Novo Resources Corp. (
Novo or the
Company) (ASX: NVO) (TSX: NVO) (OTCQX: NSRPF) is
pleased to report significant assay results received from a
relogging and infill sampling program completed across 11
previously under sampled, historic drill holes, located within
priority target corridors at the Belltopper Gold Project
(‘
Belltopper’) in Victoria (Figure 1).
Figure 1, Belltopper Gold Project location map with regional
gold occurrences and major structures.1
Novo has not conducted data verification (as
that term is defined in National Instrument 43-101 Standards of
Disclosure for Mineral Projects and JORC 2012) in respect of the
data set out in Figure 1 and therefore is not to be regarded as
reporting, adopting or endorsing those results/figures. No
assurance can be given that Novo will achieve similar results at
Belltopper.
____________________________________1 See the
following for source documents in relation to the [historical gold]
production figures for Bendigo, Fosterville, Costerfield,
Castlemaine and Ballarat. Wilson, C. J. L., Moore, D. H., Vollgger,
S. A., & Madeley, H. E. (2020). Structural evolution of the
orogenic gold deposits in central Victoria, Australia: The role of
regional stress change and the tectonic regime. Ore Geology
Reviews, 120, 103390. Phillips, G. N., & Hughes, M. J.
(1996). The geology and gold deposits of the Victorian gold
province. Ore Geology Reviews, 11(5), 255-302. Costerfield
Operation, Victoria, Australia, NI 43-101 Technical Report, March
2024; Agnico Eagle Mines Detailed Mineral Reserve and Mineral
Resources Statement (as at December 31, 2023). Agnico Eagle Mines
Limited. Fosterville Gold Mine. Retrieved August 21, 2024, from
Agnico Eagle Website For Comet and Sunday Creek exploration
results, refer: Great Pacific Gold Company TSXV release dated 11
January 2024, and Southern Cross Gold Company ASX release dated 5
March 2024, respectively.
SUMMARY
A re-logging and infill sampling program
completed on 11 previously under-sampled historic diamond drill
holes at Belltopper, has delivered multiple new significant gold
intercepts across a range of known and emerging targets.
Highlights include:
- 6.0 m @ 4.37 g/t Au
from 169 m (including 5.0 m @ 5.18 g/t Au from 169
m) in DDHMA1.
- 2.0 m @ 7.19 g/t Au
from 52 m (including 1.15 m @ 12.01 g/t Au from 52
m) in MD04.
- 2.0 m @ 3.87 g/t Au
from 43 m (including 1.0 m @ 6.92 g/t Au from 43
m) in MD04.
- 3.1 m @ 3.29 g/t Au
from 36 m (including 1.3 m @ 7.26 g/t Au from 37.3
m) in MD06A.
- 2.1 m @ 3.82 g/t Au
from 78.9 m (including 0.6 m @ 9.74 g/t Au from
79.3 m) in MD07.
- 13 m @ 0.64 g/t Au
from 90 m (including 1 m @ 1.92 g/t Au from 94 m)
in DDHMA2.
(Note: See Appendix 2 for complete assay results.)
The mineralisation presented in the body of this
news release is not necessarily representative of mineralisation
throughout the Belltopper Gold Project. Intercepts are expressed as
down-hole intersections and should not be presumed to represent
true widths, which vary from hole to hole and between reefs (refer
JORC Table 1).
New intercepts associated with the Never
Despair (e.g. DDHMA1) and West Panama
(e.g. DDHMA2) reefs (Figure 2), further highlight the unrealised
potential for a network of historic high-grade gold-reefs on the
Project that have been developed to varying degrees at surface or
underground during the mid to late 1800’s, but not extensively
mined. Most of the key historic reefs on the project have very
little (< 5 holes) to no modern drill testing.
New intercepts reported for the Butchers
Gully Fault (e.g. MD04, MD06A) showcase the potential for
this emerging +1 km steep, northwest dipping structure, that trends
in parallel with the high-grade Leven Star Reef.
The new significant intercept associated with
NW Fault 4 (MD07) is notable. This target was
mapped as a sub-vertical to steep west-south-west dipping quartz
reef and belongs to an important set of gold-bearing, west-dipping
structures that form a component of the anticline-related (e.g.
Fosterville-style) epizonal targets at Belltopper. The NW Fault 4
target may potentially link with the NW Fault 9 target mapped to
the north (Figure 2), which returned 2.0 m @ 15.18 g/t
Au from 9 m, in recently drilled BTD0042. These target
faults combined have a strike length of ~1 km.
Of further note, both NW Fault 4 and NW
Fault 9 are also modelled to interact with the Missing
Link Granite, a porphyritic felsic intrusion and hence provide
targeted structural intersections to test for intrusion hosted
mineralisation, either along the margins of, or extending into, the
Missing Link Granite itself.
Detailed information from re-logging allows
better understanding of the geology and controls on higher-grade
mineralisation at Belltopper. Data from the program has allowed
Novo to precisely locate and refine specific target reefs and key
structural features, such as modelled high-grade shoots and
high-priority target anticline corridors. This is fundamental data
that will be applied to ongoing targeting moving forward.
____________________________________2 Refer to
the Company’s news release dated June 4, 2024, released to ASX on
June 5, 2024.
RESULTS AND INTERPRETATION FROM THE
RELOGGING PROGRAM
A recent review of archived historic diamond
core has highlighted a significant opportunity to validate several
targets at Belltopper, by means of re-visiting select historic
drill core and completing a re-logging and infill sampling
exercise.
The re-logging program at Belltopper focused on
11 historic drill holes located within current priority target
areas (Figure 2). Historic sampling practices vary from hole to
hole, but as a general theme, the sampling was restricted to
specific targets, or completed as niche-style sampling, and in many
instances, what are recognised as gold-prospective zones today,
were not originally sampled.
Figure 2, Location of re-logged and infill
sampled historic drill-holes with significant new assays
highlighted. Callouts represent new assays > 5-gram x
meters.
Detailed geology and geotechnical logging were
completed on all 11 holes and included collection of magnetic
susceptibility and specific gravity data. The re-logging campaign
included a sampling component which involved gold and multi-element
assaying on previously uncut prospective intervals identified
during the re-logging exercise, or across uncut intervals where
modelled target reefs are projected to intersect the drill hole.
Samples for assay were also collected where previous historic
significant assays remained open (either at upper or lower sample
intervals), or where infill sampling was extended to cover previous
gaps in data between closely spaced historic assays.
Standard QAQC practices were adhered to as
outlined in JORC Table 1. In total some 1,643 primary and 225 QC
samples were submitted for fire assay gold and multi-element as
part of the re-logging exercise. Table 1 highlights all (+2-gram x
metre) significant intercepts returned from the recent infill
sampling program completed. Refer to Appendices for a full listing
of all anomalous (>0.3-gram x metre) intersections. The
intercepts presented in both Table 1 and Appendix 2 represent
either:
- entirely new
independent intercepts, or
- extension and
upgrading of historic intercepts, or
- extension and
integration of two or more previous intercepts by means of infill
sampling.
Table 1, Significant (+ 2-gram x metre)
intersections reported for recent infill sampling of historic drill
holes at Belltopper. Intercepts calculated with 0.3 g/t Au cut-off
and 2 m internal dilution. High grade included intercepts
calculated with 1.0 g/t Au and no internal dilution. All
significant intersections from recent infill sampling program on
historic drill holes reported.
DrillHole |
Including |
From(m) |
To(m) |
Interval(m) ^ |
Au(g/t) |
Aug*m^^ |
Intersection |
MD03 |
|
14.00 |
19.00 |
5.00 |
0.55 |
2.7 |
5.00 m @ 0.55 g/t Au from 14 m |
MD03 |
|
45.00 |
47.00 |
2.00 |
1.80 |
3.6 |
2.00 m @ 1.80 g/t Au from 45 m |
MD04 |
|
43.00 |
45.00 |
2.00 |
3.87 |
7.7 |
2.00 m @ 3.87 g/t Au from 43 m |
MD04 |
inc. |
43.00 |
44.00 |
1.00 |
6.92 |
6.9 |
1.00 m @ 6.92 g/t Au from 43 m |
MD04 |
|
52.00 |
54.00 |
2.00 |
7.19 |
14.4 |
2.00 m @ 7.19 g/t Au from 52 m |
MD04 |
inc. |
52.00 |
53.15 |
1.15 |
12.01 |
13.8 |
1.15 m @ 12.01 g/t Au from 52 m |
MD06A |
|
36.00 |
39.10 |
3.10 |
3.29 |
10.2 |
3.10 m @ 3.29 g/t Au from 36 m |
MD06A |
inc. |
37.30 |
38.60 |
1.30 |
7.26 |
9.4 |
1.30 m @ 7.26 g/t Au from 37.3 m |
MD06A |
|
420.00 |
425.50 |
5.50 |
0.70 |
3.9 |
5.50 m @ 0.70 g/t Au from 420 m |
MD07 |
|
25.00 |
30.00 |
5.00 |
0.69 |
3.4 |
5.00 m @ 0.69 g/t Au from 25 m |
MD07 |
|
78.90 |
81.00 |
2.10 |
3.82 |
8.0 |
2.10 m @ 3.82 g/t Au from 78.9 m |
MD07 |
inc. |
79.30 |
79.90 |
0.60 |
9.74 |
5.8 |
0.60 m @ 9.74 g/t Au from 79.3 m |
MD07 |
|
154.00 |
155.60 |
1.60 |
1.22 |
2.0 |
1.60 m @ 1.22 g/t Au from 154 m |
MD08A |
|
123.00 |
125.00 |
2.00 |
1.60 |
3.2 |
2.00 m @ 1.60 g/t Au from 123 m |
MD08A |
inc. |
124.00 |
125.00 |
1.00 |
2.30 |
2.3 |
1.00 m @ 2.30 g/t Au from 124 m |
LSDDH7 |
|
196.40 |
197.40 |
1.00 |
3.41 |
3.4 |
1.00 m @ 3.41 g/t Au from 196.4 m |
DDHMA1 |
|
41.10 |
45.10 |
4.00 |
0.64 |
2.6 |
4.00 m @ 0.64 g/t Au from 41.1 m |
DDHMA1 |
|
169.00 |
175.00 |
6.00 |
4.37 |
26.2 |
6.00 m @ 4.37 g/t Au from 169 m |
DDHMA1 |
inc. |
169.00 |
174.00 |
5.00 |
5.18 |
25.9 |
5.00 m @ 5.18 g/t Au from 169 m |
DDHMA2DDHMA2 |
inc. |
90.0094.00 |
103.0095.00 |
13.001.00 |
0.641.92 |
8.41.9 |
13.00 m @ 0.64 g/t Au from 90 m1.00 m @ 1.92 g/t Au from 94 m |
^ All width and intercepts are expressed as
metres downhole rather than true width. Most intersections
tabulated above will have an oblique component. Refer to drill
cross sections and JORC Table 1. Calculated as length weighted
averages. ^^ Au g/t multiplied by metres.
