.1
NCP35 238.0 255.9 17.9
NCP49 177.8 190.8 12.9
NCP07 249.0 261.0 12.0
NCP38 261.0 272.6 11.6
TRDH14-11 125.9 140.5 14.6

==> picture [451 x 90] intentionally omitted <==

NCP18A 280.5 292.2 11.6 11.6m @ 0.5% Cu & 9g/t Ag
13.1m @ 0.4% Cu & 7g/t Ag
6.0m @ 0.77% Cu & 21 g/t Ag
17m @ 0.3% Cu & 3g/t Ag
9.7m @ 0.4% Cu & 10g/t Ag
8.6m @ 0.5% Cu & 12g/t Ag
8.5m @ 0.4% Cu & 12 g/t Ag
4.5m @ 0.8% Cu & 4g/t Ag
7.9m @ 0.5% Cu & 12g/t Ag
7.9m @ 0.5% Cu & 12g/t Ag
9.2m @ 0.4% Cu & 9g/t Ag
7.7m @ 0.5% Cu & 9g/t Ag
8.9m @ 0.4% Cu & 8g/t Ag
10.8m @ 0.3% Cu & 6g/t Ag
9.1m @ 0.36% Cu & 9 g/t Ag
8.9m @ 0.35% Cu & 9 g/t Ag
10.7m @ 0.2% Cu & 16g/t Ag
6.6m @ 0.4% Cu & 11g/t Ag
6.8m @ 0.4% Cu & 9g/t Ag
13.3m @ 0.2% Cu & 3g/t Ag
11m @ 0.2% Cu & 4g/t Ag
6.6m @ 0.3% Cu & 10g/t Ag
3.6m @ 0.6% Cu & 13 g/t Ag
5.6m @ 0.3% Cu & 15g/t Ag
5.4m @ 0.4% Cu & 3g/t Ag
5.4m @ 0.2% Cu & 26g/t Ag
3.8m @ 0.5% Cu & 6g/t Ag
8.3m @ 0.2% Cu & 6g/t Ag
5.9m @ 0.3% Cu & 6g/t Ag
5.4m @ 0.2% Cu & 2g/t Ag
NCP09 108.2 121.3 13.1
MW_010 186.0 194.0 8.0
NCP37 186.0 203.0 17.0
NCP19 147.3 157.0 9.7
NCP11-B 345.0 353.6 8.6
NCP59 480.2 488.6 8.5
TRDH14-16A 169.2 173.7 4.5
NCP12 215.5 223.4 7.9
NCP10 311.3 319.2 7.9
NCP30 237.0 246.2 9.2
NCP23 424.0 431.7 7.7
NCP26 199.7 208.7 9.0
NCP48 171.2 182.0 10.8
NCP61 147.2 156.3 9.1
NCP62 430.3 439.2 8.9
NCP34 398.9 409.5 10.7
NCP17 236.8 243.5 6.6
NCP15 192.0 198.9 6.8
NCP24 178.0 191.3 13.3
NCP21 118.0 129.0 11.0
NCP14 232.0 238.6 6.6
NCP58 206.2 209.8 3.6
NCP22 144.0 149.6 5.6
NCP46 170.0 175.4 5.4
NCP44 283.0 288.4 5.4
NCP27 152.4 156.2 3.8
NCP16 188.0 196.2 8.3
NCP28 274.0 279.9 5.9
NCP13 171.4 176.8 5.4

