Wien’s Displacement Law — formula and the two peak wavelengths to know?

essential emr

Hot things glow short, cool things glow long. That’s the whole law in plain terms.

  • The Sun is super hot, so it glows in visible light (we can see it).
  • The Earth is cool, so it glows in thermal infrared (we can’t see it, but our sensors can).

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.

🔬 Science / formula

λ_max = 2897.8 / T (µm, T in K)

  • Sun (~6000 K): λ_max ≈ 0.483 µm (visible)
  • Earth (~300 K): λ_max ≈ 9.66 µm (thermal IR)

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.