Molecular Orbital Theory
Molecular Orbital (MO) theory is a quantum-mechanical method that constructs delocalized one-electron wavefunctions spanning an entire molecule to predict bond order, magnetism, photoelectron spectra, and frontier orbital reactivity.
Molecular Orbital (MO) theory—also known as Hund–Mulliken theory—is a quantum-mechanical framework in physical, inorganic, and organic chemistry that describes the electronic structure of molecules using delocalized one-electron wavefunctions (molecular orbitals, ψi) that extend across all constituent atomic nuclei rather than being confined to localized two-center bonds between pairs of atoms. Formulated between 1927 and 1932 by Friedrich Hund, Robert S. Mulliken, John E. Lennard-Jones, and Erich Hückel, MO theory complements localized Valence Bond (VB) theory, orbital hybridization, and VSEPR theory by directly explaining phenomena that localized Lewis structures cannot easily capture: the triplet paramagnetism of ground-state dioxygen (O2), fractional bond orders in one- and three-electron species (H2+, He2+), hypervalent three-center four-electron bonds, Hückel 4*n* + 2 aromaticity, ultraviolet-visible electronic excitation spectra, and Frontier Molecular Orbital (HOMO–LUMO) chemical reactivity.
🧪 Interactive Curriculum: Compare Valence Bond hybridization and Molecular Orbital models in the VSEPR & Orbital Bonding Mechanics learning module and VSEPR Lab.
Linear Combination of Atomic Orbitals (LCAO-MO) and the Secular Determinant
Constructive Bonding (ψ+) versus Destructive Antibonding (ψ−)
Within the Born–Oppenheimer approximation (which holds the heavier atomic nuclei at fixed coordinates RA while solving for the rapid motion of the electrons), each molecular orbital ψi is approximated as a Linear Combination of Atomic Orbitals (LCAO) centered on the M nuclei of the molecule:
ψi = ∑*μ*=1K cμi φμ
For a homonuclear or heteronuclear two-orbital interaction between atomic orbital φA on atom A (with Coulomb integral αA = ⟨*φ*A|*Ĥ*|*φ*A⟩) and atomic orbital φB on atom B (with αB = ⟨*φ*B|*Ĥ*|*φ*B⟩), applying the Rayleigh–Ritz variational principle (∂⟨*ψ*|*Ĥ*|*ψ*⟩/∂*c*μ = 0) yields the 2 × 2 secular determinant:
| αA − E , βAB − E SAB | = 0 (and symmetrically for row 2)
where SAB = ⟨*φ*A|*φ*B⟩ is the dimensionless overlap integral (0 ≤ SAB < 1) and βAB = ⟨*φ*A|*Ĥ*|*φ*B⟩ < 0 is the resonance (exchange) integral, which scales approximately with the overlap integral via the Mulliken–Wolfsberg–Helmholz relation βAB ≈ ½ K (αA + αB) SAB.
Solving the secular equation for a homonuclear system (αA = αB = α) yields two normalized molecular orbitals and their corresponding energy eigenvalues:
- The Bonding Molecular Orbital (ψ+, σ or π):
- ψ+ = (φA + φB) / √[ 2(1 + SAB) ]
- E+ = (α + βAB) / (1 + SAB) ≈ α − |*β*AB| + SAB|*β*AB|
- In-phase constructive interference increases electron probability density in the internuclear midpoint (ρmid = (φA + φB)2/[2(1 + SAB)] > ½(φA2 + φB2)), electrostatic shielding the two positively charged nuclei and stabilizing the molecule below α.
- The Antibonding Molecular Orbital (ψ−, σ\* or π\*):
- ψ− = (φA − φB) / √[ 2(1 − SAB) ]
- E− = (α − βAB) / (1 − SAB) ≈ α + |*β*AB| + SAB|*β*AB|
- Out-of-phase destructive interference creates a nodal plane perpendicular to the internuclear axis where electron density drops to zero (ψ− = 0), pushing electron density onto the outer flanks of the nuclei and destabilizing the orbital above α. Because the denominator (1 − SAB) is smaller than (1 + SAB), an antibonding orbital is always destabilized more than its partner bonding orbital is stabilized (Δ*E*antibonding > |Δ*E*bonding|). Consequently, filling both the bonding and antibonding orbitals with four electrons (as in hypothetical He2, 1*σ*g2 1*σ*u*2) yields a net four-electron Pauli repulsion (closed-shell steric repulsion) rather than a covalent bond.
