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This one is definitely worth a watch if you are keen to better understand the Apollo System. Brett Davis is truly one of the great structural geologists globally and we were honoured to host him at our Guayabales Project. $CNL $CNL.T @CollectiveMini1

Ramp Zone continues to ramp in size as it grows to the west $CNL $CNL.T Last night we announced new high grade results from Ramp incl 75.8m @ 8.01 g/t AuEq. tinyurl.com/2p8yva4z We are being asked about the geological model and why we believe Ramp mineralization could occur outside of the Apollo breccia over a larger area than previously envisioned. Let me answer: 1. We are only 1.75km away from Marmato Deeps deposit (6.2m ozs) which is hosted in at least two rock units (precursor porphyry diorite and schist). The most likely outcome is that Ramp and Marmato Deeps are from the same powerful intrusion engine which has already demonstrated that it overprints multiple host rock units. If this is true, why would Ramp mineralization only occur on the Apollo breccia host unit? 2. In hole APC103-D2 announced on Feb 4/25 we already hit Ramp outside of the breccia body at the end of the hole when it bottomed in 18.5m @ 3.84 g/t AuEq in precursor porphyry diorite (bigger intercept in the hole was 51.95m @ 8.38 g/t AuEq)! 3. Marmato Deeps extends for 750 meters vertical and is open. It starts in a transition zone and then improves as the depth increases. Are we only in the transition zone at Ramp given we have thus far drilled the shallowest portion of the Ramp Zone discovery? It’s clear we need to be aggressive with drilling at Ramp by stepping out laterally and vertically. Very exciting times for our team on the ground who deserve much credit for this success. Next up: 1. Apollo Subzone Assay Results 2. Trap Assay Results 3. San Antonio Assay Results 4. Additional Ramp Zone Assay Results