Hi CounterVin,We only have the one CNJ-GSR hole drilled to date...

Hi CounterVin,
We only have the one CNJ-GSR hole drilled to date (MTJV001) and no PGE assays yet. If we see PGE assays in the MTJV001 hole in the 1-3⁺g/t range over the 65m sulphide intersection (which is likely in my view) , then the PGE discovery made by GAL extends at least 400m south to the MTJV001 hole. If we get these PGE hits in MTJV001, it possibly opens up the entire length of the ultramafic cumulate and perhaps even the pyroxenite rocks in both GAL's and CNJ-GSR tenements. The ultramafic cumulate and pyroxenite comprise the Mouth Thirsty sill. Interpreted extent of the ultramafic cumulate and pyroxenite are shown on the aeromagnetic image below and underneath that the mapped extend of the rock units beneath GAL's and CNJ-GSR's tenements proximal to the Callistro discovery.

Regarding what is below the "real cheesy stuff under the sediment", I am taking a look at that over the next few days.



The mapped horizons (rocks) shown below are interpreted from the aeromagnetic image. Other geologists will very likely interpret the aeromagnetic image very differently. Just my view..........



Kind regards OldGeo