Heron Resources Limited (ASX:HRR TSX:HER, “Heron” or the
“Company”) is pleased to report the results of a
reconnaissance rotary airblast (RAB) drilling program at the Crosby
prospect within its wholly-owned Kangiara Project (EL8400), located
200km south-west of Sydney, New South Wales, Australia.
Results for first pass RAB drilling at the Crosby
Prospect have returned:
- 42m @ 0.20 g/t Au and 0.26% Cu from 4m to end of hole
(CRRB027)
- 3m 0.77 g/t Au from 33m depth to end of hole
(CRRB008)
- Several supporting anomalous results indicative of a
broad mineralised system, strong sericite and pyrite alteration
logged
- Hosted within Silurian dacitic rocks -
intrusive-related copper/gold mineralising model.
Kangiara (EL8400) RAB Program
The Kangiara Project is located 90km NW of Woodlawn and 26km NNW
of the town of Yass, and is a historical copper mine where previous
explorers (to 2014) have delineated a small, low-grade, gold,
silver, copper, lead, zinc deposit (non JORC). The geology
comprises felsic volcanic and related sedimentary rocks of the
Silurian Douro Group (Figure1).
At the Crosby Prospect (named after the nearby survey point) 5km
to the NE of the Kangiara mine, previous explorers outlined a
strong gold anomaly (up to 2.3g/t Au in rock chips and 0.17g/t Au
in soils) within a 2.5km NW-trending zone of anomalous geochemistry
(Au, As, Zn, Pb, Cu; Bi, Mo, Sb). Heron conducted check
sampling which confirmed the soil geochemistry, with levels above
150ppb Au being returned and rock-chips up to 4g/t from an area
northwest of the soil anomaly. The geological setting is
similar to the McPhillamys gold deposit (approximately 2.2Moz Au as
reported by Regis Resources Ltd http://www.regisresources.com.au/ )
located 130km to the NNE.
A program of 33 rotary air-blast (RAB) holes for 743m was
completed in May 2017 providing a first pass test of the soil
geochemical anomalies (Figure 2). The majority of the
drilling was focused on the Crosby Main target plus 2 lines to the
north providing coverage of the northern geochemical anomalies, and
was conducted with the RAB hammer which provided dry and relatively
contamination free penetration into the weathered and altered
rocks.
The drill holes encountered a thin residual regolith cover
before penetrating the Silurian sequence of dacitic intrusive rocks
with lesser intercalated breccias and shales. Pervasive
sericite alteration and fine grained disseminated pyrite (phyllic
alteration) was observed in many of the holes, with lesser biotite
and some fine-grained base metal sulphides. Where alteration
was strong, the rig was able to penetrate deeper; the deepest
intercept was in strong alteration from surface to a depth of 64m
(CRRB024) which was close to the capacity of the rig (Figure
3).
Samples were collected on 4m, 2m or 1m intervals depending on
the degree of alteration, and assayed using an aqua-regia digest
and ICP finish for gold and other elements. Some check fire
assays are being conducted to check the gold results as it may be
reporting slightly low if the mineralisation is of a refractory
nature. The drill logs and assays confirmed a broad zone of
phyllic alteration within the Silurian sequence at both the Crosby
Main and Central areas.
Better results include:
10m @ 0.11g/t Au, from 30m to end of hole
(CRRB007)
3m @ 0.77 g/t Au, from 33m depth to end of hole
(CRRB008)
4m @ 0.96% Zn, 0.36% Pb and 0.07g/t Au, from 54m
(CRRB024)
42m @ 0.20 g/t Au and 0.26% Cu from 4m to end of hole
(CRRB027)
4m @ 0.25% Cu from 24m to end of hole
(CRRB029)
The results from the Crosby Main area (CRRB007, -008 and -024)
are associated with strong sericite and fine grained disseminated
pyrite alteration and elevated zinc and lead similar to the
McPhillamys style of mineralisation.
The results from the very limited drilling in the Crosby Central
area (CRRB027 and 029) is consistent with an intrusive-related or
porphyry style of mineralisation, and the thick intercept in
CRRB0027 suggests the potential for the presence of a significant
mineralising system. Of note in the drill assays for the
central area is depletion in both Cu and Au in the top 4 metres
indicating the broad and relatively weak soil geochemical anomaly
in this area may be more significant than first thought. Strongly
anomalous silver (Ag), molybdenum (Mo), arsenic (As) levels
associated with these copper/gold results (see Appendix 1) is
encouraging and supports an intrusive-related model for the
mineralisation.
Forward Program
This first-pass reconnaissance drilling program has successfully
identified the potential for a significant, intrusive-related
copper/gold mineralised system. The fine disseminated nature
of the sulphides in the dacitic rocks can most likely be mapped
with IP geophysical methods to help target future drilling
programs.
About Heron Resources Limited:
Heron’s primary focus is the development of its 100% owned, high
grade Woodlawn Zinc-Copper Project located 250km southwest of
Sydney, New South Wales, Australia. In addition, the Company
holds a significant high quality, gold and base metal tenement
holding in central and eastern New South Wales.
Figure 1: Location of the Kangiara Project and Crosby Prospect
in relation to Woodlawn and other major deposits. Refer to link
below:
http://www.heronresources.com/tsximages/20170620/20170620_Fig1.jpg
Figure 2: Crosby Prospect showing distribution of drilling
and anomalous holes with key results highlighted. Refer to link
below:
http://www.heronresources.com/tsximages/20170620/20170620_Fig2.jpg
Figure 3: Kangiara Project, Crosby Prospect RAB drilling
rig at hole CRRB024 drilled to 64m (deepest hole of program)
showing broad zone of sericite/pyrite alteration. Refer to link
below:
http://www.heronresources.com/tsximages/20170620/20170620_Fig3.jpg
Compliance Statement (JORC 2012 and
NI43-101)
The technical information in this report relating to the
exploration results is based on information compiled by Mr. David
von Perger, who is a Member of the Australian Institute of Mining
and Metallurgy (Chartered Professional – Geology). Mr. von Perger
is a full time employee of Heron Resources Limited and has
sufficient experience, which is relevant to the style of
mineralisation and type of deposit under consideration and to the
activity which he is undertaking to qualify as a Competent Person
as defined in the 2012 edition of the “Australasian Code for
Reporting of Exploration Results and “qualified person” as this
term is defined in Canadian National Instrument 43-101 (“NI
43-101”). Mr. von Perger has approved the scientific and technical
disclosure in the news release.
