Atomic emission spectra Simplified Revision Notes for NSC Physical Sciences
Revision notes with simplified explanations to understand Atomic emission spectra quickly and effectively.
Learn about Emission and Absorption Spectra for your NSC Physical Sciences Exam. This Revision Note includes a summary of Emission and Absorption Spectra for easy recall in your Physical Sciences exam
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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 spectrumunique 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) → Yellow light.
Barium(Ba) → Green light.
Strontium(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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