1.

Each square metre of sun’s surface radiates energy at the rate of 6.27×107 Wm−2. Assuming that Stefan’s law applies to the radiation, the temperature of sun’s surface is (Stefan’s constant σ=5.7×107 Wm−2K−4)

Answer»

Each square metre of sun’s surface radiates energy at the rate of 6.27×107 Wm2. Assuming that Stefan’s law applies to the radiation, the temperature of sun’s surface is (Stefan’s constant σ=5.7×107 Wm2K4)





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