
NGEx Minerals Ltd. (TSX: NGEX) (OTCQX: NGXXF) is pleased to announce drill results from holes DPDH050 through DPDH054 from the ongoing Phase 4 drill program at its 100% owned Lunahuasi high-grade copper-gold-silver project in San Juan, Argentina. Eight rigs are currently drilling at the project.
Highlights:
Wojtek Wodzicki, President and CEO, commented, “With the Phase 4 program fully underway, assay results are now steadily coming in, and we look forward to regular updates over the coming months. The holes released today continue to support our geological interpretation and expand the size of the Mars, Jupiter and Saturn zones. They also reinforce Lunahuasi’s gold potential, with new high-grade intersections in holes DPDH050, DPDH051 and DPDH054. The gold intersections in holes 50 and 51 are in the Saturn Zone while hole 54 is 335m away in the Mars Zone, clearly demonstrating that high-grade gold occurs throughout the deposit. We are now in the middle of summer in Argentina and are taking advantage of the season to start drilling some big step outs that will test larger-scale conceptual targets and explore for new deposits in the vicinity. With over 12,000m drilled so far this season we are well on our way to accomplishing our largest program ever at Lunahuasi.”
Lunahuasi Geology Drill Plan 2026 Jan

Phase 4 Progress
The Phase 4 program continues to be ahead of schedule. To date, over 12,000m have been drilled with 12 holes completed and eight underway. Initial holes have focused on defining and expanding the three named zones, Saturn, Mars, and Jupiter, and drilling will start to pivot towards larger step-outs and test new exploration targets as the campaign progresses.
Of the completed Phase 4 holes, two have been drilled into the Jupiter Zone, two into Mars and eight into Saturn. In addition to the exploration holes, a geotechnical hole is currently being drilled down the centerline of the proposed exploration adit as planning for that project progresses.
Table 1: Significant Intersections
| Hole ID | From (m) | To (m) | Length (m) | Estimated True Width (m) |
Cu % | Au g/t | Ag g/t | CuEq % |
| DPDH050 | 592.20 | 608.60 | 16.40 | 12.0 | 1.74 | 0.77 | 8.3 | 2.38 |
| incl | 592.20 | 595.75 | 3.55 | 2.5 | 3.42 | 2.25 | 14.9 | 5.19 |
| and incl | 606.50 | 608.60 | 2.10 | 1.5 | 7.05 | 1.48 | 29.8 | 8.39 |
| plus | 649.20 | 650.70 | 1.50 | 1.1 | 9.35 | 1.51 | 33.0 | 10.73 |
| plus | 686.40 | 687.60 | 1.20 | 0.8 | 8.77 | 24.50 | 33.0 | 26.92 |
| plus | 725.00 | 758.00 | 33.00 | 23.0 | 1.51 | 0.59 | 20.5 | 2.13 |
| incl | 729.40 | 730.40 | 1.00 | 0.7 | 17.52 | 4.06 | 436.0 | 24.31 |
| DPDH051 | 188.20 | 209.00 | 20.80 | 6.2 | 0.66 | 0.99 | 42.4 | 1.76 |
| plus | 285.65 | 299.30 | 13.65 | 4.1 | 0.81 | 2.44 | 18.9 | 2.76 |
| incl | 298.00 | 299.30 | 1.30 | 0.4 | 3.55 | 11.55 | 105.0 | 12.90 |
| plus | 359.70 | 361.20 | 1.50 | 0.5 | 7.42 | 0.66 | 50.3 | 8.34 |
| plus | 436.70 | 764.10 | 327.40 | 98.0 | 2.43 | 1.53 | 21.8 | 3.74 |
| incl | 449.80 | 462.50 | 12.70 | 3.8 | 6.37 | 1.38 | 55.1 | 7.86 |
| and incl | 509.40 | 510.55 | 1.15 | 0.3 | 37.85 | 15.85 | 251.0 | 51.62 |
| and incl | 561.70 | 566.00 | 4.30 | 1.3 | 12.67 | 62.11 | 297.1 | * |
| incl | 563.30 | 564.25 | 0.95 | 0.3 | 14.85 | 254.00 | 682.0 | * |
| and incl | 628.00 | 649.00 | 21.00 | 6.3 | 4.51 | 0.93 | 15.3 | 5.33 |
| and incl | 683.00 | 688.80 | 5.80 | 1.7 | 11.97 | 2.73 | 50.8 | 14.40 |
| and incl | 716.00 | 723.30 | 7.30 | 2.2 | 10.98 | 2.49 | 193.3 | 14.50 |
| and incl | 742.00 | 745.00 | 3.00 | 0.9 | 10.15 | 1.12 | 35.7 | 11.28 |
