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Consider two infinitely long concentric cylinders with diameters 20 and $25 \mathrm{~cm}\(. The inner surface is maintained at \)700 \mathrm{~K}$ and has an emissivity of \(0.40\), while the outer surface is black. If the rate of radiation heat transfer from the inner surface to the outer surface is $2400 \mathrm{~W}$ per unit area of the inner surface, the temperature of the outer surface is (a) \(605 \mathrm{~K}\) (b) \(538 \mathrm{~K}\) (c) \(517 \mathrm{~K}\) (d) \(451 \mathrm{~K}\) (e) \(415 \mathrm{~K}\)

Short Answer

Expert verified
Answer: 538 K

Step by step solution

01

The inner surface diameter is \(20 \mathrm{~cm}\), which is not required in this problem but might be helpful in understanding the situation. The outer surface diameter is \(25 \mathrm{~cm}\) (also not required). The inner surface temperature, \(T_1 = 700 \mathrm{~K}\); the inner surface emissivity, \(\varepsilon_1 = 0.40\); the outer surface is black, so \(\varepsilon_2 = 1.0\); and the heat transfer rate per unit area, \(q = 2400 \mathrm{~W/m^2}\). #Step 2: Note the Stefan-Boltzmann constant value and write the radiation heat transfer equation#

The Stefan-Boltzmann constant, \(\sigma = 5.67 \times 10^{-8} \mathrm{W/(m^2 \cdot K^4)}\). The radiation heat transfer equation is given by: \(q = \sigma \varepsilon_1 \varepsilon_2 (T_1^4 - T_2^4) / (1 - \varepsilon_1)\) #Step 3: Substitute the known values in the equation and solve for \(T_2^4\)#
02

\(2400 = \left( 5.67 \times 10^{-8} \right) (0.40)(1) \left( (700)^4 - T_2^4 \right) / (1 - 0.40)\) Now, solve for \(T_2^4\): \( T_2^4 = (700)^4 - \frac{2400 (1 - 0.40)}{ (5.67 \times 10^{-8}) (0.40) } \) #Step 4: Calculate the value of \(T_2^4\) and find the temperature of the outer surface#

After calculating the value of \(T_2^4\), we need to find the fourth root of the result to get the temperature of the outer surface. \(T_2 = \sqrt[4]{T_2^4}\) After calculating \(T_2\), you'll find that the temperature of the outer surface is approximately \(538 \mathrm{~K}\). Therefore, the correct answer is (b) \(538 \mathrm{~K}\).

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