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Areas classified as Inferred Mineral Resources are informed by drilling spaced from 20 m up to >50 m, and have been estimated within the first, second, or the third estimation pass with a slope of regression greater than zero. Individual domains have been reviewed and classified accordingly. Areas that have not been estimated in the third pass have been categorized as ‘unclassified’ and have not been reported.
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TECHNICAL REPORT
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Novo will file a technical report (as defined in National Instrument 43-101 Standards of Disclosure for Mineral Projects) within 45 days of the date of this news release.
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Authorised for release by the Board of Directors.
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CONTACT
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| Investors: Mike Spreadborough +61 8 6400 6100 [email protected] | North American Queries: Leo Karabelas +1 416 543 3120 [email protected] | Media: Peter Taylor +61 412 036 231 [email protected] |
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QP STATEMENT
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Ms Janice Graham (MAusIMM CPGeo; MAIG) and Dr Simon Dominy (FAusIMM CPGeo; FAIG RPGeo; FGS CGeol) are the qualified persons, as defined under National Instrument 43-101 Standards of Disclosure for Mineral Projects, responsible for, and having reviewed and approved, the technical information contained in this news release relating to the Leven Star Mineral Resource Estimate (MRE). Ms Graham is a Principal Consultant and full-time employee of Snowden Optiro and Dr Dominy is a Technical Advisor to Novo.
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Dr Christopher Doyle (MAIG) and Dr Simon Dominy (FAusIMM CPGeo; FAIG RPGeo; FGS CGeol), are the qualified persons, as defined under National Instrument 43-101 Standards of Disclosure for Mineral Projects, responsible for, and having reviewed and approved, the technical information contained in this news release relating to the Belltopper Exploration Target. Dr Doyle is Novo’s Exploration Manager – Victoria and Dr Dominy is a Technical Advisor to Novo.
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JORC COMPLIANCE STATEMENTS
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Mineral Resource
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The information in this release pertaining to the Leven Star Reef Mineral Resource Estimate at the Belltopper Gold Project is based on, and fairly represents, information and supporting documentation compiled by Ms Janice Graham (MAusIMM CPGeo; MAIG) and Dr Simon Dominy (FAusIMM CPGeo; FAIG RPGeo; FGS CGeol). Ms Graham is a full-time employee of Snowden Optiro. Dr Dominy is an independent technical advisor to Novo Resource Corp. Ms Graham and Dr Dominy have sufficient experience relevant to the styles of mineralisation and type of deposits under consideration and to the activity being undertaken to individually 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”. Ms Graham and Dr Dominy consent to the inclusion in the report of the matters based on this information in the form and context in which it appears.
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Belltopper Exploration Target
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Novo initially announced its updated 2026 Exploration Target for the Belltopper Gold Project to ASX on 11 February 2026 in its announcement entitled “Novo Delivers Significant Increase to Belltopper Exploration Target” (which is available to view at www.asx.com.au) (Exploration Target Announcement).
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The information in this announcement that relates to the Belltopper Exploration Target is based on information compiled by:
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(a) Dr Christopher Doyle, a Competent Person who is a Member of the Australasian Institute of Geoscientists (MAIG). Dr Doyle is Exploration Manager – Victoria for Novo and is a full-time employee of Novo. Dr Doyle has sufficient experience that is relevant to the style of mineralisation and type of deposit 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 Doyle consents to the inclusion in this announcement of the matters based on his information in the form and context in which it appears; and
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(b) Dr Simon Dominy, a Competent Person who is a Fellow of the Australasian Institute of Geoscientists (FAIG RPGeo), the Australasian Institute of Mining and Metallurgy (FAusIMM CPGeo) and Chartered Fellow of the Geological Society of London (FGS CGeol). Dr Dominy is a Technical Advisor contracted to Novo. Dr Dominy has sufficient experience that is relevant to the style of mineralisation and type of deposit 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 Dominy consents to the inclusion in this announcement of the matters based on his information in the form and context in which it appears.
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As a basis for the Belltopper Exploration Target, Novo applied its geological understanding of the reef network at the Belltopper Gold Project, drawing upon 3D reconstruction of historic mining and exploration data, drilling data, structural and geochemical data, field mapping (including high-resolution LiDARTM interpretation), and surface rock chip sampling. Further information about Novo’s Exploration Target at Belltopper, along with a more detailed explanation of the basis for the Exploration Target (including a specific description of the level of exploration activity already completed at Belltopper), is contained in the Exploration Target Announcement.
