The latest Investing Matters Podcast episode featuring financial educator and author Jared Dillian has been released. Listen here.

Less Ads, More Data, More Tools Register for FREE

Pin to quick picksEmpire Metals Regulatory News (EEE)

Share Price Information for Empire Metals (EEE)

London Stock Exchange
Share Price is delayed by 15 minutes
Get Live Data
Share Price: 9.10
Bid: 9.00
Ask: 9.20
Change: -0.15 (-1.62%)
Spread: 0.20 (2.222%)
Open: 9.80
High: 10.05
Low: 8.90
Prev. Close: 9.25
EEE Live PriceLast checked at -

Watchlists are a member only feature

Login to your account

Alerts are a premium feature

Login to your account

Giant Copper Province Potential Confirmed by DD-IP

6 Feb 2023 07:00

RNS Number : 9179O
Empire Metals Limited
06 February 2023
 

Empire Metals Limited / LON: EEE / Sector: Natural Resources

 

06 February 2023

Empire Metals Limited

("Empire" or "the Company")

 

Geophysical Survey Results Confirm Pitfield's Potential as a Giant Copper Province

 

Empire Metals Limited (LON: EEE), the AIM-quoted resource exploration and development company, is pleased to announce the results of the Dipole - Dipole Induced Polarisation ("DD-IP") surveys carried out at the Pitfield Copper Project ("Pitfield"), located in Western Australia.

 

Highlights

· DD-IP surveys have identified multiple drilling targets and provided further evidence to support the view that Pitfield has the potential to contain multiple sediment-hosted stratabound copper ("SSC") deposits across a 40km long, massive alteration footprint.

identification of several anomalies with chargeable values that exceed the threshold that would be considered characteristic of the presence of disseminated sulphides.

these chargeable and highly resistive anomalies are closely associated with the magnetite-altered stratigraphy and are coincident with strong copper anomalism in both soils and rocks.

located in the same vicinity as the high-grade soil and rock samples that were recently collected (announced 30 January 2023) these chargeable anomalies add further evidence to support the possible presence of SCC deposits.

the highly chargeable anomaly detected in three DD-IP survey lines just southwest of Mt Scratch appears to be very extensive, covering an area of at least 1,500m in length and up to 800m wide.

A second highly chargeable anomaly was identified in a DD-IP line 12km south of and broadly along the same geological trend as Mt Scratch.

· Completion of the initial soil sampling and DD-IP surveying is expected in Q1 2023 with a view to expediting a maiden drill programme at Pitfield to better understand the geology and to determine the significance of these highly chargeable-highly resistive zones.

 

Shaun Bunn, Managing Director, said: "I am delighted to provide an update on our initial DD-IP survey activities, a reconnaissance mission focussing on areas that were previously under-explored by the major mining companies that have worked the area. These highly encouraging results from the DD-IP surveys suggest the presence of large, disseminated sulphide mineralised zones, thus providing multiple drill targets and providing another leap forward in our plans to commence drilling activities at Pitfield.

 

"Our immediate focus will be on drilling at the Mt Scratch Prospect, where we have identified a massive highly chargeable anomaly. It is important to note that the Mt Scratch Prospect on its own only represents 5% of the overall project area. The coincidence of multiple highly chargeable anomalies, extensive magnetite alteration and elevated copper in soils and rocks, extending over much of the 40km long N-S massive alteration zone, supports our view that Pitfield has the geological hallmarks of a "Giant" copper mineralised system and we intend to continue our soil sampling and DD-IP surveying activities over the coming months to identify additional drill targets."

 

DD-IP Survey Results

Induced Polarisation ("IP") is a survey technique where electrodes induce and measure a potential field in the ground. From this data, the soil chargeability and apparent resistivity can be measured (for more details on IP and DD-IP refer to the section "Dipole-Dipole Array Explained").

 

Five traverses of DD-IP for a total of 8,450 Line metres (refer Table 1 and Figure 1) were completed by contractor Kinematix Pty Ltd from 8-17 December 2022 over selected exploration targets considered geologically favourable for SSC systems.

 

 

Name

Length

Min

Easting

Min

Northing

Max

Easting

Max

Northing

Line PM01

2000

367950

6753800

369950

6753800

Line PM02

1850

368100

6753000

369950

6753000

Line PM03

1700

368300

6752250

370000

6752350

Line PM04

1200

370600

6752000

371800

6752000

Line GC01

1700

370500

6739000

372200

6739000

Table 1.DD-IP Survey Lines completed (GDA2020 MGA Z50)

 

 

 

Figure 1. Location of the five DD-IP Survey Traverses.

