An astronomer measures a star’s luminosity to be and its surface temperature to be

PHYSICS · Subjective · A Level · Physics · Astrophysics · Astrophysics

Problem

An astronomer measures a star’s luminosity to be 1.2×1028 W1.2\times10^{28}\,\text{W} and its surface temperature to be 9500 K9500\,\text{K}. Given the Sun’s luminosity L⊙=3.9×1026 WL_{\odot}=3.9\times10^{26}\,\text{W} and radius R⊙=6.96×108 mR_{\odot}=6.96\times10^{8}\,\text{m}, determine the radius of the star in units of the solar radius R⊙R_{\odot}. Use σ=5.67×10−8 W m−2K−4\sigma = 5.67\times10^{-8}\,\text{W\,m}^{-2}\text{K}^{-4}.

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