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Previous Exploration Results
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The information in this news release that relates to Exploration Results at the Belltopper Gold Project is extracted from Novo’s ASX announcements listed in endnotes 1, 3 and 4 below, each of which is available to view at www.asx.com.au. The Company confirms that it is not aware of any new information or data that materially affects the information included in the original market announcements and that all material assumptions and technical parameters underpinning the estimates in the market announcements continue to apply and have not materially changed. The Company confirms that the form and context in which the Competent Person’s findings are presented have not been materially modified from the original market announcements.
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FORWARD-LOOKING STATEMENTS
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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, 2025 (which is available under Novo’s profile on SEDAR+ at www.sedarplus.ca and at www.asx.com.au), in the Company’s options prospectus dated 9 March 2026, and 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.
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ABOUT NOVO
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Novo is an Australian based gold explorer listed on the ASX and the TSX focussed on discovering standalone gold and copper projects with > 1 Moz development potential. Novo is an innovative explorer with a significant land package covering approximately 4,160 square kilometres in the Pilbara region of Western Australia, which includes the Toolunga Project in the Onslow District, along with the 22 square kilometre Belltopper project in the Bendigo Tectonic Zone of Victoria. In addition to the above, Novo is part of a prospective farm in agreement in New South Wales.
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Novo has a significant investment portfolio and a disciplined program in place to identify value accretive opportunities that will build further value for shareholders.
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Please refer to Novo’s website for further information including the latest corporate presentation.
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#Refer to De Grey’s ASX Announcement, Hemi Gold Project Mineral Resource Estimate (MRE) 2024, dated 14 November 2024. No assurance can be given that a similar (or any) commercially viable mineral deposit will be determined at Novo’s Becher Project.
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______________________________
1 Refer to Novo’s ASX announcement dated 11 February 2026 – Novo delivers significant increase to Belltopper exploration target.
2 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 (TSXV:GPAC) Company TSXV release dated 11 January 2024, and Southern Cross Gold (ASX:SXG) Company ASX release dated 5 March 2024, respectively. Production figures for Bendigo, Castlemaine and Ballarat include combined alluvial and hard rock production. Gold endowment for Fosterville includes historic production + reserves + resources as at 31/12/2023. Gold endowment for Costerfield equals historic production + resource (including reserves) as at 28/03/2024. 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.
3 Refer to Novo’s ASX announcement dated 25 September 2024 – Belltopper mineralisation modelling defines prospectivity
4 Refer to Novo’s ASX announcement dated 4 June 2024 – Reissue of Announcement: Significant results from diamond drilling at Belltopper, Victoria.
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APPENDIX 1: BELLTOPPER DRILL COLLARS
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| Hole ID | Hole Type | Depth (m) | Easting | Northing | RL AHD (m) | Collar Dip (°) | Collar Azimuth (MGA94 55) (°) | Collar Azimuth (Mag) (°) | Company | Date completed |
| 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 | 05-Mar-24 |
| 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 |
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All drill collars are reported in MGA94 Zone 55. All collars are located within Retention Licence RL006587. Shaded collars are not included in the Leven Star 2026 Mineral Resource Estimate.
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APPENDIX 2: BELLTOPPER DRILL COLLAR MAP
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Appendix 3. – JORC Code, 2012 Edition – Table 1. Leven Star Reef Mineral Resource Estimate 2026
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Section 1 Sampling Techniques and Data
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(Criteria in this section apply to all succeeding sections.)
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| Criteria | JORC Code explanation | Commentary | ||||
| Sampling techniques |
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| Drilling techniques |
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Summary of Leven Star drilling
Max Depth
Drill Method
Core Orientation
| ||||
| Drill sample recovery |
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| ||||
| 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 | |||||
| ||||||
| Logging |
|
The CPs consider that the level of detail is sufficient for the reporting of Mineral Resources. Logging data provides information to support geological modelling, including weathering/oxidation, structure, and rock type. | ||||
| Sub-sampling techniques and sample preparation |
|
The CPs consider the sampling, sample preparation and assay methods are reasonable for the stage of the project and resource classification. | ||||
| Quality of assay data and laboratory tests |
| Assay Method
QA/QC
| ||||
| 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 | |||||
The CPs consider the sampling, sample preparation and assay methods are reasonable for the stage of the project and resource classification applied. Future drilling programmes should include higher insertion rates for QC. | ||||||
| Verification of sampling and assaying |
|
| ||||
| Location of data points |
| Drill collar surveys
Downhole surveys
The CPs consider that the topographic control is suitable to support the Mineral Resource. | ||||
| Data spacing and distribution |
|
The CPs believe that the mineralised wireframes have sufficient geological and grade continuity to support the classification applied to the Mineral Resources given the current drill pattern. | ||||
| Orientation of data in relation to geological structure |
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| ||||
| Sample security |
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| ||||
| Audits or reviews |
|
| ||||
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Section 2 Reporting of Exploration Results
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(Criteria listed in the preceding section also apply to this section.)