 

One of these key exploration targets was the Mt Scratch Prospect where Lines PM01, PM02 and PM03 were completed on 800m spaced sections to evaluate known copper anomalism and strong magnetite alteration of host sandstone and siltstone rock sequences (Figure 2).

 

Recent soils results in this area also show an association of elevated copper values with the magnetite-altered stratigraphy, and rock samples from surface float (originally shallow prospector workings which have subsequently been backfilled) recorded copper values up to 17.9% Cu and 125 g/t Ag, a very encouraging indicator that copper-silver sulphides are present in the area.

 

 

Figure 2. High copper-in-soil and rock samples collected surface in close proximity to DD-IP traverses.

 

The data quality was considered to be very good for most of the DD-IP lines at Pitfield, with the exception of PM04 where conductive overburden caused low signal levels. The chargeability highs seen in the dataset are predominantly associated closely with zones of higher resistivity which could be explained by the effects of hydrothermal alteration such as silicification.

 

The IP Inversion models were processed by Terra Resources Pty Ltd ("Terra"). Terra specialises in geophysical survey design, acquisition, processing, modelling, inversion, data integration, interpretation and drill hole targeting. Terra uses the Newmont standard chargeability for processing of time-domain IP data. The chargeability is integrated over a window of 450 - 1,100 ms. This is done to reduce the effects of EM coupling, and to provide a consistent gauge of chargeability vs sulphide content.

 

The IP Inversion models for DD-IP traverses PM01-03 and GC01 are presented below. The IP Inversion models have been coloured to highlight in red areas where the chargeability exceeds 15mV/V, which is indicative of permissive sulphide zones.

 

 

Figure 3 PM01 (L6753800N) - Sulphide Cutoff (15 mV/V) Colouring

Figure 4 PM02 (L6753000N) - Sulphide Cutoff (15 mV/V) Colouring

 

Figure 5 PM03 (L6752250N) - Sulphide Cutoff (15 mV/V) Colouring

Terra Resources description of each traverse is summarised below:

 

PM01: highly chargeable zone extends across entire 800m width of magnetic stratigraphic units The high-grade copper in rock chips returned from surface float is located on the eastern edge of the IP chargeability feature in Figure 3 which also closely matches the highest chargeability values. A second smaller IP anomaly is located close to a magnetic feature at the eastern end of the line.

 

PM02: the 800m wide chargeable zone matches PM01, with the zone shifting to the East with the strike of the magnetic stratigraphy, and highest chargeability values also close to the eastern side of the IP high feature (Figure 4)

 

PM03: highly chargeable zones developed at edges of the most magnetic unit with large East-West trending fault interpreted from the magnetic data directly to the South (Figure 5).

 

GC01: chargeable zone coincides with a subtle discrete magnetic feature with NNW strike. (Figure 6).

 

Figure 6. GC01 (L6739000N) - Sulphide Cutoff (15mV/V) Colouring

 

Figure 7: Magnetic Inversion Comparison to Chargeable Zones Plan

 

Figure 7 shows regions of high chargeability (pink > 15 mV/V) from IP survey (yellow) over magnetics in plan view. The magnetics are linearly colour stretched on different colour scales to emphasise structural features.

 

In the images presented below chargeability inversion sections are compared with 3D magnetic inversions in order to demonstrate a strong correlation in the two independent datasets between magnetite alteration and possible presence of sulphides (Figures 8 and 9.).

 

Figure 8: Magnetic Inversion Comparison to Chargeability Sections 3D View - PM01- 04

 

These images show the spatial comparison between 3D magnetic inversion volumes (pink) and 2D IP inversion sections. The IP sections have been colour-scaled to show sulphide-permissive zones (>15mV/V - Newmont standard chargeability) in red. The section spacing of the IP sections PM01-PM03 is approximately 800m, demonstrating potential continuity of the IP feature for at least 1,500m.

 

The large high magnetic susceptibility body in the western part of the area, shows a strong spatial association with high chargeability, most intensely developed in line PM02. Geological mapping shows stratigraphy is dipping moderately to steeply east, so magnetic (modelled to moderate depths of several hundred metres) and IP features (modelled to maximum of 200m depth) would be expected to extend to depth in this orientation, as would any associated SSC mineralisation.