CAUTIONARY NOTE REGARDING FORWARD-LOOKING
INFORMATION
This report contains forward-looking statements and
forward-looking information within the meaning of applicable
Canadian securities laws, which are based on expectations,
estimates and projections as of the date of this report. This
forward-looking information includes, or may be based upon, without
limitation, estimates, forecasts and statements as to management’s
expectations with respect to, among other things, the timing and
amount of funding required to execute the Company’s exploration,
development and business plans, capital and exploration
expenditures, the effect on the Company of any changes to existing
legislation or policy, government regulation of mining operations,
the length of time required to obtain permits, certifications and
approvals, the success of exploration, development and mining
activities, the geology of the Company’s properties, environmental
risks, the availability of labour, the focus of the Company in the
future, demand and market outlook for precious metals and the
prices thereof, progress in development of mineral properties, the
Company’s ability to raise funding privately or on a public market
in the future, the Company’s future growth, results of operations,
performance, and business prospects and opportunities. Wherever
possible, words such as “anticipate”, “believe”, “expect”,
“intend”, “may” and similar expressions have been used to identify
such forward-looking information. Forward-looking information is
based on the opinions and estimates of management at the date the
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such time. Forward-looking information involves significant risks,
uncertainties, assumptions and other factors that could cause
actual results, performance or achievements to differ materially
from the results discussed or implied in the forward-looking
information. These factors, including, but not limited to,
fluctuations in currency markets, fluctuations in commodity prices,
the ability of the Company to access sufficient capital on
favourable terms or at all, changes in national and local
government legislation, taxation, controls, regulations, political
or economic developments in Canada, Australia or other countries in
which the Company does business or may carry on business in the
future, operational or technical difficulties in connection with
exploration or development activities, employee relations, the
speculative nature of mineral exploration and development,
obtaining necessary licenses and permits, diminishing quantities
and grades of mineral reserves, contests over title to properties,
especially title to undeveloped properties, the inherent risks
involved in the exploration and development of mineral properties,
the uncertainties involved in interpreting drill results and other
geological data, environmental hazards, industrial accidents,
unusual or unexpected formations, pressures, cave-ins and flooding,
limitations of insurance coverage and the possibility of project
cost overruns or unanticipated costs and expenses, and should be
considered carefully. Many of these uncertainties and contingencies
can affect the Company’s actual results and could cause actual
results to differ materially from those expressed or implied in any
forward-looking statements made by, or on behalf of, the Company.
Prospective investors should not place undue reliance on any
forward-looking information. Although the forward-looking
information contained in this report is based upon what management
believes, or believed at the time, to be reasonable assumptions,
the Company cannot assure prospective purchasers that actual
results will be consistent with such forward-looking information,
as there may be other factors that cause results not to be as
anticipated, estimated or intended, and neither the Company nor any
other person assumes responsibility for the accuracy and
completeness of any such forward-looking information. The Company
does not undertake, and assumes no obligation, to update or revise
any such forward-looking statements or forward-looking information
contained herein to reflect new events or circumstances, except as
may be required by law. No stock exchange, regulation
