Need help with transfer of heat/radiation/emissivity problem

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The problem involves a concrete wall that is 0.18 m thick, with an inside temperature of 22.8°C and an outside temperature of 0.0°C. When the building is unheated, the wall emits radiant energy equal to the heat lost through conduction. To find the emissivity of the wall, the equations Q = eσAT⁴ for radiation and Q = kA(ΔT)/L for conduction are used. The calculations show that the wall emits radiant energy at a rate that indicates an emissivity of 1, meaning it behaves like a perfect emitter. Understanding these principles of heat transfer is crucial for solving the problem.
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The concrete wall of a building is 0.18 m thick. The temperature inside the building is 22.8°C, while the temperature outside is 0.0°C. Heat is conducted through the wall. When the building is unheated, the inside temperature falls to 0.0°C, and heat conduction ceases. However, the wall does emit radiant energy when its temperature is 0.0°C. The radiant energy emitted per second per square meter is the same as the heat lost per second per square meter due to conduction. What is the emissivity of the wall?


This is the problem I have to solve. I was thinking that I might need to use a combination of equations to solve this such as: H=kA(delta)T/L or Q=e(stefan-bolzmann constant)At(T^4).

But I don't even know where to start. Please help me!

thank you :smile:
 
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To solve this problem, you will need to use the equation Q = eσAT⁴, where Q is the rate of heat transfer (in watts per square meter) due to radiation, e is the emissivity of the wall, σ is the Stefan-Boltzmann constant (5.67 × 10⁻⁸ W/m²K⁴), A is the area of the wall (in square meters), and T is the temperature difference between the inside and outside (in Kelvin).Since heat conduction ceases when the inside temperature falls to 0°C, then the rate of heat transfer due to radiation must be equal to the rate of heat transfer due to conduction when the wall was still heated. This means that the rate of heat transfer due to radiation (Q) must equal the rate of heat transfer due to conduction (kA(delta)T/L), where k is the thermal conductivity of the wall, A is the area of the wall (in square meters), deltaT is the temperature difference between the inside and outside (in Kelvin), and L is the thickness of the wall (in meters).By substituting these values into the equation Q = eσAT⁴ and solving for e, you can calculate the emissivity of the wall. In this case, e = 0.042.
 


To solve this problem, we need to understand the concept of emissivity and how it relates to heat transfer. Emissivity is the measure of an object's ability to emit thermal radiation compared to a perfect emitter, which has an emissivity of 1. A perfect absorber also has an emissivity of 1.

In this problem, we know that the wall is emitting radiant energy at the same rate as the heat lost through conduction. This means that the emissivity of the wall must be equal to 1, as it is emitting the same amount of energy as a perfect emitter.

To confirm this, we can use the Stefan-Boltzmann law, which relates the radiant energy emitted by an object to its temperature and emissivity. The equation is Q = εσAT^4, where Q is the radiant energy emitted per second, A is the surface area, T is the temperature, ε is the emissivity, and σ is the Stefan-Boltzmann constant (5.67 x 10^-8 W/m^2K^4).

In this problem, the temperature inside the building is 22.8°C, which is 295.8 K, and the temperature outside is 0.0°C, which is 273.15 K. We also know that the wall is 0.18 m thick, so we can calculate the surface area as A = 0.18 m x 1 m = 0.18 m^2.

Plugging in these values into the equation, we get:

Q = (1)(5.67 x 10^-8 W/m^2K^4)(0.18 m^2)(295.8 K)^4 = 0.0093 W

This is the amount of radiant energy emitted per second per square meter by the wall. Now, we can use the heat transfer equation Q = kAΔT/L to calculate the heat lost per second per square meter through conduction. We know that the temperature difference is 22.8°C, the thickness of the wall is 0.18 m, and the thermal conductivity of concrete (k) is approximately 1 W/mK.

Plugging in these values, we get:

Q = (1 W/mK)(0.18 m^2)(22.8 K)/0.18 m = 22.8 W

Since we know that the radiant energy and heat lost through conduction are
 
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