The Never Despair Reef was
intersected at approximately 170 m down-hole in DDHMA1 and is
characterised by a 5m wide zone of silica – sericite altered
sediments with intervals of white, bleached puggy fault material
and laminated quartz veins (Figure 3). Assays returned 6.0
m @ 4.37 g/t Au from 169 m, including 5.0 m @ 5.18
g/t Au across the reef. Strongly elevated arsenic, and
elevated silver, molybdenum and antimony accompany this
interval.
Figure 3, DDHM01 from 169.15 m – 174.9 m. Never
Despair intersection returning 6.0 m @ 4.37 g/t Au
from 169 m. Strongly elevated As, and elevated Ag, Mo, and Sb
accompany this interval.
The Never Despair Reef dips to
the NE and is currently interpreted up to 675 m along strike.
Surface workings are restricted to the central portion of the trend
and along a roughly 200 m section of the Never Despair structure,
in a complex area where multiple reefs with different orientations
converge. Local underground development along the Never Despair
Reef itself is primarily within 30 m of the surface below the
significant surface workings, although additional development along
a 20 m segment of the reef occurs to depths down to 60 m in the
south, where the Never Despair Reef converges at depth with the
adjacent Panama Fault (Figure 2 and Figure 4).
The Butchers Gully Fault was
intersected at shallow depths in several re-logged historic holes,
including: MD02, MD03, MD04 and MD06A; with the best intercepts
reporting 2.0 m @ 7.19 g/t Au from 52 m (including
1.15 m @ 12.01 g/t Au) and 2.0 m @ 3.87
g/t Au from 43 m (including 1.0 m @ 6.92 g/t
Au from 43 m) in MD04; and 3.10 m @ 3.29 g/t
Au from 36 m (including 1.3 m @ 7.26 g/t
Au) in MD06A. Elevated arsenic, bismuth, and antimony
accompany these intervals. This fault typically manifests in
shallow core intervals as a limonite-rich zone, with quartz
fracture veining and intervals of iron and sulphidic tectonic
breccia.
The Butchers Gully Fault is an emerging, +1 km
long target reef that dips sub-vertical to steeply to the northwest
and trends in parallel with the high-grade Leven Star Reef, which
is located roughly 80 m to the southeast (Figure 2 and Figure 4).
Refer to Table 1 (>2-gram x metre) and Appendix 2 (>0.3-gram
x metre) for additional significant intercepts on these drill
holes.
Target NW Fault 4 was
intersected at around 80 m down-hole in MD07 (Figure 4) and is
represented by a limonite rich puggy tectonic fault breccia host
predominantly in silt (Figure 5). A significant gold interval
associated with this structure returned 2.1 m @ 3.82 g/t
Au from 78.9 m, including 0.6 m @ 9.74 g/t
Au. This intercept is bound by a 10 cm section of core
loss between 79.9 m – 80.0 m. Elevated arsenic, antimony, bismuth,
molybdenum and tungsten accompany this interval.
Figure 4, Geological cross section displaying
the portion of drill traces for re-logged holes that fall within
the field of view. Refer to Figure 2 for location of cross section
A – A’. Cross section is north-facing with a +/- 20 m field of
view. Callouts highlight significant intersections > 5-gram x
metre that are captured within the field of view. Refer to Appendix
2 for all significant (> 0.3-gram x metre) for drill holes part
depicted on section.
Target NW Fault 4 represents a
mapped, sub-vertical to steeply west-dipping quartz-bearing
tectonic breccia, which is interpreted over an ~ 320 m strike
length and modelled to interact with the Missing Link Granite
outcrop (Figure 2). Target NW Fault 9 may represent an extension of
NW Fault 4, mapped to the north, which returned 2.0 m @
15.18 g/t Au from 9 m, in previously reported assays for
drill hole BTD0043. Both faults report narrow, high-grade results
and display similar mineralisation styles and multi-element
characteristics. These faults have a combined target strike-length
of ~ 1 km (Figure 2 and Figure 4).
____________________________________3 Refer to
the Company’s news release dated June 4, 2024, released to ASX on
June 5, 2024.
Figure 5, MD07 from 76.9 m – 81.0 m. The
limonite rich puggy fault breccia represents the NW Fault 4
mineralised structure returning 2.1 m @ 3.82 g/t
Au from 78.9 m, including 0.6 m @ 9.74 g/t
Au. Elevated arsenic, antimony, bismuth, molybdenum and
tungsten accompany this interval.
The West Panama Reef was
intersected at around 41 m down-hole in DDHMA1 returning 4.0 m @
0.64 g/t Au from 41.1 m, and at 90 m down-hole in DDHMA2 returning
13 m @ 0.64 g/t Au from 90 m including 1 m
@ 1.92 g/t Au. Elevated arsenic, bismuth, antimony, and
tungsten are associated with this interval. Within DDHMA2 this
fault is represented by strongly silica and sericite altered and
annealed granulestone with well-developed quartz stockwork
veining.
The West Panama Reef is a steep to moderately
steep, NE-dipping structure that is currently interpreted to extend
for ~ 670 m (Figure 2 and Figure 5). Small segments (<10%) of
this reef were explored and developed locally down to a depth of
around 90 m.
BELLTOPPER FORWARD PROGRAM
Current work is focussed on delivering an
exploration target for the dense network of known, emerging and
newly discovered high-grade, epizonal gold-reefs that characterise
the landscape at Belltopper.
Integration of historic, recent and new
exploration data from the current logging and sampling program into
an evolving 3D target model is ongoing and fundamental to effective
targeting. This includes integration of data and interpretation
from the recent hyperspectral sampling program which is currently
being progressed and scheduled to be complete by the end of Q3
2024.
The recent re-logging program, coupled with
previous exploration, have allowed an improved understanding of the
overall prospectivity, mineralisation styles and characteristics,
and key structural controls on the higher-grade zones at
Belltopper. From these learnings, both the extensions to modelled
high-grade zones, along with well understood reefs are targeted; as
well as high-value, emerging shallow and deeper conceptual targets,
which includes both intrusion related mineralisation, and the world
class, Fosterville-style, high-grade epizonal mineralisation, of
which Belltopper displays many of these characteristics.
Authorised for release by the Board of
Directors.
CONTACT
Investors:Mike Spreadborough +61 8 6400 6100
info@novoresources.com |
North American Queries:Leo Karabelas+1 416 543
3120leo@novoresources.com |
Media:Cameron Gilenko+61 466 984
953cameron.gilenko@sodali.com |
QP STATEMENT
Dr. Christopher Doyle (MAIG), is the qualified
person, as defined under National Instrument 43-101 Standards of
Disclosure for Mineral Projects (‘NI 43-101’), responsible for, and
having reviewed and approved, the technical information contained
in this news release. Dr. Doyle is Novo’s Exploration Manager –
Victoria.
There were no limitations to the verification
process and all relevant data and records were reviewed and
verified by a qualified person (as defined in NI 43-101).
JORC COMPLIANCE STATEMENT
The information in this report that relates to
new exploration results at the Belltopper Gold Project is based on
information compiled by Dr. Christopher Doyle, who is a full-time
employee of Novo Resources Corp. Dr. Christopher Doyle is a
Competent Person who is a member of the Australian Institute of
Geoscientists. Dr. Christopher Doyle has sufficient experience that
is relevant to the style of mineralisation and the type of deposits
under consideration and to the activity being undertaken to qualify
as a Competent Person as defined in the 2012 Edition of the
'Australasian Code for Reporting of Exploration Results, Mineral
Resources and Ore Reserves'. Dr. Christopher Doyle consents to the
inclusion in the report of the matters based on her information in
the form and context in which it appears.
