Iron is the end state for nuclear fusion in the core of a star. Every element beyond iron is formed in the supernova that happens as the core of the star collapses, or in the other kinds of supernova. Some heavy elements are also formed when 2 neutron stars enter into a death spiral and collide making yet another massive explosion.
To put it simply everything beyond iron is made in massive explosions as stars die.
Iron is the end state for nuclear fusion in the core of a star. Every element beyond iron is formed in the supernova that happens as the core of the star collapses, or in the other kinds of supernova. Some heavy elements are also formed when 2 neutron stars enter into a death spiral and collide making yet another massive explosion.
To put it simply everything beyond iron is made in massive explosions as stars die.
Iron is the end state for nuclear fusion in the core of a star. Every element beyond iron is formed in the supernova that happens as the core of the star collapses, or in the other kinds of supernova. Some heavy elements are also formed when 2 neutron stars enter into a death spiral and collide making yet another massive explosion.
To put it simply everything beyond iron is made in massive explosions as stars die.
So, the idea here is that iron (specifically iron-56) has the lowest energy of any atomic nucleus. In other words, trying to fuse iron will be endothermic (absorbing energy) rather than exothermic (releasing energy) as is the case for lighter elements. So, by the time a star reaches iron, its core is no longer able to produce energy and so it collapses.
It’s long been thought that supernovas produced elements heavier than iron. So, while producing these heavier elements does absorb energy, the supernova provides enough energy to do this. More recent discoveries have suggested that collisions between neutron stars, The remnants of stellar cores following a supernova, are responsible for many of the heavier elements in the universe. These collisions take place in binary system consisting of two neutron stars orbiting each other other. They slowly spiraling towards each other and eventually meet.
Latest Answers