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The maximum energy in thermal radiation ...

The maximum energy in thermal radiation from a source occurs at the wavelength 4000Å. The effective temperature of the source

A

7000 K

B

80000 K

C

`10^(4)` K

D

`10^(6)` K

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The correct Answer is:
To find the effective temperature of the source based on the maximum energy in thermal radiation occurring at a wavelength of 4000 Å, we can use Wien's displacement law. Here’s the step-by-step solution: ### Step 1: Understand Wien's Law Wien's Law states that the wavelength at which the intensity of radiation is maximum (λm) is inversely proportional to the absolute temperature (T) of the black body. The formula is given by: \[ T = \frac{b}{\lambda_m} \] where: - \( T \) is the absolute temperature in Kelvin, - \( b \) is Wien's displacement constant, approximately \( 2.89 \times 10^{-3} \, \text{m} \cdot \text{K} \), - \( \lambda_m \) is the wavelength in meters. ### Step 2: Convert Wavelength from Angstroms to Meters The given wavelength is 4000 Å. To convert this to meters: \[ \lambda_m = 4000 \, \text{Å} = 4000 \times 10^{-10} \, \text{m} = 4.0 \times 10^{-7} \, \text{m} \] ### Step 3: Substitute Values into the Formula Now, substitute the values of \( b \) and \( \lambda_m \) into the formula: \[ T = \frac{2.89 \times 10^{-3}}{4.0 \times 10^{-7}} \] ### Step 4: Calculate the Temperature Now, perform the calculation: \[ T = \frac{2.89 \times 10^{-3}}{4.0 \times 10^{-7}} = 7225 \, \text{K} \] ### Step 5: Round the Temperature Since the question asks for the effective temperature, we can round this to the nearest thousand: \[ T \approx 7000 \, \text{K} \] ### Conclusion Thus, the effective temperature of the source is approximately 7000 Kelvin. ---

To find the effective temperature of the source based on the maximum energy in thermal radiation occurring at a wavelength of 4000 Å, we can use Wien's displacement law. Here’s the step-by-step solution: ### Step 1: Understand Wien's Law Wien's Law states that the wavelength at which the intensity of radiation is maximum (λm) is inversely proportional to the absolute temperature (T) of the black body. The formula is given by: \[ T = \frac{b}{\lambda_m} \] where: ...
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