Silver Targets defined at Black Hill project
Released
Released
Announcement PDF
10 November 2025 Accompanying video: click here
Silver Targets defined at Black Hill project
Key Points:
• Processing of detailed ground gravity survey undertaken in August completed.
• Re-processing of historical Airborne Magnetic and Electro-Magnetic surveys completed.
• Two high priority targets identified: Athena and a new prospect, Hestia.
• Prospects located within the Paris exploration corridor
Investigator Resources Limited (“Investigator” or the “Company”) is pleased to provide an update
on recent technical work at the Black Hill Project, where the Company is earning an interest under
a joint venture with Alliance Resources Pty Ltd.
With a comprehensive review of geophysical data from Investigator’s recent detailed ground
gravity survey and other historical geophysical survey data recently completed, the Company has
highlighted two high priority targets (Athena and Hestia) within the Paris Silver Corridor. A detailed
ground gravity survey covering the western half of the Black Hill tenement (EL6475) was
completed in August. The survey, comprising 1,722 new gravity stations on a 250m x 250m grid,
has significantly improved the understanding of structure and interpreted lithologies across the
area. The new dataset has been successfully merged with neighbouring gravity coverage on
EL6347 (Figure 1).
In parallel, Investigator re-processed and re-modelled existing historical airborne magnetic and
electromagnetic (AEM) datasets to provide an integrated geophysical interpretation across the
broader Black Hill area. This work has identified several key features, including:
1. The Athena magnetic target, previously drilled in 2012-13 and with previously reported 5m
@ 493 g/t Ag from 71m, is now resolved as two separate magnetic bodies.
2. The eastern magnetic body at Athena remains untested by drilling.
3. AEM data transecting the Athena historic drilling indicates a conductive structure
associated with existing skarn silver mineralisation.
4. A series of additional magnetic bodies with similar east west orientation to those observed
at Athena are present within the same trend, potentially extending the Paris Silver Corridor.
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5. The most prominent of these, located approximately 3 km to the south, shows coincident
magnetic, gravity, and AEM responses and has been designated the Hestia prospect.
6. Sub cropping magnetite calc silicate skarn style assemblages have also been observed in
recent field visits to Hestia.
These results collectively highlight a prospective structural corridor extending through Black Hill,
supporting the broader Paris Silver Corridor concept. Further work is now underway to integrate
these datasets into regional targeting and exploration planning.
Investigator Managing Director, Lachlan Wallace, commented:
“The integration of new gravity data with reprocessed magnetic and electromagnetic
surveys has provided a step-change in our understanding of the Black Hill area. The
identification of two well-defined silver targets, Athena and the newly recognised
Hestia prospect, highlights the broader potential of the Paris Silver Corridor and
strengthens the geological link between Paris and the southern prospects.
Our technical team now has a clear framework for how these systems fit within the
regional architecture, which will guide future exploration priorities across the corridor.
These results reinforce the scale and continuity of mineralising structures surrounding
Paris and provide a strong foundation for ongoing assessment of the Black Hill joint
venture area.”
Figure 1: Peterlumbo (EL6347) and Blackhill (EL6475) tenements with Silver prospects highlighted. LHS Regional Reduced to Pole (RTP)
magnetics. RHS: Total Bouger Anomaly data with a High Pass filter utilising 2.67 g/cm3 correction density. Historical Regional Drilling
demarcated by black dots.
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Figure 2: Reduced to Pole (RTP) magnetics zoom in of the Blackhill (EL6475) tenement with the Athena and newly identified Hestia targets
shown with elevated magnetic signature. Airborne Electro-Magnetic (AEM) flight lines shown by E-W lines, Gravity inversion modelling of
bodies with density 2.89 g/cm3 shown in orange compared to average rock density of 2.67 g/cm3. Cross sections of each target are shown
below.
