To "enrich the Universe", the heavy elements would need to get back out of the star - and into outer space, where it can eventually become part of new star systems. This "getting out" happens mainly in supernova explosions - i.e., in the case of very massive stars.
Also, stars with very low mass mainly convert hydrogen into helium - they didn't have time yet, given the current age of the Universe, to advance to a later stage, where they convert helium into heavier elements - and the stars with the very lowest masses never will, since they won't get hot enough.
The interstellar medium is enriched with heavy elements by the remnants of supernova explosions. Supernovae are massive stellar explosions that release heavy elements such as carbon, oxygen, and iron into space, enriching the surrounding interstellar medium with these elements.
Heavy stars produce heavier elements through nuclear fusion in their cores. As heavy stars age and undergo supernova explosions, they release these heavier elements into the surrounding space, enriching it with elements beyond hydrogen and helium. Lighter stars are not massive enough to produce heavy elements through fusion.
If massive stars did not explode at the end of their lives, they would instead collapse into black holes or neutron stars. This would have implications for the dispersal of heavy elements in the universe, as supernovae play a key role in enriching the cosmos with elements beyond hydrogen and helium. It would also impact the evolution of galaxies and the dynamics of stellar populations.
All elements , except the trans-uranic(Actinides) are atomically stable. The Actinides being the most massive elements are unstable and spontaneously breakdown into smaller less massive elements. The most massive element that is atomically stable is 'lead' ( Pb ; Plumbum).
Shocks from supernovae are abrupt changes in pressure and temperature caused by the explosion of a massive star. These shocks create powerful waves that propagate through the surrounding interstellar medium and can trigger the formation of new stars and influence the dynamics of gas and dust in galaxies. They also contribute to enriching the interstellar medium with heavy elements synthesized in the supernova explosion.
The interstellar medium is enriched with heavy elements by the remnants of supernova explosions. Supernovae are massive stellar explosions that release heavy elements such as carbon, oxygen, and iron into space, enriching the surrounding interstellar medium with these elements.
Heavy stars produce heavier elements through nuclear fusion in their cores. As heavy stars age and undergo supernova explosions, they release these heavier elements into the surrounding space, enriching it with elements beyond hydrogen and helium. Lighter stars are not massive enough to produce heavy elements through fusion.
After a supernova of a very massive star, the core collapses to form either a neutron star or a black hole. The outer layers of the star are ejected into space, enriching the surrounding environment with heavy elements. A bright burst of radiation, known as a gamma-ray burst, may also be emitted during this process.
Prof. Brian Cox provides a great explanation in episode 2 of his excellent TV series 'Wonders of The Universe'. In short, many elements can only be created in the extreme conditions which exist within stars as they burn all their internal fuel and gradually 'die'. As they die, massive changes take place within stars, creating the conditions which are required to create different types of elements.
If massive stars did not explode at the end of their lives, they would instead collapse into black holes or neutron stars. This would have implications for the dispersal of heavy elements in the universe, as supernovae play a key role in enriching the cosmos with elements beyond hydrogen and helium. It would also impact the evolution of galaxies and the dynamics of stellar populations.
Shocks from supernovae are abrupt changes in pressure and temperature caused by the explosion of a massive star. These shocks create powerful waves that propagate through the surrounding interstellar medium and can trigger the formation of new stars and influence the dynamics of gas and dust in galaxies. They also contribute to enriching the interstellar medium with heavy elements synthesized in the supernova explosion.
All elements , except the trans-uranic(Actinides) are atomically stable. The Actinides being the most massive elements are unstable and spontaneously breakdown into smaller less massive elements. The most massive element that is atomically stable is 'lead' ( Pb ; Plumbum).
Nuclear fusion.
Supernovae play a crucial role in the creation of heavy elements, including those necessary for life, such as iron and oxygen. These elements are released into the universe during the explosive death of massive stars, enriching the surrounding gas clouds from which new stars and planets, like Earth, can form. Supernovae also generate powerful shock waves that can trigger the formation of new stars and influence the evolution of galaxies.
yes
As heavier elements are formed by fusion in the core, a massive star will eventually exhaust its nuclear fuel and trigger a supernova explosion. This explosion will generate immense energy, leading to the production and dispersal of even more heavy elements into space.
Elements more massive than iron are created through processes such as supernova explosions and neutron star mergers, where extreme conditions allow for the fusion of lighter elements into heavier ones.