Planck's Blackbody Radiation Law
Also known as: Planck's law · Planck radiation formula
Heat any object and it glows — dull red, then orange, then white-hot. Classical physics predicted the glow should carry infinite energy at short wavelengths (the 'ultraviolet catastrophe'). Planck fixed it by a desperate guess: light energy comes in discrete lumps hf, not a continuum. That single assumption bends the spectrum back down at short wavelengths and matches every glowing object perfectly. It was the first crack in classical physics and the birth of the quantum.
The Planck spectrum reshapes as you change temperature; the peak slides toward shorter wavelengths as T rises.
Equivalent forms
One formula spans a campfire, the Sun, and the 2.7 K cosmic microwave background — and it forced h into physics for the first time.
Where it holds
Dimensional analysis
Planck interpolated between Wien's law (good at short wavelengths) and Rayleigh's (good at long ones), then spent months finding a physical justification. On 14 December 1900 he presented it to the German Physical Society, forced to assume oscillators exchange energy only in quanta E = hf. He called it 'an act of desperation' and spent years trying to rid physics of the quantum he had invented.
- Pyrometry: reading a furnace or star's temperature from its color
- The 2.7 K cosmic microwave background
- Incandescent-bulb and infrared-camera design
- Planck did not believe photons were real particles; Einstein took that step in 1905
- The peak wavelength shifts with temperature (Wien's law), but the whole curve rises, not just the peak
- 'Ultraviolet catastrophe' is a later name — Planck was fitting data, not resolving a paradox
What if…
The Bose factor becomes you recover Rayleigh–Jeans — the ultraviolet catastrophe returns and every warm object would blast infinite UV.
The peak wavelength halves (Wien) and the total power rises (Stefan–Boltzmann, .
Peak wavelength of the Sun
- T:
- 5778 K
- Use Wien's law \lambda _\max T = 2.898e-3 m\cdot K
- \lambda _\max = 2.898e-3 / 5778 \approx 5.0e-7\,\mathrm{m}