• atoms can receive external energy via heat, electricity, and/or EM radiation (light/photons)
  • when an electron absorbs a photon with energy equal to the difference between its current energy level and another, it enters an excited state and transitions to the higher energy level 1
    • if the energy is too high, the electron can escape the atom and the atom becomes ionized
  • excited electrons are unstable want to return to the most stable, e.g. the lowest possible, energy level, called the ground state
    • ground state — lower energy, stable
    • excited state — higher energy, unstable
  • when an electron transitions from a higher energy level to a lower one, it emits a photon
  • the energy/frequency of the emitted photon is determined by the difference in energy between the two levels the electron transitioned between
  • each element has unique discrete energy levels where its electrons can exist
    • due to having different numbers of protons and electrons
  • because of each elements’ unique energy levels, the light emitted by atoms of each element will have a distinct combination of frequencies
  • this unique signature of frequencies is the atomic spectra of an element
  • by analyzing the atomic spectra of some body [%, like a planet or star, we can determine its elemental composition
    • this is called spectral analysis
  • molecules also have unique sets of energy levels, and therefor unique spectra

Energy levels

Hydrogen energy level diagram
A transition from ‍n=6 to ‍n=2 emits a high-energy violet photon, matching the larger energy gap between those levels. A transition from n=3 to ‍n=2 emits a lower-energy red photon, matching the smaller gap. Khan Academy, CC BY-NC-SA 3.0
  • atoms have an infinite number of energy levels, but a finite amount of energy is required for an electron to escape its atom
  • an energy level diagram helps predict the photon energies by an atom

Two types of spectra

Hydrogen absorption and emission spectra
Khan Academy, CC BY-NC-SA 3.0

Absorption spectra

  • light from another source (a star) passing through cooler gas (like a planet’s atmosphere) 2
  • the cooler atoms absorb the light, but when the electrons transition down and emit their photons, the emitted photons are scattered in random directions
  • the light that was travelling from the source to us/Earth, will have fewer of the specific frequencies absorbed/emitted

Emission spectra

  • light directly emitted from excited atoms
  • only the specific photon frequencies from electrons transitioning from higher to lower energy levels

Tools

  • spectroscope — uses a diffraction grating to analyze the spectrum of a light source

Footnotes

  1. TODO — what happens if an atom receives multiple types of energy at the same time? eg. if an electron normally requires energy from an 100nm frequency photon to move from to , if the atom is heated up and receives some smaller frequency photon (<100nm), can the heat energy combine with the photon energy and transition the photon from to as well, or does the energy have to the same type?

  2. TODO — can liquids/solids produce atomic spectra?