
Nevada King Gold Corp. (TSX-V: NKG) (OTCQX: NKGFF) is pleased to announce assay results from 13 vertical, reverse circulation holes recently completed within the North Extension Target at its Atlanta Gold Mine Project, located in the prolific Battle Mountain Trend 264km northeast of Las Vegas, Nevada. Today’s holes are plotted in plan and on Sections 22-24N through 22-30N in Figures 1 to 8 below.
NET Highlights:
Hole No. | From (m) | To (m) | Interval (m) | Au (g/t) | Ag (g/t) |
AT23NS-109 | 225.6 | 239.3 | 13.7 | 3.69 | 1.3 |
AT23NS-110* | 175.3 | 201.2 | 25.9 | 1.21 | 3.3 |
AT23NS-112 | 155.5 | 176.8 | 21.3 | 4.01 | 6.7 |
AT23NS-127 | 117.4 | 146.3 | 28.9 | 0.96 | 1.5 |
AT23NS-15A | 160.1 | 179.9 | 19.8 | 1.31 | 12.1 |
Table 1. Highlight holes reported today from the North Extension Target. *Denotes hole that bottomed in mineralization. True widths are estimated to be 95% of reported intervals. |
Cal Herron, Exploration Manager of Nevada King, stated, “Sniffs of mineralization within the NET were found by past operators Kinross and Meadow Bay, but their drill patterns did not hit the higher-grade AMFZ, and consequently, the area was overlooked. By applying the Company’s new geological model, Nevada King’s drilling has consistently hit higher-grade mineralization by focusing on identifying and targeting the high-angle feeder faults responsible for channeling high-grade gold along the AMFZ. Similar to drilling conducted by the Company further south in and around the Atlanta Pit, applying the new geological model has proven key to unlocking the potential of the NET. The Company will continue to expand the gold zone eastward, westward, and southward in the coming months, paying particular attention to suspected high-angle structures adjacent to the AMFZ that might result in thicker and higher grade mineralization within the low grade horizon. It is important to note all mineralization within the NET is oxidized.”
Hole No. | From (m) | To (m) | Interval (m) | Au (g/t) | Ag (g/t) |
AT23NS-108 | 182.9 | 210.4 | 27.4 | 0.31 | 4.0 |
AT23NS-109 | 225.6 | 239.3 | 13.7 | 3.69 | 1.3 |
AT23NS-110* | 175.3 | 201.2 | 25.9 | 1.21 | 3.3 |
AT23NS-111 | 175.3 | 190.5 | 15.2 | 0.49 | 1.2 |
AT23NS-112 | 155.5 | 176.8 | 21.3 | 4.08 | 6.7 |
AT23NS-113 | 256.1 | 297.3 | 41.2 | 0.40 | 5.4 |
AT23NS-114 | 190.5 | 227.1 | 36.6 | 0.77 | 5.8 |
AT23NS-115 | 218.0 | 231.7 | 13.7 | 0.82 | 7.1 |
AT23NS-127 | 122.0 | 146.3 | 29 | 0.96 | 1.5 |
AT23NS-10A | 105.2 | 144.8 | 39.6 | 0.68 | 2.0 |
AT23NS-15A | 160.1 | 179.9 | 19.8 | 1.31 | 12.1 |
AT23NS-19A | 170.7 | 176.8 | 6.1 | 0.28 | 7.1 |
AT21-002C^ | 86.3 | 104.6 | 18.3 | 0.56 | 1.4 |
Table 2: Full list of RC drill results reported today from the NET. *Denotes hole that bottomed in mineralization. ^Denotes core hole. True widths are estimated to be 95% of reported intervals. |
Hole No. | From (m) | To (m) | Interval (m) | Au (g/t) | Ag (g/t) |
AT22NS-9 | 86.9 | 128.0 | 41.2 | 0.65 | <0.5 |
AT22NS-11 | 102.1 | 125.0 | 22.9 | 1.36 | 0.5 |
AT22NS-12 | 175.3 | 195.1 | 19.8 | 1.77 | <0.5 |
AT22NS-13 | 135.7 | 160.1 | 24.4 | 1.67 | <0.5 |
