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A metal piece is heated up to T K. The t...

A metal piece is heated up to T K. The temperature of the surrounding is t K. The heat lost to the surrounding due to radiation is proportional to

A

`T^(4)-t^(4)`

B

`(T-t^(4))`

C

`(T^(4)+t^(4))`

D

`(T^(4)+t^(4))`

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To solve the problem of determining how the heat lost to the surrounding due to radiation is proportional, we can follow these steps: ### Step 1: Understand the Concept of Radiation Heat Loss The heat lost due to radiation from a surface is described by Stefan-Boltzmann Law, which states that the power radiated per unit area of a black body is proportional to the fourth power of its absolute temperature. ### Step 2: Apply Stefan-Boltzmann Law According to Stefan-Boltzmann Law, the heat loss \( Q \) due to radiation can be expressed as: \[ Q \propto A (T^4 - t^4) \] where: - \( A \) is the surface area of the metal piece, - \( T \) is the absolute temperature of the metal piece, - \( t \) is the absolute temperature of the surroundings. ### Step 3: Identify the Proportionality From the equation \( Q \propto A (T^4 - t^4) \), we can see that the heat loss is proportional to the difference in the fourth powers of the temperatures of the metal piece and its surroundings. ### Step 4: Conclude the Proportionality Thus, the heat lost to the surrounding due to radiation is proportional to: \[ (T^4 - t^4) \] ### Final Answer The heat lost to the surrounding due to radiation is proportional to \( (T^4 - t^4) \). ---

To solve the problem of determining how the heat lost to the surrounding due to radiation is proportional, we can follow these steps: ### Step 1: Understand the Concept of Radiation Heat Loss The heat lost due to radiation from a surface is described by Stefan-Boltzmann Law, which states that the power radiated per unit area of a black body is proportional to the fourth power of its absolute temperature. ### Step 2: Apply Stefan-Boltzmann Law According to Stefan-Boltzmann Law, the heat loss \( Q \) due to radiation can be expressed as: \[ ...
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