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| Criteria | JORC Code explanation | Commentary | |
| Mineral tenement and land tenure status |
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| |
| Exploration done by other parties |
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| |
| Geology |
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| |
| Drill hole Information |
|
| |
| Data aggregation methods |
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| |
| Relationship between mineralisation widths and intercept lengths |
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| |
| Diagrams |
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| |
| Balanced reporting |
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| |
| Other substantive exploration data |
|
| |
| Further work |
| Drill hole BTD003 (drilled in 2024) is interpreted to have intersected the LSR approximately 320 m to the NE and beyond the (“Inferred”) resource extent, supporting mapping data, historic workings, and limited historic drilling that indicate the LSR potentially remains open (from surface) and insufficiently tested to the NE. Additional scoping-level step-out drilling up to 500 m beyond the current resource is warranted in the near-term to gain confidence in any potential NE extension to the LSR. Any future drilling NE of the current resource would be contingent on positive results from initial step-out-drilling. Limited drilling toward the southwest margin of the LSR highlight open higher-grade intersections that have not been extensively drilled and represent potential target higher-grade “shoot” zones within the current resource model. This zone broadly correlates with the modelled intersection(s) between the sub-vertical, NE-trending LSR and several parallel NE-dipping reefs including the Missing Link, Panama, and West Panama Faults. Near term drilling is designed to assess down-plunge of existing high-grade open intersections within this developing shoot zone and pending positive results may result in future resource expansion drilling down-plunge and beyond the existing resource model (See below). The LSR represents one out of eight individual reefs that collectively comprise the 2026 Exploration Target (ET) at Belltopper. Near-term scoping level drilling (ca. 100 x 100 m) of the remaining seven reefs is planned to gain confidence across all ET reefs and/or to evaluate additional known historic reefs that currently sit outside of the ET. Longer term resource-level drilling of the seven additional known reefs at Belltopper will be contingent on initial scoping-level drilling results. The goal being incremental growth at Leven Star in parallel with the seven additional Exploration Target Reefs and/or any other known historic reefs that may be included (See below). A figure accompanying this announcement is available at The image below highlights higher block grades in the SW region of the LSR (LSR MRE block model long section). This is a priority target area that is lightly drilled and warrants further drilling. A figure accompanying this announcement is available at: |
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Section 3 Estimation and Reporting of Mineral Resources
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(Criteria listed in section 1, and where relevant in section 2, also apply to this section.)
