Supernova form heavier elements
Carbon, oxygen, and iron nuclei are commonly found in stars because they are formed through nuclear fusion processes in the cores of stars. Carbon and oxygen are produced through fusion reactions in stars of medium mass, while iron is formed in the later stages of a star's life through various fusion processes. These elements are essential building blocks for heavier elements and are crucial for the evolution of stars.
All elements up to Iron are produced by smaller stars. heavier elements (everything heavier then iron) are produced from larger stars when they go supernova.
Elements heavier than iron are formed in super-nova explosions.
The element that has 26 protons is Iron....
Nuclear fusion in stars involves the process of combining lighter elements, such as hydrogen, to form heavier elements, such as helium. As these elements fuse together, they release energy in the form of heat and light. Over time, through a series of fusion reactions, heavier elements are synthesized, up to iron, in the core of stars.
The formation of the elements is a nuclear process that usually happens in stars. The core of the star is hot enough and has enough pressure to overcome the electric repulsion of the atomic nuclei and literally fuse the nuclei together. This process happens over and over again, but seems to stop at a certain mass. It appears that elements heavier than iron cannot be formed in the core of a star. These elements require more extreme conditions. The heavier elements on the Periodic Table (after Fe) are formed in supernova. These nuclei require tremendous energy to form, this energy must come from an event as large as a supernova.
It is said that when sun dies from hydrogen to iron elements are formed and when busted spread in space .the other elements are formed by chemical reaction by these elements
for making elements from helium to nickel and iron, thermonuclear fusionfor making elements past nickel and iron a supernova explosion is needed to force nuclei to fuse more, this destroys the star
for making elements from helium to nickel and iron, thermonuclear fusionfor making elements past nickel and iron a supernova explosion is needed to force nuclei to fuse more, this destroys the star
Chemical elements are formed in the Universe by stellar nucleosynthesis.
In cool stars, elements such as hydrogen and helium are primarily produced through nuclear fusion in their cores. Elements heavier than helium (e.g., carbon, oxygen, and iron) are formed through nucleosynthesis processes during the later stages of a star's lifecycle, such as in red giant stars or during supernova events.
Such elements are formed within stars. The heavy elements which are currently here on Earth were formed in stars some time ago, and then they were blown into space in supernova explosions.