Difference between revisions of "Terminology:Fusion (Nuclear-)"
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Nuclear Fusion is the energy-producing process which takes place continuously in suns/stars. In the core of a sun at temperatures of 10-15 million degrees Celsius, Hydrogen is converted to Helium providing enough energy to sustain life on [[Terminology:Earth|earth]]. | Nuclear Fusion is the energy-producing process which takes place continuously in suns/stars. In the core of a sun at temperatures of 10-15 million degrees Celsius, Hydrogen is converted to Helium providing enough energy to sustain life on [[Terminology:Earth|earth]]. | ||
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* [[WikiPedia:Fusion]] | * [[WikiPedia:Fusion]] | ||
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| − | [[Category:Terminology]] | + | [[Category:Terminology|Fusion (Nuclear-)]] |
Latest revision as of 20:07, 4 March 2005
 Terminology
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Nuclear Fusion is the energy-producing process which takes place continuously in suns/stars. In the core of a sun at temperatures of 10-15 million degrees Celsius, Hydrogen is converted to Helium providing enough energy to sustain life on earth.