==> picture [451 x 90] intentionally omitted <==

NCP39 333.0 338.5 5.5
NCP43 123.6 126.0 2.4
NCP35 169.0 175.0 6.0
NCP36 509.5 514.2 4.7
NCP10 211.0 213.0 2.0
NCP26 135.0 136.0 1.0
NCP31A 310.1 311.8 1.7
NCP43 152.0 155.0 3.0
NCP10 149.0 151.0 2.0
NCP11-B 338.0 340.1 2.1
NCP52 106.5 108.7 2.2
NCP52 96.0 98.3 2.3
NCP41 435.1 436.5 1.4
Intersections of > 1% Cu
Hole id FROM TO Intersection
MW_001 97.0 98.0 1m @ 1.4% Cu & 14 g/t Ag
MW_001 106.0 107.0 1m @ 1.3% Cu & 18 g/t Ag
MW_001 111.0 112.0 1m @ 1.1% Cu & 16 g/t Ag
MW_010 189.0 190.0 1m @ 2.0% Cu & 22 g/t Ag
MW_012 178.0 184.0 6m @ 1.6% Cu & 21 g/t Ag
MW_012 187.0 190.0 3m @ 1.1% Cu & 16 g/t Ag
NCP08 136.2 146.9 10.7m @ 1.3% Cu & 18g/t Ag
NCP10 318.0 319.2 1.2m @ 1.1% Cu & 26g/t Ag
NCP20A 148.7 158.0 9.3m @ 3.4% Cu & 30g/t Ag
NCP25 133.0 136.0 3m @ 1% Cu & 15g/t Ag
NCP26 207.7 208.7 1m @ 1.3% Cu & 16g/t Ag
NCP29 198.7 201.0 2.3m @ 1.1% Cu & 14g/t Ag
NCP33 240.2 242.0 1.8m @ 1% Cu & 12g/t Ag
NCP38 270.7 272.6 1.9m @ 1.1% Cu & 21g/t Ag
NCP40 296.8 298.0 1.2m @ 1.1% Cu & 1g/t Ag

==> picture [451 x 90] intentionally omitted <==

NCP55 NCP55 161.5 165.8 4.3m @ 2.2% Cu & 45g/t Ag 4.3m @ 2.2% Cu & 45g/t Ag
NCP56 188.7 189.4 0.7m @ 1.69% Cu & 28g/t Ag
PW_001 196 201 5m @ 1.2% Cu & 11 g/t Ag
PW_001 213 224 11m @ 1.1% Cu & 15 g/t Ag
PW_001 228 236 8m @ 1.1% Cu & 14 g/t Ag
TRDH14-16A 171.2 173.72 2.5m @ 1.4% Cu & 11g/t Ag
Data
aggregation
methods


















In reporting Exploration Results,
weighting averaging techniques,
maximum and/or minimum grade
truncations (eg cutting of high
grades) and cut-off grades are
usually Material and should be
stated.
Where aggregate intercepts
incorporate short lengths of high
grade results and longer lengths
of low grade results, the
procedure used for such
aggregation should be stated and
some typical examples of such
aggregations should be shown in
detail.
The assumptions used for any
reporting of metal equivalent
values should be clearly stated.

Grades were capped at 2% Cu and 30 g/t Ag
for the reporting of the Exploration Target.

Length-weighted average was used in the
reporting of the Exploration Target grade.

No aggregation of intercepts has been
reported.

Copper equivalents were not reported for the
Mineral Resource estimate or Exploration
Target.
Relationship
between
mineralisation
widths and
intercept
lengths
These relationships are
particularly important in the
reporting of Exploration Results.
If the geometry of the
mineralisation with respect to the
drill hole angle is known, its
nature should be reported.
If it is not known and only the
down hole lengths are reported,
Down hole intersection widths are used
throughout.
Diamond holes are drilled at -60o towards
150o azimuth, with mineralisation typically
oriented sub-vertical resulting in a relatively
low intersection angle.
The hydrogeological percussion drilling was
drilled down mineralisation in order to
intersect the fracture zones associated with
the mineralisation – this results in long-
intersections which are noted in the
NCP55 NCP55 161.5 165.8 4.3m @ 2.2% Cu & 45g/t Ag 4.3m @ 2.2% Cu & 45g/t Ag
NCP56 188.7 189.4 0.7m @ 1.69% Cu & 28g/t Ag
PW_001 196 201 5m @ 1.2% Cu & 11 g/t Ag
PW_001 213 224 11m @ 1.1% Cu & 15 g/t Ag
PW_001 228 236 8m @ 1.1% Cu & 14 g/t Ag
TRDH14-16A 171.2 173.72 2.5m @ 1.4% Cu & 11g/t Ag
Data
aggregation
methods


















