Juno Project, Australia

Introduction

Juno Project, Australia - Mineral Exploration Opportunity for Havieron Style Intrusion Related Gold System.

The Juno Project is located in Western Australia approximately 100km south of the town of Paraburdoo. The project area is leasehold cattle farming and access is via formed gravel roads from Meekatharra to the Pingandy pastoral lease.

Exploration Licence 08/3497 was granted and held 100% by Callum Baxter in 2023. As part of the transition into gold exploration, Geo Exploration has acquired 80% of the exploration licence.  Callum Baxter will be a consultant to the company for the exploration of the gold licence and now retains 20% of the licence.

Callum Baxter is a geologist with more than 30 years’ experience in global mineral exploration and was founding director of Greatland Gold plc, which is credited with the discovery of the Havieron deposit in Western Australia – an intrusion related gold system; which following discovery of Havieron had a peak market cap +£500m.

Background

Globally, intrusion related gold systems (IRGS) display a broad range of styles, but key components in Western Australia are Proterozoic age carbonate rich host rocks, moderate structural deformation of host rocks, proximity to basin margin faults, and proximity to post depositional granite intrusions.

Due to high sulphide content buried (not outcropping) IRGS deposits are exceptionally well detected by geophysical methods such as magnetics, gravity, induced polarisation (IP) and/or electromagnetics (EM)

The Juno project is located in carbonate rich, low to moderately deformed Proterozoic host rocks on northern margin of basin proximal to major basin structures.

The Abra deposit is located 100km south-east of Juno in the same Proterozoic basin and displays IRGS type features. Abra was discovered following airborne geophysical surveys.

The discrete magnetic feature at Juno is approximately 5km x 5km in size. By way of comparison, the discrete magnetic target at Havieron is 1km x 1km in size currently 8.4Moz AuEq.

Historic work programme

An airborne magnetic survey which was carried out in the early 90s identified the Juno target. This was followed up by ground based magnetic and gravity surveys which were completed in the mid 1990s. This work was carried out by Australian companies Newcrest Mining and Pasminco.

Pasminco recognised the coincident nature of the Juno magnetic and gravity features and applied an Iron Oxide Copper Gold (IOCG) model. IOCG deposits are large and often display coincident magnetic and gravity signatures.

Pasminco modelled the geophysical data and planned a single drillhole to test the target – HD1

HD1 failed to intersect the source of the magnetic and gravity feature as it was poorly sited. The hole also failed to achieve target depth due to the small capacity of the drilling equipment.

However, HD1 intersected rocks which displayed thermal alteration and disseminated sulphide mineralisation suggesting close to source – skarn type features as were seen at Havieron.

Follow up work in the early 2000s by Udu Resources consisted of re-evaluating  Juno as an IOCG target. Udu conducted a limited ground Electro Magnetic survey over a part of the Juno target which was successful in detecting a strong conductor. However, the aerial extent of the survey was insufficient relative to the size of the Juno target. Udu also drilled several drillholes UHC1-4 to test the target. All holes failed to penetrate the surface rocks due to the limited capacity of the drilling equipment.

Since the early 2000s there has been little to no work carried out in the Juno area. Callum Baxter applied for the current licence in 2022 and the licence was granted in 2023.

Historical data from the 90s and early 2000s is poorly constrained and more modern surveys are required to better locate and ‘see’ the target using up to date modelling techniques, as used in the Havieron discovery.

Current Status

Geo plan to use modern drilling equipment and techniques to further explore the Juno target.

An indicative timeline of activity is outlined below:

Exploration Licences 52/4391 and 08/3744

The Company has applied for two further Exploration Licences, 52/4391 and 08/3744, adjacent to the current Exploration Licence 08/3497 in Western Australia, via its wholly owned subsidiary Juno Gold Pty Ltd.

Callum Baxter, exploration geologist consulting to the Company, has identified potential exploration targets within these licences which share geophysical similarities to the target within Licence 08/3497.

