According to Stefan-Boltzmann law, the luminosity (the power of radiation) of the object can be calculated as
L=4πR2σT4=4π⋅(7.1⋅108)2⋅5.67⋅10−8⋅(5700)4=3.8⋅1026 W.L=4\pi R^2\sigma T^4 = 4\pi \cdot (7.1\cdot10^8)^2\cdot 5.67\cdot10^{-8}\cdot (5700)^4 = 3.8\cdot10^{26}\,\mathrm{W}.L=4πR2σT4=4π⋅(7.1⋅108)2⋅5.67⋅10−8⋅(5700)4=3.8⋅1026W.
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