Figure 3: Section A-A’ over the Athena targets. Strong AEM conductors are seen on the periphery of the magnetic inversion shells (green shells
representing 100,000 T). Current existing drillholes at Athena shown at surface. Core of magnetic shells and contacts with AEM signals
currently untested as is Eastern magnetic shell. Gravity inversion modelling of bodies with density 2.77 g/cm3 compared to average rock
density of 2.67 g/cm3.
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Figure 4: Section B-B’ over the Hestia Target showing strong AEM signals associated with high magnetics (green shell) and gravity anomalies
(orange shell) currently untested. Gravity inversion modelling of bodies with density 2.77 g/cm3 compared to average rock density of 2.67
g/cm3.
Black Hill and Athena Prospect Details
• The Athena Prospect (formerly known as Sunday Iron) is a prospective silver exploration
target just 11 kilometres southeast of Investigator’s flagship Paris Silver Project. Athena sits
within the broader mineralised corridor that also hosts the Perseus and Manto silver prospects,
a belt that is under-explored for silver.
• Athena lies within the Black Hill tenement (EL6475), held under an earn-in Joint Venture with
Alliance Resources Pty Ltd. While historical exploration at Athena focused exclusively on iron
(magnetite), the geology shares key similarities with Paris, including altered calc-silicate host
rocks, evidence of skarn alteration and proximity to major structural features and potential
Hiltaba age fluid sources.
• Previous drilling campaigns at Athena were undertaken between 2012–2013 by Trafford
Resources, targeting iron-rich units. These holes were terminated within magnetite units, with
no testing of the surrounding geology for precious metals.
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• Following the discovery of Paris, selected historical drill samples were re-assayed for silver,
returning encouraging results, including:
o 5m @ 493 g/t Ag from 71m, including 1m @ 950 g/t Ag (12BWRC020), and
o 3m @ 71 g/t Ag from 82m from the same hole1
• Since entering the earn in, a technical review at Athena has confirmed its strong silver
potential. In 2025, a review of historic pulps uncovered a previously unreported intersection of
7m @ 111g/t silver from 66m (13BHRC001), further validating the system.
• Petrology indicates a skarn environment with magnetite-hematite derived from hydrothermal
alteration and associated calc-silicates, while drilling west of Athena intersected a
volcanic/intrusive potential source of mineralising fluids.
Approved for release by the Board of Directors.
For further information, please contact:
Lachlan Wallace
Managing Director
+ 61 (0) 8 7325 222
lwallace@investres.com.au
About Investigator Resources
Investigator’s 100% owned Paris Silver Project is located 70km north of the rural township of
Kimba on South Australia’s Eyre Peninsula. The Paris Silver Project, with a JORC 2012 resource
of 24Mt @ 73g/t silver and 0.41% lead for 57Mozs silver and 99kt lead, is a shallow high-grade
silver deposit amenable to open pit mining, providing outstanding exposure to a metal with strong
commodity, renewable energy and manufacturing demand.
With positive outcomes of the Paris Project’s Pre-Feasibility Study as reported in November 2021,
the company is undertaking the work required to complete a Definitive Feasibility Study, whilst
continuing to progress exploration proximal to Paris and across adjacent significant ground
holdings within South Australia.
1 ASX Announcement: 1 April 2025; Strategic Earn-In to High Grade Silver Project
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Competent Person Statement
The information in this announcement relating to exploration results is based on information
compiled by Mr. Jason Murray who is a full-time employee of the company. Mr. Murray is a
member of the Australian Institute of Geoscientists. Mr. Murray has sufficient experience of
relevance to the styles of mineralisation and the types of deposits under consideration, and to the
activities undertaken, to qualify as a Competent Person as defined in the 2012 Edition of the Joint
Ore Reserves Committee (JORC) Australasian Code for Reporting of Exploration Results,
Mineral Resources and Ore Reserves. Mr. Murray consents to the inclusion in this report of the
matters based on information in the form and context in which it appears.