 

There is a subordinate, thinner high magnetic/IP zone in the eastern side of PM01-03.

 

PM04 does not show this same magnetic/IP correlation with only weak IP and magnetic anomalism present, possibly due to the highly conductive surface layer and commensurate weak basement IP signal.

 

In the case of GC01 (Figure 9) geological mapping confirmed that the strongly magnetic feature located in the centre of the section is associated with a structural repetition of the Beaconsfield conglomerate, part of the lower red-bed sequence. The location of the IP feature on the eastern end of the line is highly significant in terms of the SSC model - potentially close to the expected position of the first reduced layer within the overlying Mt Scratch sequence.

Figure 9. Magnetic Inversion Comparison to Chargeability Sections 3D View - GC01

 

Dipole-Dipole Array Explained

 

IP surveys can be acquired using a multitude of array types, including Dipole - Dipole, Pole - Dipole, Pole - Pole, Gradient, Schlumberger and Wenner. The Dipole - Dipole array is one of the more common techniques used due to a number of advantages, including its speed, its high resolution and multi-channel capability, and because it provides a very detailed image instead of providing a "big picture" image such as the Wenner array.

 

A dipole is a pair of oppositely charged electrodes that are so close together that the electric field seems to form a single electric field rather than a field from two different electric poles. The dipole-dipole array consists of a current electrode pair and a potential electrode pair and it offers a way to plot raw data in order to get an idea of a cross-section of the earth. Those using the dipole-dipole array look at a measurement value called apparent resistivity, which represents a weighted average of the resistivities under the four electrodes used to take the reading. The apparent resistivity is typically calculated by modern instruments from the geometry between the four electrodes and the injected current and measured potential.

 

The dipole-dipole method has made it easier to visualise the collected data in the form of 2D handmade contour plots. The result of a dipole-dipole survey is plotted in a pseudo-section. For each measurement, the apparent resistivity data is plotted at the midpoint between the two dipoles and at a depth half the distance between the two dipoles.

 

The value is finally contoured and colorised, which represents an image of the subsurface. So while this array doesn't provide an actual image of the ground, the data points resulting from these measurements provide an image of the cross section that can then be interpreted by the geophysicists. With the use of inversion software these apparent resistivity and chargeability values can be converted to "true" resistivity and chargeability values so that a realistic image of the ground can be created.

 

Market Abuse Regulation (MAR) Disclosure

Certain information contained in this announcement would have been deemed inside information for the purposes of Article 7 of Regulation (EU) No 596/2014, as incorporated into UK law by the European Union (Withdrawal) Act 2018, until the release of this announcement.

 

**ENDS**

 

For further information please visit www.empiremetals.co.uk or contact:

Empire Metals Ltd

Shaun Bunn / Greg Kuenzel

Tel: 020 7907 9327

S. P. Angel Corporate Finance LLP (Nomad & Broker)

Ewan Leggat / Adam Cowl

Tel: 020 3470 0470

Shard Capital Partners LLP (Joint Broker)

Damon Heath

Tel: 020 7186 9950

St Brides Partners Ltd (Financial PR)

Susie Geliher / Ana Ribeiro / Max Bennett

Tel: 020 7236 1177

 

About Empire Metals Limited

Empire Metals is an AIM-listed (LON: EEE) exploration and resource development company with a project portfolio comprising gold interests in Australia and Austria.

 

The Company's strategy is to develop a pipeline of projects at different stages in the development curve. Its initial focus has been on the high-grade Eclipse and Gindalbie Gold Projects in Western Australia. The Company expanded its exploration licence area in April 2022 from 9.5km2 to 1,728km2 with the acquisition of the Pitfield Copper-Gold Project and the Walton Copper-Gold Project in Western Australia, and the Stavely Copper-Gold Project in the Stavely Arc region of Victoria. 

 

Empire also holds a portfolio of three precious metals projects located an historically high-grade gold production region comprising the Rotgulden, Schonberg and Walchen prospects in central-southern Austria.

 

The Board continues to evaluate opportunities through which to realise the value of its wider portfolio and reviews further assets which meet the Company's investment criteria.

This information is provided by RNS, the news service of the London Stock Exchange. RNS is approved by the Financial Conduct Authority to act as a Primary Information Provider in the United Kingdom. Terms and conditions relating to the use and distribution of this information may apply. For further information, please contact rns@lseg.com or visit www.rns.com.RNS may use your IP address to confirm compliance with the terms and conditions, to analyse how you engage with the information contained in this communication, and to share such analysis on an anonymised basis with others as part of our commercial services. For further information about how RNS and the London Stock Exchange use the personal data you provide us, please see our Privacy Policy.
 
