The energy of a photon, which is the energy of the light, can be calculated using the following two formulas:

The second formula is derived from the first by using the relationship between the frequency (ν), wavelength (λ), and speed of light (c) Plank’s constant:
\[\upsilon \;{\rm{ = }}\;\frac{c}{\lambda }\]
Before going over some examples, remember the following features of the energy, wavelength, and frequency of light:

Some key correlations about the parameters of light: Higher energy means shorter wavelength (λ) and higher frequency (ν), and lower energy indicates longer wavelength (λ) and lower frequency (ν).
Calculating the Energy of One Photon
Example: A photon has a wavelength of 462 nm. Calculate the energy of the photon in joules.
Solution: Frequency (ν) is inversely proportional to the wavelength (λ) and they are correlated by the following formula:
E = hν
\[\upsilon \;{\rm{ = }}\;\frac{c}{\lambda }\]
Therefore, we can substitute the frequency (ν) with this expression and get a new formula correlating the energy and the wavelength:
\[E\; = h\upsilon \; = \;\frac{{hc}}{\lambda }\]
Always make sure all the units in the formula match! In this case, we need to match the units of wavelength to those of c (speed of light) which is 3 x 108 m/s, and because 1 nm = 10-9 m, we add the 10-9 exponent in the denominator.
\[E\; = \;\frac{{hc}}{\lambda }\; = \;\frac{{\left( {{\rm{6}}{\rm{.626}}\; \times \;{{10}^{ – 34}}\;{\rm{J}} \cdot \cancel{{\rm{s}}}} \right)\,\left( {3\; \times \,{{10}^8}\,\cancel{{\rm{m}}}{\rm{/}}\cancel{{\rm{s}}}} \right)}}{{462\, \times \,{{10}^{ – 9}}\;\cancel{{\rm{m}}}}}\; = \;4.30\, \times \;{10^{ – 19}}\,{\rm{J}}\]
Note: This is the energy of one photon and can also be written as 4.30 x 10-19 J/photon.
Calculating the Energy Based on the Moles of Photons
Example: What is the energy of 1 mol of photons, in kJ, for a 724 nm red light?
Solution: Remember, the formula correlating the energy and the wavelength is for one photon. Therefore, we can calculate the energy of one photon for the light of 724 nm wavelength. Once we find this, we can multiply the value by Avogadro’s number to determine the energy of one mole of photons.
So, first, let’s calculate the energy of one photon:
\[E\; = \;\frac{{hc}}{\lambda }\; = \;\frac{{\left( {{\rm{6}}{\rm{.626}}\; \times \;{{10}^{ – 34}}\;{\rm{J}} \cdot \cancel{{\rm{s}}}} \right)\,\left( {3\; \times \,{{10}^8}\,\cancel{{\rm{m}}}{\rm{/}}\cancel{{\rm{s}}}} \right)}}{{724\, \times \,{{10}^{ – 9}}\;\cancel{{\rm{m}}}}}\; = \;2.7\underline 4 558\, \times \;{10^{ – 19}}\,{\rm{J/photon}}\]
The underlined number is to keep track of three significant figures which we will round off the final answer to.
Now, because one mole contains 6.02 x 1023 photons, we need to multiply the energy of one photon by Avogadro’s number:
\[E\; = \;2.7\underline 4 558\,{\rm{ \times }}\;{\rm{1}}{{\rm{0}}^{{\rm{ – 19}}}}\,\frac{{\rm{J}}}{{\cancel{{{\rm{photon}}}}}}\;{\rm{ \times }}\;\frac{{{\rm{6}}{\rm{.02}}\,{\rm{ \times }}\;{\rm{1}}{{\rm{0}}^{{\rm{23}}}}\,\cancel{{{\rm{photon}}}}}}{{{\rm{1}}\;{\rm{mol}}}}\;{\rm{ = }}\,{\rm{165,284}}\,{\rm{J/mol}}\;{\rm{ = }}\;{\rm{165}}\;{\rm{kJ/mol}}\]
Calculating the Number of Photons
Example: Calculate the number of photons in a laser pulse with a wavelength of 537 nm that contains 6.29 mJ (milli Joules) of energy.