Paris Mineral Resource Estimate2
2023 Paris Silver Project Mineral Resource estimate (25g/t silver cut-off grade).
(Note: Total values may differ due to minor rounding errors in the estimation process)
2
ASX announcement 5 July 2023 “Paris Mineral Resource Estimate Update”. The Company confirms that it is not aware of any
new information or data that materially affects the information included in the original market announcement of 5 July 2023 and
that all material assumptions and technical parameters underpinning the estimates in the relevant market announcement continue
to apply and have not materially changed. The company confirms that the form and context in which the Competent Person’s
findings are presented have not been materially modified from the original market announcement.
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Appendix 5: JORC Code, 2012 Edition – Table 1
The following section is provided to ensure compliance with the JORC (2012) requirements for the reporting of
exploration results presented in the “Silver Targets defined at Black Hill project” ASX release dated 10 November
2025.
Assessment and Reporting Criteria Table Mineral Resource – JORC 2012
Section 1 Sampling Techniques and Data
(Criteria in this section apply to all succeeding sections.)
Criteria and 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.
• Include reference to measures taken to
ensure sample representivity and the
appropriate calibration of any
measurement tools or systems used.
• Aspects of the determination of
mineralisation that are Material to the
Public Report.
• In cases where ‘industry standard’ work
has been done this would be relatively
simple (e.g. ‘RC drilling was used to
obtain 1 m samples from which 3 kg was
pulverised to produce a 30 g charge for
fire assay’). In other cases more
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.
Gravity
• Gravity surveying was conducted on East-West oriented grid with stations
collected at 250 x 250m metre spacing. A total of 1722 new stations were
surveyed with a further 180 (10.5%) gravity repeat stations.
• Gravity survey measurement were conducted using calibrated Scintrex CG-5
Autograv gravity meters with location provided by Leica GX1230 GNSS
receivers for easting and northing, and reference to Australian Height Datum
(AHD) for elevations.
• Regular repeat gravity station measurement was undertaken, as well as use
of a static single gravity base station to calculate absolute and static drift of
gravity over the survey period.
Airborne Electromagnetic (AEM)
• High resolution Xcite time domain electromagnetic and magnetic survey for
Alliance Resources in 2016/2017 over its Wilcherry Hill Project which
includes EL 6475 Blackhill.
• A total of 1799 line kilometres was flown during the survey over the entire
project area in an E-W orientation. Initial spacing was at 800m with further
infill down to 200m in some areas of EL 6475.
• Electromagnetic survey utilised a Xcite Concentric Tx-Rx system with a
transmitter of 220 A (max) and a base frequency of 25 Hz.
• Location data was provided by a Novatel DL-V3L1L2 GPS positioning
system.
• Laser Altimeter type was SF-01 with a range of 0-60m and resolution of 1cm.
Magnetic Survey
• Airborne Magnetics survey was undertaken by MAGSPEC Airborne Surveys
utilsiing a Cessna 206 with a tail boom.
• Survey had a combination of 100m, 50m, 25m East-west orientated flight line
spaced data.
• A total of 18,946 line km was collected as part of the broader survey.
• The magnetometer was a single sensor tail boom mounted G-823 Cesium
vapour magnetometer with a resolution of 0.001 nT at a sample rate of 20Hz.
• Navigation utilised a integrated Novatel OEM719 DGPS receiver.
• 2 Altimeters were used with a Bendix/King KRA 405 Radar Altimeter with a
resolution of 0.3m and a Renishaw ILM-500R laser altimeter with resolution
of 0.01m.
• No new drilling or geochemical results are being reported.
• No data used to determine mineralisation material to the report.
Drilling techniques
• Drill type (e.g. core, RC, 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).
• Not applicable – geophysical survey data only.
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Criteria and JORC Code
explanation
Commentary
Drill sample recovery
• Method of recording and assessing core
and chip sample recoveries and results
assessed.
• Measures taken to maximise sample
recovery and ensure representative
nature of the samples.
• 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.
• Not applicable – geophysical survey results only discussed in this release.
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.
• Whether logging is qualitative or
quantitative in nature. Core (or costean,
channel, etc) photography.
• The total length and percentage of the
relevant intersections logged.
