Consider a surface at \(500 \mathrm{~K}\). The spectral blackbody emissive power at a wavelength of \(50 \mu \mathrm{m}\) is (a) \(1.54 \mathrm{~W} / \mathrm{m}^{2} \cdot \mu \mathrm{m}\) (b) \(26.3 \mathrm{~W} / \mathrm{m}^{2} \cdot \mu \mathrm{m}\) (c) \(108.4 \mathrm{~W} / \mathrm{m}^{2} \cdot \mu \mathrm{m}(d) 2750 \mathrm{~W} / \mathrm{m}^{2} \cdot \mu \mathrm{m}(e) 8392 \mathrm{~W} / \mathrm{m}^{2} \cdot \mu \mathrm{m}\)

Short Answer

Expert verified
Answer: The spectral blackbody emissive power at a wavelength of 50 µm for a surface at 500 K is approximately 1.54 W/m²·µm.

Step by step solution

01

Write down Planck's Law formula

Planck's Law describes the spectral distribution of blackbody radiation and can be written as: $$ E_\lambda(\lambda, T) = \frac{2 \pi h c^2}{\lambda^5} \frac{1}{e^{\frac{hc}{\lambda k_BT}} - 1} $$ Where: \(E_\lambda\) is the spectral blackbody emissive power (\(\mathrm{W} / \mathrm{m}^{2} \cdot \mu \mathrm{m}\)), \(\lambda\) is the wavelength (\(\mathrm{m}\)), \(h\) is the Planck constant (\(6.626 \times 10^{-34} \mathrm{~Js}\)), \(c\) is the speed of light (\(2.998 \times 10^{8} \mathrm{~m/s}\)), \(T\) is the temperature in Kelvin (K), \(kB\) is the Boltzmann constant (\(1.381 \times 10^{-23} \mathrm{~J/K}\)).
02

Convert given wavelength to meters

The given wavelength is 50 µm, which we need to convert to meters for the calculation: $$ \lambda = 50 \times 10^{-6} \mathrm{~m} $$
03

Calculate the spectral blackbody emissive power

Now, we can plug in the given data into the Planck's Law formula to determine the spectral blackbody emissive power \(E_\lambda\): $$ E_\lambda = \frac{2 \pi (6.626 \times 10^{-34}) (2.998 \times 10^{8})^2}{(50 \times 10^{-6})^5} \frac{1}{e^{\frac{(6.626 \times 10^{-34})(2.998 \times 10^{8})}{(50 \times 10^{-6})(1.381 \times 10^{-23})(500)}} - 1} $$ After performing the calculations, we get: $$ E_\lambda \approx 1.54 \mathrm{~W} / \mathrm{m}^{2} \cdot \mu \mathrm{m} $$ The spectral blackbody emissive power at a wavelength of 50 µm for a surface at 500 K is approximately 1.54 \(\mathrm{W} / \mathrm{m}^{2} \cdot \mu \mathrm{m}\), which corresponds to option (a).

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