AT22NS-RC14 | 99.1 | 143.3 | 44.2 | 0.71 | <0.5 |
AT22NS-15* | 155.5 | 176.8 | 21.3 | 1.83 | 5.5 |
AT22NS-16 | 91.5 | 106.7 | 15.2 | 0.54 | <0.5 |
AT22NS-17 | 85.4 | 114.3 | 28.9 | 0.59 | 2.7 |
AT22NS-19* | 166.2 | 179.9 | 16.8 | 0.31 | 2.5 |
AT21-001 | 94.5 | 131.1 | 25.9 | 1.00 | <0.5 |
AT21-002 | 82.3 | 105.2 | 22.9 | 0.71 | <0.5 |
AT21-003 | 155.5 | 173.8 | 18.3 | 4.64 | 11.18 |
AT21-004 | 85.4 | 118.9 | 33.5 | 0.735 | 1.35 |
AT21-005 | 99.1 | 103.7 | 4.6 | 0.418 | 3.37 |
AT21-006 | 163.1 | 175.3 | 12.2 | 0.959 | 9.8 |
AT21-007 | 91.5 | 111.3 | 19.8 | 1.010 | 2.18 |
KN98-10 | 198.2 | 211.9 | 13.7 | 1.19 | 1.02 |
KN98-11 | 230.2 | 247.0 | 16.8 | 2.73 | 0.83 |
DHRI-11-04RC | 103.7 | 123.5 | 19.8 | 0.474 | <.1 |
DHRI-11-05RC | 59.5 | 80.8 | 21.3 | 0.23 | 3.73 |
DHRI-11-07RC* | 105.2 | 108.2 | 3.0 | 1.15 | <0.5 |
DHRI-11-08RC | 120.4 | 143.3 | 22.9 | 0.300 | 3.8 |
DHRI-11-08C^ | 80.8 | 103.7 | 22.9 | 0.62 | <0.5 |
Table 3: Full list of previously released and historic drill results reported today from the North Extension Target. * Denotes holes that bottomed in mineralization. ^ Denotes core hole. |
Line # | Operator | No. of Holes | Average Au eq. (g/t) |
Average Thickness (m) | |
30N | NKG | 4 | 0.677 | 29.9 | |
Historical | 1 | 0.278 | 21.3 | ||
29N | NKG | 5 | 1.547 | 26.8 | |
Historical | 2 | 0.384 | 12.2 | ||
28N | NKG | 5 | 1.894 | 20.1 | |
Historical | 0 | – | – | ||
27N | NKG | 3 | 0.577 | 28.4 | |
Historical | 1 | 0.62 | 22.9 | ||
26N | NKG | 4 | 1.408 | 18.3 | |
Historical | 0 | – | – | ||
25N | NKG | 1 | 0.492 | 28.9 | |
Historical | 2 | 0.406 | 21.4 | ||
Table 4. Comparison of Nevada King and historical drill results along section lines 22-25N through 22-30N, using weighted averages. Gold equivalents calculated using Au/Ag prices of $1,925/oz and $23.52/oz, respectively, (Sep 23, 2023 $US spot prices). Only holes proximal to the AMFZ and east of the AMFZ were used in this compilation. Mineralization in holes west of the AMFZ is likely too deep and too thin to justify stripping down to it. Taken collectively, NKG’s holes average 1.025 g/t Au eq over 25.4m while the historical holes average 0.430 g/t Au eq over 19.5m. |
QA/QC Protocols
All Reverse Circulation 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 Reno, Nevada, with full custody being maintained at all times. At American Assay Lab, samples were weighed then crushed to 75% passing 2mm and pulverized to 85% passing 75 microns in order to produce a 300g pulverized split. Prepared samples are initially run using a four acid + boric acid digestion process and conventional mutli-element ICP-OES analysis. Gold assays are initially run using 30-gram samples by lead fire assay with an OES finish to a 0.003 ppm detection limit, with samples greater than 10 ppm finished gravimetrically. Every sample is also run through a cyanide leach for gold with an ICP-OES finish. The QA/QC procedure involves regular submission of Certified Analytical Standards and property-specific duplicates.
Qualified Person
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.
About Nevada King Gold Corp.
