As stars approach the end of their life cycles, they undergo several stages depending on their mass. For low to medium-mass stars, like our Sun, they expand into red giants, shedding outer layers to form planetary nebulas, with the core remaining as a white dwarf. Massive stars, however, experience a more violent end, going supernova and leaving behind either a neutron star or a black hole. Throughout these stages, nuclear fusion processes change, leading to the formation of heavier elements.
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