An astronomer measures a star’s luminosity to be 1.2×1028W and its surface temperature to be 9500K. Given the Sun’s luminosity L⊙=3.9×1026W and radius R⊙=6.96×108m, determine the radius of the star in units of the solar radius R⊙. Use σ=5.67×10−8Wm−2K−4.