The most common fusion in the sun is two hydrogen atoms fusing to produce helium. There are different ways this can happen. Two deuterium atoms may fuse, or a deuterium atom may fuse with a tritium atom, or two tritium atoms may fuse. Since the half life of tritium is rather short, the overwhelming majority of these atoms are deuterium atoms. The commonest form of hydrogen, known as protium, does not take part in the process.
In the most common stellar fusion, helium gas is formed from the fusion of hydrogen nuclei.
Hydrogen is the element that is most likely to undergo nuclear fusion.
Light elements - most commonly hydrogen.
iron
Nuclear fusion is the process that powers stars, such as our sun.
In the most common stellar fusion, helium gas is formed from the fusion of hydrogen nuclei.
Hydrogen is the element that is most likely to undergo nuclear fusion.
Nuclear fusion. The most common process is making helium nuclei from hydrogen nuclei.
Nuclear fusion. In the most common case, hydrogen-1 is converted to helium-4.
Where: In supernovae. How: by nuclear fusion.
Fusion and fission nuclear reactions.
Sun
Instead of making insults like the person who initially posted, here is an answer. Nuclear fusion is most commonly found in stars, such as our sun.
fusion nuclear reaction followed by fission nuclear reaction
nuclear fusion
The Sun gets its energy from nuclear fusion.The Sun gets its energy from nuclear fusion.The Sun gets its energy from nuclear fusion.The Sun gets its energy from nuclear fusion.
Initially as radiation (all types), most of which becomes heat.