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The hot glowing surfaces of stars emit energy in the form of electromagnetic radiation. It is a good approximation to assume that the Emissivity e is equal to 1 for these surfaces.
Find the radius RRigel of the star Rigel, the bright blue star in the constellation Orion that radiates energy at a rate of 2.7 x 1031 W and has a surface temperature of 11,000 K. Assume that the star is spherical Use σ = 5.67 × 10-8 w/m2-K4 for the Stefan-Boltzmann constant and express your answer numerically in meters to two significant figures.
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