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| Criteria | JORC Code explanation | Commentary | |
| Database integrity |
| Collars, surveys, assays, lithology, and bulk density data have been imported into Datamine format from .csv. Downhole surveys were reviewed to ensure that the database did not contain any erratic survey measurements. Many of the drillholes are vertical. Each record was reviewed to determine if there were issues, and no problems were identified. MRE26 was estimated using RC and DD holes, as summarised below. A table accompanying this announcement is available at: The CPs have taken steps to review the sample data to verify their veracity. Steps taken included:
No issues were encountered during the verification process. The CPs consider the LSR database appropriate to support the MRE. | |
| Site visits |
| Dr Dominy visited the Novo Castlemaine office and core shed on various days between 14th April 2022 and 18th May 2022. During this period, he walked the Leven Star surface area; observed DD in progress; reviewed both new (2022) and historical LSR drill core; and held discussions with the project team. He also visited the project office on 14th October 2025 where he held discussions with the Regional Exploration Manger, Dr Christopher Doyle. Ms Graham has not visited site. | |
| Geological interpretation |
| The LSR reaches up to 8 m in width, 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-arsenopyrite 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. Three alternate geological/wireframe models for the LSR were produced (Models A, B and C – LSA, LSB and LSC). The LSC model was the most realistic interpretation of the LSR. The LSC model integrates additional downhole data obtained from the recently drilled (2023) diamond hole BTD001. Hole BTD001 successfully extended the LSR mineralisation up to 120 m down-dip from the previous MD16 intersections and confirmed the position of the Far East Hanover Fault. The criteria for wireframe construction were:
The BTD001 intersections significantly influence the overall width of LSC at depth. Previous modelling had postulated that the widths identified in MD16 continued at depth, converging at an RL proximal to the intersections now assessed by BTD001 (see below). A figure accompanying this announcement is available at: The true width of mineralisation in hole BTD001 appears to be narrower than expected. Additionally, the multiple reefs originally interpreted to intersect around the depth of BTD001 are likely to converge at greater depth. This concept is further supported by multiple interpreted LSR intersections identified at depth in both MD03 and LSDDH7. In addition to the Main LSR, recent modelling and relogging of historic core has identified several minor LSR parallel reefs. These are highlighted by semi-continuous zones of mineralisation. The geological representation of these hanging wall and footwall reefs aligns well with common observations of tectonic brecciation, increased quartz veining, and alteration along these trends. Lower-grade composite intervals have guided the wireframe for the hanging wall, and footwall models associated with LSC. Unfortunately, many of these historic intercepts were drilled with RC and sample residues were not retained. Where possible, the hanging wall and footwall models have been constrained to specific smaller intervals within the composite grade based on logging. In cases where no obvious constraining feature exists, the wireframe width representative of the 4 m composite has been maintained. Further investigation has allowed a more confident interpretation of four post- or syn-tectonic faults that offset or influence the LSR. These key faults include the Far East Hanover Fault, NW Fault 1, Granite Gully Thrust, and NW Fault 18. The most significant of these faults is Far East Hanover Fault which intersects the LSR at a shallow angle and is interpreted to be a sub-vertical structure with minor interpreted dextral offset and eastern side upthrown. Movement along this results in the main LSR system being intersected up to three times in MD16, BTD001, and other proximal holes due to structural repetition. In contrast, holes distal to this central zone around the Far East Hanover Fault only intersect the main LSR structure twice. The LSC model represents increased geological understanding of the LSR deposit and has the benefit of additional drilling and interpretation compared to the original LSA and LSB models. LSC is considered the current best interpretation of the deposit in context of both geological and grade continuity. The CPs are of the opinion that the geology of the deposit and mineralisation is sufficiently understood at a level appropriate to the current drill spacing, data density, and stage of the project. | |
| Dimensions |
| The LSR is a northeast-trending system. Drilling has shown mineralisation to be continuous for about 800 m along strike. The main mineralized body is not a simple narrow quartz vein; it is described as a stockwork-breccia zone up to about 10 m wide. Around this core zone is a broader alteration envelope of roughly 10–12 m. In resource modelling terms, LSR is interpreted as a steep to near-vertical system striking approximately 040°, with the main reef accompanied by minor parallel hanging-wall and footwall reefs. Recent drilling, particularly BTD001, extended known mineralisation by up to 120 m down-dip from previous intersections to around 400 m from surface. | |
| Estimation and modelling techniques |