• Not applicable – geophysical survey results only discussed in this release.
Sub-sampling techniques and sample
preparation
• If core, whether cut or sawn and whether
quarter, half or all core taken.
If non-core, whether riffled, tube sampled,
rotary split, etc and whether sampled wet
or dry.
For all sample types, the nature, quality
and appropriateness of the sample
preparation technique.
Quality control procedures adopted for all
sub-sampling stages to maximise
representivity of samples.
• 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.
• Whether sample sizes are appropriate to
the grain size of the material being
sampled.
• Not applicable – geophysical survey results only discussed in this release.
Quality of assay data and laboratory
tests
Gravity
• Scintrex CG-5 Autograv gravity meters were used for field acquisition.
• For each gravity observation the CG-5 gravity meter was levelled, restricting
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Criteria and JORC Code
explanation
Commentary
• The nature, quality and appropriateness
of the assaying and laboratory
procedures used and whether the
technique is considered partial or total.
• 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.
• 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.
the vertical and horizontal levels to 5 arc seconds.
• Two gravity observations of 20-second stacking time were read and
recorded at each location.
• The instrument was monitored for any seismic or instrumental noise and the
X/Y tilts, temperature and tolerance between readings monitored during the
reading time.
• The tolerance between readings was set at 0.030 of a dial reading and any
readings falling outside of this were re-read.
• Field readings were manually recorded by the field crews in Daishsat gravity
field books along with any observations that may affect the reading.
• During the day the field crews monitored any internal repeat gravity stations
collected for abnormal drift as well as the drift closure at the end of the day.
• A new GNSS base station, numbered 1904, was utilised for reduction and
drift control for the survey.
• The new base was tied with existing Daishsat base 1018 in a gravity control
loop. This base has been tied into the Australian Fundamental Gravity
Network (AFGN).
• A base station reading was taken in the morning before surveying
commenced, and after the last field observation of the day. When taking a
base station reading, the observed gravity values were stacked over 120
seconds to ensure accuracy. Observations were repeated until the readings
repeated to 0.010 of a dial reading or less.
• Data was downloaded on a daily basis and quality control checked for
repeatability of positional and observational data.
• Once data was downloaded, Daishsat’s in-house software was used to
average the two 20-second readings for each gravity station, remove the
Scintrex Earth Tide Correction and assign each gravity positional data from
the processed GNSS data (matched by timestamp). Geosoft GRAVRED
software was then used to perform gravity reductions to produce a set of
observed gravity values that can be used for gridding, imaging, and further
analysis.
AEM
• Xcite Concentric Tx-Rx system with a transmitter of 220 A (max) and a base
frequency of 25 Hz.
• Location data was provided by a Novatel DL-V3L1L2 Gps positioning system
utilising a 12 satellite system.
• Laser Altimeter type was SF-01 with a range of 0-60m and resolution of
1cm.
• Pre Survey QC tests included lag test, alitimeter calibration, high altitude
check.
• During Survey daily field QC incudes monitoring of line path deviation;
altitude deviation; late time noise; GPS satellites
• Results are compared against diurnal base station. The diurnal magnetic
field was recorded at 1 Hz to monitor for excessive diurnal variation. If the
measured diurnal field varied by more than 10 nT per 10 min chord against
the base the data collected during this period was reflown.
• Two high altitude sections are flown with each flight of data acquisition.
These sections are used to determine the system response as a function of
time for each flight. The system response is removed from the measured
data to isolate the true earth response.
• The laser Altimeter is calibrated at the start of every survey.
Magnetics
• The magnetometer was a single sensor tail boom mounted G-823 Cesium
vapour magnetometer with a resolution of 0.001 nT, 0.01 nT sensitivity at a
sample rate of 20Hz with a compensation of 3 axis fluxgate magnetometer.
• Navigation utilised a integrated Novatel OEM719 DGPS receiver with L1/L2
+ GLONASS Multi Frequency across 555- channels.