Solution: Remember, the formula correlating the energy and the wavelength is for one photon. Therefore, we can calculate the energy of one photon for the light of 537 nm wavelength. Once we find this, we can compare it with 6.29 mJ to determine how many photons would make that much energy.
So, first, let’s calculate the energy of one photon:
\[E\; = \;\frac{{hc}}{\lambda }\; = \;\frac{{\left( {{\rm{6}}{\rm{.626}}\; \times \;{{10}^{ – 34}}\;{\rm{J}} \cdot \cancel{{\rm{s}}}} \right)\,\left( {3\; \times \,{{10}^8}\,\cancel{{\rm{m}}}{\rm{/}}\cancel{{\rm{s}}}} \right)}}{{537\, \times \,{{10}^{ – 9}}\;\cancel{{\rm{m}}}}}\; = \;3.7\underline 0 167\, \times \;{10^{ – 19}}\,{\rm{J/photon}}\]
Next, we need to match the units of energy. We can convert the J to mJ (1 J = 1000 mJ).
\[E\; = \;3.7\underline 0 167\;{\rm{ \times }}\;{\rm{1}}{{\rm{0}}^{{\rm{ – 19}}}}\,\cancel{{\rm{J}}}\,{\rm{ \times }}\;\frac{{{\rm{1000}}\;{\rm{mJ}}}}{{{\rm{1}}\;\cancel{{\rm{J}}}}}\, = \;3.7\underline 0 167\;{\rm{ \times }}\;{\rm{1}}{{\rm{0}}^{{\rm{ – 16}}}}\;{\rm{mJ}}\]
And now, we use this energy as a conversion factor to determine the number of photons:
\[{\rm{N(photons)}}\;{\rm{ = }}\,\;\frac{{{\rm{1}}\,{\rm{photon}}}}{{3.7\underline 0 167\;{\rm{ \times }}\;{\rm{1}}{{\rm{0}}^{{\rm{ – 16}}}}\;\cancel{{{\rm{mJ}}}}}}\;{\rm{ \times }}\,6.29\,\cancel{{{\rm{mJ}}}}\;{\rm{ = }}\;1.70\, \times \;{10^{16}}\;{\rm{photons}}\]
Alternatively, you can set up a cross-multiplication correlation for the energy and the number of photons:
1 photon – 3.701675 x 10-16 mJ
x photons – 6.29 mJ
Cross multiplying x with 3.701675 x 10-16 mJ, and 1 with 6.29 mJ, we can find the x:
\[{\rm{x}}\; = \;\frac{{{\rm{1}}\;{\rm{photon}}\;{\rm{ \times }}\;{\rm{6}}{\rm{.29}}\,\cancel{{{\rm{mJ}}}}}}{{3.701675\;{\rm{ \times }}\;{\rm{1}}{{\rm{0}}^{{\rm{ – 16}}}}\;\cancel{{{\rm{mJ}}}}}}\;{\rm{ = }}\;{\rm{1}}{\rm{.70}}\,{\rm{ \times }}\;{\rm{1}}{{\rm{0}}^{{\rm{16}}}}\;{\rm{photons}}\]
Check this 95-question, Multiple-Choice Quiz on the Electronic Structure of Atoms including questions on properties of light such as wavelength, frequency, energy, quantum numbers, atomic orbitals, electron configurations, and more.
Periodic Table and Periodic Trends
Electronic Structure of Atoms Quiz
Check Also
- Atomic Orbitals
- Electron Configurations
- Electron Configurations of Ions
- Orbital Diagrams
- Aufbau’s Principle, Hund’s Rule, and Pauli’s Exclusion Principle
- Hund’s Rule
- Pauli Exclusion Principle
- Quantum Numbers (n, l, ml, ms)
- Bohr Model of the Hydrogen Atom
- Rydberg Formula
- The Photoelectric Effect
- Ionization Energy
- Electron Affinity
- Energy, Wavelength, and Frequency Practice Problems
Practice
What is the wavelength of the photon needed to excite an electron from the E1 to E4 level for a hypothetical atom given the following energy levels:






