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Midnight Sun Extends Dumbwa Copper Deposit to Over 5.3 Kilometres; Remains Open Along Strike With Drilling Ongoing

Exploration Programs

Midnight Sun Extends Dumbwa Copper Deposit to Over 5.3

Kilometres; Remains Open Along Strike With Drilling Ongoing

Results include: 93m @ 0.40% Cu, 80m @ 0.39% Cu, 44m @ 0.53% Cu,

and 36m @ 0.58% Cu

Vancouver, British Columbia, May 13 , 2026 – Midnight Sun Mining Corp. (TSXV:

MMA / OTC QX: MDNGF) (“Midnight Sun” or the “Company”) is pleased to report

results from drillholes completed on its wholly owned Dumbwa copper deposit,

located in Solwezi, Zambia. Dumbwa is in the southeast portion of the Company’s

Solwezi Project, centered in the heart of the prolific Domes Region - flanked to the

north by First Quantum’s Kansanshi mine and west by Barrick’s Lumwana mine.

Drilling has now surpassed 200 holes for a total of over 42,000 metres (“m”) and

results to date confirm near surface copper sulphide mineralisation, over a

continuous strike length of 5.3 kilometres (“km”) ( see Figures 2 and 3 ), with assays

received for the first ~4km of drilled strike. The initial discovery and delineation drill

program continues with 4 rigs focussed on growing the deposit to the north along

strike and to extend previously drilled mineralisation east and west. Quality control

issues related to laboratory analysis have been resolved, and the related backlog of

assays are now largely caught up (see below).

The Company plans to host a technical webinar with Midnight Sun ’s COO, Dr. Kevin

Bonel, to discuss the results announced in this news release. Details will be included

in a separate news release.

Top 20 Drill Highlights:

Hole ID From (m) To (m) Interval (m) Cu (%)

DBW-25-099R 58 60 2 0.54

152 245 93 0.40

29 33.78 4.78 0.31

DBW-25-123 59 67 8 0.44

127 207 80 0.39

DBW-25-036 0 44 44 0.53

and 119.54 137 17.46 0.37

DBW-25-111

52 57 5 1.75

63 79 16 0.35

132 221 89 0.25

DBW-25-122

11 20.6 9.6 0.18

77 91 14 0.19

106 142 36 0.58

including 127 142 15 1.03

171 238 67 0.30

DBW-25-147

0 17 17 0.20

41 102 61 0.34

including 41 47 6 1.30

82 85 3 1.38

111 126 15 0.27

154 168.05 14.05 0.51

182 183 1 1.34

DBW-25-064 0.7 47 46.3 0.42

DBW-25-114 26 32 6 0.21

43 87 44 0.37

122 208.5 86.5 0.15

DBW-25-149

23 40.84 17.84 0.85

Including 31 39 8 1.71

50.58 72 21.42 0.38

171 197.65 26.65 0.38

DBW-25-110

42 77 35 0.36

89 102 13 0.34

145 154 9 0.20

DBW-25-065 91 98 7 0.16

127 163 36 0.33

DBW-25-106

38 43 5 0.19

59 67 8 0.4

173 210 37 0.31

DBW-25-031

27 36 9 0.34

119 142 23 0.49

160 181 21 0.34

DBW-25-037 0 42 42 0.25

DBW-25-127

42 72 30 0.32

96 107 11 0.53

174.95 180 5.05 0.29

DBW-25-117

42 46 4 0.51

67 95 28 0.30

103 109 6 0.19

143 182 39 0.15

DBW-25-120

13 19 6 0.54

89 144.5 55.5 0.15

164 172 8 0.46

DBW-25-108 10 51 41 0.20

106 153 47 0.14

DBW-25-054

14 20 6 0.19

37 54 17 0.47

including 37 38 1 5.94

64.3 66 1.7 0.57

79 86 7 1.01

DBW-25-148

72.2 78 5.8 0.18

86 102 16 0.17

119 139.7 20.7 0.17

169 190 21 0.33

• Assay results based on four-acid digest, ICP-OES finish. Intervals listed are based on drilling intervals

and therefore are considered relative rather than true widths.

• The full table of assays including locations is available on the Company’s website and can be accessed

through this link: Dumbwa Drill Hole Location and Assay Table.

“What began as a geological concept has now been established as a significant

discovery, with over 5.3km of strike now tested and supported by more than 40,000m

of drilling. Our team is rapidly defining what is emerging as an exceptionally large,

near-surface, structurally controlled copper sulphide deposit” stated COO, Kevin

Bonel.

“We are developing a clear understanding of Dumbwa and can see the hallmark

‘pinch-and-swell’ geometry typical of major structurally controlled systems and have

confirmed unequivocally that Dumbwa is a basement-hosted, strain-related deposit,

geologically comparable in every way to Barrick’s Lumwana. We also recognize a

predictable grade distribution along strike, with broader higher- grade zones

separated by narrower lower- grade domains. Most importantly, we are continuing

to establish meaningful scale with each step north expanding the system and

mineralisation remaining open, alongside a clear plan to unlock additional

mineralisation within zones identified through earlier drilling.”

Figure 1: Dumbwa drilling to date, plotted on 11.2km Phase One copper-in-soil anomaly, target area.

Figure 2: Dumbwa drilling to date, magnified to show current 5.3km drilled strike extent, plotted on Phase One copper -in-

soil anomaly, target area.

Dumbwa Today – Geological Model Verified

The Company’s drilling has now surpassed 200 holes for a total of more than

42,000m over 5.3km of strike, and continues to confirm that Dumbwa is an

exceptionally large, very near surface, structurally controlled copper sulphide deposit

which remains open for growth. Drill testing has focussed on the upper ~220m of the

deposit with the intent of defining a resource amenable to rapid, low strip ratio, low-

cost future development. It is noted that some areas of similar mineralisation at the

nearby Lumwana pro ject can be traced to vertical depths well beyond 200m. At

Dumbwa, east-west width of the mineralised corridor ranges from 200m to greater

than 500m. Copper grades are variable ranging from thick lower grade intercepts (>

50 m @ <0.3%) to thick higher -grade intercepts (>25m@>0.5%). Grade variability is

pronounced along strike (north-south) and is influenced by cross-cutting northwest-

southeast structures that adversely affect the strain regime and subsequent

development of mineralised schists. In contrast, grades are relatively consistent east-

west within the higher, medium and lower grade zones, and across the width of the

mineralised corridor.

Figure 3: Assay grade shells superimposed on the Dumba soil anomaly showing the correlation between high soil anomalies

and medium to high grade mineralised intercepts at Dumbwa. Drilling continues to follow the soil anomaly north.