The information in this news release that
relates to previously reported exploration results at Belltopper is
extracted from Novo's announcement released to ASX on 5 June 2024
and which is available to view at www.asx.com.au. The Company
confirms that it is not aware of any new information that
materially affects the information included in the original market
announcement and that all material assumptions and technical
parameters underpinning the estimates in the market announcement
continue to apply and have not materially changed.
FORWARD-LOOKING STATEMENTS
Some statements in this news release may contain
“forward-looking statements” within the meaning of Canadian and
Australian securities law and regulations. In this news release,
such statements include but are not limited to planned exploration
activities and the timing of such. These statements address future
events and conditions and, as such, involve known and unknown
risks, uncertainties and other factors which may cause the actual
results, performance or achievements to be materially different
from any future results, performance or achievements expressed or
implied by the statements. Such factors include, without
limitation, customary risks of the resource industry and the risk
factors identified in Novo’s annual information form for the year
ended December 31, 2023 (which is available under Novo’s profile on
SEDAR+ at www.sedarplus.ca and at www.asx.com.au) in the Company’s
prospectus dated 2 August 2023 which is available at
www.asx.com.au. Forward-looking statements speak only as of the
date those statements are made. Except as required by applicable
law, Novo assumes no obligation to update or to publicly announce
the results of any change to any forward-looking statement
contained or incorporated by reference herein to reflect actual
results, future events or developments, changes in assumptions or
changes in other factors affecting the forward-looking statements.
If Novo updates any forward-looking statement(s), no inference
should be drawn that the Company will make additional updates with
respect to those or other forward-looking statements.
ABOUT NOVO
Novo is an Australian based gold explorer listed
on the ASX and the TSX focused on discovering standalone gold
projects with > 1 Moz development potential. Novo is an
innovative gold explorer with a significant land package covering
approximately 6,700 square kilometres in the Pilbara region of
Western Australia, along with the 22 square kilometre Belltopper
project in the Bendigo Tectonic Zone of Victoria, Australia.
Novo’s key project area is the Egina Gold Camp,
where De Grey Mining is farming-in to form a JV at the Becher
Project and surrounding tenements through exploration expenditure
of A$25 million within 4 years for a 50% interest. The Becher
Project has similar geological characteristics as De Grey’s 12.7
Moz Hemi Project1. Novo is also advancing gold exploration at
Nunyerry North, part of the Croydon JV (Novo 70%: Creasy Group
30%), where 2023 exploration drilling identified significant gold
mineralisation. Novo continues to undertake early-stage exploration
across its Pilbara tenement portfolio.
Novo has also formed lithium joint ventures with
both Liatam and SQM in the Pilbara which provides shareholder
exposure to battery metals.
Novo has a significant investment portfolio and
a disciplined program in place to identify value accretive
opportunities that will build further value for shareholders.
Please refer to Novo’s website for further
information including the latest corporate presentation.
1. Refer to De Grey ASX Announcement, Hemi Gold
Project Resource Update, dated 21 November 2023. No assurance can
be given that a similar {or any) commercially mineable deposit will
be determined at Novo’s Becher project.
APPENDIX 1: BELLTOPPER DRILL COLLARS
Hole ID |
HoleType |
Depth(m) |
Easting |
Northing |
RLAHD(m) |
CollarDip (°) |
CollarAzimuth(MGA9455) (°) |
CollarAzimuth(Mag) (°) |
Company |
Datecompleted |
BTD001 |
DD |
323.7 |
263866.02 |
5880369.85 |
524.18 |
-66 |
128.484 |
118.984 |
NOVO |
28-Nov-23 |
BTD002 |
DD |
594 |
263701.31 |
5881202.77 |
457.18 |
-60 |
145.117 |
135.617 |
NOVO |
21-Dec-23 |
BTD003 |
DD |
389.7 |
264162.29 |
5880827.97 |
489.97 |
-51.05 |
135.07 |
125.57 |
NOVO |
18-Jan-24 |
BTD004 |
DD |
521 |
263530.06 |
5880820.71 |
471.69 |
-45 |
90.23 |
80.73 |
NOVO |
08-Feb-24 |
BTD005 |
DD |
299.9 |
263394.65 |
5880825.96 |
471.94 |
-50 |
90.495 |
80.995 |
NOVO |
19-Feb-24 |
BTD006 |
DD |
400.6 |
263263.53 |
5880606.13 |
470.22 |
-37.88 |
144.53 |
135.03 |
NOVO |
08-Jan-87 |
MD01 |
DD |
352.2 |
263787.47 |
5880326.69 |
526.36 |
-57 |
144.5 |
135 |
GBM |
20-Dec-07 |
MD02 |
DD |
262 |
263787.42 |
5880326.77 |
526.39 |
-50 |
144.5 |
135 |
GBM |
10-Jan-08 |
MD03 |
DD |
478.5 |
263787.36 |
5880326.85 |
526.39 |
-65 |
144.5 |
135 |
GBM |
01-Nov-08 |
MD04 |
DD |
255 |
263788.00 |
5880328.62 |
526.37 |
-51.5 |
124.5 |
115 |
GBM |
26-Jan-08 |
MD05 |
DD |
266.9 |
263785.35 |
5880325.81 |
526.34 |
-50 |
166.5 |
157 |
GBM |
08-Feb-08 |
MD06A |
DD |
426.8 |
263785.10 |
5880326.89 |
526.36 |
-66 |
165.5 |
156 |
GBM |
24-Feb-08 |
MD07 |
DD |
249 |
263783.43 |
5880326.00 |
526.32 |
-55.5 |
239.5 |
230 |
GBM |
03-Mar-08 |
MD08 |
DD |
241.2 |
263575.14 |
5880074.01 |
434.02 |
-54.9 |
134.7 |
125.2 |
GBM |
09-Apr-08 |
MD08A |
DD |
450.3 |
263574.36 |
5880074.15 |
434.05 |
-55.5 |
134.5 |
125 |
GBM |
02-May-08 |
MD09 |
DD |
259.8 |
263573.87 |
5880074.24 |
434.07 |
-65.9 |
134.5 |
125 |
GBM |
12-May-08 |
MD10 |
DD |
191.3 |
263680.28 |
5878848.91 |
475.87 |
-60 |
254.5 |
245 |
GBM |
25-May-08 |
MD11 |
DD |
261 |
263680.66 |
5878849.04 |
475.87 |
-70 |
259.3 |
249.8 |
GBM |
05-Jun-08 |
MD12 |
DD |
999.8 |
263587.00 |
5880641.00 |
471.52 |
-85.5 |
279.5 |
270 |
GBM |
17-Mar-10 |
MD13 |
DD |
112.4 |
263795.58 |
5880084.40 |
457.50 |
-30 |
315 |
305.5 |
GBM |
23-Dec-21 |
MD14 |
DD |
365.5 |
263797.55 |
5880078.04 |
456.24 |
-50 |
270 |
260.5 |
GBM |
24-Jan-22 |
MD15 |
DD |
131.2 |
263853.37 |
5880118.38 |
452.71 |
-50 |
315 |
305.5 |
GBM |
03-Feb-22 |
MD16 |
DD |
204 |
263921.11 |
5880337.81 |
518.16 |
-73 |
135 |
125.5 |
GBM |
15-Feb-22 |
