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How do you calculate the constant in Wien's law? - Answers
Wien's law states that the wavelength at which the intensity of radiation emitted by a black body is maximized is inversely proportional to its temperature. The constant in Wien's law, known as Wien's displacement constant, is approximately (2.898 \times 10^{-3}) m·K. To calculate this constant, you can use the formula (\lambda_{max} = \frac{b}{T}), where (b) is the constant, (\lambda_{max}) is the peak wavelength, and (T) is the absolute temperature in Kelvin. This relationship can be derived from experimental data on black body radiation.
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How do you calculate the constant in Wien's law? - Answers
Wien's law states that the wavelength at which the intensity of radiation emitted by a black body is maximized is inversely proportional to its temperature. The constant in Wien's law, known as Wien's displacement constant, is approximately (2.898 \times 10^{-3}) m·K. To calculate this constant, you can use the formula (\lambda_{max} = \frac{b}{T}), where (b) is the constant, (\lambda_{max}) is the peak wavelength, and (T) is the absolute temperature in Kelvin. This relationship can be derived from experimental data on black body radiation.
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How do you calculate the constant in Wien's law? - Answers
Wien's law states that the wavelength at which the intensity of radiation emitted by a black body is maximized is inversely proportional to its temperature. The constant in Wien's law, known as Wien's displacement constant, is approximately (2.898 \times 10^{-3}) m·K. To calculate this constant, you can use the formula (\lambda_{max} = \frac{b}{T}), where (b) is the constant, (\lambda_{max}) is the peak wavelength, and (T) is the absolute temperature in Kelvin. This relationship can be derived from experimental data on black body radiation.
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- og:descriptionWien's law states that the wavelength at which the intensity of radiation emitted by a black body is maximized is inversely proportional to its temperature. The constant in Wien's law, known as Wien's displacement constant, is approximately (2.898 \times 10^{-3}) m·K. To calculate this constant, you can use the formula (\lambda_{max} = \frac{b}{T}), where (b) is the constant, (\lambda_{max}) is the peak wavelength, and (T) is the absolute temperature in Kelvin. This relationship can be derived from experimental data on black body radiation.
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