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A body at a temperature of 727^(@)C and ...

A body at a temperature of `727^(@)C` and having surface area `5 cm^(2)`, radiations `300 J` of energy each minute. The emissivity is(Given Boltzmann constant `=5.67xx10^(-8) Wm^(-2)K^(-4)`

A

`e= 0.18`

B

`e= 0.02`

C

`e= 0.2`

D

`e= 0.15`

Text Solution

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The correct Answer is:
To find the emissivity of the body, we can use the Stefan-Boltzmann law, which states: \[ Q = e \sigma A T^4 t \] Where: - \( Q \) = total energy radiated (in joules) - \( e \) = emissivity (dimensionless) - \( \sigma \) = Stefan-Boltzmann constant (\( 5.67 \times 10^{-8} \, \text{W/m}^2\text{K}^4 \)) - \( A \) = surface area (in square meters) - \( T \) = absolute temperature (in Kelvin) - \( t \) = time (in seconds) ### Step-by-Step Solution: 1. **Convert Temperature to Kelvin**: The given temperature is \( 727^\circ C \). To convert it to Kelvin: \[ T = 727 + 273 = 1000 \, K \] 2. **Convert Surface Area to Square Meters**: The surface area is given as \( 5 \, \text{cm}^2 \). To convert it to square meters: \[ A = 5 \, \text{cm}^2 = 5 \times 10^{-4} \, \text{m}^2 \] 3. **Convert Time to Seconds**: The energy is radiated per minute, so we need to convert minutes to seconds: \[ t = 1 \, \text{minute} = 60 \, \text{seconds} \] 4. **Substitute Values into the Stefan-Boltzmann Law**: We know that \( Q = 300 \, J \), \( \sigma = 5.67 \times 10^{-8} \, \text{W/m}^2\text{K}^4 \), \( T = 1000 \, K \), \( A = 5 \times 10^{-4} \, \text{m}^2 \), and \( t = 60 \, s \). Plugging these values into the formula: \[ 300 = e \cdot (5.67 \times 10^{-8}) \cdot (5 \times 10^{-4}) \cdot (1000)^4 \cdot 60 \] 5. **Calculate \( T^4 \)**: \[ T^4 = (1000)^4 = 10^{12} \, K^4 \] 6. **Calculate the Right Side**: \[ \text{Right Side} = (5.67 \times 10^{-8}) \cdot (5 \times 10^{-4}) \cdot (10^{12}) \cdot 60 \] \[ = (5.67 \times 5 \times 60) \times 10^{-8 -4 + 12} \] \[ = (1701) \times 10^{0} = 1701 \, W \] 7. **Solve for Emissivity \( e \)**: Rearranging the equation to find \( e \): \[ e = \frac{Q}{\text{Right Side}} = \frac{300}{1701} \] \[ e \approx 0.176 \] 8. **Final Result**: The emissivity \( e \) is approximately \( 0.18 \). ### Conclusion: The emissivity of the body is approximately \( 0.18 \).

To find the emissivity of the body, we can use the Stefan-Boltzmann law, which states: \[ Q = e \sigma A T^4 t \] Where: - \( Q \) = total energy radiated (in joules) - \( e \) = emissivity (dimensionless) - \( \sigma \) = Stefan-Boltzmann constant (\( 5.67 \times 10^{-8} \, \text{W/m}^2\text{K}^4 \)) ...
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Knowledge Check

  • A body at a temperature of 728^@C and having surface area 5 cm^2 , radiates 300 J of energy each minute. The emissivity is [Given Boltzmann constant : = 5.67xx10^(-8) Wm^(-2) K–4^(-4) ]

    A
    e = 0.18
    B
    e = 0.02
    C
    e = 0.2
    D
    e = 0.15
  • A body having a surface area of 50cm^2 radiates 300J of energy per minute at a temperature of 727^(@)C . The emissivity of the body is ( Stefan's constant =5.67xx10^(-8)W//m^2K^4 )

    A
    0.09
    B
    0.018
    C
    0.36
    D
    0.54
  • The surface of a black body is at a tempera ture 727^(@)C and its cross section is 1m^(2) Heat radi ated from this surface in one minute in Joules is (Stefan's constant =5.7 xx 10^(-8) W//m^(2)//k^(4)) .

    A
    `34.2xx10^(5)`
    B
    `2.5xx10^(5)`
    C
    `3.42xx10^(5)`
    D
    `2.5xx10^(6)`
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