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"The stars above us, govern our conditions"
 

Computer simulation of a Red Giant star.
Computer simulation of a Red Giant star.

The origins of chemical elements found on Earth-nuclear reactions that take place in stars—were discovered and confirmed by researchers supported by the Office of Science and predecessor agencies. The late William Fowler of the California Institute of Technology won half of the 1983 Nobel Prize in physics for his work in elucidating this process of nucleosynthesis. Fowler carried out experimental studies of nuclear reactions of astrophysical interest as well as theoretical calculations. During the 1950s, he and co-workers developed a complete theory of the formation of the chemical elements in the universe. (Their paper opens with the above quote from Shakespeare's King Lear.) An extensive series of neutron capture measurements performed at the Oak Ridge Electron Linear Accelerator since the 1970s further substantiated the theory. Other research conducted at national laboratories using reactions involving unstable nuclei also has contributed to understanding of the inner workings of astrophysical objects.

Scientific Impact: This work has yielded fundamental understanding of the chemical evolution of the galaxy and formation and age of the solar system. Fowler's theory remains the basis of knowledge in this field, and recent progress in nuclear physics and space research has further confirmed its correctness.

Social Impact: Scientists now know that half of the chemical elements heavier than iron were synthesized in Red Giant stars and dispersed throughout the galaxy as stardust blown by stellar winds. These elements are essential to human life; in other words, humans are made of stardust.

Reference: "Synthesis of the Elements in Stars," E. M. Burbidge et al., Rev. Mod. Phys. 29: 547 (1957).

URL: http://library.thinkquest.org/17940/texts/nucleosynthesis/nucleosynthesis.html

Technical Contact: Dr. Gene Henry, gene.henry@science.doe.gov

Press Contact: Jeff Sherwood, DOE Office of Public Affairs, 202-586-5806

SC-Funding Office: Office of High Energy and Nuclear Physics

http://www.science.doe.gov
Back to Decades of Discovery home Updated: March 2001

 

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