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Journal of Radioanalytical and Nuclear Chemistry

, Volume 266, Issue 2, pp 159–163 | Cite as

Nuclear systematics

Part IV. Neutron-capture cross sections and solar abundance
  • O. Manuel
  • M. Pleess
  • Y. Singh
  • W. A. Myers
Article

Summary

The abundance pattern of s-process nuclides confirms severe mass separation in the Sun and in the parent star that gave birth to the Solar System. The most abundant elements in the interior of the Sun are Fe, Ni, O, Si and S. These five, even-Z elements with high nuclear stability comprize the bulk material of ordinary meteorites and rocky planets close to the Sun. The Sun and other stars operate as giant, magnetic mass-separators that selectively move lightweight elements, and the lighter mass isotopes of each element, to the surface.

Keywords

Physical Chemistry Inorganic Chemistry Solar System Bulk Material Abundant Element 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag/Akadémiai Kiadó 2005

Authors and Affiliations

  • O. Manuel
    • 1
  • M. Pleess
    • 2
  • Y. Singh
    • 3
  • W. A. Myers
    • 4
  1. 1.Nuclear Chemistry, University of Missouri
  2. 2.Nuclear Chemistry, University of Missouri
  3. 3.Nuclear Chemistry, University of Missouri
  4. 4.Department of Chemical Engineering, University of Arkansas

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