Skip to content
Exercises · 8.9

Q.The terminology of different parts of the electromagnetic spectrum is given in the text. Use the formula E=hνE = h\nu (for energy of a quantum of radiation: photon) and obtain the photon energy in units of eV for different parts of the electromagnetic spectrum. In what way are the different scales of photon energies that you obtain related to the sources of electromagnetic radiation?

Karnataka PUCTextbookSubjective· 3mImportance★★★★★
24% · 11/46 Questions
🔒 Locked · start free trial →

You're viewing a preview — the full solution, concept, methods & PYQ mapping are locked.

Start your 14-day free trial to unlock the full solution →

Photon energy is E=hν=hc/λE=h\nu=hc/\lambda. Using representative wavelengths for each band (radio ~1 m, microwave ~1 cm, infrared ~10 μ\mum, visible 400-700 nm, UV ~100 nm, X-ray ~0.1 nm, gamma ray ~1 pm), photon energies range from about 10−610^{-6} eV (radio) to over 10610^{6} eV (gamma rays) -- this huge range directly reflects the different physical processes (from oscillating currents to nuclear transitions) that generate each band.

The formula

E=hν=hcλE=h\nu=\frac{hc}{\lambda}

with h=6.63×10−34h=6.63\times10^{-34} J*s, c=3×108c=3\times10^{8} m/s. Converting to electronvolts (11 eV =1.6×10−19=1.6\times10^{-19} J) gives the handy shortcut

E(eV)=1240λ(nm)E(\text{eV})=\frac{1240}{\lambda(\text{nm})}

Photon energy across the spectrum (one representative wavelength per band)

RegionRepresentative λ\lambdaEE (eV)Typical source
Radio1 m1.24×10−61.24\times10^{-6}Oscillating currents in antennas
Microwave1 cm1.24×10−41.24\times10^{-4}Molecular rotation, oscillators
Infrared10 μ\mum0.1240.124Molecular vibration, thermal emission
Visible400-700 nm1.81.8-3.13.1Electronic transitions in atoms/molecules
Ultraviolet100 nm12.412.4Atomic ionisation, hot sources
X-ray0.1 nm1.24×1041.24\times10^{4}Inner-shell transitions, bremsstrahlung
Gamma ray1 pm1.24×1061.24\times10^{6}Nuclear transitions, particle annihilation

Sample calculations: radio E=1240/(1×109)=1.24×10−6E=1240/(1\times10^{9})=1.24\times10^{-6} eV; gamma ray E=1240/(0.001)=1.24×106E=1240/(0.001)=1.24\times10^{6} eV.

How photon energy relates to the source

Each energy scale matches the energy scale of the physical process that produces it:

  • Radio/microwave (μ\mueV-meV): energies of oscillating currents in circuits/antennas or molecular rotations -- very small, so these come from low-energy motions.
  • Infrared (~0.1 eV): matches the spacing of molecular vibrational energy levels and thermal (blackbody) emission from warm objects. …

Unlock everything free for 14 days

  • Full step-by-step solutions
  • Concept-first explanations
  • Methods, shortcuts & mistakes
  • PYQ mapping + timed mock tests

Full access for 14 days. No credit card required.