- Non-Bonding Molecular Orbitals (n): If two atomic orbitals have orthogonal symmetries (SAB = 0, such as a px orbital meeting an s orbital along the z-axis) or carry a large energy mismatch (|*α*A − αB| ≫ |*β*AB|), no mixing occurs, leaving a non-bonding molecular orbital at its original atomic energy E ≈ α (corresponding to a localized lone pair).
Bond Order, Diatomic Correlation Diagrams, and *s*–*p* Mixing
Formal Bond Order and Second-Period Homonuclear Diatomics
In MO theory, the covalent bond order (BO) is defined as half the difference between the number of electrons occupying bonding orbitals (Nb) and the number occupying antibonding orbitals (Na*):
Bond Order (BO) = ½ ( Nbonding − Nantibonding )
Across the second-period homonuclear diatomic series (Li2 through Ne2), the valence 2*s* and 2*p* subshells combine into eight molecular orbitals: two σ orbitals from 2*s* (2*σ*g and 2*σ*u*), two coaxial σ orbitals from 2*p*z (3*σ*g and 3*σ*u*), and two degenerate pairs of lateral π orbitals from 2*p*x and 2*p*y (1*π*u and 1*π*g*). Here the subscripts g (gerade, even) and u (ungerade, odd) denote whether the wavefunction retains (+1) or inverts (−1) its sign upon inversion through the molecular center of symmetry (i): σ bonding orbitals are g (σg) and *σ*\* antibonding orbitals are u (σu*), whereas π bonding orbitals are u (πu) and *π*\* antibonding orbitals are g (πg*).
In the lighter diatomics (Li2, Be2, B2, C2, and N2), the atomic 2*s*–2*p* energy separation is relatively small (from 1.85 eV in Li to 10.9 eV in N). Because the 2*σ*g (from 2*s*) and 3*σ*g (from 2*p*z) molecular orbitals share identical σg symmetry, they undergo second-order s–p mixing: 2*σ*g is pushed lower in energy while 3*σ*g is pushed upward above the degenerate 1*π*u(2px,*y*) pair, producing the "inverted" (π-below-σ) ordering (1*π*u < 3*σ*g) for B2, C2, and N2. In O2 and F2, the large effective nuclear charge (Zeff) widens the atomic 2*s*–2*p* energy gap (>15–20 eV), suppressing s–p mixing and restoring the "normal" (σ-below-π) ordering (3*σ*g < 1*π*u).
| Diatomic Species | Valence Electrons | Ground-State Valence MO Configuration | Bond Order | Unpaired Spins & Magnetism | Bond Length (r0) | Dissociation Energy (*D*°0) |
|---|---|---|---|---|---|---|
| H2+ | 1 | (1*σ*g)1 | 0.5 | 1 (Paramagnetic, 2Σg+) | 1.052 Å | 255 kJ mol−1 |
| H2 | 2 | (1*σ*g)2 | 1.0 | 0 (Diamagnetic, 1Σg+) | 0.741 Å | 436 kJ mol−1 |
| He2+ | 3 | (1*σ*g)2 (1*σ*u*)1 | 0.5 | 1 (Paramagnetic, 2Σu+) | 1.081 Å | 228 kJ mol−1 |
| B2 | 6 | (2*σ*g)2 (2*σ*u*)2 (1*π*u)2 | 1.0 (π bond) | 2 (Paramagnetic triplet, 3Σg−) | 1.590 Å | 290 kJ mol−1 |
| C2 | 8 | (2*σ*g)2 (2*σ*u*)2 (1*π*u)4 | 2.0 (two π) | 0 (Diamagnetic singlet, 1Σg+) | 1.243 Å | 602 kJ mol−1 |
| N2 | 10 | (2*σ*g)2 (2*σ*u*)2 (1*π*u)4 (3*σ*g)2 | 3.0 | 0 (Diamagnetic, 1Σg+) | 1.098 Å | 945 kJ mol−1 |