MD17 |
DD |
380 |
263849.25 |
5880561.10 |
523.92 |
-50 |
265 |
255.5 |
GBM |
09-Mar-22 |
MD18 |
DD |
320 |
263569.06 |
5880639.13 |
470.11 |
-50 |
260 |
250.5 |
GBM |
29-Mar-22 |
MD18A |
DD |
35 |
263569.46 |
5880639.23 |
470.13 |
-50 |
260 |
250.5 |
GBM |
30-Mar-22 |
MD19 |
DD |
553.9 |
263831.60 |
5879274.76 |
472.01 |
-50 |
260 |
250.5 |
GBM |
03-May-22 |
MD20 |
DD |
551.4 |
263828.50 |
5878871.91 |
477.38 |
-58 |
260 |
250.5 |
GBM |
07-Jun-22 |
MD21 |
DD |
255.5 |
263959.98 |
5880254.29 |
481.10 |
-68.4 |
318.6 |
309.1 |
GBM |
27-Jun-22 |
MD22 |
DD |
252.8 |
263587.28 |
5880638.16 |
471.78 |
-45.9 |
93.9 |
84.4 |
GBM |
10-Jul-22 |
LSRC1 |
RC |
87 |
264059.03 |
5880480.22 |
492.41 |
-60 |
135.5 |
126 |
Eureka |
20-Aug-94 |
LSRC2 |
RC |
111 |
264004.09 |
5880453.50 |
495.34 |
-55 |
135.5 |
126 |
Eureka |
22-Aug-94 |
LSRC3 |
RC |
111 |
263987.44 |
5880430.88 |
498.14 |
-55 |
135.5 |
126 |
Eureka |
26-Aug-94 |
LSRC4 |
RC |
110 |
263977.25 |
5880409.48 |
501.61 |
-55 |
135.5 |
126 |
Eureka |
27-Aug-94 |
LSRC5 |
RC |
110 |
263960.40 |
5880390.00 |
507.44 |
-55 |
135.5 |
126 |
Eureka |
28-Aug-94 |
LSRC6 |
RC |
70 |
263993.79 |
5880335.47 |
496.58 |
-56 |
315.5 |
306 |
Eureka |
29-Aug-94 |
LSRC7 |
RC |
105 |
263989.42 |
5880302.66 |
491.44 |
-55 |
315.5 |
306 |
Eureka |
29-Aug-94 |
LSRC8 |
RC |
112 |
263960.64 |
5880254.82 |
481.32 |
-55 |
315.5 |
306 |
Eureka |
30-Aug-94 |
LSRC9 |
RC |
73 |
263888.69 |
5880235.61 |
474.55 |
-60 |
315.5 |
306 |
Eureka |
01-Sep-94 |
LSRC10 |
RC |
112 |
263860.81 |
5880200.34 |
469.75 |
-55 |
315.5 |
306 |
Eureka |
04-Sep-94 |
LSRC11 |
RC |
96 |
263857.09 |
5880170.10 |
463.53 |
-55 |
315.5 |
306 |
Eureka |
05-Sep-94 |
LSRC12 |
RC |
82 |
263852.64 |
5880119.70 |
452.86 |
-50 |
315.5 |
306 |
Eureka |
07-Sep-94 |
LSRC13 |
RC |
118 |
263828.12 |
5880095.91 |
454.24 |
-50 |
315.5 |
306 |
Eureka |
08-Sep-94 |
LSRC14 |
RC |
100 |
263798.14 |
5880084.18 |
456.59 |
-50 |
315.5 |
306 |
Eureka |
09-Sep-94 |
LSRC15 |
RC |
100 |
263926.07 |
5880344.94 |
517.80 |
-50 |
135.5 |
126 |
Eureka |
11-Sep-94 |
LSRC16/D14 |
RC/DD |
101.1 |
263908.39 |
5880335.61 |
518.96 |
-60 |
135.5 |
126 |
Eureka |
23-Sep-94 |
LSRC17/D15 |
RC/DD |
84 |
263909.51 |
5880334.60 |
518.75 |
-50 |
135.5 |
126 |
Eureka |
03-Oct-94 |
HMDDH1 |
DD |
180.7 |
263933.48 |
5880659.32 |
512.75 |
-50 |
279.5 |
270 |
Pittson |
16-Dec-91 |
HMDDH2 |
DD |
70 |
263872.24 |
5880377.30 |
523.19 |
-50 |
99.5 |
90 |
Pittson |
22-Dec-91 |
HMDDH3 |
DD |
176.5 |
263853.66 |
5880488.54 |
526.55 |
-50 |
279.5 |
270 |
Pittson |
31-Dec-91 |
LSDDH1 |
DD |
100.6 |
263942.09 |
5880228.14 |
474.18 |
-50 |
311.5 |
302 |
Pittson |
01-May-90 |
LSDDH2 |
DD |
162.4 |
263942.09 |
5880228.14 |
474.18 |
-65 |
311.5 |
302 |
Pittson |
09-May-90 |
LSDDH3 |
DD |
110.4 |
263894.70 |
5880179.43 |
450.94 |
-50 |
311.5 |
302 |
Pittson |
13-May-90 |
LSDDH4 |
DD |
49.5 |
263989.89 |
5880343.02 |
500.13 |
-55 |
311.5 |
302 |
Pittson |
15-May-90 |
LSDDH5 |
DD |
140.7 |
264045.76 |
5880359.72 |
473.23 |
-65 |
311.5 |
302 |
Pittson |
18-May-90 |
LSDDH6 |
DD |
60.5 |
264073.00 |
5880423.93 |
476.30 |
-55 |
311.5 |
302 |
Pittson |
19-May-90 |
LSDDH7 |
DD |
333 |
263977.71 |
5880144.28 |
431.21 |
-60 |
311.5 |
302 |
Pittson |
03-May-91 |
LSDDH8 |
DD |
199 |
263799.51 |
5880084.94 |
457.06 |
-62 |
311.5 |
302 |
Pittson |
12-May-91 |
LSDDH9 |
DD |
201 |
263894.14 |
5880430.78 |
517.00 |
-50 |
141.5 |
132 |
Pittson |
18-May-91 |
LSDDH10 |
DD |
98.5 |
264192.32 |
5880515.60 |
501.26 |
-55 |
310.5 |
301 |
Pittson |
23-May-91 |
LSDDH11 |
DD |
9 |
264114.83 |
5880499.34 |
496.16 |
-52.5 |
303.5 |
294 |
Pittson |
23-May-91 |
LSDDH12 |
DD |
106.2 |
264319.66 |
5880637.86 |
487.26 |
-55 |
319.5 |
310 |
Pittson |
28-May-91 |
LSDDH13 |
DD |
247.8 |
264007.53 |
5880606.35 |
499.33 |
-50 |
131.5 |
122 |
Pittson |
08-Jun-91 |
DDHMA1 |
DD |
298.6 |
263526.83 |
5880314.86 |
431.11 |
-45 |
74.5 |
65 |
Molopo |
18-Jan-87 |
DDHMA2 |
DD |
182.3 |
263489.40 |
5880328.73 |
433.31 |
-45 |
74.5 |
65 |
Molopo |
28-Jan-87 |
DDHMA3 |
DD |
260.65 |
263688.97 |
5880516.92 |
499.41 |
-53 |
244.5 |
235 |
Molopo |
11-Feb-87 |
All drill collars are reported in MGA94 Zone 55. All collars are
located within Retention Licence RL006587
APPENDIX 2: BELLTOPPER RELOGGING
SIGNIFICANT INTERSECTIONS
Standard Intercepts calculated with 0.3 g/t Au
cut-off and 2 m internal dilution. High grade included intercepts
calculated with 1.0 g/t Au and no internal dilution.
^ All width and intercepts are expressed as
metres downhole rather than true width. Calculated as length
weighted averages.
^^ Au g/t multiplied by metres.
Logged core loss treated as 0 g/t Au grade in
all calculations. The gold assay of a primary sample from a
duplicate pair will be used in all calculations. Any isolated gold
intersections separated by internal dilution must independently be
above the average cut-off grade when including the grades of the
internal dilution.
All new or updated significant
intersections > 0.3 GM from recent relogging and sampling
exercise
Drill Hole |
Including |
From(m) |
To(m) |
Interval(m) ^ |
Au (g/t) |
Au g*m ^^ |
Intersection |
MD02 |
|
42.00 |
43.00 |
1.00 |
0.44 |
0.4 |
1.00 m @ 0.44 g/t Au from 42 m |
MD02 |
|
75.40 |
77.00 |
1.60 |
0.33 |
0.5 |
1.60 m @ 0.33 g/t Au from 75.4 m |
MD02 |
|
83.00 |
85.00 |
2.00 |
0.58 |
1.2 |
2.00 m @ 0.58 g/t Au from 83 m |
MD02 |
|
141.00 |
142.00 |
1.00 |
0.47 |
0.5 |
1.00 m @ 0.47 g/t Au from 141 m |
MD03 |
|
14.00 |
19.00 |
5.00 |
0.55 |
2.7 |
5.00 m @ 0.55 g/t Au from 14 m |
MD03 |
|
22.00 |
23.00 |
1.00 |
0.39 |
0.4 |
1.00 m @ 0.39 g/t Au from 22 m |
MD03 |
|
27.00 |
28.00 |
1.00 |
0.44 |
0.4 |
1.00 m @ 0.44 g/t Au from 27 m |
MD03 |
|
31.00 |
32.00 |
1.00 |
0.34 |
0.3 |
1.00 m @ 0.34 g/t Au from 31 m |
MD03 |
|
36.00 |
37.00 |
1.00 |
0.43 |
0.4 |
1.00 m @ 0.43 g/t Au from 36 m |
MD03 |
|
45.00 |
47.00 |
2.00 |
1.80 |
3.6 |
2.00 m @ 1.80 g/t Au from 45 m |
MD03 |
|
129.90 |
131.00 |
1.10 |
0.38 |
0.4 |
1.10 m @ 0.38 g/t Au from 129.9 m |
MD04 |
|
15.00 |
16.00 |
1.00 |
0.38 |
0.4 |
1.00 m @ 0.38 g/t Au from 15 m |
MD04 |
|
43.00 |
45.00 |
2.00 |
3.87 |
7.7 |
2.00 m @ 3.87 g/t Au from 43 m |
MD04 |
inc. |
43.00 |
44.00 |
1.00 |