Nevada King is the third largest mineral claim holder in the State of Nevada, behind Nevada Gold Mines (Barrick/Newmont) and Kinross Gold. Starting in 2016 the Company has staked large project areas hosting significant historical exploration work along the Battle Mountain trend located close to current or former producing gold mines. These project areas were initially targeted based on their potential for hosting multi-million-ounce gold deposits and were subsequently staked following a detailed geological evaluation. District-scale projects in Nevada King’s portfolio include (1) the 100% owned Atlanta Mine, located 100km southeast of Ely, (2) the Lewis and Horse Mountain-Mill Creek projects, both located between Nevada Gold Mines’ large Phoenix and Pipeline mines, and (3) the Iron Point project, located 35km east of Winnemucca, Nevada.
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, Lincoln County, NV” with an effective date of October 6, 2020, and a report date of December 22, 2020, as prepared by Gustavson Associates and filed under the Company’s profile on SEDAR+ (www.sedarplus.ca).
Resource Category | Tonnes
(000s) |
Au Grade
(ppm) |
Contained Au Oz |
Ag Grade
(ppm) |
Contained Ag Oz |
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 5. NI 43-101 Mineral Resources at the Atlanta Mine |
Figure 1. Location map for holes reported in this news release along drill sections22-24N, 25N, 26N, 27N, 28N, 29N and 30N relative to the perimeter of the historical Atlanta Pit and footprint of the Gustavson 2020 NI 43-101 resource. Shallow drillholes on the mine dumps have been removed from the plot for clarity. (CNW Group/Nevada King Gold Corp.)
Figure 2. Cross section 22-30N looking north along the AMFZ at the vertically displaced mineralized horizon. Au/Ag mineralization is hosted within a silica breccia layer developed on top of Paleozoic dolomite and underneath the Tertiary volcanic cover. Higher grade and mineralized thickness tend to occur proximal to the AMFZ. (CNW Group/Nevada King Gold Corp.)
Figure 3. Cross section 22-29N looking north along the AMFZ at the vertically displaced mineralized horizon. Au/Ag mineralization is hosted within a silica breccia layer developed on top of Paleozoic dolomite and underneath the Tertiary volcanic cover. Higher grade and mineralized thickness tend to occur proximal to the AMFZ. (CNW Group/Nevada King Gold Corp.)
Figure 4. Cross section 22-28N looking north along the AMFZ at the vertically displaced mineralized horizon. Au/Ag mineralization is hosted within a silica breccia layer developed on top of Paleozoic dolomite and underneath the Tertiary volcanic cover. Higher grade and mineralized thickness tend to occur proximal to the AMFZ. (CNW Group/Nevada King Gold Corp.)
Figure 5. Cross section 22-27N looking north along the AMFZ at the vertically displaced mineralized horizon. Au/Ag mineralization is hosted within a silica breccia layer developed on top of Paleozoic dolomite and underneath the Tertiary volcanic cover. Higher grade and mineralized thickness tend to occur proximal to the AMFZ. (CNW Group/Nevada King Gold Corp.)
Figure 6. Cross section 22-26N looking north along the AMFZ at the vertically displaced mineralized horizon. Au/Ag mineralization is hosted within a silica breccia layer developed on top of Paleozoic dolomite and underneath the Tertiary volcanic cover. Higher grade and mineralized thickness tend to occur proximal to the AMFZ. (CNW Group/Nevada King Gold Corp.)
Figure 7. Cross section 22-25N looking north along the AMFZ at the vertically displaced mineralized horizon. Au/Ag mineralization is hosted within a silica breccia layer developed on top of Paleozoic dolomite and underneath the Tertiary volcanic cover. Higher grade and mineralized thickness tend to occur proximal to the AMFZ. (CNW Group/Nevada King Gold Corp.)
Figure 8. Cross section 22-24N looking north along the AMFZ at the vertically displaced mineralized horizon. Au/Ag mineralization is hosted within a silica breccia layer developed on top of Paleozoic dolomite and underneath the Tertiary volcanic cover. Higher grade and mineralized thickness tend to occur proximal to the AMFZ. (CNW Group/Nevada King Gold Corp.)
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