services provider, securities commission or other regulatory
authority has approved or disapproved the information contained in
this report.
Appendix 1
Table 1: Drill hole details for RAB holes
completed
Hole No. |
MGAEast (m) |
MGANorth (m) |
RL (m)(approx.) |
Dip |
Azimuth(approx.) |
EOHDepth (m) |
Target |
CRRB001 |
665100 |
6171720 |
620 |
-60 |
270 |
22 |
Crosby Main |
CRRB002 |
665140 |
6171720 |
620 |
-60 |
270 |
30 |
Crosby Main |
CRRB003 |
665180 |
6171720 |
620 |
-60 |
270 |
35 |
Crosby Main |
CRRB004 |
665220 |
6171720 |
620 |
-60 |
270 |
13 |
Crosby Main |
CRRB005 |
665260 |
6171720 |
620 |
-60 |
270 |
10 |
Crosby Main |
CRRB006 |
665080 |
6171800 |
620 |
-60 |
270 |
13 |
Crosby Main |
CRRB007 |
665120 |
6171800 |
620 |
-60 |
270 |
40 |
Crosby Main |
CRRB008 |
665160 |
6171800 |
620 |
-60 |
270 |
35 |
Crosby Main |
CRRB009 |
665200 |
6171800 |
620 |
-60 |
270 |
22 |
Crosby Main |
CRRB010 |
665240 |
6171800 |
620 |
-60 |
270 |
4 |
Crosby Main |
CRRB011 |
665060 |
6171720 |
620 |
-60 |
270 |
13 |
Crosby Main |
CRRB012 |
665120 |
6171640 |
620 |
-60 |
270 |
13 |
Crosby Main |
CRRB013 |
665160 |
6171635 |
620 |
-60 |
270 |
14 |
Crosby Main |
CRRB014 |
665200 |
6171640 |
620 |
-60 |
270 |
16 |
Crosby Main |
CRRB015 |
665240 |
6171640 |
620 |
-60 |
270 |
13 |
Crosby Main |
CRRB016 |
665140 |
6171555 |
620 |
-60 |
270 |
16 |
Crosby Main |
CRRB017 |
665180 |
6171560 |
620 |
-60 |
270 |
14 |
Crosby Main |
CRRB018 |
665140 |
6171760 |
620 |
-60 |
270 |
28 |
Crosby Main |
CRRB019 |
665065 |
6171880 |
620 |
-60 |
270 |
28 |
Crosby Main |
CRRB020 |
665020 |
6171880 |
620 |
-60 |
270 |
28 |
Crosby Main |
CRRB021 |
664980 |
6171880 |
620 |
-60 |
270 |
37 |
Crosby Main |
CRRB022 |
664960 |
6171800 |
620 |
-60 |
270 |
4 |
Crosby Main |
CRRB023 |
665000 |
6171800 |
620 |
-60 |
270 |
19 |
Crosby Main |
CRRB024 |
665020 |
6171800 |
620 |
-60 |
270 |
64 |
Crosby Main |
CRRB025 |
665020 |
6171720 |
620 |
-60 |
270 |
11 |
Crosby Main |
CRRB026 |
664960 |
6171880 |
620 |
-60 |
270 |
25 |
Crosby Main |
CRRB027 |
664572 |
6172672 |
620 |
-60 |
270 |
46 |
Crosby Central |
CRRB028 |
664540 |
6172680 |
620 |
-60 |
270 |
11 |
Crosby Central |
CRRB029 |
664590 |
6172671 |
620 |
-60 |
270 |
28 |
Crosby Central |
CRRB030 |
664020 |
6172993 |
620 |
-60 |
270 |
25 |
Crosby North |
CRRB031 |
664065 |
6173002 |
620 |
-60 |
270 |
25 |
Crosby North |
CRRB032 |
664086 |
6173016 |
620 |
-60 |
270 |
19 |
Crosby North |
CRRB033 |
664005 |
6172986 |
620 |
-60 |
270 |
22 |
Crosby North |
Table 2: Selected assay results for the RAB program –
holes not included contained no significant assay
results
Hole ID |
From |
To |
Au ppm |
Cu ppm |
Pb ppm |
Zn ppm |
Ag ppm |
As ppm |
Mo ppm |
CRRB002 |
0 |
4 |
0.031 |
58.1 |
191.5 |
389 |
0.2 |
11.1 |
2 |
CRRB002 |
4 |
8 |
0.007 |
38.3 |
61.2 |
443 |
0.2 |
8.2 |
0.7 |
CRRB002 |
8 |
12 |
0.005 |
32.3 |
84.9 |
396 |
0.3 |
9.5 |
0.9 |
CRRB002 |
12 |
16 |
0.008 |
94.4 |
547 |
445 |
0.6 |
63.6 |
3.3 |
CRRB002 |
16 |
20 |
0.005 |
29.1 |
393 |
772 |
0.4 |
29 |
1.7 |
CRRB002 |
20 |
24 |
0.005 |
65 |
369 |
552 |
0.6 |
22.7 |
1.6 |
CRRB002 |
24 |
28 |
0.026 |
156.5 |
905 |
656 |
1.9 |
34.5 |
19.3 |
CRRB002 |
28 |
30 |
0.063 |
78.7 |
654 |
649 |
1.4 |
31.3 |
14.8 |
CRRB005 |
4 |
8 |
0.004 |
20.8 |
24.3 |
118 |
0.1 |
30.6 |
<0.5 |
CRRB005 |
8 |
10 |
0.006 |
16.4 |
14.9 |
130 |
0.1 |
32.6 |
<0.5 |
CRRB006 |
0 |
4 |
0.016 |
41.9 |
1645 |
652 |
3 |
41 |
2.7 |
CRRB006 |
4 |
8 |
0.015 |
35.9 |
870 |
671 |
7.7 |
23.9 |
2.2 |
CRRB006 |
8 |
12 |
0.014 |
30.5 |
309 |
886 |
2.1 |
13.2 |
1.8 |
CRRB006 |
12 |
13 |
0.006 |
32.9 |
267 |
575 |
0.8 |
11.7 |
1 |
CRRB007 |
0 |
4 |
0.020 |
57.9 |
977 |
518 |
0.6 |
15.6 |
2.7 |
CRRB007 |
4 |
8 |
0.012 |
38.7 |
684 |
807 |
0.5 |
11.9 |
1.9 |
CRRB007 |
8 |
12 |
0.015 |
29.6 |
794 |
1165 |
0.8 |
11.7 |
1.9 |
CRRB007 |
12 |
16 |
0.041 |
64.6 |
1715 |
1220 |
4.2 |
19.3 |
11.2 |
Hole ID |
From |
To |
Au ppm |
Cu ppm |
Pb ppm |
Zn ppm |
Ag ppm |
As ppm |
Mo ppm |
CRRB007 |
16 |
20 |
0.055 |
39.4 |
1255 |
1000 |
7 |
26.5 |
6.1 |
CRRB007 |
20 |
24 |
0.069 |
57.2 |
1145 |
1960 |
3.7 |
15.9 |
7.5 |
CRRB007 |
24 |
28 |
0.048 |
10.3 |
1125 |
1490 |
0.6 |
22.9 |
4 |
CRRB007 |
27 |
28 |
0.012 |
12.4 |
918 |
856 |
1 |
24.3 |
1.7 |
CRRB007 |
28 |
29 |
