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Borexino collaboration reported about first measurement of solar CNO-$\nu$interaction rate in Borexino detector. This result is consistent with HydridicEarth model prediction about the contribution of $^{40}$K geo-antineutrinointeractions in single Borexino events. The potassium abundance in the Earth inthe range $1 \div 1.5$\% of the Earth mass could give the observed enhancementof counting rate above expected CNO-$\nu$ counting rate. The Earth intrinsicheat flux must be in the range $200 \div 300$ TW for this potassium abundance.This value of the heat flux can explain the ocean heating observed by theproject ARGO. We consider that Hydridic Earth model actually corresponds betterto CNO-$\nu$ Borexino results than Silicate Earth model.

On first detection of solar neutrinos from CNO cycle with Borexino