Wien’s Displacement Law describes the relationship between the temperature of a black body and the wavelength at which it emits radiation most strongly. The law states that the peak emission wavelength (lambda_{max}) is inversely proportional to the absolute temperature (T). This relationship is expressed by the formula:
b = Wien’s displacement constant (approximately 2.89777 Γ 10β»Β³ mΒ·K)
T = absolute temperature in Kelvin
This law is fundamental in understanding the thermal radiation properties of objects and plays a crucial role in various fields such as astrophysics, spectroscopy, and thermodynamics.
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