Wien’s Displacement Law — formula and the two peak wavelengths to know?
essential emrHot things glow short, cool things glow long. That’s the whole law in plain terms.
That’s exactly why we use VIS/NIR sensors to capture reflected sunlight, and thermal infrared sensors to capture Earth’s own heat — at night, in the dark, all the time.
λ_max = 2897.8 / T (µm, T in K)
Hotter → shorter peak wavelength.
Hot = short, cool = long. Sun hot → 0.48 µm (visible). Earth cool → 9.66 µm (thermal IR). That's why we use VIS/NIR for reflected solar and thermal IR for emitted Earth.