NEVADA KING INTERCEPTS 4.51 G/T AU OVER 86.3M INCLUDING 7.77 G/T AU OVER 43M, FURTHER EXPANDS HIGH-GRADE ZONE 200M NORTH OF THE ATLANTA PIT
- High-grade gold intercepts reported, such as 4.51 g/t Au over 86.3m in core hole AT23WS-23C.1.
- Mineralization along near-horizontal horizons with thick mineralized thicknesses estimated.
- Multiple high-grade zones identified, indicating significant mineralization potential.
- Success attributed to full penetration of low-angle unconformity hosting mineralization.
- Continuous drilling and exploration efforts aim to define and expand high-grade zones.
- Qualified Person Calvin R. Herron approves the scientific and technical information in the release.
- None.
Highlights:
Hole No. | From (m) | To (m) | Interval (m) | Au (g/t) | Ag (g/t) |
AT23WS-23C.1*+ | 226.2 | 312.5 | 86.3 | 4.51 | 50.7 |
Includes | 256.3 | 299.2 | 43 | 7.77 | 25.1 |
Includes | 256.3 | 261.3 | 5 | 18.34 | 1.9 |
AT23WS-58 | 213.4 | 297.2 | 83.8 | 0.75 | 5.4 |
AT23WS-61* | 243.8 | 294.1 | 50.3 | 1.56 | 13.2 |
Table 1: Highlight holes released on section 22N-17N(2). Mineralization occurs along near-horizontal horizons with true mineralized thicknesses estimated to be |
- Core hole AT23WS-23C.1 intercepted 4.51 g/t Au over 86.3m including 7.77 g/t Au over 48.6m and was collared 6m north of RC hole AT23WS-23, which intercepted 2.45 g/t Au over 102.1m, (released June 6, 2023). AT23WS-23C.1 was planned to provide metallurgical material for the ongoing Phase II test work program, as well as to verify the RC drilling.
- While core hole AT23WS-23C.1 shows a
60% increase in overall grade, a comparison of gold distribution in AT23WS-23C.1 with AT23WS-23 (see Table 4 below) reveals close lateral correlation. This is particularly evident when comparing elevations of the upper high-grade zones (highlighted in yellow in Table 4) and the lower high-grade zones (highlighted in magenta). The sub-horizontal geometry of these zones suggests higher grade mineralization along low-angle bedding features or breccia horizons. - As shown below in Figure 1, the high-grade intercepts in AT23WS-23C.1 and adjacent AT23WS-23 also add definition to a developing, northwest-trending high-grade zone along the axis of the WAGZ that currently spans 200m long by 70m wide. Relative to the location of AT23WS-23C.1, other previously reported holes of note within this zone include:
- AT23WS-44 (11.64 g/t Au over 108.2m) located 56m southeast;
- AT23WS-53 (2.72 g/t Au over 64m) located 34m to south;
- AT23WS-62 (6.09 g/t Au over 41.5m) located 41m southwest;
- AT23WS-34 (1.74 g/t Au over 114.3m) located 82m to the southeast; and
- AT23WS-56 (1.55 g/t Au over 94.5m) located 108m southeast.
- At least two high-grade feeder zones appear to be responsible for this well mineralized zone. Holes AT23WS-23C.1, AT23WS-44, AT23WS-34, and AT23WS-56 most likely share the same NW-trending basement structure, whereas AT23WS-62 probably tapped into a different structure with a different orientation. It is also important to note the high proportion of holes shown in Figure 1 that bottomed in mineralization and did not fully penetrate both of the high-grade horizons described above. The Company is currently re-drilling these holes along the NW trend connecting AT23WS-23C.1 and AT23WS-44 in order to obtain representative Au/Ag grade averages through the entire mineralized sequence.
- Holes AT23WS-58 and AT23WS-59 intercepted 0.75 g/t Au over 83.8m and 0.86 g/t Au over 61.7m, respectively, filling in a previously untested 45m-wide gap between the WAGZ and the Atlanta Mine Fault Zone ("AMFZ"). As shown in Figure 3, both holes extend the thick mineralization found in the centre of the WAGZ eastward to the West Atlanta Fault, thus building additional tonnage potential.