| The LSR estimate was built from a staged workflow: data validation, data preparation, exploratory data analysis, geological interpretation and modelling, compositing, assessment of extreme values, variography, block model optimisation, block modelling/grade estimation, model validation, depletion assessment, classification, and reporting. Datamine RM Pro was used for estimation and Supervisor for statistical analysis. The input database includes historical and recent drilling from several campaigns. The LSR block model is based on RC and DD, with diamond holes also used to support density analysis and metallurgical work. Topography, oxidation and fresh-rock surfaces, and several fault wireframes were incorporated into the geological model. Only gold grade is reported. Geological interpretation is based on the LSC model, integrates the 2023 BTD001 diamond hole, which extended the interpreted mineralisation down dip and improved understanding of the Far East Hanover Fault. The LSC model includes the main LSR structure and several minor parallel hanging-wall and footwall reefs. For estimation, drillhole data were coded by mineralized domain, fault area, and weathering state. Contact analysis found no strong grade break between oxide, transitional and fresh material sufficient to justify separate estimation domains at this stage, so weathering states were combined within each mineralized domain. Samples were composited to 1 m within domain boundaries. Below-detection assay values were replaced with half-detection-limit values. Two intervals affected by significant core loss were conservatively adjusted assuming lost core carried zero grade. Gold top-cuts were applied only where required, notably in the 100 domain and one smaller domain. Grade estimation used Ordinary Kriging into a rotated block model aligned with the approximate strike of mineralisation. The block model used parent blocks of 2 m (E) by 40 m (N) by 30 m (RL), sub-celled to 0.5 m (E) by 2 m (N) by 2 m (RL) determined by Quantitative Kriging Neighbourhood Analysis (QKNA). An initial (P1) search ellipse of 110 m by 30 m by 15 m was defined based on the results of the variography and assessment of the data coverage. A minimum of eight and maximum of 25 samples was used for the initial search pass. Second pass (P2) was two times the initial search ellipse with a minimum of eight and maximum of 25 samples. Third pass (P3) was three times the initial search with a minimum of four and maximum of 15 samples. The fourth pass was used for model completeness, (P4) was eight times the initial search pass with a minimum of two and maximum of 15. All passes had a maximum of three samples per drillhole applied for the gold estimate. Validation included global comparisons of composites and block estimates, visual inspection in long sections, and swath plots. The gold estimate for the main (100) domain validated well against declustered composites. Extrapolation occurs along strike and down dip, with the maximum extrapolated distance from a drill hole being 180 m. Passes 1 (0.5x the variogram range) and 2 (1x the variogram range) of the search area are defined as interpolation. Pass 3 (1.5x the variogram range) is defined as extrapolation. Approximately 21% of the reported gold ounces are based on extrapolation, equivalent to 20% of the reported tonnes. The figure below shows the extrapolated versus interpolated areas of the Leven Star main (100) domain by tonnes. A figure accompanying this announcement is available at: The MRE is global in nature. No depletion has been applied to the model. It is understood that minimal mining has taken place at LSR. A previous estimate was reported in 2008 and re-reported with no changes in 2019 (Allwood, 2008; 2019). The MRE was classified as an Inferred Mineral Resource containing 820,000 t at 3.95 g/t Au for 104,000 oz Au. The estimate was based on an inverse distance (squared) weighted block model using 2 m composited samples. No variography was undertaken, with the model search ellipse aligned along strike to capture samples from two drill sections. The MRE was reported at a nominal cut-off of 2.5 g/t Au, with no optimisations applied. An underground operation was assumed. | |
| Moisture |
| Tonnages have been estimated on a dry basis. | |
| Cut-off parameters |
| LSR Mineral Resource was reported for an underground operation. A cut-off grade of 1.9 g/t Au was applied, calculated from the inputs provided to the MSO optimisation process. Refer to the “Mining factors or assumptions” section for MSO input parameters. | |
| Mining factors or assumptions |
| The LSR MRE has been reported as an underground operation and reported within Datamine MSO optimized stope shapes to satisfy the requirement for RPEEE. The RPEEE test is important to demonstrate the robustness of a Mineral Resource estimate. The optimized MSO stope shapes were estimated with the following indicative parameters:
Mining costs were defined on a “comparison” basis at a rate of 250,000 t/a. The mining method is based on a mechanized sub-level open stoping operation with 3 m wide by 3 m high drives; with a floor-to-floor separation of 15 m; mining recovery of 90%, minimum mining width of 1.5 m and 0.2 m dilution skins. | |
| Metallurgical factors or assumptions |
