Atomic absorption spectra Simplified Revision Notes for NSC Physical Sciences
Revision notes with simplified explanations to understand Atomic absorption 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 absorption spectra
1. Definition and Key Concepts
An atomic absorption spectrum is a continuous spectrum with missing frequencies (dark lines).
These dark lines occur when specific wavelengths of light are absorbed by atoms in a cool gas.
Electrons in the gas absorb energy from the light and move to a higher (excited) energy state.
The energy absorbed is equal to the energy difference between electron energy levels.
2. Characteristics of Atomic Absorption Spectra
The missing wavelengths correspond to specific elements in the gas.
Each element has a unique absorption spectrum, acting as a "fingerprint".
Absorption lines appear at the same positions as emission lines for the same element.
The higher the frequency of light absorbed, the higher the energy level of electrons.
3. Applications of Atomic Absorption Spectra
Identifying Elements in Stars:
Astronomers use absorption spectra to determine which elements are present in stars and galaxies.
Chemical Analysis:
Used in flame tests to identify metals.
Medical and Industrial Uses:
Analysing blood samples or detecting metal contamination in water.
4. Key Takeaways
Absorption spectra are unique for each element.
Dark lines in a spectrum indicate which wavelengths have been absorbed.
Combining an element's emission and absorption spectra results in a continuous spectrum.
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