- AT23WS-61 (50.3m of 1.56 g/t Au) was lost just short of entering the lower high-grade zone (Figure 3), but the hole did demonstrate continuance of the thick mineralization seen in the middle of the WAGZ westward to the West Atlanta Fault #2 ("WAF2"), which bounds the western margin of the WAGZ. This is particularly important when taking into account the low-grade intercepts in two historical holes located only 32m west of AT23WS-61 but on the western side of the WAF2. Neither DHRI-11-15C (67.1m @ 0.28 g/t Au) nor DHRI-11-NRC01 (27.4m @ 0.42 g/t Au) indicated potential for the thick, much higher-grade mineralization encountered in AT23WS-61, much less in the centre of the WAGZ.
Cal Herron, Exploration Manager of
Hole No. | From (m) | To (m) | Interval (m) | Au (g/t) | Ag (g/t) |
AT23WS-23C.1*+ | 226.2 | 312.5 | 86.3 | 4.51 | 50.7 |
Includes | 256.3 | 299.2 | 43 | 7.77 | 25.1 |
Includes | 256.3 | 261.3 | 5 | 18.34 | 1.9 |
AT23WS-58 | 213.4 | 297.2 | 83.8 | 0.75 | 5.6 |
AT23WS-59 | 216.5 | 283.5 | 67.1 | 0.86 | 10.9 |
AT23WS-61* | 243.9 | 294.2 | 50.3 | 1.56 | 13.2 |
AT23NS-149 | 175.3 | 193.6 | 18.3 | 0.45 | 10.3 |
Table 2. All holes released today on section 22-17N(2). Mineralization occurs along near-horizontal horizons with true mineralized thickness in vertical holes estimated to be |
Hole No. | From (m) | To (m) | Interval (m) | Au (g/t) | Ag (g/t) |
AT21-10* | 150.9 | 152.4 | 1.5 | 0.24 | 0.7 |
AT21-11^ | 15.2 | 21.3 | 6.1 | 0.45 | 10.9 |
AT22WS-1* | 239.3 | 304.9 | 65.5 | 1.52 | 11.6 |
AT22WS-12*^ | 204.3 | 259.1 | 54.9 | 0.21 | 1.2 |
AT23WS-15 | 213.4 | 248.5 | 35.1 | 0.50 | 8.4 |
AT22NS-26T+ | 119.2 | 138.3 | 19.1 | 0.39 | 11.6 |
AT22NS-27 | 51.8 | 71.6 | 19.8 | 0.41 | 12.5 |
AT23WS-23 | 230.2 | 332.3 | 102.1 | 2.45 | 10.1 |
Includes | 288.1 | 300.3 | 12.2 | 8.78 | 11.8 |
AT23WS-18 | 225.6 | 283.5 | 57.9 | 1.48 | 8.5 |
DHRI-11-NRC1* | 310.9 | 338.3 | 27.4 | 0.42 | 5.93 |
DHRI-11-15C+ | 266.7 | 333.8 | 67.1 | 0.28 | 8.4 |
Table 3. Previously released and historical holes used on section 22-17N (2). AT series holes drilled by |
AT23WS-23C.1 | AT23WS-23 | ||||||
From (m) | To (m) | Interval (m) | Au (g/t) | From (m) | To (m) | Interval (m) | Au (g/t) |
232.3 | 233.8 | 1.5 | 0.376 | 230.1 | 231.7 | 1.5 | 0.239 |
233.8 | 235.3 | 1.5 | 0.749 | 231.7 | 233.2 | 1.5 | 0.145 |
235.3 | 236.8 | 1.5 | 0.547 | 233.2 | 234.7 | 1.5 | 0.507 |
236.8 | 238.4 | 1.5 | 0.409 | 234.7 | 236.2 | 1.5 | 0.447 |
238.4 | 239.9 | 1.5 | 1.67 | 236.2 | 237.7 | 1.5 | 0.481 |
239.9 | 241.3 | 1.4 | 1.1 | 237.7 | 239.3 | 1.5 | 0.496 |
241.3 | 242.8 | 1.5 | 0.8 | 239.3 | 240.8 | 1.5 | 0.393 |
242.8 | 244.0 | 1.2 | 1.57 | 240.8 | 242.3 | 1.5 | 0.38 |
244.0 | 245.2 | 1.2 | 2.88 | 242.3 | 243.8 | 1.5 | 0.428 |
245.2 | 246.7 | 1.5 | 1.94 | 243.8 | 245.4 | 1.5 | 0.427 |