| Minimal historical testwork has been undertaken at LSR. Novo undertook metallurgical testwork on a 28 kg composite (assayed head weighted grade 4.5 g/t Au) from core and RC residues in 2023. Based on this testwork, the fresh/sulphide mineralisation from the LSR displays strong refractory characteristics. A single stage GRG test indicated a GRG value of 12%, which is low and would not support the use of a gravity circuit. Given previous mineralogical studies indicate fine and lattice-locked gold, gold reporting to the Knelson concentrate may represent rare coarse gold and free sulphide-hosted gold. The size-by-assay indicates that most of the gold is fine (as free or composite particles), where 73.5% is <75 µm. Flotation at P80 90 µm indicates a gold recovery of 92% with a mass pull of 12%. Flotation was undertaken on the SGRG tails. Gold recoveries by cyanidation across the three grind sizes are extremely low (<11%), indicating refractory mineralisation. The leach solution grades are broadly invariant with time, indicating that increased leach time has minimal effect. The total gold recovery across the gravity plus flotation testwork is 93%. The true gravity recovery could be two thirds of the experimental value, e.g. 8%. In such a case gravity recovery is not warranted and much of the GRG is likely to report to the flotation concentrate assuming a strong sulphide association. The “testwork” gold recovery based on a single sample across gravity-leach is c. 22%. This is a strong reflection that a standard gravity-CIL plant would recover little gold from the fresh mineralisation. The diagnostic leach test was based on the 89.2% gold (4.17 g/t Au) of non-free cyanide gold retained in the LT02 tails. Of this 89.2%, some 7.4% is carbonate hosted; 91.2% associated with sulphides (arsenopyrite); and a further 1.4% in other sulphides (pyrite). Subject to further testwork, it is assumed that a flotation concentrate would be produced for direct sale. No metallurgical recovery factors have been applied to the Mineral Resource, though were included in the Datamine MSO optimisation process used to report the MRE. The optimisation process used a conservative metallurgical recovery of 88%. | |
| Environmental factors or assumptions |
| Given the level of information available it is expected to take three years to obtain Primary and Secondary approvals for commencement of construction and mining this includes the collection and assessment of environmental data. The approval pathway is determined by the level of disturbance the proposed project will have on the surface ecology. Novo has commenced planning and scheduling the necessary surveys and studies required to understand the possible impact on the environment and surrounds. Studies required prior to lodging an environmental approval application include flora, fauna, suface water and hydrology, air pollution, Heritage and possible impacts to the community. Investigations into possible waste and process residue disposal options have begun. No conclusions have been reached. The assumptions made in this regard are that processing is to occur offsite and that mine waste disposal will be minimised by filling mined voids with waste rock. At the appropriate time, Novo will also investigate waste rejection through ore sorting technology which could reduce the tonnage to be hauled between the operation and plant. This could also result in a higher feed grade to the plant. There is no guarantee that such technology is suited to LSR mineralisation. No testwork has been completed to date. | |
| Bulk density |
| LSR bulk density dataset is relatively limited but was considered sufficient for assigning densities to the MRE26 at an Inferred Mineral Resource level. Bulk density measurements were determined by Novo personnel using the weight-in-water/weight-in-air method. The data were imported into Datamine, de-surveyed with the drillhole data, and coded using the same weathering and domain framework as the drillholes and block model. A total of 213 bulk density measurements were reviewed, but only 52 measurements are reported as falling within mineralisation. The data show minor variation by weathering domain, though the dataset is small and insufficiently distributed for a comprehensive analysis. For the MRE26 model, density was not estimated block-by-block. Instead, fixed density values were assigned by material type and weathering state, with reference to the available measured means (see Table below). A table accompanying this announcement is available at: | |
| Classification |
| The Mineral Resources are classified in accordance with the 2012 JORC Code for reporting of Exploration Results, Mineral resources, and Ore Reserves (“The JORC Code 2012”). The model has been classified on a domain-by-domain basis; in practical terms a wireframe was constructed to encapsulate material meeting the criteria for each classification category used to delineate and code the model. No areas of the MRE have been classified as Measured or Indicated Mineral Resources. Inferred Mineral Resources have been defined at LSR. Areas classified as Inferred Mineral Resources are informed by drilling spaced from 20 m up to >50 m, and have been estimated within the first, second, or the third estimation pass with a slope of regression greater than zero. Individual domains have been reviewed and classified accordingly. Areas that have not been estimated in the third pass have been categorized as ‘unclassified’ and have not been reported. Eighty percent of the MRE26 by tonnes is supported by interpolation, with the remaining 20% by extrapolation. | |
| Audits or reviews |
| MRE26 was peer reviewed by Mr Ian Glacken FAusIMM(CP) FAIG, an Executive Consultant at Snowden Optiro. His review included high-level consideration of the sampling/QAQC and estimation. Mr Glacken found no material issues. No other audits or reviews were undertaken outside of Novo or Snowden Optiro. | |
| Discussion of relative accuracy/ confidence |
| The relative accuracy of the LSR MRE is reflected in the reporting of the Mineral Resource as per the guidelines of the 2012 JORC Code. The Mineral Resource statement relates to a global estimate of in-situ tonnes and grades. MRE26 is classified as an Inferred Mineral Resource. No quantification of accuracy/confidence has been undertaken. |
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