UV-Visible spectroscopy

Why is a carrot orange and a sugar cube colourless, when both are made of ordinary carbon, hydrogen and oxygen atoms? The answer lies in how far an electron has to jump. UV-Visible spectroscopy watches electrons absorb a photon and leap from a filled molecular orbital to an empty one — and the energy gap for that jump, set by how much a molecule's double bonds are conjugated, decides whether the absorbed light is invisible UV or visible colour. This article builds the electronic-transition picture (which orbitals, which energies, which intensities), the chromophore/auxochrome vocabulary, the qualitative conjugation trend, and the quantitative Beer-Lambert law used to turn an absorbance reading into a concentration.

The core insight

An electron absorbs a UV or visible photon to jump from a filled orbital to an empty one, with π→π∗\pi\to\pi^* transitions growing stronger and shifting to longer wavelength as conjugation extends the delocalized π\pi system, while the absorbance itself obeys the Beer-Lambert law A=εclA=\varepsilon c l.

The core idea

Four transition types, ranked by energy. Absorbing a photon in the UV-visible range promotes an electron from a bonding or non-bonding orbital into an antibonding orbital. Highest energy (shortest wavelength) to lowest:

  • σ→σ∗\sigma\to\sigma^*: out of a σ\sigma-bond, needs very high energy (<150 nm<150~\text{nm}, far/vacuum UV), seen in saturated hydrocarbons only.
  • n→σ∗n\to\sigma^*: a heteroatom lone pair into a σ∗\sigma^* orbital, typically 150150-250 nm250~\text{nm}, seen in alcohols, amines, alkyl halides.
  • π→π∗\pi\to\pi^*: out of a π\pi-bond, needs an unsaturated group (C=C, C=O, aromatic ring); strongest absorptions (ε∼103\varepsilon\sim10^3-105 L mol−1cm−110^5~\text{L mol}^{-1}\text{cm}^{-1}), and the one that moves into the visible with conjugation.
  • n→π∗n\to\pi^*: a lone pair (e.g. carbonyl oxygen) into a π∗\pi^* orbital; weak and symmetry-disfavoured (ε∼10\varepsilon\sim10-100 L mol−1cm−1100~\text{L mol}^{-1}\text{cm}^{-1}), at longer wavelength than the π→π∗\pi\to\pi^* of the same group.

Chromophores and auxochromes. A chromophore is the functional group that itself absorbs (an isolated C=C or C=O). An auxochrome does not absorb strongly on its own but, attached to a chromophore, donates electron density into the π\pi system and shifts/intensifies its absorption (-OH, -NH2_2, -Cl on a benzene ring or conjugated chromophore).

Conjugation narrows the gap. As more alternating double bonds link together, the π\pi electrons delocalize over a longer system. Delocalization lowers the energy of the bonding combinations and raises the energy of the antibonding ones less steeply, so the HOMO-LUMO gap shrinks and λmax\lambda_{max} moves to longer wavelength. Four standard shift terms describe this:

  • Bathochromic (red) shift — λmax\lambda_{max} to longer wavelength.
  • Hypsochromic (blue) shift — λmax\lambda_{max} to shorter wavelength.
  • Hyperchromic effect — absorption intensity (ε\varepsilon) increases.
  • Hypochromic effect — absorption intensity (ε\varepsilon) decreases.
Figure
Energy level diagram showing four molecular orbital transitions ranked by increasing wavelength from sigma star to n pi star
Electronic transitions, ranked by energy orbital energy sigma* sigma sigma to sigma* (below 150 nm) n n to sigma* (150-250 nm) pi pi to pi* (shifts into visible) n n to pi* (weak, longest wavelength) Longer arrows = smaller energy gap = longer absorbed wavelength

Quantitatively, once a chromophore is chosen, the absorbance measured at its λmax\lambda_{max} follows the Beer-Lambert law:

A=ε c lA = \varepsilon\, c\, l

where: AA is absorbance (dimensionless), ε\varepsilon is the molar absorptivity (L mol−1cm−1\text{L mol}^{-1}\text{cm}^{-1}, characteristic of the transition), cc is molar concentration (mol L−1\text{mol L}^{-1}), and ll is the path length through the sample (cm, usually 1.00 cm1.00~\text{cm} for a standard cuvette).

