This article begins with the historical problem of how the sun kept warm for so long. It then explains the discovery of radioactivity and how it solved this problem. The final section provides graphs and information about the sun and the chemical reactions that take place within it.
Jet Propulsion Laboratory. (2004). The Nuclear Fire of the Sun. Retrieved February 20, 2017, from http://genesismission.jpl.nasa.gov/educate/scimodule/SunandSolar/Final%20Linked%20SSW/6AppendicesCari/a.pdf
%0 Electronic Source %A Jet Propulsion Laboratory, %D 2004 %T The Nuclear Fire of the Sun %V 2017 %N 20 February 2017 %9 application/pdf %U http://genesismission.jpl.nasa.gov/educate/scimodule/SunandSolar/Final%20Linked%20SSW/6AppendicesCari/a.pdf
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