In reporting Exploration Results,
weighting averaging techniques,
maximum and/or minimum grade
truncations (eg cutting of high
grades) and cut-off grades are
usually Material and should be
stated.
Where aggregate intercepts
incorporate short lengths of high
grade results and longer lengths
of low grade results, the
procedure used for such
aggregation should be stated and
some typical examples of such
aggregations should be shown in
detail.
The assumptions used for any
reporting of metal equivalent
values should be clearly stated.

Grades were capped at 2% Cu and 30 g/t Ag
for the reporting of the Exploration Target.

Length-weighted average was used in the
reporting of the Exploration Target grade.

No aggregation of intercepts has been
reported.

Copper equivalents were not reported for the
Mineral Resource estimate or Exploration
Target.
Relationship
between
mineralisation
widths and
intercept
lengths
These relationships are
particularly important in the
reporting of Exploration Results.
If the geometry of the
mineralisation with respect to the
drill hole angle is known, its
nature should be reported.
If it is not known and only the
down hole lengths are reported,
Down hole intersection widths are used
throughout.
Diamond holes are drilled at -60o towards
150o azimuth, with mineralisation typically
oriented sub-vertical resulting in a relatively
low intersection angle.
The hydrogeological percussion drilling was
drilled down mineralisation in order to
intersect the fracture zones associated with
the mineralisation – this results in long-
intersections which are noted in the

==> picture [451 x 90] intentionally omitted <==

there should be a clear statement
to this effect (eg ‘dow hole
length, true width not k ow ’).
intersection tables.
Diagrams Appropriate maps and sections
(with scales) and tabulations of
intercepts should be included for
any significant discovery being
reported These should include,
but not be limited to a plan view
of drill hole collar locations and
appropriate sectional views.
Section and plan maps of the appropriate drill
hole are provided in the text.
Plan map illustrating the position of drill holes coloured by total Cu.m%.
Balanced
reporting
Where comprehensive reporting
of all Exploration Results is not
practicable, representative
reporting of both low and high
grades and/or widths should be
practiced to avoid misleading
reporting of Exploration Results.
Results from the previous exploration
programmes are summarised in the target
priorities which are based on an
interpretation of these results.
The accompanying document is considered to
be a balanced and representative report.

==> picture [451 x 90] intentionally omitted <==

Other
substantive
exploration
data
Other exploration data, if
meaningful and material, should
be reported including (but not
limited to): geological
observations; geophysical survey
results; geochemical survey
results; bulk samples – size and
method of treatment;
metallurgical test results; bulk
density, groundwater,
geotechnical and rock
characteristics; potential
deleterious or contaminating
substances.
The project area has been surveyed using high
resolution magnetic data, airborne
electromagnetics and airborne gravity
gradient surveys. These results provide a
guide to identifying the mineralised contact
including evidence for further untested
mineralised contact
11,400 soil samples, collected across the
property have been analysed using a
combination of pXRF, ICPMS and partial
leach analysis. This data has been used
successfully to target portions of the contact
_deemed to be better mineralised. _
Further work •The nature and scale of planned
further work (eg tests for lateral
extensions or depth extensions or
large-scale step-out drilling).
• Diagrams clearly highlighting
the areas of possible extensions,
including the main geological
interpretations and future drilling
areas, provided this information is
not commercially sensitive
An EIA is currently in progress
Further hydrogeological work is planned to
test the lateral continuity of fractures zones
associated with mineralisation.
Additional diamond exploration drilling along
the NCP Exploration Target