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The Sun is a main-sequence star, and thus generates its energy by nuclear fusion of hydrogen nuclei into helium.
The sun generates energy from a process called nuclear fusion. During nuclear fusion, the high pressure and temperature in the sun's core cause nuclei to separate from their electrons. Hydrogen nuclei fuse to form one helium atom. During the fusion process, radiant energy is released.
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=> The reaction responsible for large energy production in the sun is called as NUCLEAR FUSSION REACTION which is totally differ from nuclear fission reaction.
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