• Navigation information was supplied to the pilot via an LCD Steering
indicator. All data were synchronised to one pulse per second triggered by
GPS.
• 2 Altimeters were used with a Bendix/King KRA 405 Radar Altimeter with a
resolution of 0.3m sampling at 20Hz with a defined range between 0-760M
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Criteria and JORC Code
explanation
Commentary
and a Renishaw ILM-500R laser altimeter with resolution of 0.01m
SAMPLING UP TO 20Hz and a range of 0-500m
• Magnetics base stations consisted of GEM GSM-19 Overhauser and
Scintrex Envi Mag proton precession base station magnetometers with
resolutions of 0.01 nT and 0.1 nT accuracy at a sample rate of 0.1-0.5Hz.
• Calibration of the Magnetometer included flight of a compensation box prior
to survey. The compensation consisted of a series of pitch, roll and yaw
manoeuvres in reciprocal survey headings at high altitude. The measured
output from the 3-axis fluxgate magnetometer was recorded and used to
resolve a compensation solution. This solution was applied when post-
compensating all survey magnetometer data to remove manoeuvre effects
and heading error.
• GPS accuracy tests were performed by accumulating GPS readings for
approximately 5 minutes whilst the aircraft was static. All readings (X, Y, Z)
were within 2 meters
• Prior to commencement of survey production, the radar altimeter was
checked for linearity by way of a swoop test over flat terrain
• During survey, the pilot monitored system health from prompts on the
navigation screen. The diurnal base stations were monitored by ground
crew.
• Upon completion of each flight all survey data were transferred from the
acquisition system to the infield data processing computer. Using
customised techniques, the data were checked for any errors and
compliance with specifications.
Verification of sampling and assaying
• The verification of significant intersections
by either independent or alternative
company personnel.
• The use of twinned holes.
• Documentation of primary data, data entry
procedures, data verification, data storage
(physical and electronic) protocols.
• Discuss any adjustment to assay data.
• AEM, Magnetics and Gravity data were verified and further processed by
geophysical consultancy, Montana G.I.S.
• Gravity data was QC checked, terrain corrected and processed utilising a
series of industry accepted algorithms to produce a series of gravity images
including Bouguer, Total Bouguer (includes terrain correction), 1VD.
Smoothing and trend removal algorithms were utilised to create residual
gravity images.
• Magnetic Data underwent a number of first order reduction to remove
remove the influence of the modern-day magnetic field inclination &
declination. These included Reduced to Pole, Vertical integration of
Analytical signal and Vector Residual magnetic Intensity.
• These First order reductions are then filtered usining transforms to enhance
their visual character these include Band Pass, High Pass, Tilt filters.
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.
• Specification of the grid system used.
• Quality and adequacy of topographic
control.
Gravity
• Set out of the survey grid was done concurrently with gravity data
acquisition using Leica GX1230 GNSS receivers operating in
autonomous mode. Each individual crew had this ‘roving’ receiver
mounted on a vehicle.
• Raw kinematic GNSS data was logged by the roving receiver(s) at 5
second intervals during acquisition to determine the precise location of
the GNSS antenna. Repeat stations were strategically placed
throughout the survey to monitor and control positional accuracy.
• Where possible, the readings were taken as close as possible to the
nominated coordinates. Some stations were moved from their
nominated coordinates for various reasons including inaccessible (trees
and scrub), topographical features that could introduce severe local
gravity terrain effects and other topographical issues making access to
the station difficult or unsafe.
• Raw GNSS data was processed using Waypoint’s (Novatel) GrafNav
GNSS post-processing software to produce positions accurate to within
a couple centimetres for the roving antenna location at each five second
interval (epoch). This technique is known as Post Process Kinematic
(PPK).
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Criteria and JORC Code
explanation
Commentary
AEM
• Flight survey lines were followed using the onboard Novatel Dl-v3L1L2
real time GPS which utilises 12 satellites with a recording rate of 20 Hz.
• The SF-01 laser altimeter was quality check before initiation of survey
and monitored flight height throughout with a resolution of 1cm.
