A supernova. It is an explosion that crushes the core of the star into a black hole or neutron star, and blasts all of the remaining mass of the star out into space.
We know that our Sun is a 3rd generation star, because the Earth contains elements like iron, gold, lead, or uranium that can ONLY be produced in a supernova.
And us? We're star-stuff; the iron atoms in our blood and the calcium atoms in our bones has already been through at least ONE supernova explosion.
Fusing hydrogen atoms into heavier elements produces helium and releases a large amount of energy in the form of heat and light. This process, known as nuclear fusion, occurs in the core of stars like our sun and is responsible for the sun's energy output.
Lighter elements are composed of fewer protons and neutrons compared to heavier elements. They tend to have fewer total nucleons and lower atomic numbers. Lighter elements are typically found at the beginning of the periodic table, while heavier elements are found towards the end.
What basically happens is that the "dying star" has enormous energy production at the end of its life, due to a kind of instability. The resulting heat will fuse lighter elements into heavier elements - resulting in production of elements at least up to element number 92 (uranium).
The heavier elements in the universe were primarily formed through processes such as stellar nucleosynthesis and supernova explosions. In stars, nuclear fusion combines lighter elements like hydrogen and helium into heavier elements up to iron. Elements heavier than iron are typically formed during supernovae, where the intense energy and neutron capture processes create these elements. Additionally, some heavy elements may also form through the merging of neutron stars.
They were formed in supernovae.
That is called "nuclear fusion".
The fusion of iron into heavier elements cannot support a star because it requires more energy than it produces, leading to a loss of energy and the collapse of the star.
Heavier elements are formed through nuclear fusion processes that take place in the core of a star. Hydrogen atoms undergo fusion to form helium, and then this process continues to create heavier elements by fusing helium atoms together. As the star fuses lighter elements, it produces heavier elements through a series of nuclear reactions.
Fusing hydrogen atoms into heavier elements produces helium and releases a large amount of energy in the form of heat and light. This process, known as nuclear fusion, occurs in the core of stars like our sun and is responsible for the sun's energy output.
The stellar process in which the fusion of hydrogen produces other elements is called nucleosynthesis. This is a key process in the evolution of stars, where lighter elements such as hydrogen and helium are fused together to form heavier elements like carbon, oxygen, and iron.
Heavier atoms which could not be formed as a result of fusion are produced as the result of a star that has run out of fuel exploding. It essentially forces atoms which do not release energy to fuse together.
Elements heavier than iron are formed in super-nova explosions.
They were formed in supernovae.
Earth acquired its heavier elements through a process called nucleosynthesis, which occurred in the cores of stars. During the life cycle of a star, nuclear fusion reactions create heavier elements from lighter ones. When these stars eventually explode in supernovae, they release these heavier elements into space. Over time, these elements are incorporated into new stars and planets, including Earth.
Lighter elements are composed of fewer protons and neutrons compared to heavier elements. They tend to have fewer total nucleons and lower atomic numbers. Lighter elements are typically found at the beginning of the periodic table, while heavier elements are found towards the end.
What basically happens is that the "dying star" has enormous energy production at the end of its life, due to a kind of instability. The resulting heat will fuse lighter elements into heavier elements - resulting in production of elements at least up to element number 92 (uranium).
This process is known as nuclear fusion. It occurs in stars like the sun when lighter elements such as hydrogen are combined to form heavier elements like helium, releasing a large amount of energy in the process.