Great Western Exploration Hits Outer Shell of New VHMS System Near DeGrussa

Great Western Exploration's maiden RC drilling at the Juggernaut Project has returned zinc-silver mineralisation interpreted as the outer margin of a new VHMS system just 70km from Sandfire's DeGrussa deposit — with the copper-gold core still untested and squarely in the crosshairs of follow-up drilling.
By William Hadrian -
  • Maiden RC drilling at the Seymour Target returned zinc-silver intercepts including 12m @ 0.33% Zn, 7g/t Ag from 77m and 5m @ 0.22% Zn, 2g/t Ag from 98m, interpreted as the outer margin of a new VHMS mound system.
  • The copper-gold core of the interpreted VHMS system — the highest-value target — has not yet been drilled and sits between and below the two key holes, making it the primary focus of follow-up work.
  • The Seymour Target sits 70km from Sandfire Resources' DeGrussa copper-gold VHMS deposit in the adjacent Bryah Basin, a globally recognised benchmark VHMS discovery.
  • GTE identified this mineralisation through geological mapping and interpretation alone, without a pre-existing geophysical bullseye — a meaningful validation of the company's exploration methodology in a largely untested basin.
  • The forward programme includes airborne infill magnetics, potential down-hole EM surveys, and follow-up RC drilling, with permitting being progressed as a priority before the next drill campaign can begin.
Summarise with AI:

Maiden drilling at Juggernaut flags new VHMS system on the doorstep of DeGrussa

Great Western Exploration (ASX: GTE) has returned zinc-silver mineralisation from its maiden RC drilling programme at the Seymour Target within the Juggernaut Copper-Gold Project, with results interpreted to represent the outer margin of a new seafloor “mound” type Volcanic Hosted Massive Sulphide (VHMS) system. The critical hook for investors: the copper-gold core of that system has not yet been intersected.

The Seymour Target sits 70km from Sandfire Resources’ (ASX: SFR) DeGrussa VHMS copper-gold deposit in the adjacent Bryah Basin, one of the world’s benchmark VHMS discoveries. The Juggernaut project is located on the western portion of the Yerrida Basin, approximately 800km north-east of Perth.

Key assay results from the programme include:

  • 12m @ 0.33% Zn, 7g/t Ag, and 0.09% Pb from 77m (drill-hole 26GJGRC006), including 1m @ 1.02% Zn from 81m and 2m @ 20g/t Ag from 85m
  • 5m @ 0.22% Zn, 2g/t Ag, and 0.15% Pb from 98m (drill-hole 26GJGRC002)

The copper-gold core, interpreted to lie between and below these two holes, remains the primary target for follow-up drilling.

What is a VHMS system, and why does zinc at the edges matter?

A Volcanic Hosted Massive Sulphide system forms on the ancient seafloor when superheated mineral-rich fluids (hydrothermal fluids) vent through cracks in the ocean crust and mix with cold seawater. As the fluids cool rapidly, metals precipitate out and accumulate in layered deposits directly on the seafloor. The result is a “mound” of stacked mineralisation, with different metals concentrating at different temperatures and distances from the vent.

Reading the mineralisation signature

Think of a VHMS mound like a target with concentric rings. The hottest zone sits closest to the vent and is enriched in copper and gold. Moving outward, as temperatures drop, the mineralisation transitions to zinc, lead, and silver. This zoning is predictable and well-documented across VHMS deposits globally.

The geochemical signature recorded at Seymour, a Zn-Ag-Pb-Cd-S +/- Tl fingerprint, is characteristic of the outer, cooler margins of this style of system. In the schematic diagram of a VHMS mound (Figure 3 in the announcement), the outer zone is represented by “black ore” rich in zinc, lead, and silver, while the hotter inner core is represented by “yellow ore” enriched in copper. The Seymour intercepts, as annotated in that figure, plot in the outboard position relative to the interpreted copper core.

Two additional geological features support this interpretation. First, the drilled intercepts contain 1–5% sulphide mineralisation within the host rocks, a positive indicator of a fertile VHMS system rather than a barren zone. Second, and critically, these intercepts were recorded at a shale-mafic volcanic rock contact, the ideal geological boundary for mound-type VHMS development.

GTE interprets the high-temperature copper-gold core to lie between drill-holes 26GJGRC002 and 26GJGRC006, and below the current drilled depth. That gap between the two holes is precisely where follow-up drilling is now being prioritised.

Why Seymour is a genuine discovery-stage opportunity

The Yerrida Basin remains largely untested for VHMS

The Yerrida Basin is geologically similar to and of comparable age to the Bryah Basin, the basin that hosts both DeGrussa and the Monty copper-gold VHMS deposit. Despite this geological kinship, very little systematic VHMS exploration has been conducted in the Yerrida.

What makes the Seymour result particularly notable is the absence of a clear discrete geophysical or surface geological target guiding the maiden programme. GTE defined a new potential VHMS system through sustained geological mapping, interpretation, and modelling alone. Finding mineralisation interpreted as part of a VHMS system in a maiden campaign, without a pre-existing geophysical bullseye to aim at, is a meaningful validation of the company’s systematic exploration methodology.

The copper-gold core is the next target

The cross-section interpretation (Figure 4 in the announcement) illustrates how the two key drill-holes are interpreted to have intersected opposite edges of the same stratigraphy, which appears to be folded. This geometry places the highest-priority copper-gold target in the zone between and below 26GJGRC002 and 26GJGRC006.

