Respuesta :
Answer:
Stage 5 - A star of one solar mass remains in main sequence for about 10 billion years, until all of the hydrogen has fused to form helium.
Stage 6 - The helium core now starts to contract further and reactions begin to occur in a shell around the core.
Answer:
a star with 2-3 stellar masses would become a red supergiant
then a supernova and then become a neutron star.