246.7 | 247.7 | 0.9 | 0.624 | 245.4 | 246.9 | 1.5 | 0.755 |
247.7 | 248.6 | 0.9 | 0.147 | 246.9 | 248.4 | 1.5 | 8.74 |
248.6 | 249.6 | 1.1 | 0.426 | 248.4 | 249.9 | 1.5 | 12.98 |
249.6 | 250.5 | 0.9 | 1.2 | 249.9 | 251.5 | 1.5 | 8.61 |
250.5 | 252.1 | 1.5 | 5.94 | 251.5 | 253.0 | 1.5 | 0.643 |
252.1 | 253.6 | 1.5 | 3.52 | 253.0 | 254.5 | 1.5 | 0.39 |
253.6 | 255.1 | 1.5 | 4.52 | 254.5 | 256.0 | 1.5 | 0.683 |
255.1 | 256.2 | 1.1 | 4.03 | 256.0 | 257.6 | 1.5 | 3.32 |
256.2 | 257.7 | 1.5 | 15.87 | 257.6 | 259.1 | 1.5 | 2.88 |
257.7 | 258.8 | 1.1 | 11.90 | 259.1 | 260.6 | 1.5 | 1.69 |
258.8 | 259.7 | 0.9 | 26.97 | 260.6 | 262.1 | 1.5 | 1.64 |
259.7 | 261.2 | 1.5 | 20.13 | 262.1 | 263.7 | 1.5 | 1.55 |
261.2 | 262.7 | 1.5 | 1.35 | 263.7 | 265.2 | 1.5 | 1.05 |
262.7 | 263.7 | 0.9 | 1.3 | 265.2 | 266.7 | 1.5 | 0.861 |
263.7 | 265.5 | 1.8 | 2.53 | 266.7 | 268.2 | 1.5 | 0.542 |
265.5 | 267.0 | 1.5 | 4.19 | 268.2 | 269.8 | 1.5 | 1.27 |
267.0 | 268.5 | 1.5 | 5.02 | 269.8 | 271.3 | 1.5 | 1.61 |
268.5 | 270.1 | 1.5 | 1.53 | 271.3 | 272.8 | 1.5 | 1.18 |
270.1 | 271.6 | 1.5 | 4.59 | 272.8 | 274.3 | 1.5 | 1.97 |
271.6 | 273.3 | 1.7 | 6.78 | 274.3 | 275.8 | 1.5 | 1.5 |
273.3 | 274.8 | 1.5 | 12.6 | 275.8 | 277.4 | 1.5 | 2.86 |
274.8 | 275.4 | 0.6 | 11.45 | 277.4 | 278.9 | 1.5 | 3.08 |
275.4 | 276.9 | 1.5 | 12.37 | 278.9 | 280.4 | 1.5 | 1.64 |
276.9 | 278.0 | 1.1 | 8.34 | 280.4 | 281.9 | 1.5 | 2.22 |
278.0 | 279.5 | 1.5 | 10.42 | 281.9 | 283.5 | 1.5 | 5.41 |
279.5 | 281.0 | 1.5 | 14.28 | 283.5 | 285.0 | 1.5 | 4.44 |
281.0 | 282.6 | 1.5 | 5.02 | 285.0 | 286.5 | 1.5 | 2.09 |
282.6 | 283.8 | 1.2 | 6.25 | 286.5 | 288.0 | 1.5 | 4.86 |
283.8 | 285.3 | 1.5 | 9.82 | 288.0 | 289.6 | 1.5 | 7.95 |
285.3 | 286.8 | 1.5 | 6.71 | 289.6 | 291.1 | 1.5 | 9.53 |
286.8 | 287.7 | 0.9 | 5.29 | 291.1 | 292.6 | 1.5 | 13.97 |
287.7 | 289.3 | 1.5 | 3.89 | 292.6 | 294.1 | 1.5 | 11.4 |
289.3 | 290.5 | 1.2 | 1.75 | 294.1 | 295.7 | 1.5 | 7.66 |
290.5 | 291.7 | 1.2 | 4.61 | 295.7 | 297.2 | 1.5 | 6.68 |
291.7 | 293.5 | 1.8 | 4.24 | 297.2 | 298.7 | 1.5 | 5.93 |
293.5 | 295.0 | 1.5 | 3.53 | 298.7 | 300.2 | 1.5 | 7.1 |
295.0 | 296.6 | 1.5 | 8.13 | 300.2 | 301.8 | 1.5 | 1.44 |
296.6 | 297.8 | 1.2 | 13.28 | 301.8 | 303.3 | 1.5 | 1.93 |
297.8 | 299.2 | 1.4 | 5.02 | 303.3 | 304.8 | 1.5 | 0.565 |
299.2 | 300.8 | 1.7 | 0.762 | 304.8 | 306.3 | 1.5 | 0.543 |
300.8 | 302.4 | 1.5 | 0.976 | 306.3 | 307.9 | 1.5 | 0.423 |
302.4 | 303.6 | 1.2 | 1.66 | 307.9 | 309.4 | 1.5 | 0.299 |
303.6 | 305.1 | 1.5 | 0.702 | 309.4 | 310.9 | 1.5 | 0.306 |
305.1 | 306.8 | 1.7 | 0.262 | 310.9 | 312.4 | 1.5 | 0.224 |
306.8 | 308.0 | 1.2 | 0.368 | 312.4 | 313.9 | 1.5 | 0.176 |
308.0 | 310.0 | 2.0 | 0.171 | 313.9 | 315.5 | 1.5 | 0.231 |
310.0 | 312.4 | 2.4 | 0.412 | 315.5 | 317.0 | 1.5 | 0.27 |