Derivation AGetting Beer-Lambert from light passing through a solution

Show that if each thin slice of an absorbing solution removes a fixed fraction of the light passing through it, the total light lost across a finite path length grows exponentially with concentration and path length, and that taking a logarithm of the transmitted fraction turns this exponential relationship into the linear law A=εclA=\varepsilon c l used to read off concentration from a single absorbance measurement.

Step 1. Consider light of intensity II travelling through a thin slice of solution of thickness dxdx, containing absorbing molecules at concentration cc. Each slice removes a fraction of the light proportional to both the number of absorbing molecules present (proportional to c dxc\,dx) and the intensity arriving, since more molecules or more incident photons both mean more absorption events: −dI=k c I dx-dI = k\, c\, I\, dx, where kk is a proportionality constant tied to how strongly the molecule absorbs at that wavelength.

Step 2. Separate variables and integrate from the incident intensity I0I_0 at x=0x=0 to the transmitted intensity II at x=lx=l: ∫I0IdII=−kc∫0ldx\int_{I_0}^{I}\frac{dI}{I} = -k c\int_0^l dx, which gives ln⁡ ⁣(II0)=−kcl\ln\!\left(\dfrac{I}{I_0}\right) = -k c l, an exponential decay of intensity with path length, exactly the pattern expected if each successive slice absorbs the same fraction of whatever light reaches it.

Step 3. Define the transmittance T=I/I0T = I/I_0 (the fraction of light that gets through) and the absorbance A=−log⁡10T=log⁡10(I0/I)A = -\log_{10}T = \log_{10}(I_0/I), a base-10 logarithm chosen purely by convention. Converting Step 2's natural log to base 10 by dividing by ln⁡10\ln 10, and absorbing the constants k/ln⁡10k/\ln 10 into a single new constant ε\varepsilon (the molar absorptivity), gives A=ε c lA = \varepsilon\, c\, l: absorbance is directly, linearly proportional to concentration and path length, which is why a single absorbance reading at known ε\varepsilon and ll is enough to solve for an unknown cc.

Worked example

Problem: A dye solution has λmax=480 nm\lambda_{max}=480~\text{nm} with molar absorptivity ε=2.10×104 L mol−1cm−1\varepsilon = 2.10\times10^4~\text{L mol}^{-1}\text{cm}^{-1}. In a 1.00 cm1.00~\text{cm} cuvette at 480 nm480~\text{nm}, a sample of unknown concentration gives A=0.630A=0.630. Find the concentration, identify the likely transition type, and then find what path length would be needed to read exactly A=1.000A=1.000 for the same solution.

Step 1. Rearrange Beer-Lambert for concentration: c=Aεl=0.630(2.10×104 L mol−1cm−1)(1.00 cm)=3.00×10−5 mol L−1c = \dfrac{A}{\varepsilon l} = \dfrac{0.630}{(2.10\times10^4~\text{L mol}^{-1}\text{cm}^{-1})(1.00~\text{cm})} = 3.00\times10^{-5}~\text{mol L}^{-1}.

Step 2. Identify the transition: λmax=480 nm\lambda_{max}=480~\text{nm} is in the visible region, and ε≈2×104 L mol−1cm−1\varepsilon\approx2\times10^4~\text{L mol}^{-1}\text{cm}^{-1} is large, the signature of a fully allowed transition. This is a π→π∗\pi\to\pi^* transition in an extensively conjugated chromophore (typical of azo dyes) rather than a weak n→π∗n\to\pi^* transition, which would give ε\varepsilon two to three orders of magnitude smaller.

