Which stars typically undergo core-collapse supernovae, designated as Type II, Ib, or Ic?
Answer
Stars significantly heftier than the Sun, generally exceeding about eight times its mass
Core-collapse supernovae mark the end for stars significantly heftier than the Sun, specifically those generally exceeding about eight times its mass.
Related Questions
Which characteristic distinguishes the fusion of iron in a star's core compared to lighter elements?What mechanism initially provides resistance against gravitational compression in a massive star before core collapse?What process is responsible for forcing electrons into atomic nuclei during the immediate onset of collapse?During the rapid collapse phase, what size does the core shrink down to in milliseconds?What is the direct consequence when the infalling material slams into the ultra-dense, newly formed neutron core?What major problem did stellar models show regarding the initial shock wave following core collapse?If the initial shock wave stalls permanently, what is the likely outcome instead of a supernova explosion?What is the essential mechanism credited with reviving the stalled shock wave to drive the supernova explosion?Which stars typically undergo core-collapse supernovae, designated as Type II, Ib, or Ic?What is the fate of a remnant core whose mass exceeds roughly three solar masses after the supernova?What fraction of the total explosion energy is carried away by neutrinos that stream away unimpeded?