312.4 | 313.3 | 0.9 | 0.06 | 317.0 | 318.5 | 1.5 | 0.155 |
313.3 | 314.9 | 1.5 | 0.159 | 318.5 | 320.0 | 1.5 | 0.183 |
Table 4. Comparison of Au assays from core hole AT23WS-23C.1 and RC hole AT23WS-23 including drill depths and sample interval lengths. RC sampling is done on 1.5-metre intervals while core drilling varies in interval size with the ability to tighten or broaden sample size with relation to structure, contacts, and strong mineralization. Yellow highlighted intervals indicate the Upper High-Grade Zone, while magenta highlighted intervals denote the Lower High-Grade Zone. Both high grade zones often occur together throughout the |
All RC samples from the Atlanta Project are split at the drill site and placed in cloth and plastic bags utilizing a nominal 2kg sample weight. CRF standards, blanks, and duplicates are inserted into the sample stream on-site on a one-in-twenty sample basis, meaning all three inserts are included in each 20-sample group. Samples are shipped by a local contractor in large sample shipping crates directly to American Assay Lab in
The PQ-diameter core was sampled in the Company's warehouse in
The scientific and technical information in this news release has been reviewed and approved by Calvin R. Herron, P.Geo., who is a Qualified Person as defined by National Instrument 43-101.
The Atlanta Mine is a historical gold-silver producer with a NI 43-101 compliant pit-constrained resource of 460,000 oz Au in the measured and indicated category (11.0M tonnes at 1.3 g/t) plus an inferred resource of 142,000 oz Au (5.3M tonnes at 0.83 g/t). See the NI 43-101 Technical Report on Resources titled "Atlanta Property,
Resource Category | Tonnes (000s) | Au Grade (ppm) | Contained Au | Ag Grade (ppm) | Contained Ag |
Measured | 4,130 | 1.51 | 200,000 | 14.0 | 1,860,000 |
Indicated | 6,910 | 1.17 | 260,000 | 10.6 | 2,360,000 |
Measured + Indicated | 11,000 | 1.30 | 460,000 | 11.9 | 4,220,000 |
Inferred | 5,310 | 0.83 | 142,000 | 7.3 | 1,240,000 |
Table 3. NI 43-101 Mineral Resources at the Atlanta Mine |
Please see the Company's website at www.nevadaking.ca.
Neither the TSX Venture Exchange nor its Regulation Services Provider (as that term is defined in the policies of the TSX Venture Exchange) accepts responsibility for the adequacy or accuracy of this release.
This news release contains certain "forward-looking information" and "forward-looking statements" (collectively "forward-looking statements") within the meaning of applicable securities legislation. All statements, other than statements of historical fact, included herein, without limitation, statements relating the future operations and activities of
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SOURCE Nevada King Gold Corp.
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