The Company is using an intrusion related deposit exploration model seeking to locate precious and base metal mineralisation, similar to that at the Havieron and Telfer deposits in northern Western Australia.

Progress to Date

  • October 2024 – Commencement of the Airborne Geophysical Survey.
  • October 2024 – Site visit by Callum Baxter and team with initial area of interest deemed good, via historical tracks. Meeting with the local pastoralist very positive, and he is very supportive of proposed exploration activities.
  • November 2024 – Results of Airborne Geophysical Survey received
  • November 2024 – Ground Based Gravity Survey Commencement at Juno Project
  • December 2024 – Completion of airborne Light Detection and Ranging (Lidar) acquisition data.

Aeromagnetic Results

The Company’s main focus at Juno is targeting Intrusion Related Gold Systems (IRGS) similar to Havieronand Telfer. Havieron and Telfer are large gold and copper deposits located in the north of Western Australia.
Gold and copper mineralisation at Havieron was discovered following exploration drilling of a strong discrete magnetic feature. Havieron also displays a coincident gravity response.
Geo has targeted the northern parts of E08/3497 as its initial area of focus. Processing and imaging of aeromagnetic data covering the northern portion of the main Juno magnetic feature is complete (Figure 1). Imaging has revealed the data is of high quality and very detailed in nature.
The new aeromagnetic data confirms the location, highlights the strong intensity and verifies the large size of the Juno magnetic feature. This new detailed aeromagnetic data reveals structures and other features not seen in historical, lower resolution, magnetic data. The aeromagnetic survey was carried out during October 2024 using a fixed wing aircraft at 50m line spacing.

Figure 1 – Newly acquired 50m line spaced data overlayed on historic 400m line spaced data.

Final Ground Gravity Data Received for Juno Project

  • Analysis confirms a significantly large residual gravity response
  • Large gravity response spatially aligns with prominent magnetic feature at Juno
  • Alignment is typical signature of IRGS style mineralisation as per Havieron copper gold deposit.
Ground gravity data was collected over the central north of the Juno Project area from late November to mid December 2024. A total of 1400 ground gravity observations were taken at station spacings of 400m x200m, and 200m x 200m where added resolution was required. Post processing and imaging of the gravity data was completed during late December 2024 and early January 2025. Delivered products include high resolution raw and residual gravity data.
The newly acquired 2024 ground gravity data has successfully confirmed the gravity response that was initially suggested by the historic work from the 1990s. Importantly, the Company’s recent detailed and spatially accurate gravity work has successfully identified a significant residual gravity response that is coincident with the large magnetic response at Juno (Figure 1).
The residual gravity response covers an area of approximately 4km x 2km (8sq kms) with a peak amplitude of 2mgal. The magnetic feature covers an area of approximately 5km x 2km (10sq kms) with a peak response of +1000nT. Coincident magnetic and gravity response of this size and amplitudes is consistent with IRGS and IOCG (Iron Oxide Copper-Gold) type deposits.
 The Company is targeting IRGS type mineralisation at Juno. By comparison, Havieron, a large IRGS gold and copper deposit (+8Moz gold equivalent) located in the north of Western Australia, displays a 1km x 1km (1 sq km) magnetic response with a coincident gravity response peaking at 0.5mgal. The intensity of the gravity response at Juno is more elevated than Havieron, and the footprint of the coincident response at Juno is several times larger which illustrates the significant size of the opportunity at Juno.

Figure 1 – Juno Aeromagnetics and Ground Gravity

Several historic exploration holes have been attempted at Juno since the mid 1990s to the early 2000s (Figure 2). Several holes targeted the large Juno magnetic feature but failed to reach the target depth due to limited capacity drilling equipment. Modern drilling equipment has the ability to overcome these earlier shortcomings, and advanced modelling of detailed subsurface geophysical data provides accurate 3D models for efficient drill targeting.

Figure 2 – Juno Project Aeromagnetics (image) with Residual Ground Gravity (contour) and historic drilling.