6.92 |
6.9 |
1.00 m @ 6.92 g/t Au from 43 m |
MD04 |
|
50.00 |
51.00 |
1.00 |
0.31 |
0.3 |
1.00 m @ 0.31 g/t Au from 50 m |
MD04 |
|
52.00 |
54.00 |
2.00 |
7.19 |
14.4 |
2.00 m @ 7.19 g/t Au from 52 m |
MD04 |
inc. |
52.00 |
53.15 |
1.15 |
12.01 |
13.8 |
1.15 m @ 12.01 g/t Au from 52 m |
MD04 |
|
81.00 |
82.00 |
1.00 |
0.33 |
0.3 |
1.00 m @ 0.33 g/t Au from 81 m |
MD04 |
|
109.00 |
110.00 |
1.00 |
1.90 |
1.9 |
1.00 m @ 1.90 g/t Au from 109 m |
MD06A |
|
28.50 |
30.00 |
1.50 |
0.35 |
0.5 |
1.50 m @ 0.35 g/t Au from 28.5 m |
MD06A |
|
32.00 |
32.80 |
0.80 |
1.06 |
0.9 |
0.80 m @ 1.06 g/t Au from 32 m |
MD06A |
|
36.00 |
39.10 |
3.10 |
3.29 |
10.2 |
3.10 m @ 3.29 g/t Au from 36 m |
MD06A |
inc. |
37.30 |
38.60 |
1.30 |
7.26 |
9.4 |
1.30 m @ 7.26 g/t Au from 37.3 m |
MD06A |
|
173.75 |
174.08 |
0.33 |
0.36 |
0.1 |
0.33 m @ 0.36 g/t Au from 173.75 m |
MD06A |
|
350.00 |
351.00 |
1.00 |
0.30 |
0.3 |
1.00 m @ 0.30 g/t Au from 350 m |
MD06A |
|
409.73 |
410.03 |
0.30 |
0.40 |
0.1 |
0.30 m @ 0.40 g/t Au from 409.73 m |
MD06A |
|
420.00 |
425.50 |
5.50 |
0.70 |
3.9 |
5.50 m @ 0.70 g/t Au from 420 m |
MD06A |
inc. |
423.50 |
424.40 |
0.90 |
1.17 |
1.1 |
0.90 m @ 1.17 g/t Au from 423.5 m |
MD06A |
inc. |
425.10 |
425.50 |
0.40 |
1.08 |
0.4 |
0.40 m @ 1.08 g/t Au from 425.1 m |
MD07 |
|
25.00 |
30.00 |
5.00 |
0.69 |
3.4 |
5.00 m @ 0.69 g/t Au from 25 m |
MD07 |
inc. |
26.00 |
26.70 |
0.70 |
1.33 |
0.9 |
0.70 m @ 1.33 g/t Au from 26 m |
MD07 |
|
53.90 |
55.00 |
1.10 |
0.85 |
0.9 |
1.10 m @ 0.85 g/t Au from 53.9 m |
MD07 |
|
78.90 |
81.00 |
2.10 |
3.82 |
8.0 |
2.10 m @ 3.82 g/t Au from 78.9 m |
MD07 |
inc. |
79.30 |
79.90 |
0.60 |
9.74 |
5.8 |
0.60 m @ 9.74 g/t Au from 79.3 m |
MD07 |
inc. |
80.00 |
81.00 |
1.00 |
1.59 |
1.6 |
1.00 m @ 1.59 g/t Au from 80 m |
MD07 |
|
114.80 |
116.90 |
2.10 |
0.51 |
1.1 |
2.10 m @ 0.51 g/t Au from 114.8 m |
MD07 |
|
154.00 |
155.60 |
1.60 |
1.22 |
2.0 |
1.60 m @ 1.22 g/t Au from 154 m |
MD07 |
inc. |
155.00 |
155.60 |
0.60 |
2.33 |
1.4 |
0.60 m @ 2.33 g/t Au from 155 m |
MD08 |
|
202.00 |
203.00 |
1.00 |
0.72 |
0.7 |
1.00 m @ 0.72 g/t Au from 202 m |
MD08 |
|
206.00 |
207.00 |
1.00 |
0.38 |
0.4 |
1.00 m @ 0.38 g/t Au from 206 m |
MD08 |
|
222.52 |
223.42 |
0.90 |
0.35 |
0.3 |
0.90 m @ 0.35 g/t Au from 222.52 m |
MD08A |
|
114.21 |
114.60 |
0.39 |
2.44 |
1.0 |
0.39 m @ 2.44 g/t Au from 114.21 m |
MD08A |
|
123.00 |
125.00 |
2.00 |
1.60 |
3.2 |
2.00 m @ 1.60 g/t Au from 123 m |
MD08A |
inc. |
124.00 |
125.00 |
1.00 |
2.30 |
2.3 |
1.00 m @ 2.30 g/t Au from 124 m |
MD08A |
|
134.00 |
135.00 |
1.00 |
0.61 |
0.6 |
1.00 m @ 0.61 g/t Au from 134 m |
MD08A |
|
152.78 |
153.09 |
0.31 |
0.35 |
0.1 |
0.31 m @ 0.35 g/t Au from 152.78 m |
MD08A |
|
173.05 |
174.00 |
0.95 |
0.42 |
0.4 |
0.95 m @ 0.42 g/t Au from 173.05 m |
MD08A |
|
285.00 |
285.44 |
0.44 |
0.71 |
0.3 |
0.44 m @ 0.71 g/t Au from 285 m |
MD08A |
|
291.03 |
292.00 |
0.97 |
0.40 |
0.4 |
0.97 m @ 0.40 g/t Au from 291.03 m |
MD08A |
|
298.00 |
298.70 |
0.70 |
0.61 |
0.4 |
0.70 m @ 0.61 g/t Au from 298 m |
MD08A |
|
301.00 |
302.00 |
1.00 |
0.63 |
0.6 |
1.00 m @ 0.63 g/t Au from 301 m |
MD08A |
|
342.88 |
344.00 |
1.12 |
0.32 |
0.4 |
1.12 m @ 0.32 g/t Au from 342.88 m |
MD08A |
|
422.00 |
423.00 |
1.00 |
0.87 |
0.9 |
1.00 m @ 0.87 g/t Au from 422 m |
LSDDH7 |
|
196.40 |
197.40 |
1.00 |
3.41 |
3.4 |
1.00 m @ 3.41 g/t Au from 196.4 m |
DDHMA1 |
|
20.60 |
22.00 |
1.40 |
0.31 |
0.4 |
1.40 m @ 0.31 g/t Au from 20.6 m |
DDHMA1 |
|
41.10 |
45.10 |
4.00 |
0.64 |
2.6 |
4.00 m @ 0.64 g/t Au from 41.1 m |
DDHMA1 |
|
62.40 |
63.40 |
1.00 |
0.89 |
0.9 |
1.00 m @ 0.89 g/t Au from 62.4 m |
DDHMA1 |
|
146.00 |
148.00 |
2.00 |
0.30 |
0.6 |
2.00 m @ 0.30 g/t Au from 146 m |
DDHMA1 |
|
157.95 |
158.80 |
0.85 |
0.43 |
0.4 |
0.85 m @ 0.43 g/t Au from 157.95 m |
DDHMA1 |
|
169.00 |
175.00 |
6.00 |
4.37 |
26.2 |
6.00 m @ 4.37 g/t Au from 169 m |
DDHMA1 |
inc. |
169.00 |
174.00 |
5.00 |
5.18 |
25.9 |
5.00 m @ 5.18 g/t Au from 169 m |
DDHMA1 |
|
176.00 |
177.00 |
1.00 |
0.34 |
0.3 |
1.00 m @ 0.34 g/t Au from 176 m |
DDHMA2 |
|
8.60 |
10.10 |
1.50 |
0.60 |
0.9 |
1.50 m @ 0.60 g/t Au from 8.6 m |
DDHMA2 |
|
90.00 |
103.00 |
13.00 |
0.64 |
8.4 |
13.00 m @ 0.64 g/t Au from 90 m |
DDHMA2 |
inc. |
94.00 |
95.00 |
1.00 |
1.92 |
1.9 |
1.00 m @ 1.92 g/t Au from 94 m |
DDHMA2 |
|
105.00 |
106.00 |
1.00 |
0.34 |
0.3 |
1.00 m @ 0.34 g/t Au from 105 m |
DDHMA2 |
|
115.00 |
116.00 |
1.00 |
0.50 |
0.5 |
1.00 m @ 0.50 g/t Au from 115 m |
DDHMA2 |
|
118.00 |
119.10 |
1.10 |
0.41 |
0.5 |
1.10 m @ 0.41 g/t Au from 118 m |
DDHMA2 |
|
148.00 |
150.00 |
2.00 |
0.37 |
0.7 |
2.00 m @ 0.37 g/t Au from 148 m |
DDHMA2 |
|
156.00 |
157.00 |
1.00 |
0.40 |
0.4 |
1.00 m @ 0.40 g/t Au from 156 m |
DDHMA2 |
|
168.00 |
169.00 |
1.00 |
0.82 |
0.8 |
1.00 m @ 0.82 g/t Au from 168 m |
DDHMA3 |
|
2.00 |
3.00 |
1.00 |
0.40 |
0.4 |
1.00 m @ 0.40 g/t Au from 2 m |
DDHMA3 |
|
52.30 |
53.30 |
1.00 |
0.40 |
0.4 |
1.00 m @ 0.40 g/t Au from 52.3 m |
DDHMA3 |
|
94.00 |
98.00 |
4.00 |
0.38 |
1.5 |
4.00 m @ 0.38 g/t Au from 94 m |
DDHMA3 |
|
99.00 |
100.00 |
1.00 |
0.36 |
0.4 |
1.00 m @ 0.36 g/t Au from 99 m |
DDHMA3 |
|
103.00 |
105.00 |
2.00 |
0.48 |
1.0 |
2.00 m @ 0.48 g/t Au from 103 m |
DDHMA3 |
|
110.00 |
111.00 |
1.00 |
0.75 |
0.8 |
1.00 m @ 0.75 g/t Au from 110 m |
DDHMA3 |
|
112.00 |
113.00 |
1.00 |
0.31 |
0.3 |
1.00 m @ 0.31 g/t Au from 112 m |
DDHMA3 |
|
116.00 |
120.20 |
4.20 |
0.44 |
1.8 |
4.20 m @ 0.44 g/t Au from 116 m |
DDHMA3 |
|
122.30 |
124.30 |
2.00 |
0.38 |
0.8 |
2.00 m @ 0.38 g/t Au from 122.3 m |
DDHMA3 |
|
133.30 |
134.40 |
1.10 |
0.43 |
0.5 |
1.10 m @ 0.43 g/t Au from 133.3 m |
DDHMA3 |
|
135.60 |
136.10 |
0.50 |
0.40 |
0.2 |
0.50 m @ 0.40 g/t Au from 135.6 m |
DDHMA3 |
|
148.00 |
148.75 |
0.75 |
0.45 |
0.3 |
0.75 m @ 0.45 g/t Au from 148 m |
DDHMA3 |
|
152.60 |
153.10 |
0.50 |
2.22 |
1.1 |
0.50 m @ 2.22 g/t Au from 152.6 m |
DDHMA3 |
|
207.00 |
208.75 |
1.75 |
0.65 |
1.1 |
1.75 m @ 0.65 g/t Au from 207 m |
DDHMA3 |
inc. |
207.00 |
207.50 |
0.50 |
1.19 |
0.6 |
0.50 m @ 1.19 g/t Au from 207 m |
JORC Code, 2012 Edition – Table 1
Belltopper Gold Project
Section 1 Sampling Techniques and Data
(Criteria in this section apply to all succeeding sections.)
