Question:medium

A star radiates heat as a black body at temperature ' (T) '. The total radiant energy per unit area received at a distance ' (R) ' from the centre of a star of radius ' (r) ' is : ((\sigma =) Stefan's constant)

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Intensity follows the inverse square law ($I \propto 1/R^2$).
Updated On: May 12, 2026
  • (\frac{\sigma r^2 T^4}{R^2})
  • (\frac{\sigma r^2 T^4}{4\pi R^2})
  • (\frac{\sigma r^2 T^4}{R^4})
  • (\frac{4\pi \sigma r^2 T^4}{R^2})
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The Correct Option is A

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