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A sphere of radius 0.350m, temperature 2...

A sphere of radius 0.350m, temperature `27.0^(@)C` , and emissivity 0.850 is located in an environment of temperature `77.0^(@)C`. At what rate does the sphere (a) emit and (b) absorb thermal radiation ? (c ) What is the sphere's net change in energy in 3.50 min ?

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To solve the problem, we will break it down into three parts: (a) calculating the rate at which the sphere emits thermal radiation, (b) calculating the rate at which the sphere absorbs thermal radiation, and (c) determining the net change in energy over a specified time period. ### Given Data: - Radius of the sphere, \( r = 0.350 \, m \) - Temperature of the sphere, \( T_s = 27.0 \, ^\circ C \) - Emissivity of the sphere, \( \epsilon = 0.850 \) - Temperature of the environment, \( T_e = 77.0 \, ^\circ C \) ### Step 1: Convert Temperatures to Kelvin To use the Stefan-Boltzmann law, we need to convert the temperatures from Celsius to Kelvin. \[ T_s = 27.0 + 273.15 = 300.15 \, K \] \[ T_e = 77.0 + 273.15 = 350.15 \, K \] ### Step 2: Calculate the Surface Area of the Sphere The surface area \( A \) of a sphere is given by the formula: \[ A = 4\pi r^2 \] Substituting the radius: \[ A = 4\pi (0.350)^2 \approx 1.539 \, m^2 \] ### Step 3: Calculate the Rate of Emission of Thermal Radiation (Part a) The power emitted by the sphere can be calculated using the Stefan-Boltzmann law: \[ P_{\text{emit}} = \sigma \epsilon A T_s^4 \] Where: - \( \sigma = 5.6704 \times 10^{-8} \, W/m^2K^4 \) (Stefan-Boltzmann constant) Substituting the values: \[ P_{\text{emit}} = (5.6704 \times 10^{-8}) \times 0.850 \times (1.539) \times (300.15)^4 \] Calculating \( (300.15)^4 \): \[ (300.15)^4 \approx 8.073 \times 10^9 \, K^4 \] Now substituting back: \[ P_{\text{emit}} \approx (5.6704 \times 10^{-8}) \times 0.850 \times (1.539) \times (8.073 \times 10^9) \approx 602 \, W \] ### Step 4: Calculate the Rate of Absorption of Thermal Radiation (Part b) The power absorbed by the sphere from the environment is given by: \[ P_{\text{absorb}} = \sigma \epsilon A T_e^4 \] Substituting the values: \[ P_{\text{absorb}} = (5.6704 \times 10^{-8}) \times 0.850 \times (1.539) \times (350.15)^4 \] Calculating \( (350.15)^4 \): \[ (350.15)^4 \approx 1.5 \times 10^{10} \, K^4 \] Now substituting back: \[ P_{\text{absorb}} \approx (5.6704 \times 10^{-8}) \times 0.850 \times (1.539) \times (1.5 \times 10^{10}) \approx 1115 \, W \] ### Step 5: Calculate the Net Change in Energy (Part c) The net power change is given by: \[ P_{\text{net}} = P_{\text{absorb}} - P_{\text{emit}} = 1115 \, W - 602 \, W = 513 \, W \] To find the net change in energy over 3.50 minutes, we convert minutes to seconds: \[ \text{Time} = 3.50 \times 60 = 210 \, s \] Now, calculate the net energy change: \[ \Delta E = P_{\text{net}} \times \text{Time} = 513 \, W \times 210 \, s = 107730 \, J \approx 1.08 \times 10^5 \, J \] ### Summary of Answers: (a) Rate of emission: \( 602 \, W \) (b) Rate of absorption: \( 1115 \, W \) (c) Net change in energy in 3.50 minutes: \( 1.08 \times 10^5 \, J \)
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