| O2 | 12 | (2*σ*g)2 (2*σ*u*)2 (3*σ*g)2 (1*π*u)4 (1*π*g*)2 | 2.0 | 2 (Paramagnetic triplet, 3Σg−) | 1.208 Å | 498 kJ mol−1 |
| O2− (Superoxide) | 13 | … (3*σ*g)2 (1*π*u)4 (1*π*g*)3 | 1.5 | 1 (Paramagnetic radical, 2Πg) | 1.33 Å | 395 kJ mol−1 |
| O22− (Peroxide) | 14 | … (3*σ*g)2 (1*π*u)4 (1*π*g*)4 | 1.0 | 0 (Diamagnetic, 1Σg+) | 1.49 Å | 146 kJ mol−1 |
| F2 | 14 | (2*σ*g)2 (2*σ*u*)2 (3*σ*g)2 (1*π*u)4 (1*π*g*)4 | 1.0 | 0 (Diamagnetic, 1Σg+) | 1.412 Å | 159 kJ mol−1 |
Frontier Molecular Orbitals (HOMO–LUMO), Aromaticity, and Woodward–Hoffmann Rules
Perturbation Theory and HOMO–LUMO Donor-Acceptor Reactivity
In heteronuclear bonds (A–B where χB > χA, so αB < αA), second-order perturbation theory gives the stabilization energy Δ*E* ≈ −|*β*AB|2 / |*α*A − αB|:
- The lower-energy bonding MO (ψ+) has a larger coefficient on the more electronegative atom B (|*c*B| > |*c*A|), polarizing bonding electrons toward B.
- The higher-energy antibonding MO (ψ−, σ\* or π\*) has a larger coefficient on the less electronegative atom A (|*c*A| > |*c*B|), explaining why nucleophilic attack on a polar C=O or C–Br bond always occurs at the electropositive carbon atom where the LUMO lobe is largest.
As formulated by Kenichi Fukui (1952) and Roald Hoffmann and Robert B. Woodward (1965, awarded the 1981 Nobel Prize in Chemistry), most bimolecular chemical reactions are governed by the interaction between the Highest Occupied Molecular Orbital (HOMO) of the electron-donor nucleophile and the Lowest Unoccupied Molecular Orbital (LUMO) of the electron-acceptor electrophile:
- Nucleophilic Substitution (SN2): The nucleophile's HOMO (lone pair n) attacks the backside lobe of the substrate's C–X *σ*\* LUMO at 180°, populating *σ*\* to cleave the C–X bond while forming the new C–Nu σ bond with stereochemical Walden inversion.
- Woodward–Hoffmann Conservation of Orbital Symmetry: Concerted pericyclic reactions (such as the [4+2] Diels–Alder cycloaddition between a 4π diene HOMO and a 2π dienophile LUMO, or electrocyclic ring closures of vitamin D precursors in human skin under ultraviolet light) proceed with low activation energy only when the terminal lobes of the interacting frontier orbitals have matching algebraic phase signs (suprafacial/antarafacial selection rules).
- Hückel's 4*n* + 2 Aromaticity Rule: In planar cyclic conjugated polyenes (CmHm), solving the Hückel secular determinant yields a Frost circle of π molecular orbitals with a unique lowest orbital (a2u in benzene) followed by degenerate pairs (e1g, e2u, …). Planar rings containing 4*n* + 2 π electrons (n = 0, 1, 2, …; e.g., 6 π electrons in benzene, adenine, and tryptophan, or 18 π electrons in the porphyrin macrocycle of heme and chlorophyll) completely fill all bonding shells to achieve closed-shell aromatic stabilization, whereas 4*n* rings (such as 4π cyclobutadiene) leave half-filled non-bonding degenerate orbitals that undergo Jahn–Teller distortion (antiaromaticity).
