Question: The power density radiated by a star [Fig. E3.11(a)] decreases radially as S(R) = S0 / R2, where R is the radial distance from the
(a)
![The power density radiated by a star [Fig. E3.11(a)] decreases](https://dsd5zvtm8ll6.cloudfront.net/si.question.images/image/images10/751-E-E-E(443)-1.png)
(b)
![The power density radiated by a star [Fig. E3.11(a)] decreases](https://dsd5zvtm8ll6.cloudfront.net/si.question.images/image/images10/751-E-E-E(443)-2.png)
7S Figure E3.11
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