The potential energy of a nuclide is enhanced by about 10 MeV per nucleon f
rom the repulsion between like nucleons, and diminished by about 20 MeV per
nucleon from the attraction between unlike nucleons. Nuclear stability res
ults mostly from the interplay of these opposing forces, plus Coulomb repul
sion of positive charges. Whereas fusion may be the primary mechanism by wh
ich first generation stars produce energy, repulsion between like nucleons
may cause neutron emission from the collapsed core (neutron star) produced
in a terminal supernova explosion and initiate luminosity in second generat
ion stars that accrete on such objects. As noted earlier [1], the scarcity
of solar neutrinos, the enrichment of light isotopes in the solar wind, and
the presence of abundant short-lived nuclides and interlinked chemical and
isotopic heterogeneities in the early solar system might also be explained
if the Sun formed in this manner.