IRON
The final elements fused in a star of the mass of our Sun are Oxygen then Carbon. Therefore a white dwarf core could be regarded as a solid, gigantic diamond.
The final stage in the evolution of the most massive stars is a supernova explosion, where the star collapses and then rebounds in a powerful explosion. This explosion can lead to the formation of either a neutron star or a black hole, depending on the mass of the collapsing core.
The process of core collapse to form iron from silicon in a massive star can occur in a matter of days to weeks. This phase, known as core-collapse supernova, is an explosive event where the iron core rapidly collapses and rebounds, leading to the synthesis of heavier elements.
When the gravity of a massive star overcomes neutron degeneracy pressure, the core collapses under its own gravity, leading to the formation of a black hole or a neutron star, depending on the initial mass of the star. This process releases a tremendous amount of energy in the form of a supernova explosion.
When a star explodes in a supernova, its core can collapse into either a neutron star or a black hole, depending on the mass of the original star. For stars with masses less than about 3 times that of the Sun, the core collapses into a neutron star, which is an extremely dense and compact object. For more massive stars, the core collapses further into a singularity, forming a black hole.
The final elements fused in a star of the mass of our Sun are Oxygen then Carbon. Therefore a white dwarf core could be regarded as a solid, gigantic diamond.
A massive star with iron in its core will stop nuclear fusion, leading to its collapse and eventual explosion as a supernova. Iron is the element at which fusion becomes endothermic, meaning energy is no longer released in the process.
Iron. Iron is the heaviest element that can be produced through nuclear fusion in a star, and once the core of a massive star is mostly composed of iron, it can no longer sustain fusion reactions. This triggers its collapse and ultimately leads to a supernova explosion.
Once fusion ceases in a massive star, it takes only a few seconds for the core to collapse and undergo a supernova explosion.
Assuming I've understood the question, it would be nickel. Nickel is the end product of the silicon burning process, since going any further (the next step up would be zinc) is endergonic.
an expanding Shell of hydrogen gas envelop the core of the star which collapses ,it becomes a red giant. In more massive star with hotter core ,helium fuses to carbon,silicon or oxygen, synthesizing the heavier element .even more massive stars may burns iron generating a cooling effect . The core implodls and the outer layer of the stars are bloom away as a supernova
The final stage in the evolution of the most massive stars is a supernova explosion, where the star collapses and then rebounds in a powerful explosion. This explosion can lead to the formation of either a neutron star or a black hole, depending on the mass of the collapsing core.
Yes, if the star is massive enough when the core collapses a supernova explosion happens.
Neutron Star
The process of core collapse to form iron from silicon in a massive star can occur in a matter of days to weeks. This phase, known as core-collapse supernova, is an explosive event where the iron core rapidly collapses and rebounds, leading to the synthesis of heavier elements.
When a massive star runs out of fuel, it undergoes a supernova explosion. The core of the star collapses under gravity, leading to the formation of a neutron star or black hole, depending on the final mass of the star. The outer layers of the star are expelled into space, enriching the surrounding environment with heavy elements.
A supernova occurs in a star's lifecycle when it runs out of fuel and its core collapses, causing a massive explosion.