A star can be modeled as a spherical blackbody that emits and has a peak-emission…

PHYSICS · Subjective · CBSE · Physics · Thermal Properties of Matter · Thermal Properties of Matter

Problem

A star can be modeled as a spherical blackbody that emits 3.9×1026 W3.9\times10^{26}\,\text{W} and has a peak-emission wavelength of 520 nm520\,\text{nm}. Determine the star’s radius. (Use σ=5.67×10−8 W m−2 K−4\sigma = 5.67\times10^{-8}\,\text{W\,m}^{-2}\,\text{K}^{-4} and b=2.90×10−3 m Kb = 2.90\times10^{-3}\,\text{m\,K}.)

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