The principle of UV-Visible spectroscopy is based on the absorption of ultraviolet (UV) and visible light by molecules.
Here’s how it works:
- Light source: UV (200–400 nm) and visible (400–800 nm) light is passed through a sample.
- Absorption of photons: Molecules absorb light energy if it matches the energy needed to promote electrons from a lower-energy orbital (usually bonding or non-bonding) to a higher-energy orbital (usually anti-bonding).
- Examples:
- π → π* transitions (in double bonds).
- n → π* transitions (in molecules with lone pairs, like C=O).
- Examples:
- Measurement: The instrument measures how much light is absorbed at each wavelength.
- Spectrum: A plot of absorbance vs. wavelength is obtained, showing peaks at wavelengths where absorption occurs.
From a UV-Vis spectrum, we can learn:
- The presence of conjugated systems (double bonds, aromatic rings).
- The concentration of a compound in solution (using the Beer-Lambert Law).
🔹 Applications:
- Identifying organic and inorganic compounds.
- Measuring concentrations of colored or UV-absorbing substances.
- Studying reaction kinetics and biological molecules like DNA and proteins.
In short: UV-Visible spectroscopy works on the principle that molecules absorb light of specific wavelengths, causing electronic transitions, and the amount of absorption reveals both structural and quantitative information.