/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 13 A copper sphere is suspended in ... [FREE SOLUTION] | 91Ó°ÊÓ

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A copper sphere is suspended in an evacuated chamber maintained at \(300 \mathrm{~K}\). The sphere is maintained at constant temperature of \(900 \mathrm{~K}\) by heating electrically. A total of \(300 \mathrm{~W}\) electric power is needed to do this. When half of the surface of the copper sphere is completely blackened, \(600 \mathrm{~W}\) is needed to maintain the same temperature of sphere. The emissivity of copper is (A) \(1 / 4\) (B) \(1 / 3\) (C) \(1 / 2\) (D) 1

Short Answer

Expert verified
The emissivity of copper is \(\frac{1}{3}\).

Step by step solution

01

Write down the Stefan-Boltzmann Law for the power radiated

The power radiated by an object is given by the Stefan-Boltzmann Law: \[P = \epsilon A \sigma T^4\] Where: - \(P\) is the power (in Watts) - \(\epsilon\) is the emissivity (dimensionless) - \(A\) is the area of the object (in m²) - \(\sigma\) is the Stefan-Boltzmann constant, approximately \(5.67 \times 10^{-8} \mathrm{W \cdot m^{-2} \cdot K^{-4}}\) - \(T\) is the temperature of the object (in K)
02

Set up the equations for the two situations

Initially, with the entire sphere non-blackened, we need 300 W to maintain the sphere's temperature. Let's denote the initial emissivity as \(\epsilon_c\), for the initial copper surface. The equation becomes: \[P_1 = 300 = \epsilon_c A\sigma T^4\] When half of the sphere is blackened, we need 600 W to maintain the temperature. The blackened part has an emissivity of 1. Let's denote the black and non-black areas as \(A_b\) and \(A_c\), respectively, and the total area as \(A\), we get: \[P_2 = 600 = (1 \cdot A_b + \epsilon_c A_c) \sigma T^4\]
03

Simplify the equations and solve for the emissivity of copper

First, we know that half the sphere is blackened, so \(A_b = \frac{A}{2}\) and \(A_c = \frac{A}{2}\). We can plug that into the second equation: \[600 = \left(1 \cdot \frac{A}{2} + \epsilon_c \cdot \frac{A}{2}\right) \sigma T^4\] Now, divide the second equation by the first equation: \[\frac{600}{300} = \frac{\left(1 \cdot \frac{A}{2} + \epsilon_c \cdot \frac{A}{2}\right) \sigma T^4}{\epsilon_c A\sigma T^4}\] Simplify the equation: \[\frac{600}{300} = \frac{1 + \epsilon_c}{2\epsilon_c}\] Solve for \(\epsilon_c\): \[\epsilon_c = \frac{1}{3}\] So the correct answer is (B). The emissivity of copper is \(\frac{1}{3}\).

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