END
 
 
DRLDZGGZFFZGFZM
Date   Source Headline
7th Feb 202212:26 pmRNSHolding(s) in Company
28th Jan 202212:14 pmRNSUpdate on Central Menzies Gold Project
26th Jan 20227:19 amRNSTribute Agreement for the Eclipse Gold Project
20th Dec 20217:00 amRNSExploration Update for the Eclipse Gold Project
2nd Dec 20217:00 amRNSPhase 2 Drilling Commences at Central Menzies
3rd Nov 202111:06 amRNSSecond Price Monitoring Extn
3rd Nov 202111:00 amRNSPrice Monitoring Extension
3rd Nov 20217:00 amRNSDrill Results for the Central Menzies Gold Project
12th Oct 20217:00 amRNSInvestor Presentation
1st Oct 20217:00 amRNSSoil Sampling Results - Central Menzies Project
30th Sep 20217:00 amRNSInterim Results
15th Sep 20217:00 amRNSTechnical update for the Eclipse Gold Project
9th Sep 20217:00 amRNSDrilling Commences at the Central Menzies Project
7th Sep 20217:11 amRNSAppointment of Key Personnel to Exploration Team
31st Aug 20215:12 pmRNSHolding(s) in Company
31st Aug 20217:00 amRNSDirector Dealings
25th Aug 202111:05 amRNSSecond Price Monitoring Extn
25th Aug 202111:00 amRNSPrice Monitoring Extension
25th Aug 20217:00 amRNSProgress update for the Eclipse Gold Project
19th Aug 20217:00 amRNSDrilling to Commence: Central Menzies Gold Project
28th Jul 20217:00 amRNSIdentification of new Twin Shafts Lode at Eclipse
7th Jul 20212:50 pmRNSHolding(s) in Company
17th Jun 20219:00 amRNSPublication of New Investor Presentation
16th Jun 20219:30 amRNSCentral Menzies Gold Project Update
10th Jun 20212:05 pmRNSCompletion of Sale of 50% Interest in CGC
9th Jun 20217:00 amRNSInvestor Presentation
7th Jun 202112:49 pmRNSFinalised Sale of 50% Interest in Georgian Assets
20th May 20212:05 pmRNSSecond Price Monitoring Extn
20th May 20212:00 pmRNSPrice Monitoring Extension
20th May 20217:00 amRNSOption to Acquire Highly Prospective Gold Project
17th May 202111:06 amRNSSecond Price Monitoring Extn
17th May 202111:00 amRNSPrice Monitoring Extension
17th May 20217:00 amRNSAppointment of Managing Director
27th Apr 20217:00 amRNSDrilling Recommences at Eclipse Gold Project
19th Apr 20217:00 amRNSFinal Results
17th Mar 20211:35 pmRNSNext Phase to Commence at Eclipse Gold Project
16th Mar 20217:00 amRNSNext Phase at Eclipse Gold Project
25th Feb 20212:06 pmRNSSecond Price Monitoring Extn
25th Feb 20212:00 pmRNSPrice Monitoring Extension
22nd Feb 20217:00 amRNSEclipse Acquisition Completion & Issue of Equity
18th Feb 20217:00 amRNSFurther Drilling Results at Eclipse Gold Project
1st Feb 202110:10 amRNSGrant of Options and Director Shareholding
1st Feb 20217:00 amRNSCorporate Update, Drilling Update & Board Changes
7th Jan 202112:30 pmRNSSecond Phase Drilling Commences at Eclipse Project
30th Dec 202010:30 amRNSFIRB Approval
10th Dec 20207:00 amRNSDrilling Results & 75% Acquisition of Eclipse
27th Nov 20203:06 pmRNSHolding(s) in Company
24th Nov 20201:26 pmRNSPlacing to Acquire 75% of Eclipse Gold Project
11th Nov 20203:30 pmRNSResult of General Meeting
6th Nov 20207:00 amRNSDrilling Update at Eclipse Gold Project

Due to London Stock Exchange licensing terms, we stipulate that you must be a private investor. We apologise for the inconvenience.

To access our Live RNS you must confirm you are a private investor by using the button below.

Login to your account

Don't have an account? Click here to register.

Quickpicks are a member only feature

Login to your account

Don't have an account? Click here to register.