Answered: (4) (i) Using the solar compositions… | bartleby

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(4) (i) Using the solar compositions from Lecture 3, derive the mean atomic mass of stellar
material and the number of free electrons per nucleon for the Sun
(ii) Repeat this
calculation assuming the cases of a) all Hydrogen, b) all Helium, and c) all heavy elements.

For Solar composition, μ = 0.61

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