Properties of Photons
Quick Notes
- When a photon is absorbed, an atom or molecule gains energy and may undergo an electronic transition to a higher energy level.
- When a photon is emitted, the atom or molecule loses energy as the electron drops to a lower energy level.
- Photon energy (E) is related to its frequency (f) by Planck’s equation:
- E = h × f
- Where E is Energy, h is Planck's constant and f is frequency
- Wavelength (λ) and frequency are related to the speed of light (c) by the equation:
- c = λ × f
- Where c is speed of light, λ is wavelength and f is frequency
- Note that freqency is also shown as v in equations
Full Notes
Photons are packets of electromagnetic energy. When atoms or molecules absorb or emit photons, electrons can transition between different energy levels.
Energy Transitions and Photons

- If a photon is absorbed, the energy of the atom or molecule increases, and an electron moves to a higher energy level.
- If a photon is emitted, the energy of the atom or molecule decreases, and an electron falls to a lower energy level.
The amount of energy absorbed or released corresponds exactly to the energy of the photon.
Planck’s Equation – Photon Energy
The energy of a photon is directly proportional to its frequency:

E = h × v
- E = energy of the photon (in joules)
- h = Planck’s constant (6.626 × 10-34 J·s)
- v = frequency of the electromagnetic wave (in s-1)
Speed of Light and Wavelength
The frequency of a wave is related to its wavelength (λ) and the speed of light (c):

c = λ × v
- c = speed of light (3.00 × 108 m/s)
- λ = wavelength (in meters)
- v = frequency (in s-1)
Using both equations together allows us to calculate the energy of a photon from either its frequency or wavelength.
Worked Example
Question: What is the energy of a photon with a wavelength of 400 nm?
- Step 1: Convert wavelength to meters
λ = 400 nm = 4.00 × 10-7 m - Step 2: Use c = λ × f to find frequency
f = c ÷ λ = (3.00 × 108 m/s) ÷ (4.00 × 10-7 m) = 7.50 × 1014 s-1 - Step 3: Use Planck’s equation to find energy
E = h × f = (6.626 × 10-34 J·s) × (7.50 × 1014 s-1)
E = 4.97 × 10-19 J
Answer: 4.97 × 10-19 J

Always check your units when working with wavelength or frequency. If you’re given nm, convert to meters before using c = λ × f. Also remember that shorter wavelengths = higher energy photons.
Summary
- Photons carry energy that can be absorbed or emitted by atoms and molecules during electronic transitions.
- The energy of a photon (E) depends on its frequency (f): E = h × f
- c = λ × f
- These relationships allow us to calculate how much energy is transferred during absorption or emission.
- Understanding these equations is essential for interpreting electronic transitions in spectroscopy.