| DPDH052 | 216.25 | 248.00 | 31.75 | 13.0 | 0.41 | 0.75 | 14.7 | 1.08 |
| plus | 338.00 | 427.40 | 89.40 | 36.0 | 1.04 | 0.95 | 38.9 | 2.08 |
| incl | 349.00 | 356.00 | 7.00 | 2.8 | 1.07 | 2.52 | 51.7 | 3.36 |
| and incl | 395.40 | 427.40 | 32.00 | 13.0 | 2.09 | 1.01 | 71.7 | 3.46 |
| incl | 395.40 | 408.40 | 13.00 | 5.2 | 3.90 | 1.44 | 118.2 | 5.99 |
| DPDH053 | 103.90 | 108.70 | 4.80 | 3.4 | 1.08 | 3.27 | 211.5 | 5.33 |
| plus | 209.80 | 213.20 | 3.40 | 2.4 | 2.84 | 1.30 | 30.0 | 4.06 |
| plus | 242.00 | 266.00 | 24.00 | 17.0 | 1.04 | 1.88 | 17.9 | 2.57 |
| plus | 285.00 | 286.70 | 1.70 | 1.2 | 0.37 | 5.68 | 401.0 | 8.04 |
| DPDH054 | 175.00 | 176.35 | 1.35 | 1.0 | 2.32 | 4.60 | 35.0 | 5.98 |
| plus | 271.00 | 365.00 | 94.00 | 71.0 | 3.88 | 6.66 | 29.6 | 8.99 |
| incl | 284.10 | 305.80 | 21.70 | 16.0 | 12.70 | 25.21 | 95.5 | 31.92 |
| incl | 284.10 | 293.10 | 9.00 | 6.8 | 14.98 | 42.73 | 89.2 | 46.92 |
| incl | 298.80 | 305.80 | 7.00 | 5.3 | 19.05 | 21.43 | 173.5 | 36.21 |
| and incl | 335.00 | 336.30 | 1.30 | 1.0 | 7.39 | 8.05 | 91.0 | 14.06 |
| and incl | 355.00 | 363.50 | 8.50 | 6.4 | 4.21 | 2.78 | 32.3 | 6.52 |
Copper equivalent (CuEq) for drill intersections is calculated based on US$3.00/lb Cu, US$1,500/oz Au and US$18/oz Ag, with 80% metallurgical recoveries assumed for all metals. The formula is: CuEq % = Cu % + (0.7292 * Au g/t) + (0.0088 * Ag g/t). A * indicates that no CuEq was calculated as samples within the interval and/or the entire interval returned >100% CuEq.
Estimated true widths are rounded to the nearest metre for widths over 10m and to the nearest 0.1m for widths less than 10m, as this better reflects the precision of the estimates. True widths should be regarded as approximate as these are derived from an estimation that uses a preliminary interpretation of the geological model and are subject to change as more information becomes available.
A * indicates that no CuEq was calculated as one or more samples in the interval returned > 100% CuEq.
DPDH050 was targeted at the Saturn Zone. It intersected the zone between 592.20m and 687.60m where it was comprised of three main high-grade zones as shown in Table 1. A deeper zone starting at 725.00m may represent the southern extension of the Jupiter Zone.
DPDH051 was drilled from north to south along the Saturn zone, below hole DPDH044 from Phase 3, to investigate the geometry of the zone and test for directional bias in the grade. Results were consistent with those modeled from drilling in other directions and the hole intersected a long interval of good grade along the zone punctuated by some very high-grade sub-intervals as shown in Table 1. Of particular note is the very high-grade gold interval from 561.70m to 566.00m which correlates well with similar intervals in holes DPDH028, DPDH046 and DPDH048.
DPDH052 was drilled towards the southwest across the Saturn Zone, which it intersected between 338.00m and 427.40m.
DPDH053 targeted the Jupiter Zone, 60m north of the discovery hole DPDH002, successfully intersecting it from 242.00m to 266.00m.
DPDH054 targeted the Mars Zone 30m to the northeast of DPDH035 (21.50m @ 26.68% CuEq; April 24, 2025 News Release) and 90m down-dip from DPDH024 (12.3m @ 23.35% CuEq; December 18, 2024 News Release). The hole intersected a wide, high-grade interval from 284.10m to 305.80m which correlates well with the two intersections noted above and, similar to them, forms a very high-grade core to a much wider envelope of good grade.