GTE’s planned next steps are:

  1. Airborne infill magnetics survey planned prior to and concurrently with drilling
  2. Potential down-hole EM survey planned to further refine the mineralisation model
  3. Follow-up RC drilling targeting the zone between 26GJGRC002 and 26GJGRC006, plus extensions north and south (Figure 5)
  4. Permitting being progressed as quickly as possible
  5. Geophysical surveys to be undertaken concurrently to optimise drill targeting

Baroo: a secondary copper target also advancing

The Baroo Target, identified during earlier regional geological mapping and rock-chipping, was also tested in this programme. Two shallow RC holes intersected a quartz vein below surface, returning 1m @ 0.2% Cu from 24m (26GBBRC002) and 1m @ 514ppm Cu from 25m (26GBBRC001).

The results are modest, but GTE interprets the width and tenor of copper mineralisation to increase at depth below the drilled intercepts. Further drilling is planned concurrently with Juggernaut follow-up. Seymour remains the primary story; Baroo is a secondary thread worth watching.

Key results at a glance

Drill Hole Target From (m) Interval (m) Key Grades
26GJGRC006 Seymour, Juggernaut 77m 12m 0.33% Zn, 7g/t Ag, 0.09% Pb
26GJGRC006 (incl.) Seymour 81m 1m 1.02% Zn
26GJGRC006 (incl.) Seymour 85m 2m 20g/t Ag
26GJGRC002 Seymour, Juggernaut 98m 5m 0.22% Zn, 2g/t Ag, 0.15% Pb
26GBBRC002 Baroo 24m 1m 0.2% Cu

All reported intervals are downhole lengths. True widths are not yet known at this stage of exploration.

What’s next for Great Western Exploration

The focus now shifts to permitting and geophysics. GTE has stated it is moving as quickly as possible to secure the permits required for follow-up drilling at Seymour, with that permitting being progressed as a priority. A market update is expected once permitting is completed.

The forward programme, in sequence, is:

  1. Permitting for follow-up drilling at Seymour progressing as a priority
  2. Airborne infill magnetics and potentially down-hole EM surveys prior to and concurrent with drilling
  3. Follow-up drill targets defined between and around 26GJGRC002 and 26GJGRC006, plus along-strike extensions north and south
  4. Baroo follow-up drilling planned concurrently
  5. Market update to follow once permitting is completed

No resource estimates have been defined at this stage, and no timelines beyond the permitting and survey sequence have been disclosed.

Juggernaut Project Forward Work Program

GTE’s Oval Copper-Gold Target, tested through diamond drilling as a separate programme, returned preliminary observations consistent with a significant copper-gold system, adding another thread to the company’s expanding discovery pipeline across its Yerrida Basin tenure.

The geological logic here is straightforward: GTE has found the outer shell of what is interpreted to be a new VHMS system in its very first drilling campaign at Seymour, conducted without a pre-existing geophysical target. The company holds a prominent tenement package over the largely underexplored Yerrida Basin, a basin considered geologically similar to and of comparable age to the Bryah Basin, host to both DeGrussa and Monty. The copper-gold core interpreted to lie between and below the current holes is the prize that the next phase of work is designed to test.

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Frequently Asked Questions

What is a VHMS system and why does it matter for copper-gold exploration?

A Volcanic Hosted Massive Sulphide (VHMS) system forms when superheated mineral-rich fluids vent through ancient ocean crust and cool rapidly, depositing layered metals including copper, gold, zinc, lead, and silver. They matter because they can host large, high-grade copper-gold deposits — Sandfire's DeGrussa mine in Western Australia is a globally recognised example of this deposit style.

What did Great Western Exploration find at the Juggernaut Project?

Great Western Exploration's maiden RC drilling at the Seymour Target returned zinc-silver mineralisation, including 12m at 0.33% zinc and 7g/t silver from 77m depth, interpreted as the outer margin of a new VHMS mound system. The copper-gold core of the system, which is the primary target, has not yet been drilled and sits between and below the two key holes.

How close is the Juggernaut Project to Sandfire's DeGrussa deposit?

The Seymour Target within the Juggernaut Project sits approximately 70km from Sandfire Resources' DeGrussa copper-gold VHMS deposit, which is located in the adjacent Bryah Basin. The Yerrida Basin, where Juggernaut is located, is considered geologically similar to and of comparable age to the Bryah Basin.

What are the next steps for Great Western Exploration at the Juggernaut Project?

GTE is prioritising permitting for follow-up drilling at the Seymour Target, after which it plans airborne infill magnetics and potentially down-hole EM surveys to refine drill targeting. Follow-up RC drilling will focus on the zone between and below the two existing holes, where the copper-gold core is interpreted to sit, with along-strike extensions also planned.

Why does zinc mineralisation at the edges of a VHMS system indicate a copper-gold core might exist?

VHMS deposits are zoned by temperature: copper and gold concentrate closest to the hydrothermal vent where temperatures are highest, while zinc, lead, and silver deposit further out where fluids have cooled. Finding zinc-silver mineralisation at the outer margin of a VHMS system is a geological indicator that a hotter copper-gold core may exist closer to the original vent source.

William Hadrian
By William Hadrian
Partnerships Director
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