Criteria |
JORC Code explanation |
Commentary |
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.
- In cases where ‘industry standard’ work has been done this
would be relatively simple (eg ‘reverse circulation drilling was
used to obtain 1 m samples from which 3 kg was pulverised to
produce a 30 g charge for fire assay’). In other cases more
explanation may be required, such as where there is coarse gold
that has inherent sampling problems. Unusual commodities or
mineralisation types (eg submarine nodules) may warrant disclosure
of detailed information.
|
- All drill holes within the Belltopper Project were drilled as
either diamond or reverse circulation holes. The detail of the
various phases of drilling are discussed under drilling technique
in the section below.
- Details of sampling and assay methods are discussed in the
sections below under the headings sub-sampling techniques and
sample preparation and quality of assay data and laboratory tests
respectively.
|
Criteria |
JORC Code explanation |
Commentary |
Drilling techniques |
- Drill type (eg core, reverse circulation, open-hole hammer,
rotary air blast, auger, Bangka, sonic, etc) and details (eg core
diameter, triple or standard tube, depth of diamond tails,
face-sampling bit or other type, whether core is oriented and if
so, by what method, etc).
|
- Drilling at the Belltopper Project includes both diamond
drilling (DD) (88.83%) and reverse circulation drilling (RC)
(11.17% of drilling) across nine phases of drilling:
|
|
|
Summary of Belltopper Drilling |
|
|
PhasesofDrilling |
Holes |
Type |
Company |
Year |
HoleCount |
TotalMetres |
MaxDepth(m) |
% ofdrilling |
|
|
BTD Series |
BTD001-BTD006 |
DD |
Novo |
2024 |
6 |
2528.9 |
594 |
16.80% |
|
|
MD Series |
MD13-MD22 |
DD |
Novo/GBM |
2022 |
11 |
3161.7 |
553.9 |
21.00% |
|
|
MD12 |
DD |
GBM |
2010 |
1 |
999.8 |
999.8 |
6.64% |
|
|
MD1-MD11 |
DD |
GBM |
2008 |
12 |
3694 |
478.5 |
24.54% |
|
|
LSRC/D Series |
LSRC16/D14, LSRC17/D15 |
RC with DD Tails |
Eureka |
1994 |
2 |
185.1 |
101.1 |
1.23% |
|
|
LSRC Series |
LSRC1-LSRC15 |
RC |
Eureka |
1994 |
15 |
1497 |
118 |
9.94% |
|
|
HMDDH Series |
HMDDH1-HMDDH3 |
DD |
Pittson |
1992 |
3 |
427.2 |
180.7 |
2.84% |
|
|
LSDDH Series |
LSDDH1-LSDDH13 |
DD |
Pittson |
1990 |
13 |
1818.6 |
333 |
12.08% |
|
|
DDHMA Series |
DDHMA1-DDHMA2 |
DD |
Molopo |
1987 |
3 |
741.55 |
298.6 |
4.93% |
|
|
|
|
|
|
Total |
66 |
15053.85 |
|
100% |
|
|
Max Depth
- MD12 is the deepest DD hole from the project at 999.8 m. The
deepest RC hole was drilled to 118 m. The overall average hole
depth from Belltopper is 228 m.
Drill Method
- All diamond drilling utilised standard wireline drilling
methods.
- The MD Series (MD13-MD22) was drilled with triple tube HQ3 and
NQ3 core diameter, all other drill phases were drilled with
conventional HQ core (63.5 mm diameter) from surface with
occasional NQ or NQ2 Core tails.
Core Orientation
- All diamond core from the MD Series onwards was orientated to
varying degrees. The BTD series utilised a REFLEX ACT III™ digital
core orientation system, while DD core from the MD13-MD22 series
was orientated with a Boort Longyear TruCore™ orientation tool.
Earlier DD core used varying methods of core orientation including
a traditional spear method. Bedding and key foliation relationships
are well understood and were often used to calibrate the
orientation of drill core.
|
Criteria |
JORC Code explanation |
Commentary |
Drill sample recovery |
- Method of recording and assessing core and chip sample
recoveries and results assessed.
- Measures taken to maximise sample recovery and ensure
representative nature of the samples.
- Whether a relationship exists between sample recovery and grade
and whether sample bias may have occurred due to preferential
loss/gain of fine/coarse material.
|
- Diamond core recovery was recorded in logs run by run and, in
general, core loss greater than or equal to 0.2 m was recorded in
geological logs. Core loss zones were treated as zero grade in any
significant intersection calculation.
- Drilling recovery data for RC drilling is recorded in drill
logs as good, medium or poor with recovery generally considered by
the geologist logging as ‘good’.
|
|
|
|
Summary of drilling recovery |
|
|
|
|
|
% Recovery |
|
|
|
|
BTD Series |
99.6 |
|
|
|
|
MD Series |
95.4 |
|
|
|
|
HMDDH Series |
90.7 |
|
|
|
|
LSRC/D Series |
99.6 |
|
|
|
|
LSRC Series |
Good |
|
|
|
|
DDHMA Series |
Good |
|
|
|
|
|
|
- The sampling methods utilised are appropriate and
representative of the of the drilled ground.
- Particularly in historical drilling, occasional core loss was
observed within ore zones. More recent drilling efforts focused on
ensuring good recovery in these zones.
- Significant sample bias or “High grading” due to any core loss
has not been observed.
|
Criteria |
JORC Code explanation |
Commentary |
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.
- Whether logging is qualitative or quantitative in nature. Core
(or costean, channel, etc) photography.
- The total length and percentage of the relevant intersections
logged.
|
- All diamond drill core was washed and metre-marked, orientated
(where appropriate), and then selectively logged for geotechnical
parameters (RQD, recovery and rock strength), lithology,
mineralisation, weathering, alteration, quartz vein style and
percentage and number of quartz veins per metre. Later core logging
( BTD and MD series and relogging of historic core) included
measurements for magnetic susceptibility, and representative
density measurements. Additional comments relating to specific
mineralised intervals were added once assays were received.
- Since 2020, many of the historic drilled DD holes have been
relogged and infill sampled to ensure consistent interpretation of
key features and the identification of any previously missed
mineralised zones.
- Both wet and dry photographs are available for all MD and BTD
series holes and for the vast majority of historic core.
- All logging is of a standard that allows identification and
interpretation of key geological features to a level appropriate to
support a possible mineral resource estimation in the future.
|
Sub-sampling techniques and sample
preparation |
- If core, whether cut or sawn and whether quarter, half or all
core taken.
- If non-core, whether riffled, tube sampled, rotary split, etc
and whether sampled wet or dry.
- For all sample types, the nature, quality and appropriateness
of the sample preparation technique.
- Quality control procedures adopted for all sub-sampling stages
to maximise representivity of samples.
- Measures taken to ensure that the sampling is representative of
the in situ material collected, including for instance results for
field duplicate/second-half sampling.
- Whether sample sizes are appropriate to the grain size of the
material being sampled.
|
- DD core was sampled by cutting it using a diamond saw
longitudinally in half. Samples were cut to geological boundaries
or to a preferred length of 1.0 m. Where a core orientation line
was present, core was cut 2 cm to the left of the line (when
looking down hole). When no cut line was present, core was cut
longitudinally down the apex line of the most prominent geological
feature (such as bedding or vein boundaries). Once cut, the upper
half of core (left side of the tray when looking down hole) is
placed in a pre-labelled calico bag and dispatched for analysis.
The lower half of core is returned to the core tray in its original
orientation.
- In general, sample intervals ranged from 0.3 m to 1.3 m.
- RC samples (LSRC series) were split using a Jones riffle
splitter to a nominal 3-5 kg sample weight.
- Field duplicates were representative of the original primary
pair either as a quarter core duplicate or RC riffle-split
duplicate.
- Once at the laboratory, all sample material was crushed and
pulverized prior to analysis. Samples from the BTD and MD13-MD22
Series were coarse crushed using the ALS method CRU-21 and
pulverise up to 3 kg to 85 % passing 75 microns (ALS Method
PUL-23).
