The range of applicability of non-relativistic K Auger transition probability calculations has been established by comparing experimental data, relativistic Hartree-Fock-Slater calculations (RHFS) and conclusions on non-relativistic theories with jj and intermediate coupling. As is shown, relativistic effects play the most important role in K Auger transitions resulting in the formation of s vacancies, and they should be taken into account when calculating the probabilities of such transitions for atoms with Z>or approximately=30. An error has been observed in the RHFS calculations of the KL1M4,5, KM1M4,5 transition probabilities made by Bhalla et al. (1970).