Electron Energy Levels
- A continuous spectrum is a spectrum that appears to contain all frequencies over a comparatively wide range
- The Sun’s spectrum is not continuous as it shows dark lines where some frequencies are missing
- Bohr explained the existence of spectral lines using the new photon model of electromagnetic radiation
- In addition, Bohr proposed a model of the atom which includes:
- Electrons orbiting the nucleus
- Electrons only occupying specific orbits associated with a discrete set of energies
- The orbits are also called shells or energy levels
- Electrons can gain or lose energy by moving from one allowed energy level to another
Electrons in an atom can have only certain specific (discrete) energies within an atom
- Energy is required for an electron to move from a lower to a higher energy level
- This transition is called an excitation
- Energy is released if the electron moves from a higher to a lower energy level
- This transition is called a de–excitation
- Electrons can move to a higher or lower energy level by absorbing or emitting electromagnetic radiation with a frequency, f
- The energy required for excitation of a gas can be provided by:
- A photon of a specific frequency
- Energy absorbed from the surroundings (through heating)
- Energy supplied by an electric field
- The energy released during de–excitation is emitted as electromagnetic radiation of a specific frequency
- This frequency depends on the difference of energy between the specific energy levels involved in the transition
Examiner Tip
The values of energy level are all given using the unit electron volt (eV), because we are dealing with very small energy values. 1 eV is equal to 1.6 × 10–19 Joules, so to convert between J and eV, remember: