AP | A-Level | IB | NCERT 11 + 12 – FREE NOTES, RESOURCES AND VIDEOS!
S1.1 - Introduction to the particulate nature of matter S1.2 - The nuclear atom S1.3 - Electron configurations S1.4 - Counting particles by mass - The mole S1.5 - Ideal gases S2.1 - The ionic model S2.2 - The covalent model S2.3 - The metallic model S2.4 - From models to materials S3.1 - The periodic table - Classification of elements S3.2 - Functional groups - Classification of organic compounds R1.1 - Measuring enthalpy changes R1.2 - Energy cycles in reactions R1.3 - Energy from fuels R1.4 - Entropy and spontaneity AHL R2.1 - How much? The amount of chemical change R2.2 - How fast? The rate of chemical change R2.3 - How far? The extent of chemical change R3.1 - Proton transfer reactions R3.2 - Electron transfer reactions R3.3 - Electron sharing reactions R3.4 - Electron-pair sharing reactions

S1.3 - Electron configurations

1.3.1 Emission Spectra 1.3.2 Hydrogen Emission Spectrum and Energy Levels 1.3.3 Main Energy Levels 1.3.4 Sublevels and Atomic Orbital 1.3.5 Electron Configuration 1.3.6 Ionization Energy and Spectral Interpretation (AHL) 1.3.7 Successive Ionization Energies and Electron Configuration (AHL)

Emission Spectra and Electromagnetic Radiation

Specification Reference S1.3.1

Quick Notes

  • Emission spectra are produced when electrons fall from higher to lower energy levels, releasing energy as photons.
  • Each photon corresponds to a specific wavelength (or frequency) of light.
  • The electromagnetic spectrum includes all types of light, from radio waves to gamma rays.
  • Energy, frequency, and wavelength are all related:
    • Higher frequency = shorter wavelength = higher energy
    • Lower frequency = longer wavelength = lower energy
  • Visible light ranges from:
    • Red: longest wavelength, lowest energy
    • Violet: shortest wavelength, highest energy
  • A continuous spectrum shows all wavelengths (e.g., white light through a prism).
  • A line spectrum shows only specific wavelengths emitted by excited atoms.

Full Notes:

What Is an Emission Spectrum?

When an atom absorbs energy (e.g., from heat or electricity), its electrons jump to higher energy levels – this is called the excited state.

But electrons don’t stay excited forever. They soon fall back to lower energy levels, and when they do, they release energy in the form of light (photons).

IB Chemistry diagram showing electrons absorbing energy, moving to higher energy levels, and releasing photons as they fall back down.

Each jump from one energy level to another releases a photon of a specific energy, which corresponds to a specific wavelength and colour of light.

This can be observed in an emission spectrum — a set of bright lines against a dark background, each one representing a specific transition.

Example – Hydrogen Emission Spectrum

The hydrogen emission spectra shows the specific energies emitted by electrons as they fall to the n = 2 energy level from higher energy levels in an atom of hydrogen.

IB Chemistry hydrogen emission spectrum showing lines corresponding to electron transitions to n=2 energy level.

Continuous vs Line Spectra

A continuous spectrum (like sunlight passed through a prism) contains all visible wavelengths without gaps – it looks like a rainbow.

A line spectrum (like that from hydrogen gas) shows only specific wavelengths. Each line corresponds to an electron transition.

IB Chemistry diagram comparing a continuous rainbow spectrum with a line spectrum showing discrete lines for hydrogen.

Line spectra are like fingerprints – unique to each element.

The Electromagnetic Spectrum: Key Relationships

The electromagnetic spectrum includes many types of radiation, from radio waves to gamma rays. These differ in their:

General relationships:

The section of the electromagnetic spectrum we can see is the visible light range (approx. 400–700 nm):

IB Chemistry electromagnetic spectrum diagram showing wavelength, frequency, and energy from radio waves through visible light to gamma rays.

So, in visible light:

Summary