The kinetic energy of electrons produced during beta decay is not constant and varies based on the specific nuclide involved. The total energy available in the decay is fixed, determined by the mass difference between the initial and final nuclei, but is randomly distributed between the emitted electron and the neutrino. For example, tritium decays yield an average kinetic energy of about 5.7 keV for the electron, while heavier isotopes can produce electrons with significantly higher energies. The discussion also touches on the complexities of calculating velocities and energies, highlighting the importance of careful arithmetic in such calculations. Overall, beta decay results in variable kinetic energies for electrons, influenced by the properties of the decaying atom.