0.042 |
12.2 |
478 |
764 |
0.5 |
16.6 |
1.5 |
CRRB007 |
29 |
30 |
0.013 |
6.6 |
222 |
570 |
0.5 |
10.4 |
1.3 |
CRRB007 |
30 |
31 |
0.020 |
13.4 |
1445 |
1060 |
1.7 |
35.9 |
8.2 |
CRRB007 |
31 |
32 |
0.122 |
37.4 |
2080 |
3220 |
5.2 |
200 |
109.5 |
CRRB007 |
32 |
33 |
0.361 |
162.5 |
6200 |
4240 |
9.1 |
164 |
224 |
CRRB007 |
32 |
36 |
0.332 |
163 |
6130 |
4110 |
9.5 |
144.5 |
295 |
CRRB007 |
33 |
34 |
0.021 |
17.3 |
649 |
1130 |
0.8 |
24.7 |
12 |
CRRB007 |
34 |
35 |
0.076 |
34 |
391 |
882 |
1.4 |
56.6 |
12.4 |
CRRB007 |
35 |
36 |
0.067 |
81 |
341 |
1000 |
1.1 |
27.5 |
9 |
CRRB007 |
36 |
37 |
0.161 |
321 |
1015 |
2880 |
2.6 |
55.9 |
29.5 |
CRRB007 |
36 |
40 |
0.143 |
395 |
879 |
2300 |
2.5 |
51.7 |
22.4 |
CRRB007 |
37 |
38 |
0.159 |
562 |
837 |
2360 |
2.7 |
48.6 |
16.9 |
CRRB007 |
38 |
39 |
0.058 |
197 |
923 |
1430 |
1.7 |
54.8 |
12.1 |
CRRB007 |
39 |
40 |
0.061 |
169 |
950 |
1805 |
2.3 |
81.4 |
17.8 |
CRRB008 |
0 |
4 |
0.154 |
35.6 |
756 |
454 |
0.6 |
31 |
7.2 |
CRRB008 |
4 |
8 |
0.035 |
24.9 |
631 |
906 |
0.8 |
31.6 |
2.9 |
CRRB008 |
8 |
12 |
0.033 |
47 |
514 |
1295 |
1.4 |
18.9 |
2 |
CRRB008 |
12 |
16 |
0.141 |
32.6 |
972 |
1050 |
2.5 |
40.3 |
4.9 |
CRRB008 |
16 |
20 |
0.013 |
36.5 |
470 |
1110 |
0.3 |
10.2 |
1.5 |
CRRB008 |
20 |
24 |
0.165 |
69.9 |
947 |
866 |
1.3 |
23.4 |
9.9 |
CRRB008 |
24 |
25 |
0.023 |
34.9 |
1080 |
1120 |
0.4 |
13.6 |
1.6 |
CRRB008 |
25 |
26 |
0.035 |
29.1 |
841 |
1080 |
0.8 |
19.5 |
2.5 |
CRRB008 |
26 |
27 |
0.020 |
27.3 |
623 |
2070 |
2.4 |
41.6 |
3.3 |
CRRB008 |
27 |
28 |
0.031 |
28.9 |
638 |
423 |
1.9 |
89.3 |
9.9 |
CRRB008 |
28 |
29 |
0.026 |
29.6 |
133 |
440 |
1.7 |
116.5 |
4.4 |
CRRB008 |
29 |
30 |
0.045 |
109.5 |
557 |
1120 |
4.3 |
284 |
4.3 |
CRRB008 |
30 |
31 |
0.048 |
167 |
554 |
1130 |
4.1 |
213 |
4.8 |
CRRB008 |
31 |
32 |
0.024 |
215 |
670 |
1510 |
2.3 |
32 |
2.1 |
CRRB008 |
32 |
33 |
0.523 |
189.5 |
486 |
1120 |
3.1 |
28.8 |
5.5 |
CRRB008 |
33 |
34 |
1.230 |
143 |
474 |
1220 |
3.4 |
55.5 |
13.7 |
CRRB008 |
34 |
35 |
0.541 |
46 |
389 |
1020 |
1.7 |
41.6 |
8.2 |
CRRB012 |
0 |
2 |
0.004 |
17.4 |
123 |
35 |
0.1 |
65.7 |
<0.5 |
CRRB012 |
2 |
4 |
0.012 |
24.7 |
592 |
44 |
0.4 |
98.8 |
<0.5 |
CRRB012 |
4 |
6 |
0.011 |
79.3 |
2150 |
60 |
1.3 |
54.9 |
0.5 |
CRRB012 |
6 |
8 |
0.009 |
32.4 |
991 |
130 |
0.5 |
53.8 |
0.6 |
CRRB012 |
8 |
10 |
0.020 |
80.6 |
1365 |
112 |
1.5 |
61.5 |
<0.5 |
CRRB012 |
10 |
12 |
0.009 |
172.5 |
4200 |
177 |
3.2 |
68.5 |
<0.5 |
CRRB012 |
12 |
13 |
0.007 |
45.4 |
1810 |
192 |
2.3 |
50.8 |
<0.5 |
CRRB013 |
0 |
2 |
0.006 |
14.5 |
147.5 |
69 |
0.1 |
121 |
0.8 |
CRRB013 |
2 |
4 |
0.016 |
24.6 |
288 |
128 |
0.3 |
82.6 |
1.6 |
CRRB013 |
4 |
6 |
0.024 |
21.9 |
442 |
73 |
0.8 |
91.2 |
3.5 |
CRRB013 |
6 |
8 |
0.015 |
21.8 |
162 |
83 |
1.3 |
206 |
3.4 |
CRRB013 |
8 |
10 |
0.015 |
11 |
29.8 |
178 |
0.9 |
119 |
1.7 |
CRRB013 |
10 |
12 |
0.007 |
12 |
13 |
231 |
0.3 |
25.6 |
0.8 |
CRRB013 |
12 |
14 |
0.006 |
24.6 |
14.6 |
337 |
0.3 |
23.4 |
0.8 |
CRRB014 |
0 |
2 |
0.030 |
41.1 |
201 |
149 |
0.1 |
18.6 |
3.6 |
CRRB014 |
2 |
4 |
0.020 |
42.7 |
171.5 |
199 |
0.1 |
28.6 |
5.2 |
CRRB014 |
4 |
6 |
0.024 |
65.7 |
593 |
295 |
0.3 |
26.9 |
4.2 |
CRRB014 |
6 |
8 |
0.086 |
134 |
2290 |
573 |
2.5 |
33.5 |
25.6 |
CRRB014 |
8 |
10 |
0.038 |
117 |
1855 |
734 |
1.3 |
46.5 |
25.2 |
CRRB014 |
10 |
12 |
0.022 |
79 |
933 |
266 |
1.4 |
60.6 |
3.7 |
CRRB014 |
12 |
14 |
0.013 |
135.5 |
353 |
253 |
1.1 |
59.7 |
2.6 |
CRRB014 |
14 |
16 |
0.040 |
154 |
149.5 |
408 |
1.8 |
26.8 |
4 |
Hole ID |
From |
To |
Au ppm |
Cu ppm |
Pb ppm |
Zn ppm |
Ag ppm |
As ppm |
Mo ppm |
CRRB018 |
0 |
4 |
0.033 |
39.8 |
389 |
432 |
0.4 |
21.4 |
3.2 |
CRRB018 |
4 |
8 |
0.004 |
4.7 |
109.5 |
516 |
0.3 |
11.2 |
<0.5 |
CRRB018 |
8 |
12 |
0.002 |
2.6 |
9 |
270 |
-0.1 |
1.5 |
<0.5 |
CRRB018 |
12 |
16 |
0.003 |
4.9 |
29.8 |
423 |
0.2 |
10.4 |
0.7 |
CRRB018 |
16 |
20 |
0.003 |
13 |
69 |
982 |
0.2 |
10.1 |
0.6 |
CRRB018 |
20 |
22 |
0.086 |
21.3 |
232 |
754 |
0.3 |
6.1 |
1.1 |
CRRB018 |
22 |
24 |
0.111 |
20 |
155.5 |
979 |
0.3 |
5.7 |
1 |
CRRB018 |
24 |
26 |
0.078 |
20.5 |
97 |
999 |
0.4 |
33.5 |
1 |
CRRB018 |
26 |
28 |
0.016 |
32.6 |
579 |
851 |
0.8 |
39.4 |
0.9 |
CRRB019 |
0 |
4 |
0.079 |
28.5 |
153 |
111 |
0.1 |
14.8 |
0.9 |
CRRB019 |
4 |
8 |
0.006 |
40.5 |
148 |
224 |
0.1 |
17.5 |
1.2 |
CRRB019 |
