According to Wien's displacement law
\(\lambda_{m}=\frac{b}{T} \Rightarrow T=\frac{b}{\lambda_{m}}=\frac{2.93 \times 10^{-3}}{4000 \times 10^{-10}}=7325 \mathrm{K}\)
KEY CONCEPTS
Wien's Displacement Law According to Wien's law the product of wavelengths corresponding to maximum intensity of radiation and temperature of body (in Kelvin) is constant, ie., \(\lambda_{\mathrm{m}} \mathrm{T}=\mathrm{b}=\) constant where \(\mathrm{b}\) is Wien's constant and has value \(2.89 \times 10^{-3} \mathrm{m}-\mathrm{K}\)

Wien's displacement Law According to Wien's law the product of wavelength corresponding to maximum intensity of radiation and temperature of body (in Kelvin) is constant, i.e.
\(\lambda_{\mathrm{m}} \mathrm{T}=\mathrm{b}=\) constant
Where b is Wien's constant and has value \(2.89 \times 10^{-3} \mathrm{mk}\)
As the temperature of the body increases, the wavelength at which the spectral intensity \(\left(\mathrm{E}_{\lambda}\right)\) is maximum shifts towards left. Therefore it is also called Wien's displacement law.

\(\mathrm{T}_{3}>\mathrm{T}_{2}>\mathrm{T}_{1}\)
\(\lambda_{\mathrm{m}_{2}}<\lambda_{\mathrm{m}_{2}}<\lambda_{\mathrm{m}_{2}}\)
This law is of great importance in 'Astrophysics' as through the analysis of radiations coming from a distant star, by finding \(\lambda_{\mathrm{m}}\) the temperature of the star \(\mathrm{T}\left(=\frac{\mathrm{b}}{\lambda_{\mathrm{m}}}\right)\) is determined
Examples on Wien's law The sun has a temperature of \(5800 \mathrm{K}\). What is the sun's wavelength of maximum emission?
Wavelength of maximum emission \(=2900 /\) Object's temperature in Kelvin
Sun's wavelength of maximum emission \(=2900 / 5800=0.5\) microns