- The sampling methods and sample sizes are appropriate to the
style of mineralisation (fine-grained free gold, fine grained
disseminated auriferous sulphides or the oxidized
equivalents).
|
Criteria |
JORC Code explanation |
Commentary |
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.
- For geophysical tools, spectrometers, handheld XRF instruments,
etc, the parameters used in determining the analysis including
instrument make and model, reading times, calibrations factors
applied and their derivation, etc.
- 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.
|
Assay Method
- For the recent BTD series, drilling of MD13-MD22, MD12 and any
recent infill sampling of historic holes, samples have been
submitted to ALS Laboratories Adelaide for analysis using the
methods described below:
- Gold was analysed with a 50 g ore grade (DL of 0.01 g/t Au) Au
fire assay and an atomic absorption spectroscopy (AAS) finish (ALS
Method Au-AA26). Original assaying of MD12 used trace level (DL of
0.001 g/t Au) ALS Lab Method Au-AA21 with a nominal 30 g sample
weight.
- Multielement geochemistry was analysed for a suite of 48
elements obtained by a four-acid near-total digestion with a
combination of Inductively coupled plasma (ICP) Mass Spectrometry
(MS) and Atomic Emission Spectroscopy (AES) finish on a 0.25 g pulp
sample (ALS Lab Method ME-MS61).
- Samples from GBM MD01 to MD11 series holes were originally
assayed at Amdel Laboratories in Adelaide
- Gold was analysed with Fire Assay method FA1 (DL of 0.01 g/t
Au)
- Multielement geochemistry was analysed with method IC3E using a
sample of up to 0.2 g of the analytical pulp digested using a
HF/multi acid digest, with solution presented for analysis with ICP
Optical Emission Spectroscopy (OES).
- Samples from original LSRC, LSRC/D, LSDDH and HMDDH series
utilised ALS lab method PM203 for gold analysis (DL of 0.02 g/t Au)
based on the aqua regia digestion of a 50 g charge and a fire assay
with an Atomic Absorption Spectroscopy (AAS) finish.
- The original lab method for DDHMA series holes could not be
determined with confidence. Any gold assay of significant grade
(0.1 g/t Au) has been resampled using the same lab method as used
by the BTD series (Au-AA26 and ME-MS61).
- All assays were performed at external laboratories.
- A portable XRF available on site during recent drilling has
only been used to assist with mineral identification.
QAQC Method
- For the recent BTD series drilling, drilling of MD13-MD22 and
any recent infill sampling of historic holes (Includes earlier MD,
LSDDH DDHMA series holes), staff used an industry accepted QAQC
methodology incorporating blind field duplicates, blanks, and
certified reference materials (CRM) standards. Standards and blanks
were inserted at a rate of four each per hundred samples (see
Standard ID table) and field duplicates were inserted at a nominal
rate of four per hundred with geologist discretion for duplicate
placement.
|
|
|
|
Table of CRM standard insertion rate |
|
|
|
|
Standard ID |
Sample ID ending in |
|
|
|
|
OREAS 232 |
33, 83 |
|
|
|
|
OREAS 239 or OREAS 232b |
58 |
|
|
|
|
OREAS 264 |
08 |
|
|
|
|
BLANK OREAS C26d Or OREAS C26e |
16, 41, 66, 91 |
|
|
|
|
|
|
- Laboratory QAQC involves the use of internal lab standards
using certified reference material, blanks, splits and replicates
as part of the in-house procedures.
- QAQC insertion rates for early-stage drilling are in line with
industry standards at the time.
- The LSRC series included the insertion of field blanks and
standards at a rate of approximately 5 per 100 samples and
conducted riffle split field duplicates nominally at 20 to 30 m
intervals.
- Original LSDDH and HMDDH series sampling included the insertion
of approximately 12 % field duplicates and the occasional insertion
of field blanks and standards.
- No QAQC assay data was reported with original DDHMA series
samples.
- No issues of concern were identified in a comprehensive review
of QAQC data associated with the Belltopper project.
|
Criteria |
JORC Code explanation |
Commentary |
Verification of sampling and assaying |
- The verification of significant intersections by either
independent or alternative company personnel.
- The use of twinned holes.
- Documentation of primary data, data entry procedures, data
verification, data storage (physical and electronic)
protocols.
- Discuss any adjustment to assay data.
|
- All significant intersections were checked and verified
internally by senior qualified Novo staff.
- Twinned holes were not completed.
- All primary drill data was documented, verified (including QAQC
analysis) and stored within an industry-standard SQL database.
|
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.
- Specification of the grid system used.
- Quality and adequacy of topographic control.
|
Drill collar surveys
- All BTD and MD series collars were initially surveyed by
company staff using a hand-held GPS. At the completion of each
program all collars were surveyed in MGA94 Zone 55 and MGA2020 zone
55 by a Registered Licensed Surveyor using a Differential GPS
system (DGPS).
- Holes drilled by Eureka and the majority of holes drilled by
Pittson in the mid 1990’s (LSRC/D & LSRC Series and HMDDH &
LSDDH Series respectively) were surveyed in AMG84 Zone 55 by a
Registered Licensed Surveyor using a theodolite.
- The collar positions for the DDHMA Series are considered less
reliable, as they have been digitised off old plan maps. Although
the general drill pads for these holes could be located, Novo staff
were unable to locate the collar positions.
- Most collar positions, except for the DDHMA series collars,
have been validated in the field.
- A high-resolution LIDAR survey flown in Dec 2022 over the
Belltopper project has assisted in validating the collar position
of all Belltopper drill holes.
- All drill collars have been converted to and are presented in
MGA94 Zone 55.
Downhole surveys
- Downhole surveying of DD for the MD and BTD series were carried
out at a nominal depth of 6 m, then every 25 m from thereon and at
end of hole. The BTD series drilling used a REFLEX EZ-TRAC™ digital
magnetic hole survey system, while the MD13-MD22 series used a
Boart Longyear TruShot™ magnetic multi-shot tool. DD holes
MD01-MD11 were surveyed with a magnetic single shot camera
- Earlier DD holes were surveyed using a magnetic single shot
camera at the collar, then at nominal 50 m intervals down hole and
at end of hole depth. RC holes were surveyed at collar and end of
hole depth.
|
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 at the Belltopper project has primarily focused on the
Leven Star prospect area. Drilling along this mineralised trend has
been at a nominal 30-50 m spacing along strike and down-dip. The
deepest Leven Star intersection occurs approximately 400 m below
the surface topography.
- Drilling outside the Leven Star mineralised trend has been of a
scout nature testing narrow lode mineralisation styles.
- Coupled with a comprehensive understanding of the historic
workings and detailed geological mapping there is good confidence
in the continuity of mineralised structures and other geological
features outside of the Leven Star mineralised trend.
- DD core samples were not physically composited.
- RC samples were physically composited into four-meter intervals
for initial sampling. Any composited samples returning grade were
subsequently resampled at a one-meter infill intervals.
|
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.
- If the relationship between the drilling orientation and the
orientation of key mineralised structures is considered to have
introduced a sampling bias, this should be assessed and reported if
material.
|
- In most cases, holes were drilled across strike at a high angle
to the interpreted mineralisation geometry.
- No sampling bias is considered to have been introduced by the
drilling orientation.
- Further discussion regarding drilling orientation is presented
under the heading Relationship between mineralisation widths and
intercept lengths.
|
Sample security |
- The measures taken to ensure sample security.
|
- All samples from the BTD and MD13-MD22 series were transported
by a commercial courier directly to ALS Laboratories in Adelaide
from the Novo/GBM core facility in Castlemaine, Victoria.
- During previous drill programs, samples were either delivered
via courier or directly delivered by staff to the appropriate
laboratory.
- Available core, coarse rejects and pulps are stored at the Novo
core facility in Castlemaine, Victoria.
|
Audits or reviews |
- The results of any audits or reviews of sampling techniques and
data.
|
- No audits of either the data or the methods used in this
program have been undertaken to date.
|
Section 2 Reporting of Exploration Results
(Criteria listed in the preceding section also apply to this
section.)
Criteria |
JORC Code explanation |
Commentary |
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.
|
- The Belltopper Project is enclosed within retention license
RL006587 (Originally granted on 23rd September 2020 for a period of
10 years) and EL007112 (Originally granted on 3rd of July 2020 for
a period of 5 years). All reported drilling associated with the
Belltopper Project is located within RL006587
- The rights, title and interest of RL006587 and EL007112 are
held under Rocklea Gold Pty Ltd (100% subsidiary of Novo resources
Corp.)
- Part of retention license RL006587 is located within the Fryers
Ridge Conservation Reserve. The Reserve is classified as
‘restricted Crown land’ under the Mineral Resources Development Act
1990 and may be used for mineral exploration and mining, subject to
the approval of the Minister for Environment and Conservation.
- Novo has accepted the Schedule 4 conditions of the Land Use
Activity Agreement between the Dja Dja Wurrung Clans Aboriginal
Corporation and the State of Victoria applying to all Crown land
including road reserves within the retention license.
|
Exploration done by other parties |
- Acknowledgment and appraisal of exploration by other
parties.
|
- The project area has been explored by several companies since
the 1970s. In 1987 Molopo/Paringa drilled 3 DD holes for 741.55 m.