8 |
12 |
0.006 |
46.2 |
138 |
276 |
0.2 |
9.8 |
1.1 |
CRRB019 |
12 |
16 |
0.009 |
17 |
58.9 |
223 |
0.3 |
4.1 |
<0.5 |
CRRB019 |
16 |
20 |
0.005 |
18 |
50.4 |
208 |
0.1 |
8.5 |
1 |
CRRB019 |
20 |
22 |
0.002 |
15.2 |
56.6 |
507 |
0.2 |
7.9 |
0.9 |
CRRB019 |
22 |
24 |
0.002 |
22.6 |
83 |
842 |
0.2 |
6.7 |
1 |
CRRB019 |
24 |
26 |
0.195 |
194 |
759 |
822 |
1.3 |
93.8 |
5.1 |
CRRB019 |
26 |
28 |
0.073 |
16.2 |
146.5 |
749 |
0.3 |
28.5 |
1.8 |
CRRB020 |
0 |
4 |
0.006 |
24 |
247 |
395 |
0.1 |
12.9 |
0.6 |
CRRB020 |
4 |
8 |
0.090 |
13.8 |
273 |
408 |
0.1 |
19.8 |
<0.5 |
CRRB020 |
8 |
12 |
0.015 |
8.3 |
107 |
482 |
0.2 |
29.8 |
0.6 |
CRRB020 |
12 |
16 |
0.005 |
38.4 |
134 |
511 |
0.2 |
5.8 |
0.6 |
CRRB020 |
16 |
20 |
0.004 |
20.9 |
576 |
469 |
0.3 |
14.1 |
0.8 |
CRRB020 |
20 |
22 |
0.003 |
19.9 |
734 |
664 |
0.3 |
7.5 |
<0.5 |
CRRB020 |
22 |
24 |
0.005 |
16.5 |
233 |
434 |
0.2 |
7.5 |
<0.5 |
CRRB020 |
24 |
26 |
0.004 |
14.3 |
205 |
393 |
0.2 |
8.7 |
0.5 |
CRRB020 |
26 |
28 |
0.006 |
17.9 |
521 |
725 |
0.2 |
10.7 |
0.7 |
CRRB021 |
0 |
4 |
0.739 |
154.5 |
819 |
190 |
0.5 |
61 |
8.1 |
CRRB021 |
4 |
8 |
0.072 |
139.5 |
1180 |
350 |
0.5 |
24 |
6.3 |
CRRB021 |
8 |
12 |
0.026 |
110.5 |
520 |
236 |
0.4 |
38.1 |
6.4 |
CRRB021 |
12 |
16 |
0.058 |
28.7 |
177.5 |
454 |
0.2 |
38.1 |
2.1 |
CRRB021 |
16 |
20 |
0.005 |
13 |
198.5 |
627 |
0.1 |
9.5 |
0.7 |
CRRB021 |
20 |
21 |
0.008 |
7.4 |
37.6 |
428 |
0.1 |
20.6 |
6.1 |
CRRB021 |
21 |
22 |
0.014 |
87.7 |
124.5 |
1090 |
0.2 |
20.5 |
19.9 |
CRRB021 |
22 |
23 |
0.013 |
3.5 |
32.6 |
703 |
0.1 |
27.3 |
11.5 |
CRRB021 |
23 |
24 |
0.022 |
2.3 |
48.7 |
329 |
0.2 |
56.3 |
8.2 |
CRRB021 |
24 |
25 |
0.005 |
1.8 |
13.1 |
257 |
0.1 |
15.4 |
2.6 |
CRRB021 |
25 |
26 |
0.005 |
1.3 |
18.9 |
454 |
0.1 |
16.8 |
5 |
CRRB021 |
26 |
27 |
0.003 |
4 |
8.9 |
472 |
0.1 |
11.9 |
1.5 |
CRRB021 |
27 |
28 |
0.040 |
1.6 |
10 |
267 |
0.1 |
15.5 |
1.9 |
CRRB021 |
28 |
29 |
0.025 |
7.7 |
38.6 |
494 |
0.3 |
28.2 |
6.4 |
CRRB021 |
29 |
30 |
0.013 |
5.2 |
50 |
568 |
1.2 |
23.9 |
10.4 |
CRRB021 |
30 |
31 |
0.006 |
2.3 |
19.8 |
373 |
0.2 |
3.6 |
0.7 |
CRRB021 |
31 |
32 |
0.029 |
4.4 |
29.4 |
294 |
0.8 |
18.4 |
2.9 |
CRRB021 |
32 |
33 |
0.057 |
5.4 |
34.3 |
326 |
0.4 |
25.2 |
6.3 |
CRRB021 |
33 |
34 |
0.027 |
4.7 |
59.1 |
273 |
0.8 |
31.4 |
13.2 |
CRRB021 |
34 |
35 |
0.030 |
10.9 |
109.5 |
264 |
0.7 |
30.8 |
9.2 |
CRRB021 |
35 |
36 |
0.030 |
7.1 |
60.8 |
250 |
0.8 |
33.1 |
4.4 |
CRRB021 |
36 |
37 |
0.031 |
30.6 |
47.2 |
198 |
0.4 |
16.5 |
3.8 |
CRRB022 |
0 |
1 |
0.048 |
90.6 |
19 |
17 |
-0.1 |
2.5 |
<0.5 |
CRRB022 |
1 |
2 |
0.002 |
116.5 |
9.3 |
16 |
-0.1 |
1.8 |
<0.5 |
CRRB022 |
2 |
3 |
0.003 |
67.3 |
8.8 |
19 |
-0.1 |
2.2 |
0.5 |
CRRB022 |
3 |
4 |
0.049 |
154 |
57.5 |
19 |
0.1 |
0.7 |
<0.5 |
CRRB023 |
0 |
2 |
0.008 |
73.8 |
138.5 |
236 |
0.1 |
21.8 |
1.5 |
CRRB023 |
2 |
4 |
0.007 |
108 |
215 |
343 |
0.1 |
16.4 |
1.4 |
CRRB023 |
4 |
6 |
0.006 |
80 |
135.5 |
305 |
0.3 |
14.9 |
0.9 |
CRRB023 |
6 |
8 |
0.010 |
321 |
183 |
393 |
0.8 |
37.8 |
1.3 |
Hole ID |
From |
To |
Au ppm |
Cu ppm |
Pb ppm |
Zn ppm |
Ag ppm |
As ppm |
Mo ppm |
CRRB023 |
8 |
10 |
0.041 |
218 |
376 |
299 |
0.9 |
37.3 |
3.1 |
CRRB023 |
10 |
12 |
0.042 |
181 |
739 |
343 |
1 |
24.6 |
2.2 |
CRRB023 |
12 |
14 |
0.036 |
181.5 |
213 |
345 |
0.6 |
17.2 |
2.1 |
CRRB023 |
14 |
16 |
0.030 |
190.5 |
169 |
439 |
0.8 |
26.5 |
1.7 |
CRRB023 |
16 |
18 |
0.105 |
35.5 |
199.5 |
350 |
0.5 |
34.6 |
8 |
CRRB023 |
18 |
19 |
0.162 |
17.6 |
127 |
431 |
0.2 |
23.6 |
5.3 |
CRRB024 |
0 |
4 |
0.023 |
147.5 |
224 |
215 |
0.3 |
59.1 |
2 |
CRRB024 |
4 |
8 |
0.102 |
290 |
115 |
319 |
0.9 |
37.6 |
3.4 |
CRRB024 |
8 |
12 |
0.011 |
189 |
83.1 |
281 |
0.2 |
45.7 |
3.8 |
CRRB024 |
12 |
16 |
0.023 |
332 |
125.5 |
394 |
0.3 |
36.2 |
8.8 |
CRRB024 |
16 |
20 |
0.008 |
30.7 |
46 |
279 |
0.2 |
34.4 |
12.6 |
CRRB024 |
20 |
24 |
0.087 |
72 |
125 |
209 |
0.3 |
31.7 |
5.8 |
CRRB024 |
24 |
28 |
0.015 |
34.3 |
61.7 |
600 |
0.1 |
57.4 |
4.7 |
CRRB024 |
28 |
30 |
0.029 |
167.5 |
180 |
1105 |
0.4 |
177.5 |
4.3 |
CRRB024 |
30 |
32 |
0.045 |
190.5 |
105 |
494 |
1.6 |
447 |
3.3 |
CRRB024 |
32 |
34 |
0.038 |
519 |
62.6 |
373 |
2.3 |
147 |
2.9 |
CRRB024 |
34 |
36 |
0.036 |
1355 |
60.7 |
563 |
5 |
92.6 |
3.9 |
CRRB024 |
36 |
38 |
0.017 |
471 |
72.4 |
454 |
2.1 |
57.2 |
0.9 |
