The question asks for the peak wavelength ($\lambda_{max}$) of radiation emitted by a black body at a specific temperature. This can be determined using Wien's displacement law.
Wien's displacement law relates the peak wavelength of emitted radiation to the temperature of the black body:
$ \lambda_{max} = \frac{b}{T} $
Where:
Given the temperature $ T = 4000 $ K:
$ \lambda_{max} = \frac{2.898 \times 10^{-3} \text{ m·K}}{4000 \text{ K}} $
$ \lambda_{max} = \frac{2.898 \times 10^{-3}}{4 \times 10^3} \text{ m} $
$ \lambda_{max} = \frac{2.898}{4} \times 10^{-6} \text{ m} $
$ \lambda_{max} = 0.7245 \times 10^{-6} \text{ m} $
Since $ 1 \text{ μm} = 10^{-6} $ m, the result is:
$ \lambda_{max} = 0.7245 \text{ μm} $
Comparing the calculated value $ 0.7245 $ $\mu$m to the options provided, it is closest to $ 0.72 $ $\mu$m.
| A. | Rainbows | P. | Refraction |
| B. | Mirage | Q. | Refraction and Reflection |
| C. | Corona | R. | Refraction, Reflection, Dispersion in ice crystals |
| D. | Halo | S. | Diffraction |