"Ultra-high-energy cosmic ray electrons " (defined as electrons with energies of ≥10 eV) might be explained by the Centrifugal mechanism of acceleration in the magnetospheres of the Crab -like Pulsars. The feasibility of electron acceleration to this energy scale in the Crab pulsar magnetosphere is supported by the 2019 observation of ultra-high-energy gamma rays coming from the Crab Nebula, a young pulsar with a spin period of 33 ms.