Frequently Asked Questions
Why does ionizing an electron from nitric oxide (NO → NO+) or dioxygen (O2 → O2+) shorten and strengthen the bond instead of weakening it?
In most molecules (such as N2 → N2+, where bond order drops from 3.0 to 2.5 and bond length stretches from 1.098 Å to 1.116 Å), removing a valence electron ejects it from a bonding molecular orbital. However, in nitric oxide (NO, 11 valence electrons) and dioxygen (O2, 12 valence electrons), the Highest Occupied Molecular Orbital (HOMO) is the antibonding *π*\*2*p* orbital (occupied by one electron in NO and two unpaired electrons in O2). Ionizing NO to the nitrosonium cation (NO+, isoelectronic with N2 and CO) or O2 to the dioxygenyl cation (O2+) removes an antibonding *π*\* electron, increasing the formal bond order from 2.5 to 3.0 in NO+ (shortening the N–O bond from 1.15 Å to 1.06 Å and raising the IR stretching frequency from 1,876 cm−1 to 2,377 cm−1) and from 2.0 to 2.5 in O2+ (r0 drops from 1.208 Å to 1.116 Å; *D*° rises from 498 to 643 kJ mol−1).
How does ground-state triplet oxygen (3O2) differ chemically from reactive singlet oxygen (1O2)?
In its lowest-energy ground state (3Σg− triplet dioxygen, 3O2), the two degenerate antibonding 1*π*g* orbitals each contain one electron with parallel spins (↑ and ↑) in accordance with Hund's rule. Because nearly all organic biomolecules (lipids, proteins, DNA) have closed-shell singlet ground states (all electrons spin-paired, ↑↓), a direct concerted two-electron reaction between triplet 3O2 and a singlet organic molecule to give singlet products is spin-forbidden by conservation of angular momentum, creating a kinetic barrier that prevents spontaneous combustion of living tissue in air. When a photosensitizer (such as excited triplet chlorophyll or porphyrin) transfers energy (94.3 kJ mol−1 / 0.98 eV) to 3O2, it flips one spin to generate singlet oxygen (1Δg, 1O2), in which both electrons are paired in one πg* orbital while the second πg* orbital is completely vacant—turning 1O2 into a spin-allowed electrophile (reactive oxygen species) that rapidly attacks alkene double bonds in polyunsaturated membrane lipids.
What is the relationship between canonical Molecular Orbitals and the localized bonds of Valence Bond / VSEPR theory?
For any closed-shell single-determinant wavefunction (such as Hartree–Fock or Kohn–Sham Density Functional Theory), the total many-electron Slater determinant Ψ(1, 2, …, N), the total 3D electron density ρ(r), the molecular energy E, and the equilibrium nuclear geometry are invariant under any unitary linear transformation among the occupied molecular orbitals. Canonical Molecular Orbitals diagonalize the Fock energy matrix to yield delocalized symmetry-adapted orbitals (such as the a1 and t2 orbitals of CH4) that directly predict vertical ionization energies (Koopmans' theorem) and electronic absorption spectra. Applying a unitary localization transformation (such as Boys, Edmiston–Ruedenberg, or Natural Bond Orbital localization) to those exact same occupied canonical MOs transforms them into localized bonding and lone-pair orbitals that match the two-center σ/π bonds and lone pairs of VSEPR theory and orbital hybridization.
References
- Mulliken, R. S. (1967). "Spectroscopy, molecular orbitals, and chemical bonding." Science, 157(3784), 13–24. https://doi.org/10.1126/science.157.3784.13
- Hoffmann, R., & Woodward, R. B. (1968). "The conservation of orbital symmetry." Accounts of Chemical Research, 1(1), 17–22. https://doi.org/10.1021/ar50001a003
- Fukui, K. (1982). "Role of frontier orbitals in chemical reactions." Science, 218(4574), 747–754. https://doi.org/10.1126/science.218.4574.747
- Albright, T. A., Burdett, J. K., & Whangbo, M.-H. (2013). Orbital Interactions in Chemistry (2nd ed.). John Wiley & Sons. ISBN 978-0471080398