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The energy radiated per unit surface area (across all wavelengths) for a black body with temperature 2200. Use 5.67 x 10-8 for the Stefan-Bo
Question
The energy radiated per unit surface area (across all wavelengths) for a black body with temperature 2200. Use 5.67 x 10-8 for the Stefan-Boltzmann constant.The ____________ describes the power radiated from a black body in terms of its temperature. Specifically, the total energy radiated per unit surface area of a black body across all wavelengths per unit time is proportional to the fourth power of the black body’s thermodynamic temperature
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2021-07-29T17:06:57+00:00
2021-07-29T17:06:57+00:00 1 Answers
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Answer:
Stefan-Boltzmann Law describes the power radiated from a black body in terms of its temperature. Specifically, the total energy radiated per unit surface area of a black body across all wavelengths per unit time is proportional to the fourth power of the black body’s thermodynamic temperature
Explanation:
So we now know that
energy per unit area is = zigma x T^4
From this
T = temperature in kelvin
zigma is stefan boltzman constant
So
E/A = 5.67 x 10^-8 x (2200)⁴
= 1.33x 10^6 W/m^2