Azimut and KGHM Drill High-Grade Nickel-PGE Mineralization on the Kukamas Property, James Bay Region, Quebec

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Exploration Azimut Inc
Exploration Azimut Inc

8.42% Ni, 0.55% Cu, 7.25 g/t PGE over 1.9 m
6.06% Ni, 0.38% Cu, 3.34 g/t PGE over 2.6 m
3.55% Ni, 0.19% Cu, 2.19 g/t PGE over 2.5 m
0.81% Ni, 0.07% Cu, 0.52 g/t PGE over 24.2 m

LONGUEUIL, Quebec, Jan. 20, 2025 (GLOBE NEWSWIRE) -- Azimut Exploration Inc. (“Azimut” or the “Company”) (TSXV: AZM) (OTCQX: AZMTF) is pleased to announce the results of the maiden 2,000-metre diamond drilling program on the Kukamas Property (the “Property”) in the Eeyou Istchee James Bay (“James Bay”) region of Quebec. The Property is subject to an option agreement with KGHM International Ltd (“KGHM”), with Azimut as the operator.

The drilling program consisted of 9 holes (KUK24-001 to -009) for a total of 1,998.5 metres to complete a first assessment of the Perseus and Halley magmatic nickel sulphide surface discoveries (see press release of April 2, 2024, and September 23, 2024) and other strong conductors defined by airborne and ground electromagnetic (“EM”) geophysical surveys.

This phase confirms the Perseus Zone as a significant high-grade nickel and platinum group element (“PGE”) discovery, likely associated with komatiitic volcanics. A second mineralized horizon, also hosted in komatiites, has been intersected approximately 80 metres deeper (along hole) from the Perseus horizon. Both zones remain open in all directions. The features of the mineralization (high-grade Ni, high Ni/Cu ratio, high Pd/Pt ratio) and the lithological context highlight a fertile system, with similarities to Archean Kambalda-type komatiitic nickel deposits, exemplified by the Kambalda district in Western Australia.

These initial results underscore the potential of Kukamas, which also hosts several under-explored, kilometre-scale, high-quality nickel targets. A work plan for 2025 is currently being developed to further advance the Perseus discovery and test surrounding targets.

HIGHLIGHTS (see Figures 1 to 6, Tables 1 and 2)

• Hole KUK24-001:

Perseus Zone

 

1.64% Ni, 0.11% Cu, 1.12 g/t PGE over 8.5 m (from 16.5 m to 25.0 m), including

 

3.55% Ni, 0.19% Cu, 2.19 g/t PGE over 2.5 m (from 22.5 m to 25.0 m)

 

 

 

New sulphide horizon

 

0.90% Ni, 0.32 g/t PGE over 9.05 m (from 126.65 m to 135.70 m)

 

 

• Hole KUK24-002:

Perseus Zone

 

8.42% Ni, 0.55% Cu, 7.25 g/t PGE over 1.9 m (from 27.0 m to 28.9 m)

 

 

• Hole KUK24-003:

Perseus Zone

 

0.81% Ni, 0.52 g/t PGE over 24.2 m (from 30.0 m to 54.2 m), including

 

1.63% Ni, 0.14% Cu, 1.61 g/t PGE over 1.25 m (from 42.5 m to 43.75 m) and

 

3.46% Ni, 0.21% Cu, 2.44 g/t PGE over 0.75 m (from 52.4 m to 53.15 m)

 

 

• Hole KUK24-007:

Perseus Zone

 

6.06% Ni, 0.38% Cu, 3.34 g/t PGE over 2.6 m (from 32.4 m to 35.0 m), including

 

19.6% Ni, 0.81% Cu, 9.43 g/t PGE over 0.75 m (from 33.4 m to 34.15 m)

 

 

 

New sulphide horizon

 

3.18% Ni, 0.15% Cu, 1.17 g/t PGE over 1.7 m (from 109.3 m to 111.0 m)

Perseus Target Area (see Figure 4)