Magnetics
• Flight Survey Lines were followed utilising an integrated Novatel
OEM719 DGPS receiver with L1/L2 + GLONASS Multi Frequency
across 555- channels with flight height monitored by the 2 onboard
altimeters.
• Navigation information was supplied to the pilot via an LCD Steering
indicator. All data were synchronised to one pulse per second triggered
by GPS.
• The GDA94 datum and MGA Zone 53 projection system was used for all
data
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.
• Whether sample compositing has been
applied.
• Gravity is appropriately spaced (250 x 250m) to allow regional and broad
prospect scale interpretations of geology and structure.
• AEM data has variable line spacing from 800m down to 200m and provides
regional scale information on conductors in addition to some limited prospect
scale information where flight lines intersect areas of interest.
• Magnetic Survey spacing between lines is 25m, 50m and 100m and is
determined to be appropriate for regional and prospect scale interpretation.
• No information from this geophysical survey is used to establish geological
or grade continuity assumptions.
• No sample compositing as geophysical technique only.
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.
• 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.
• Gravity data oriented to allow merge with existing surrounding surveys and is
regarded as a best fit orientation for the survey coverage and for dominant
structural and lithological controls known in the region.
• AEM and Magnetic data is regarded as best fit orientation for dominant
structural and lithological orientations in the region.
• No drilling reported and as such no relationship between orientation of
drilling and mineralised structures is made.
Sample security
• The measures taken to ensure sample
security.
• Geophysical surveys only.
• Geophysical data security via cloud hosted and redundancy backed up
datasets.
Audits or reviews
• The results of any audits or reviews of
sampling techniques and data.
• Geophysical data was audited by Montana G.I.S Geophysics and found to
be acceptable.
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Section 2 Reporting of Exploration Results
(Criteria listed in the preceding section also apply to this section.)
Criteria and 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.
• Exploration was within the Blackhill EL 6475, granted to Alliance (Eyre) Pty
Ltd, a wholly owned subsidiary of Alliance Resources Pty Ltd
• Investigator Resources currently has a Earn-In to Joint Venture agreement
with Alliance Resources who manages EL 6475 holding 100% interest.
• EL 6475 is located on Crown Land covered by several pastoral leases.
• An NTMA has been signed between Alliance (Eyre) Pty Ltd and the
Gawler Ranges Aboriginal Corporation allowing for further
exploration activity to occur.
• There are no registered Conservation or National Parks on EL 6475.
Exploration done by other parties
• Acknowledgment and appraisal of
exploration by other parties.
• The Athena prospect (at the time referred to as
“Sunday Iron”) referenced in this release was originally
explored for magnetite mineralisation by Ironclad Mining
and subsequently Trafford Resources. Shortly after 2013 Trafford changed
name to
Tyranna Resources prior to disposal of the Black Hill and other
tenements in the vicinity to Alliance (Eyre) Pty Ltd, a unlisted
company who are now developing the Weednanna gold project.
• In addition to a number of small RC and aircore drill programs,
additional geophysical surveying included aeromagnetic and
electromagnetic surveys in the region.
• In other areas of the tenement, not subject to the current release
historic work has been undertaken by other parties including
Aberfoyle, Shell, Acacia and MIM Ltd with a focus on base and
precious metals exploration.
Geology
• Deposit type, geological setting and style
of mineralisation.
• The Athena prospect is associated with a magnetic high attributed to
magnetite enrichment that may be associated with potential iron rich
metasedimentary units of the Hutchison Group with historic drilling
identifying iron in the 30-60% range.
• Silver mineralisation appears to be associated with calc silicate
sequences that host a magnetite skarn that may be closely
associated with a proximal granite inferred to be Hiltaba age, and at
a structural junction in magnetics.
• The prospect is along the south-eastern extension of a structural and
stratigraphic corridor that links it with the Paris silver deposit
approximately 12km to the north-west. The Paris Project is a Ag-Pb
deposit that is hosted predominantly within a sequence of flat lying
polymict
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