VANCOUVER, BC, April 3,
2024 /CNW/ - Nevada King Gold Corp.
(TSXV: NKG) (OTCQX: NKGFF) ("Nevada
King" or the "Company") is pleased to announce
results from four vertical, reverse circulation ("RC") holes
and one vertical, PQ-diameter diamond core hole completed in the
northern portion of the West Atlanta Graben Zone ("WAGZ") at
its at its 5,166 hectares (51.6km2), 100% owned Atlanta
Gold Mine Project, located in the prolific Battle Mountain Trend
264km northeast of Las Vegas,
Nevada.
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 85% to 95% of reported
drill intercept length. *Denotes hole bottoming in
mineralization. +Denotes core
hole.
|
- 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 Nevada King, stated, "The Company's multiple
structure model continues to lead to thick, high-grade mineralized
zones. In addition to following high-angle structures that served
as loci for higher grade Au-Ag mineralization, Nevada King's success at increasing both grade
and thickness can also be attributed to achieving full penetration
of the low-angle unconformity that hosts most of the mineralization
at Atlanta. The occurrence of two
separate, sub-horizontal high-grade horizons as illustrated in
Table 4 is replicated throughout the Atlanta system but is most often observed in
the WAFZ where the deeper high-grade occurs in the carbonate
section at or directly above the unconformable basement contact,
while the shallower high-grade is hosted in the volcanic sequence
above the unconformity. Higher grade and thicker intercepts occur
close to feeder structures controlling the mineralization, as seen
in AT23WS-23C.1, while grades decrease and thin laterally away from
the feeders as seen in AT23WS-23."
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 85% to 95%
of reported drill intercept length. *Denotes holes that bottomed in
mineralization. + Denotes core holes.
|
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 Nevada King
in 2021 and 2022. DHRI series holes drilled by Meadow Bay in 2011.
*Denotes hole that bottomed in mineralization.
+Denotes core hole. ^Denotes aggregate assay
interval.
|
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 Atlanta deposit.
|
QAQC Protocols
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 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 multi-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. Silver
samples that run greater than 100ppm are also 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.
The PQ-diameter core was sampled in the Company's warehouse in
Winnemucca, Nevada, with whole
core samples being placed in heavy canvas bags and sent to American
Assay Lab in Reno, Nevada, in
heavy shipping bags by a Company contractor with full custody being
maintained at all times. CRF standards and coarse blanks were
inserted into the sample stream on a one-in-twenty sample basis,
meaning both inserts are included in each 20-sample group. At
American Assay Lab, samples were weighted then completely crushed
to -1 inch. The coarse-crushed sample was quarter-split and one
quarter was reduced to 75% passing 2mm. A 300g split was
subsequently pulverized to 85% passing 75 microns. Prepared samples
are initially run using a four acid + boric acid digestion process
and conventional multi-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 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.
Cautionary Statements Regarding
Forward Looking Information
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 Nevada King, are forward-looking statements.
Forward-looking statements are frequently, but not always,
identified by words such as "expects", "anticipates", "believes",
"intends", "estimates", "potential", "possible", and similar
expressions, or statements that events, conditions, or results
"will", "may", "could", or "should" occur or be achieved.
Forward-looking statements in this news release relate to, among
other things, the Company's exploration plans and the Company's
ability to potentially expand mineral resources and the impact
thereon. There can be no assurance that such statements will prove
to be accurate, and actual results and future events could differ
materially from those anticipated in such statements.
Forward-looking statements reflect the beliefs, opinions and
projections on the date the statements are made and are based upon
a number of assumptions and estimates that, while considered
reasonable by Nevada King, are
inherently subject to significant business, economic, competitive,
political and social uncertainties and contingencies. Many factors,
both known and unknown, could cause actual results, performance or
achievements to be materially different from the results,
performance or achievements that are or may be expressed or implied
by such forward-looking statements and the parties have made
assumptions and estimates based on or related to many of these
factors. Such factors include, without limitation, the ability to
complete proposed exploration work, the results of exploration,
continued availability of capital, and changes in general economic,
market and business conditions. Readers should not place undue
reliance on the forward-looking statements and information
contained in this news release concerning these items. Nevada King does not assume any obligation to
update the forward-looking statements of beliefs, opinions,
projections, or other factors, should they change, except as
required by applicable securities laws.
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SOURCE Nevada King Gold Corp.