Asked • 06/05/19

How to explain the existence of heavier elements in Population I stars and in Population II stars contain lighter one?

Recently I read Astrophysics Notes where I found a statement that young stars are classified as Population I stars and relatively older one as Population II stars. Population I stars contain heavier elements or "Metals" - that means elements other than helium and hydrogen. While Population II contain older stars and they contain Hydrogen and Helium - lighter elements more in abundance.My doubt is that, stars begin their journey from Hydrogen in nebula. In course of time due to nuclear reactions more and more heavier nuclei are created,and hence Population I stars which should contain lighter elements in much abundance and the older Population II stars should contain heavier elements. Whether the explanation of the Notes is wrong? or any other plausible explanation? Please clarify.

1 Expert Answer

By:

Allen P. answered • 06/08/19

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