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From the Initial to the Present Sun

  • Rudolf Kippenhahn
  • Alfred Weigert
Chapter
Part of the Astronomy and Astrophysics Library book series (AAL)

Abstract

There is evidence on Earth that the sun has shone for more than 3000 million years with about the same luminosity. From radioactive decay in different materials of the solar system, one nowadays assumes that it was formed 4.65 × 109 years ago. Since then, the sun has lived on hydrogen burning, predominantly according to the pp chain, and its interior has been appreciably enriched in 4He. In the following we show how a model of the present sun can be constructed.

Keywords

Solar Neutrino Solar Model Helium Content Neutrino Flux Hydrogen Burning 
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 Berlin Heidelberg 1990

Authors and Affiliations

  • Rudolf Kippenhahn
    • 1
  • Alfred Weigert
  1. 1.GöttingenGermany

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