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Atomic emission spectra Simplified Revision Notes

Revision notes with simplified explanations to understand Atomic emission spectra quickly and effectively.

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Atomic emission spectra

1. Definition and Key Concepts

  • Atomic emission spectra are produced when a gas is heated or an electric current is passed through it.
  • Electrons in atoms absorb energy and move to a higher energy level (excited state), which is unstable.
  • When electrons return to their ground state, they emit energy in the form of light (photons).

2. Characteristics of Atomic Emission Spectra

  • The wavelength (colour) of emitted light depends on the energy difference between the excited and ground states.
  • Only certain frequencies of light are emitted, producing a line spectrum unique to each element.
  • Colours outside the visible range, such as ultraviolet and infrared, are not visible.

3. Applications of Atomic Emission Spectra

  • Element Identification: Each element has a unique emission spectrum, allowing scientists to identify substances.
    • Sodium (Na)(Na) → Yellow light.
    • Barium (Ba)(Ba) → Green light.
    • Strontium (Sr)(Sr) → Red light.
  • Fireworks: Colours are produced by different metallic salts.
  • Astronomy: Scientists use emission spectra to analyse distant stars and planets.

4. Key Takeaways

  • Emission spectra are unique "fingerprints" for elements.
  • Excited electrons release photons when returning to lower energy levels.
  • Used in chemical analysis, fireworks, and astronomy.
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