CRRB024 |
38 |
40 |
0.014 |
69.2 |
157 |
541 |
0.8 |
52 |
0.5 |
CRRB024 |
40 |
42 |
0.009 |
52 |
188 |
1260 |
1 |
28.1 |
0.7 |
CRRB024 |
42 |
44 |
0.006 |
69.1 |
89 |
546 |
0.7 |
32.3 |
0.7 |
CRRB024 |
44 |
46 |
0.021 |
91.6 |
23.4 |
921 |
1.3 |
79.8 |
0.8 |
CRRB024 |
46 |
48 |
0.023 |
19.1 |
41.7 |
557 |
0.5 |
232 |
1.1 |
CRRB024 |
48 |
50 |
0.020 |
15.1 |
28.1 |
412 |
0.2 |
50 |
1.5 |
CRRB024 |
50 |
52 |
0.005 |
6.8 |
107.5 |
448 |
0.4 |
27 |
1.6 |
CRRB024 |
52 |
54 |
0.009 |
294 |
721 |
2940 |
2.5 |
56.4 |
7.3 |
CRRB024 |
54 |
56 |
0.026 |
310 |
3630 |
9490 |
8.1 |
40.2 |
14.5 |
CRRB024 |
56 |
58 |
0.117 |
185.5 |
5380 |
9800 |
7.9 |
53 |
7.8 |
CRRB024 |
58 |
60 |
0.013 |
90.5 |
536 |
1390 |
1.3 |
31.3 |
6.6 |
CRRB024 |
60 |
62 |
0.009 |
172.5 |
216 |
609 |
0.9 |
24.3 |
2.1 |
CRRB024 |
62 |
64 |
0.012 |
31.8 |
106 |
411 |
0.3 |
31.5 |
1.3 |
CRRB027 |
0 |
2 |
0.032 |
1350 |
468 |
192 |
0.4 |
50.1 |
7.4 |
CRRB027 |
2 |
4 |
0.013 |
1950 |
408 |
198 |
0.6 |
19.8 |
2.3 |
CRRB027 |
4 |
6 |
0.256 |
2960 |
920 |
223 |
1.5 |
203 |
16 |
CRRB027 |
6 |
8 |
0.215 |
3780 |
1045 |
229 |
1.2 |
83 |
16.4 |
CRRB027 |
8 |
10 |
0.230 |
2860 |
874 |
197 |
3.2 |
87.9 |
18 |
CRRB027 |
10 |
12 |
0.065 |
2430 |
769 |
273 |
1.6 |
60.3 |
8.4 |
CRRB027 |
12 |
14 |
0.095 |
2820 |
521 |
172 |
2.3 |
42.5 |
12.8 |
CRRB027 |
14 |
16 |
0.090 |
1575 |
1030 |
372 |
1.9 |
54.3 |
10.4 |
CRRB027 |
16 |
18 |
0.344 |
3290 |
1305 |
243 |
3.6 |
107.5 |
18.1 |
CRRB027 |
18 |
20 |
0.100 |
2810 |
655 |
216 |
2.4 |
67.5 |
10.4 |
CRRB027 |
20 |
22 |
0.055 |
1565 |
1210 |
213 |
1.6 |
47.3 |
10 |
CRRB027 |
22 |
24 |
0.175 |
7000 |
1590 |
263 |
6 |
78.3 |
16.3 |
CRRB027 |
24 |
26 |
0.053 |
2250 |
746 |
390 |
1.8 |
88.8 |
7 |
CRRB027 |
26 |
28 |
0.684 |
8460 |
2030 |
1030 |
9.8 |
160 |
21.4 |
CRRB027 |
28 |
30 |
0.228 |
2140 |
1015 |
733 |
1.2 |
38.3 |
14.7 |
CRRB027 |
30 |
32 |
0.455 |
1945 |
1135 |
474 |
2.4 |
118 |
14.3 |
CRRB027 |
32 |
34 |
0.157 |
1485 |
834 |
650 |
1.3 |
51 |
10.8 |
CRRB027 |
34 |
36 |
0.073 |
2100 |
1470 |
354 |
1.2 |
36.8 |
10.4 |
CRRB027 |
36 |
38 |
0.135 |
1175 |
1420 |
772 |
0.9 |
43.1 |
9.8 |
CRRB027 |
38 |
40 |
0.216 |
1100 |
1355 |
754 |
0.9 |
41.1 |
9.2 |
CRRB027 |
40 |
42 |
0.264 |
878 |
189 |
307 |
0.5 |
20.6 |
7.4 |
CRRB027 |
42 |
44 |
0.214 |
698 |
85 |
346 |
0.6 |
27.3 |
12.2 |
CRRB027 |
44 |
46 |
0.078 |
955 |
100.5 |
573 |
0.9 |
83.6 |
8.3 |
CRRB028 |
0 |
4 |
0.007 |
75 |
674 |
79 |
0.3 |
13.9 |
2.2 |
CRRB028 |
4 |
8 |
0.012 |
132.5 |
827 |
68 |
0.6 |
35.1 |
5.8 |
CRRB028 |
8 |
11 |
0.077 |
198.5 |
1455 |
133 |
1.1 |
35.1 |
10.8 |
Hole ID |
From |
To |
Au ppm |
Cu ppm |
Pb ppm |
Zn ppm |
Ag ppm |
As ppm |
Mo ppm |
CRRB029 |
0 |
4 |
0.014 |
242 |
46.7 |
96 |
0.1 |
72.9 |
5.4 |
CRRB029 |
4 |
8 |
0.013 |
137 |
21.8 |
104 |
0.1 |
24.3 |
1.2 |
CRRB029 |
8 |
12 |
0.017 |
405 |
18.5 |
108 |
0.1 |
34.5 |
2.6 |
CRRB029 |
12 |
16 |
0.010 |
740 |
16.9 |
97 |
0.2 |
23 |
2.4 |
CRRB029 |
16 |
20 |
0.006 |
245 |
7.8 |
108 |
0.2 |
19.9 |
1.8 |
CRRB029 |
20 |
22 |
0.007 |
232 |
9.7 |
99 |
0.3 |
17.3 |
3.4 |
CRRB029 |
22 |
24 |
0.004 |
277 |
10.2 |
102 |
0.2 |
12.9 |
4.5 |
CRRB029 |
24 |
26 |
0.010 |
3440 |
16.1 |
81 |
1.1 |
16.6 |
3.9 |
CRRB029 |
26 |
28 |
0.009 |
1565 |
13.6 |
88 |
0.4 |
14.6 |
3.8 |
JORC 2012 Table 1
Section 1 Sampling Techniques and Data
(Criteria in this section applies to all succeeding
sections)
Criteria |
JORC Code
explanation |
|
Sampling
techniques |
· Nature and
quality of sampling (eg cut channels, random chips, or specific
specialised industry standard measurement tools appropriate to the
minerals under investigation, such as down hole gamma sondes, or
handheld XRF instruments, etc). These examples should not be taken
as limiting the broad meaning of sampling.· Include reference
to measures taken to ensure sample representivity and the
appropriate calibration of any measurement tools or systems
used.· Aspects of the determination of mineralisation that
are Material to the Public Report. |
· Samples for
analysis were taken from rotary airblast (RAB) drill
cuttings. The majority (~90%) of the drill cutting were
produced from the RAB hammer which provided better penetration into
the harder bedrock materials. The samples were essentially
all dry with little or no ground water being encountered. All drill
cuttings were collected via a cyclone using manual choke or
collected at the top of the collar and placed on the ground in
separate 1m piles. Samples were taken as mostly 4m scoop composite
samples with potentially mineralised intervals samples at either 2m
or 1m intervals. Samples were collected from the 1m piles on an
equal volume basis to approximately 2.5kg of total sample size per
numbered calico bag.· One quality control sample (alternating
between assay standards, blank assay material and field duplicates)
was inserted on a nominal 10 sample basis. |
Drilling
techniques |
· Drill type (eg
core, reverse circulation, open-hole hammer, rotary air blast,
auger, Bangka, sonic, etc) and details. |
· The drilling
was undertaken by a rotary airblast (RAB) system, mostly employing
the hammer to achieve penetration in bedrock materials.· The
drilling rig was Mole Pioneer 160 rig with 600cfm and 200psi
compressor, with a maximum depth to 100m.· A 4.5 inch bit was
used for the drilling and holes were drilled to target
depth.· All holes were drilled under geological
supervision. |
Drill sample
recovery |
· Method of
recording and assessing core and chip sample recoveries and results
assessed. |
· A geologist
supervised the drilling and sampling of the holes and recorded the
lithologies intersected.· There were no issues with either
sample recovery or sample condition in the drilling program and
ground conditions were generally good for the drilling method
employed. |
Logging |
· Whether core
and chip samples have been geologically and geotechnically logged
to a level of detail to support appropriate Mineral Resource
estimation, mining studies and metallurgical studies. |
· All drill holes
were geologically logged at the time they were drilled by the
supervising geologist using the Heron Geological Legend. Selected
drill chips were collected for each hole and stored in chip trays
for future reference. |
Sub-sampling techniques
and sample preparation |
· For all sample
types, the nature, quality and appropriateness of the sample
preparation technique. |
· All samples
weighed, dried and reconciled against company submission.·
All samples pulverised in a ring pulveriser (LM5) to a nominal 85%
passing 75 micron. |
Quality of assay data
and laboratory tests |
· The nature,
quality and appropriateness of the assaying and laboratory
procedures used and whether the technique is considered partial or
total.· Nature of quality control procedures adopted (eg
standards, blanks, duplicates, external laboratory checks) and
whether acceptable levels of accuracy (ie lack of bias) and
precision have been established. |
· Sample
preparation and assaying was conducted through ALS Laboratories in
Orange NSW· Gold determined by aqua-regia digestion with
ICP-AES analysis to 1ppb LLD.· Other elements by aqua-regia
digestion followed by ICP-AES analysis. · Laboratory
quality control standards (blanks, standards and duplicates) are
inserted at a rate of 5 per 35 samples. |
Verification of
sampling and assaying |
· The
verification of significant intersections by either independent or
alternative company personnel.· Documentation of primary
data, data entry procedures, data verification, data storage
(physical and electronic) protocols.· Discuss any adjustment
to assay data. |
· An internal
review of results was undertaken by company personnel. No
independent verification was undertaken at this stage.· All
field and laboratory data is in the process of being entered into
an industry standard database using a contract database
administrator (DBA). In-house validation of both the field
and laboratory data is undertaken prior to final acceptance and
reporting of the data.· Quality control samples from both the
Company and the Laboratory are assessed by the DBA and reported to
the Company geologists for verification. All assay data must
pass this data verification and quality control process before
being reported. |
Location of data
points |
· Accuracy and
quality of surveys used to locate drill holes (collar and down-hole
surveys), trenches, mine workings and other locations used in
Mineral Resource estimation. |
· All sample
points located with handheld GPS, with accuracy of about 5m.
