Photon Energy from Wavelength (E = hc/λ)

E=hcλE = \frac{h c}{\lambda}

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Combining E = hf with c = fλ gives the spectroscopist's favorite form. The product hc ≈ 1240 eV·nm is worth memorizing: a 620 nm red photon carries 2 eV, a 124 nm ultraviolet photon 10 eV, a 0.1 nm X-ray photon 12.4 keV. Silicon solar cells have a 1.1 eV band gap, so photons with wavelengths longer than about 1100 nm — a third of sunlight's energy — pass straight through and can never be harvested.

Photon Energy from Wavelength (E = hc/λ)
E=hcλE = \frac{h c}{\lambda}
Where
  • EE= Photon energy
  • λ\lambda= Wavelength
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