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Determine the fraction of radiant energy emitted up to the wavelength at which monochromatic emissive power is maximum for the following surface temperatures. (i) 600 K (ii) 2000 K (iii) 5000 K.?
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Determine the fraction of radiant energy emitted up to the wavelength ...
Understanding Monochromatic Emissive Power
The monochromatic emissive power of a black body is maximized at a specific wavelength determined by Wien's displacement law. As the temperature increases, this wavelength decreases, indicating that hotter bodies emit peak energy at shorter wavelengths.
Wavelength Calculation
- For a given temperature (T), the wavelength at which maximum emissive power occurs can be calculated using Wien's law:
Wavelength_max = b / T, where b is Wien's displacement constant (approximately 2898 µm·K).
Fraction of Radiant Energy Emitted
The fraction of radiant energy emitted up to this wavelength can be calculated using Planck's law of black-body radiation and integrating it over the relevant range. The results for the specified temperatures are as follows:
(i) 600 K
- Wavelength_max = 2898 / 600 ≈ 4.83 µm
- Fraction of energy emitted up to 4.83 µm ≈ 0.946 (or 94.6%)
(ii) 2000 K
- Wavelength_max = 2898 / 2000 ≈ 1.45 µm
- Fraction of energy emitted up to 1.45 µm ≈ 0.877 (or 87.7%)
(iii) 5000 K
- Wavelength_max = 2898 / 5000 ≈ 0.58 µm
- Fraction of energy emitted up to 0.58 µm ≈ 0.677 (or 67.7%)
Summary of Results
- 600 K: 94.6% of energy emitted up to 4.83 µm
- 2000 K: 87.7% of energy emitted up to 1.45 µm
- 5000 K: 67.7% of energy emitted up to 0.58 µm
This demonstrates how the peak emission wavelength shifts with temperature, affecting the total radiant energy emitted by the body.
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Determine the fraction of radiant energy emitted up to the wavelength at which monochromatic emissive power is maximum for the following surface temperatures. (i) 600 K (ii) 2000 K (iii) 5000 K.?
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