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The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
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Let your stars shine

Vanessa Sung1

  • 1Vanessa Sung is a Ph.D. candidate at McGill University in Montreal, Canada, and co-president of Science & Policy Exchange. Do you have an interesting career story? Send it to SciCareerEditor@aaas.org.

Science (New York, N.Y.)
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PubMed
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No abstract available in PubMed .

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