Step 3. For the follow-up, hold ε\varepsilon and cc fixed (same solution, same wavelength) and solve for ll: l=Aεc=1.000(2.10×104)(3.00×10−5)=1.0000.630≈1.587 cml=\dfrac{A}{\varepsilon c}=\dfrac{1.000}{(2.10\times10^4)(3.00\times10^{-5})}=\dfrac{1.000}{0.630}\approx1.587~\text{cm}. The concentration is 3.00×10−5 mol L−13.00\times10^{-5}~\text{mol L}^{-1}, the transition is a conjugated π→π∗\pi\to\pi^*, and a 1.59 cm1.59~\text{cm} cuvette would give exactly A=1.000A=1.000.

Competitive stretch

Unconjugated alkenes absorb near λmax≈175 nm\lambda_{max}\approx175~\text{nm} (π→π∗\pi\to\pi^*); 1,3-butadiene, with two conjugated double bonds, absorbs at λmax≈217 nm\lambda_{max}\approx217~\text{nm}. In the delocalized picture, the four 2p2p orbitals of the four sp² carbons combine into four π\pi molecular orbitals (π1,π2,π3∗,π4∗\pi_1,\pi_2,\pi_3^*,\pi_4^*); the filled HOMO is π2\pi_2 and the empty LUMO is π3∗\pi_3^*. Delocalization narrows this HOMO-LUMO gap below the localized π\pi-π∗\pi^* gap of an isolated double bond, giving the observed bathochromic shift from 175175 to 217 nm217~\text{nm} — the same mechanism, extended over roughly eleven conjugated double bonds, that makes carotenoids strongly coloured.

Common traps

  • Assuming "colourless" means "no UV-Vis absorption." Acetone is colourless yet absorbs strongly in the UV (its carbonyl transitions sit below about 350 nm350~\text{nm}, outside the visible range the eye detects); UV-Vis absorption and visible colour are not synonyms.
  • Mixing up which transition is intense. n→π∗n\to\pi^* is weak (symmetry-disfavoured) and π→π∗\pi\to\pi^* is strong (allowed); do not assume all electronic transitions give comparably sized peaks.
  • Calling an auxochrome a chromophore. An auxochrome (-OH, -NH2_2) has no strong absorption of its own; it only modifies an existing chromophore's absorption once attached to it.
  • Trusting Beer-Lambert at high concentration. The linear A=εclA=\varepsilon cl relationship holds only in the dilute regime; aggregation and intermolecular interactions cause real deviations at high cc.

Ask the tutor: if you want more practice converting between conjugation length and lambda max, or extra Beer-Lambert rearrangement problems, just ask.

Why does conjugation length affect colour but a single isolated double bond never does

A single isolated C=C has only one π\pi and one π∗\pi^* orbital, so its HOMO-LUMO gap stays large and its π→π∗\pi\to\pi^* transition needs a high-energy UV photon (around 175 nm175~\text{nm}), far outside visible light. As more double bonds conjugate, the π\pi electrons delocalize over more orbitals, the gap keeps shrinking, and eventually the absorbed photon energy drops into the visible range, which is why long conjugated systems like carotenoids or dyes are coloured while single alkenes never are.

Is molar absorptivity the same thing as absorbance

No. Absorbance AA is what you actually read off the instrument for a specific sample, and it changes with concentration and path length. Molar absorptivity ε\varepsilon is a fixed property of the molecule at a given wavelength, independent of how concentrated your particular sample is or how thick your cuvette is; it is the proportionality constant that links AA to cc and ll in A=εclA=\varepsilon c l.

Why is an n to pi star transition allowed at all if it is symmetry disfavoured

Symmetry-disfavoured does not mean symmetry-forbidden in a strict sense the way some spin-forbidden transitions are; the lone pair (n) orbital and the pi orbital have relatively poor spatial overlap, so the transition probability is low but not zero. That is why n to pi bands are real, observable, and useful diagnostically (they are how carbonyl compounds are distinguished from purely conjugated hydrocarbons), just consistently weaker than the well-overlapping pi to pi* bands of the same molecule.

Before this

Where this leads