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Table 2: Drillhole Information |
|||||||
| Hole ID | UTM East | UTM North | Elev (masl) | Azimuth | Dip | Length Drilled (m) |
Drill Status |
| DPDH048 | 439,217 | 6,855,999 | 4,703 | 277.4 | -55.4 | 761.0 | Complete |
| DPDH049 | 439,224 | 6,855,908 | 4,742 | 273.5 | -60.6 | 1,487.0 | Complete |
| DPDH050 | 439,204 | 6,855,918 | 4,742 | 290.5 | -62.0 | 796.1 | Complete |
| DPDH051 | 438,851 | 6,856,236 | 4,767 | 157.3 | -71.5 | 790.5 | Complete |
| DPDH052 | 439,092 | 6,856,132 | 4,663 | 225.6 | -47.6 | 560.4 | Complete |
| DPDH053 | 439,077 | 6,856,286 | 4,655 | 287.0 | -48.5 | 301.5 | Complete |
| DPDH054 | 439,299 | 6,856,194 | 4,631 | 289.4 | -48.4 | 383.0 | Complete |
| DPDH055 | 439,226 | 6,855,998 | 4,703 | 273.5 | -68.3 | 925.0 | Complete |
| DPDH056 | 439,092 | 6,856,134 | 4,663 | 255.3 | -70.0 | 877.4 | Complete |
| DPDH057 | 439,203 | 6,855,918 | 4,742 | 280.1 | -45.2 | 799.0 | Complete |
| DPDH058 | 439,081 | 6,856,287 | 4,654 | 327.9 | -67.3 | 577.0 | Complete |
| DPDH059 | 438,851 | 6,856,236 | 4,768 | 164.8 | -68.7 | 776.0 | In Progress |
| DPDH060 | 439,297 | 6,856,195 | 4,632 | 304.8 | -50.3 | 488.5 | Complete |
| DPDH061 | 439,297 | 6,856,193 | 4,632 | 289.1 | -54.9 | 662.0 | In Progress |
| DPDH062 | 439,226 | 6,855,995 | 4,702 | 256.4 | -63.8 | 560.4 | In Progress |
| DPDH063 | 439,222 | 6,855,907 | 4,743 | 259.1 | -54.3 | 632.0 | In Progress |
| DPDH064 | 439,204 | 6,855,913 | 4,742 | 260.3 | -46.5 | 476.0 | In Progress |
| DPDH065 | – | In Progress | |||||
| DPDH066 | – | In Progress | |||||
| DPGT004 | 439,561 | 6,856,232 | 4,572 | 266.2 | -11.8 | 543.0 | In Progress |
Additional assay results will be released once assays are received, analyzed, and confirmed by the Company.
Qualified Persons and Technical Notes
The scientific and technical disclosure included in this news release have been reviewed and approved by Bob Carmichael, B.A.Sc., P.Eng. who is the Qualified Person as defined by NI 43-101. Mr. Carmichael is Vice President, Exploration for the Company.
Samples were cut at NGEx’s operations base in San Juan, Argentina by Company personnel. Diamond drill core was sawed and then sampled in maximum 2-meter intervals, stopping at geological boundaries. Core diameter is a mix of PQ, HQ and NQ depending on the depth of the drill hole. Samples were bagged, tagged, and packaged for shipment by truck to the ALS preparation laboratory in Mendoza, Argentina where they were crushed and a 500g split was pulverized to 85% passing 200 mesh. The prepared sample splits were sent to the ALS assay laboratory in Lima, Peru for copper, gold and silver assays, and multi-element ICP. ALS is an accredited laboratory which is independent of the Company. Gold assays were by fire assay fusion with AAS finish on a 30g sample (Au-AA23). Any samples returning > 10 g/t were then reanalyzed by fire assay with gravimetric finish on a 30g sample (Au-GRA21). Copper and silver were assayed by atomic absorption following a 4-acid digestion. Samples were also analyzed for a suite of 48 elements with ME-MS61 plus mercury and a sequential copper leach analysis was completed on each sample with copper greater than 500ppm (0.05%). Sequential copper analysis involves the sequential leaching of the sample by acid, followed by a cyanide solution. It can be used to differentiate copper speciation, with copper oxide minerals leachable with acid and secondary copper minerals (enargite, chalcocite, covellite) leachable by cyanide. The residual copper remaining following the sequential leaches it typically contained in chalcopyrite and bornite. Copper and gold standards as well as blanks and duplicates (field, preparation, and analysis) were randomly inserted into the sampling sequence for Quality Control. On average, 10% of the submitted samples are Quality Control samples. No data quality problems were indicated by the QA/QC program.
About NGEx Minerals
NGEx Minerals is a copper and gold exploration company based in Canada, focused on exploration of the Lunahuasi copper-gold-silver project in San Juan Province, Argentina, and the nearby Los Helados copper-gold project located approximately nine kilometres to the northeast in Chile’s Region III. Both projects are located within the Vicuña District, which includes the Caserones mine, and the Josemaria and Filo del Sol deposits.
NGEx owns 100% of Lunahuasi and is the majority partner and operator for the Los Helados project, subject to a Joint Exploration Agreement with Nippon Caserones Resources LLC, which is the indirect 30% owner of the operating Caserones open pit copper mine located approximately 17 kilometres north of Los Helados. Lundin Mining Corporation holds the remaining 70% stake in Caserones.
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