Respuesta :
The answer is nuclear fusion.
Nuclear fusion is the process that produces the energy in the stars. The simplest example of this process is the hydrogen-to-helium fusion, where two nuclei of hydrogen combine together into a nucleum of helium. In the process, a huge amount of energy is released, according to Einstein's famous equivalence:
[tex]E=mc^2[/tex]
where m is the mass difference between the total mass of the initial nuclei and the mass of the final products, and c is the speed of light.
Nuclear fusion is the process that produces the energy in the stars. The simplest example of this process is the hydrogen-to-helium fusion, where two nuclei of hydrogen combine together into a nucleum of helium. In the process, a huge amount of energy is released, according to Einstein's famous equivalence:
[tex]E=mc^2[/tex]
where m is the mass difference between the total mass of the initial nuclei and the mass of the final products, and c is the speed of light.
Nuclear fission is the process that produces the largest amount of energy given off by stars. It happens when a large nucleus undergoes collision with any other particle.
What is Nuclear Fission?
When a heavier nucleus splits simultaneously due to the impact of with another particle, then some energy is released and this phenomenon is known as Nuclear fission.
In stars, nuclear fission takes place on the account of the interaction between hydrogen and helium. The two nuclei of hydrogen combine together into a nucleus of helium. In the process, a huge amount of energy is released, according to Einstein's famous equivalence:
[tex]E = mc^{2}[/tex]
Here, m is the mass difference between the total mass of the initial nuclei and the mass of the final products, and c is the speed of light.
Thus, we can conclude that nuclear fission is the process that produces the largest amount of energy given off by stars.
Learn more about Nuclear fission here:
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