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Nuclear Fusion Nuclear Fusion is the energy-producing process which takes place continuously in the sun and stars. In the core of the sun at temperatures of 10-15 million degrees Celsius, Hydrogen is converted to Helium providing enough energy for us to sustain life on earth. For energy production on earth, different fusion reactions are involved. The most suitable reaction occurs between the nuclei of the two light forms (isotopes) of Hydrogen - Deuterium and Tritium; eventually reactions involving just Deuterium or Deuterium and Helium may be used. A brief breakdown of the fuels used are as follows, Deuterium is a very abundant isotope of hydrogen and can be extracted from all forms of water, Tritium is not as abundant and is not a natural isotope, instead a machine is needed to extract it from lithium.
Approximate Word count = 500
Approximate Pages = 2
(250 words per page double spaced)
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