Decreasing nuclear stability terminates the r -process when its heaviest nuclei become unstable to spontaneous fission, when the total number of nucleons approaches 270. The fission barrier may be low enough before 270 such that neutron capture might induce fission instead of continuing up the neutron drip line. After the neutron flux decreases, these highly unstable radioactive nuclei undergo a rapid succession of beta decays until they reach more stable, neutron-rich nuclei. While the s -process creates an abundance of stable nuclei having closed neutron shells, the r -process, in neutron-rich predecessor nuclei, creates an abundance of radioactive nuclei about 10 amu below the s -process peaks. These abundance peaks correspond to stable isobars produced from successive beta decays of waiting point nuclei having N = 50, 82, and 126—which are about 10 protons removed from the line of beta stability.