+Wien's Law quantifies the inverse relationship between a black body's temperature and the peak wavelength of its emitted [Thermal Radiation](/wiki/thermal_radiation). This fundamental principle explains why hotter objects, like stars, appear bluer, shifting their peak emission towards shorter wavelengths, a cornerstone of [Astrophysics](/wiki/astrophysics).
+## See also
+- [Black Body](/wiki/black_body)
+- [Planck's Law](/wiki/plancks_law)
+- [Stefan-Boltzmann Law](/wiki/stefan-boltzmann_law)
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