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A black body at 1000°c radiates 14.89 watt per square centimetre of its surface. The surfaceof a certain star radiates 10 kW per square centimetre. Assuming that the star’s surface behaves as a perfect blackbody, estimate its temperature.

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Data: T1 = 273 + 1000 = 1273K,

R1 = 14.89 watt/cm2 = 14.89 × 104 watt/m2,

R2 = 10 kW/cm2 = 107 watt/cm2

Emissive power of a blackbody, R = σT4

∴ This is the temperature of the star’s surface.

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