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explain why heavy elements are nucleosynthesized in the interior layer of the stars
Stars are hot and dense enough to burn hydrogen-1 (1H) to helium-4 (4He). The formation of heavy elements by fusion of lighter nuclei in the interior of stars is called “stellar nucleosynthesis”. ... Layers near core of stars have very high temperatures enough to nucleosynthesize heavy elements such as silicon and iron.
Stars are hot and dense enough to burn hydrogen-1 (1H) to helium-4 (4He). The formation of heavy elements by fusion of lighter nuclei in the interior of stars is called “stellar nucleosynthesis”. ... Layers near core of stars have very high temperatures enough to nucleosynthesize heavy elements such as silicon and iron.
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