Electronic absorption spectrum of iodine vapour: dissociation energy
Aim: to record the B ³Π0u+ ← X ¹Σg+ absorption band system of I₂, assign the vibrational progressions, construct a Birge–Sponer plot, locate the convergence limit, and determine the dissociation energies D₀′ (B state) and D₀″ (ground state).
Absorption spectrometer
Transmission spectrum of the iodine cell
Each dip is the violet-side band head of a v′ ← v″ band. Click a band to mark it. Drag to zoom (the bands crowd together toward 500 nm); double-click to reset.
Observation table
For the convergence limit, enter "conv" as v′Birge–Sponer plot (v″ = 0 progression)
Results
Theory
A band v′ ← v″ lies at
$$ \tilde\nu(v',v'') = T_e + G'(v') - G''(v''),\qquad G(v) = \omega_e(v+\tfrac12) - \omega_ex_e(v+\tfrac12)^2 + \dots $$For a progression from v″ = 0, the spacing between successive bands is the vibrational quantum of the upper state:
$$ \Delta G'(v'+\tfrac12) = \tilde\nu(v'+1,0)-\tilde\nu(v',0) = \omega_e' - 2\omega_e'x_e'(v'+1) .$$The spacing shrinks as the molecule nears dissociation. Plotting ΔG against (v′+1) and extrapolating to zero is the Birge–Sponer method. The area under the line is the dissociation energy of the B state measured from v′ = 0:
$$ D_0' = \sum_{v'} \Delta G'(v'+\tfrac12) \approx \frac{\omega_e'^2}{4\omega_e'x_e'} .$$Above the convergence limit the spectrum turns into a continuum: the molecule dissociates into I(²P₃/₂) + I*(²P₁/₂). Energy conservation then gives the ground-state dissociation energy:
$$ \tilde\nu_{conv} = D_0'' + E(\mathrm I^*) \;\Rightarrow\; D_0'' = \tilde\nu_{conv} - 7603\ \text{cm}^{-1} .$$Accepted values: \(\tilde\nu_{conv}\) ≈ 20 043 cm⁻¹ (≈ 499 nm), \(D_0''\) = 12 440 cm⁻¹ = 1.542 eV, \(\omega_e'\) = 125.7 cm⁻¹, \(\omega_e''\) = 214.5 cm⁻¹.
Procedure
- Warm the cell (40–60 °C) so the vapour pressure gives a peak absorbance of about 0.5–1.
- Record the spectrum from 490 to 650 nm with a narrow slit.
- Identify the v″ = 0 progression (the stronger bands below about 560 nm) and assign v′. Hot bands from v″ = 1 lie 213 cm⁻¹ lower and become stronger as the cell is heated.
- Convert each λ (air) to ν̃ (vacuum), compute ΔG′ for successive bands, and make the Birge–Sponer plot.
- Mark the onset of the continuum (convergence limit) directly as well, and compare it with the extrapolation.
Notes on the model
The X- and B-state constants are from Huber & Herzberg. The B-state vibrational ladder includes a cubic anharmonic term, so the Birge–Sponer plot curves downward near dissociation, as it does for real I₂. A linear extrapolation from low v′ therefore overestimates D₀′, a well-known limitation of the method. Band intensities follow a Franck–Condon envelope (reflection approximation), the hot-band populations a Boltzmann distribution, and the vapour pressure the Clausius–Clapeyron law.
Viva questions
Why are the bands degraded to the red?
B′ < B″ (the B-state bond is longer), so the R-branch forms a head on the high-wavenumber side and the rotational lines spread toward lower wavenumber.
Why does heating change the spectrum?
Heating raises the vapour pressure (more absorption) and the population of v″ = 1 and 2, so the hot bands at longer wavelength grow.
Why add E(I*)?
The B state correlates with one ground-state and one spin–orbit-excited atom. The convergence limit is therefore D₀″ plus the I* excitation energy.