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SOLVED: Fill in the cquation for thc Stefan-Boltzmann law for the luminosity L of a blackbody using R for the radius, for the Stefan Boltzmann constant; and for temperature04T"IncontcctWhat part of the equation describes the surface area of sphere?sut fuce area of sphere;IncottecMultiplying the radius by . fuctor of 3 will increase the luminosity by what fuctor?

SOLVED: Fill in the cquation for thc Stefan-Boltzmann law for the lumi…

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The Stefan-Boltzmann law predicts the power of total electromagnetic radiation (including light) emitted by a heated body from a unit area: P=σT^4 , where or =5.67 ·10^-5 W /(m^2 K^4). Here the power is measured in watts (W) and temperature T is in the Kelvin scale. a) Use the size of the Sun and its surface temperature of 6,000 K to estimate the total energy emitted per second. b) Use the scaling that was discussed in section 4.5 to determine the power per unit area away from the Sun at Ear

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