In 1990-92 Pittson drilled 16 DD holes for 2245.8m. In 1994 Eureka
drilled 15 RC holes for 1682.1m and 2 RC holes with DD tails for a
further 185.1m.
- GBM Resources drilled 12 DD holes (MD01 to MD11 including
MD08A) for 3694 m in 2008 followed by a single 999.8 m hole (MD12)
which was drilled in March 2010).
- In joint venture with GBM Resources, Novo Resources drilled
3161.7 m of HQ and NQ diamond core across 11 holes (MD13 to MD22
including MD18A).
|
Geology |
- Deposit type, geological setting and style of
mineralisation.
|
- The geology within the project area consists of a series of
Early Ordovician turbidites that form part of the Castlemaine
Supergroup within the Ballarat-Bendigo Structural Zone of the
Lachlan Fold Belt. The sediments comprise of a very uniform and
well-bedded sequence of marine sandstone and mudstone interbedded
with fossiliferous black shale. The Drummond North goldfield is a
north-trending belt of fault-related mineralised zones, extending
from the Humboldt reef in the north to the Queen’s Birthday reef in
the south, a distance of around 4 kilometres. Approximately 30 % of
the tenement area is covered by basalt cover.
- Historically two styles of mineralisation have been
investigated at Belltopper Hill, located within the Drummond North
Goldfield. One comprises steeply dipping, north-west to
north-trending quartz veins with associated stockwork zones (e.g.
Panama and Missing Link) that were worked to shallow depths in the
late 1800s. The other is a northeast-striking zone that cuts
obliquely across bedding in the Ordovician sedimentary rocks and
was worked for a short time in the 1930s as Andrews Lode but more
recently as the Leven Star Zone. Most modern exploration has
targeted the Leven Star lode with only modest attention paid to the
other reefs on Belltopper or to the reef lines south of the hill
where the bulk of historical production occurred.
- Recent drilling has also highlighted the potential of saddle
reef style mineralisation within the Belltopper corridor.
- At Leven Star, the GBM 2008 resource work determined that the
reef, up to 8m wide, follows a narrow, brittle fault zone with
associated intense fracturing and quartz vein development in the
country rock. Deformity and reef width are controlled by lithology
with the best development in coarser-grained sandstone units.
Sulphide mineralisation occurs as; fine-grained
pyrite/stibnite/bismuth-telluride/bismuthinite in quartz veins and
country rock fractures, disseminated clots of
pyrite-arsenopyrite-stibnite-pyrrhotite-chalcopyrite, and as fine
needles and radial clots associated with sericite. Pyrite is most
widespread while stibnite-arsenpyrite are restricted to stockwork
veins and larger-scale quartz veins. Alteration is dominated by
sericite, within quartz veins and as vein selvedge.
Carbonate/sulphide alteration is extensive as haloes around breccia
zones. Skarn-like assemblages of scheelite/fluorite/cassiterite
with coarse bladed calcite and muscovite are also present.
- The Drummond/Belltopper mineralisation shares similarities with
the Fosterville gold field; mapped distribution and scale of
workings, reef geometry, gold in arsenopyrite disseminated in
country rocks, sulphide-carbonate alteration and gold antimony
association, and mineralisation age (370 Ma).
- Mineralisation may be associated with buried intrusion(s) of
IRG or porphyry affinity. Evidence for intrusion-related
mineralisation includes; outcropping auriferous and altered
porphyritic monzogranite with overprinting gold-bearing sheet
veins, a Falcon gravity low anomaly spatially associated with the
hill and mineralisation, presence of Mo-Bi-W-Te-Sb in soils and
rocks on Belltopper, and anomalous Mo-Bi-Sn-W-Cu-Sb-Zn to
significant depth in the deep exploration hole MD12.
|
Drill hole Information |
- 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:
- easting and northing of the drill hole collar
- elevation or RL (Reduced Level – elevation above sea level in
metres) of the drill hole collar
- dip and azimuth of the hole
- down hole length and interception depth
- hole length.
- If the exclusion of this information is justified on the basis
that the information is not Material and this exclusion does not
detract from the understanding of the report, the Competent Person
should clearly explain why this is the case.
|
- Detailed drill hole information is provided in the accompanying
table.
|
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.
- The assumptions used for any reporting of metal equivalent
values should be clearly stated.
|
- Reported gold intersections have been calculated with
length-weighted averages using the following
parameters: Standard intersectionsº
0.3 g/t Au cut-off and 2 m internal dilution. º
High grade included intercepts calculated with 1.0 g/t
Au and no internal dilution.Granite/intrusive
intersectionsº Significant intersections
across broad intrusive zones in MD17, MD22 and DDHMA3 were
calculated using a 0.1g/t Au cut-off grade and no more than 5m
internal dilution.
- All width and intercepts are expressed as metres downhole.
Calculated as length weighted averages.
- Reported core loss was treated as 0 g/t Au grade in all
calculations.
- The gold assay of a primary sample from a duplicate pair was
used in all calculations.
- Any isolated gold intersections separated by internal dilution
must independently be above the average cut-off grade when
including the grades of the internal dilution.
- Metal equivalents were not reported.
|
Relationship between mineralisation 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.
- If it is not known and only the down hole lengths are reported,
there should be a clear statement to this effect (eg ‘down hole
length, true width not known’).
|
- Reported gold intersections from drilling represent apparent
downhole widths.
- Most targeted mineralised trends for the Belltopper Project are
interpreted to be vertical to sub-vertical with many drill holes
intersecting mineralisation at an acute angle of between 30 ° and
65 °. As a result, true widths of most significant intersections
are likely to be a reduced factor of reported apparent downhole
widths. In general, it is estimated that true width twill be
between 40 % and 85 % less than the reported downhole widths.
- In summary of more recent drilling:
- BTD001 intersects Leven Star at a shallow angle. True widths
for these intersections will be between 50 % and 60 % lower than
the reported downhole widths.
- BTD002 was drilled shallow along the strike of geology with the
aim of increasing the potential of intersecting anticline related
mineralisation. The two most elevated intersection in BTD002 were
Welcome Fault (4.1 m @ 2.4 g/t Au from 36.1 m) and Hanover fault
(19.15 m @ 0.7 g/t Au from 216 m in BTD002). BTD002 intersected
both structures at a shallow angle and the true width of these
structures are likely to be around 40% less than the reported down
hole width.
- Cross section interpretation of BTD003 indicates that BTD003
intersected Butcher Gully fault at a high angle, while other key
intersections from this hole were likely intersected at a shallower
angle, and the true width of these structures are likely to be
around 20% to 30 % less than the reported down hole width.
- Cross section interpretation of BTD004 and BTD005 indicate most
drill intersections were at a high angle to intersected reefs with
the notable exception of the Missing Link (12.26 m @ 1.4 g/t Au
from 185 m) and Missing Link Footwall (3.17 m @ 1.1 g/t Au from
164.11 m) which were both intersected at a shallow angle of around
30 degrees. True widths for these intersections will be
approximately 40 % less than the reported downhole widths.
- BTD006 intersected Piezzi Reef Fault (7 m @ 1.9 g/t Au from 179
m) at a shallow angle. The true width of this intersection is
likely to be between 50 % and 40 % less than the reported downhole
width.
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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.
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- Collar plans showing drill collar locations are included.
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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
Exploration Results.
|
- A table of significant intersections with a gram metre
intersection of greater than 0.3 GM with the detailed parameters is
presented within this report.
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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.
|
- Other recent phases of exploration at Belltopper include:
- Detailed geological mapping.
- 2801 soil geochemistry samples at a nominal spacing of 100 m by
50 m, increasing to 25 m by 25 m spacing in areas of
anomalism.
- 1084 multielement rock chip samples.
- Compilation and 3D digitisation of historic production
workings.
- Recent geophysics surveys including:
- 15.2 line km of 2D dipole-dipole induced polarisation.
- 83.1 line km of ground magnetics.
- 121 new stations of ground gravity (merged with GBM 2008 ground
gravity survey).
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Further work |
- The nature and scale of planned further work (eg tests for
lateral extensions or depth extensions or large-scale step-out
drilling).
- Diagrams clearly highlighting the areas of possible extensions,
including the main geological interpretations and future drilling
areas, provided this information is not commercially
sensitive.
|
- Work by Novo has identified strong potential for the discovery
of additional resource ounces within the Drummond and Belltopper
Hill goldfields.
- Potential targets can be classified into categories based on
structural domains and target models;
- Incremental increases to the current Leven Star resource where
shoots are open at depth and along strike.
- Step over or repeat of Leven Star parallel structures defined
by geophysics, mapping, and soils data.
- Intersection between key mineralised structures (including
Leven Star reef, the Missing Link, Hanover Reef, and Welcome Fault
structures) and project scale anticlines (Mostly notably,
Belltopper Anticline)
- Blind mineralisation associated with north-northwest trending
mineralised structures including; Piezzi Reef, O'Connors Reef, and
Panama Reef under the west dipping regional Taradale Fault.
- Poorly tested 1.5+ km system strike length from Queen’s
Birthday to O’Connor’s Reefs.
- Further investigation of intrusion related gold system (IRGS)
model; mineralisation in sheeted veins, breccias or disseminations
at margin or within near-surface dykes or deeper-seated
intrusion(s).
- Unrealised potential for intrusion hosted gold (e.g. modelled
intersections of high-grade gold reefs with the Missing Link
Granite are untested at Belltopper).
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