This is considered appropriate at this early stage of
exploration. Elevations for collars are not determined at
this stage and a nominal elevation is used. |
Data spacing and
distribution |
· Data spacing
for reporting of Exploration Results.· Whether the data
spacing and distribution is sufficient to establish the degree of
geological and grade continuity appropriate for the Mineral
Resource and Ore Reserve estimation procedure(s) and
classifications applied.· Whether sample compositing has been
applied. |
· Drilling was
performed on a nominal 80m spaced east-west lines and 40m along the
line with some closer spaced holes in places. All holes were
angled at 60 degrees to the west.· Sampling and compositing
was appropriate for the early stage of exploration. |
Orientation of data in
relation to geological structure |
· Whether the
orientation of sampling achieves unbiased sampling of possible
structures and the extent to which this is known, considering the
deposit type. |
· Sampling
orientation was appropriate for the early stage of exploration and
was not designed to take into account specific structures. |
Sample security |
· The measures
taken to ensure sample security. |
· Samples were
secured in green plastic bags and transported to the laboratory by
company employed personnel. Beyond this there were no
specific security measures. |
Audits or reviews |
· The results of
any audits or reviews of sampling techniques and data. |
· No audits or
reviews were undertaken due to the early stage of exploration. |
Section
2
Reporting of Exploration Results
(Criteria listed in the preceding section also apply to this
section.)
Criteria |
JORC Code
explanation |
|
Mineral tenement and
land tenure status |
· Type, reference
name/number, location and ownership including agreements or
material issues with third parties such as joint ventures,
partnerships, overriding royalties, native title interests,
historical sites, wilderness or national park and environmental
settings.· The security of the tenure held at the time of
reporting along with any known impediments to obtaining a licence
to operate in the area. |
· All work was
undertaken on granted exploration licences EL8400 in the name of
Ochre Resources Pty Ltd which is a wholly owned subsidiary of Heron
Resources Ltd. The tenement is in good standing· The
Kangiara Project area is on privately owned farm land and the
Company has entered into compensation agreements with the
landowners to access their properties.· There are no known
specific environmental or heritage impediments for the current
phase of exploration. |
Exploration done by
other parties |
· Acknowledgment
and appraisal of exploration by other parties. |
· Previous
exploration at the Crosby Prospect appears to have been limited
with no previous drilling of the geochemical had been
undertaken.· The soil geochemical anomaly was first outlined
in the mid 1970s (Esso Exploration) and then better defined
(including gold analysis) by Oakland Resources Ltd in 2013. |
Geology |
· Deposit type,
geological setting and style of mineralization. |
· The Crosby
Prospect is underlain by rocks of the in felsic-intermediate
Silurian volcanics of the Douro Group.· The drilling
intersected the Silurian sequence of dacitic intrusive and breccia
rocks with minor intercalated shale and other fine-grained
sediments. Pervasive sericite and fine grained disseminated
pyrite (phyllic alteration) was observed in many of the holes with
lesser biotite and some fine grained base metal sulphides.·
The style/model of mineralisation is McPhillamy’s (Orogenic) or
intrusive related (including porphyry style) styles. |
Drill hole
Information |
o A summary of
all information material to the understanding of the exploration
results including a tabulation of the following information for all
Material drill holes: |
· Drilling
location information is provided in Table 1 and collars shown in
Figure 2.· The drilling was designed to provide information
as to the source of the strong surface geochemical anomaly and
provide guidance for deeper drilling. |
Data aggregation
methods |
· In reporting
Exploration Results, weighting averaging techniques, maximum and/or
minimum grade truncations (eg cutting of high grades) and cut-off
grades are usually Material and should be stated.· Where
aggregate intercepts incorporate short lengths of high grade
results and longer lengths of low grade results, the procedure used
for such aggregation should be stated and some typical examples of
such aggregations should be shown in detail. |
· Assays results
for the various programs are reported in summary form only, which
is considered appropriate for this early stage of
exploration. · Only relevant elements are reported here,
however, a larger suite of elements were assayed for. |
Relationship between
mineralization widths and intercept lengths |
· These
relationships are particularly important in the reporting of
Exploration Results.· If the geometry of the mineralisation
with respect to the drill hole angle is known, its nature should be
reported. |
· See comments
above – at this stage, actual mineralised intercepts are not
considered relevant to the report. |
Diagrams |
· Appropriate
maps and sections (with scales) and tabulations of intercepts
should be included for any significant discovery being reported
These should include, but not be limited to a plan view of drill
hole collar locations and appropriate sectional views. |
· Maps relevant
for current phase of exploration are included in the release. |
Balanced reporting |
· Where
comprehensive reporting of all Exploration Results is not
practicable, representative reporting of both low and high grades
and/or widths should be practiced to avoid misleading reporting of
Results. |
· The reporting
is considered to be balanced and all relevant/material results have
been disclosed for this current phase of exploration. |
Other substantive
exploration data |
· Other
exploration data, if meaningful and material, should be reported
including (but not limited to): geological observations;
geophysical survey results; geochemical survey results; bulk
samples – size and method of treatment; metallurgical test results;
bulk density, groundwater, geotechnical and rock characteristics;
potential deleterious or contaminating substances. |
· Open-file
aeromagnetic data, geological maps, and other geological datasets
have been used to guide the drilling program and the interpretation
of the results. |
Further work |
· The nature and
scale of planned further work (eg tests for lateral extensions or
depth extensions or large-scale step-out drilling). |
· Gold by fire
assay determination of selected anomalous intervals will be
undertaken to check if gold is potentially refractory and may lead
to slightly higher reportable gold levels.· Further deeper
and step out drilling is being considered given these initial
results, however, a full review will be undertaken prior to
commitment of a follow-up program. |
For further information, please visit www.heronresources.com.au or contact:
Australia:
Mr Wayne Taylor
Managing Director and Chief Executive Officer
Tel: +61 2 9119 8111 or +61 8 6500 9200
Email: heron@heronresources.com.au
Jon Snowball
FTI Consulting
+61 2 8298 6100
jon.snowball@fticonsulting.com
Canada:
Tel: +1 647 862 1157 (Toronto)