18-electron rule
The 18-electron rule is a fundamental guideline in organometallic chemistry stating that stable transition metal complexes typically possess 18 valence electrons around the central metal atom, mimicking the inert gas electronic configuration and promoting thermodynamic stability.[1] This rule, first articulated by Irving Langmuir in 1921 as an extension of valence theory to transition metals, posits that the metal achieves a closed-shell structure by coordinating ligands that donate the requisite electrons to fill its valence shell, specifically the (n-1)d, ns, and np orbitals.[1] Refined by Nevil Sidgwick in 1927 through the effective atomic number (EAN) concept, it emphasizes that the total electron count, derived from the metal's d electrons plus ligand donations, correlates with observed stability in diamagnetic complexes.[2] Electron counting under the 18-electron rule involves two common methods: the neutral ligand formalism, where ligands are treated as neutral donors (e.g., CO as a 2-electron donor), and the ionic formalism, which assigns formal charges to adjust the metal's oxidation state before adding ligand electrons.[3] For instance, in Vaska's complex ([IrCl(CO)(PPh₃)₂]), the iridium center (group 9, d⁸ in oxidation state +1) receives 2 electrons from Cl, 2 from CO, and 2 each from the two phosphines, totaling 16 electrons, highlighting a common exception for square-planar d⁸ species.[3] The rule applies primarily to low-spin, octahedral complexes of second- and third-row transition metals, where it rationalizes formulas like [Mn(CO)₆]⁺ (18 electrons) versus unstable alternatives.[3] Beyond prediction, the 18-electron rule informs reaction mechanisms in homogeneous catalysis, such as olefin hydrogenation and hydroformylation, where intermediates often alternate between 16-electron (unsaturated, reactive) and 18-electron (saturated, stable) configurations to facilitate steps like oxidative addition or ligand substitution.[3] Exceptions abound, including 16-electron tetrahedral or square-planar complexes (e.g., Pd(0) catalysts), 14-electron species in early transition metals, and rare 20-electron cases stabilized by steric effects, as seen in a stable 20-electron ferrocene derivative synthesized in July 2025 by Satoshi Takebayashi and colleagues at the Okinawa Institute of Science and Technology (OIST), challenging the rule's upper limit.[3][4][5] These deviations underscore the rule's empirical nature, influenced by factors like metal identity, ligand type, and geometry, yet it remains a cornerstone for designing organometallic compounds in synthesis and industry.[3]Fundamentals
Electron Counting Methods
Electron counting in transition metal complexes is essential for applying the 18-electron rule, which posits that stable organometallic compounds typically achieve a total of 18 valence electrons around the central metal atom.[3] Two equivalent conventions are widely used to perform this count: the neutral ligand method (also known as the covalent model) and the ionic ligand method (also known as the oxidation state formalism).[6] These methods assign electron contributions from the metal and ligands in a manner that ensures consistency in the final tally, facilitating the prediction of complex stability without regard to bonding details.[3] In the neutral ligand method, the metal is considered in its formal zero oxidation state, contributing a number of valence electrons equal to its group number in the periodic table (e.g., iron in group 8 contributes 8 electrons).[6] Ligands are treated as neutral molecules or fragments, donating electrons based on their typical Lewis basicity: even-electron donors like carbon monoxide (CO) or phosphines (PR₃) contribute 2 electrons each, while odd-electron donors like halides (X) or hydrogen (H) contribute 1 electron each.[3] The total electron count is the sum of the metal's contribution and all ligand donations, with adjustments for the overall charge of the complex if anionic or cationic (subtract or add electrons accordingly).[6] This approach emphasizes covalent bonding character and is particularly straightforward for complexes with neutral ligands.[3] The ionic ligand method, in contrast, begins by determining the oxidation state of the metal, which is calculated by assigning full charges to ligands (e.g., halides as X⁻, cyclopentadienyl as Cp⁻) and balancing the complex's overall charge.[6] The metal then contributes its d-electrons, given by the formula: d-electron count = group number - oxidation state.[3] Ligands are classified as L-type (neutral, 2-electron donors like CO or PR₃) or X-type (anionic, 2-electron donors like Cl⁻ or H⁻ in their closed-shell form), with odd-electron ligands such as allyl often treated as 3-electron donors when neutral or 2-electron donors when anionic.[6] The total is again the sum of metal d-electrons and ligand contributions, adjusted for charge; this method highlights ionic character and is useful for complexes with charged ligands.[3] To perform the count using either method, the steps are as follows: (1) identify the metal and its relevant group number or oxidation state; (2) classify and tally electron donations from each ligand; (3) sum the metal and ligand electrons; and (4) adjust for the complex's net charge if necessary (e.g., subtract 1 electron for a +1 charge).[6] Common ligand donations vary by method but are standardized for consistency:| Ligand | Neutral Method Donation | Ionic Method Donation | Notes |
|---|---|---|---|
| CO | 2e (neutral σ-donor/π-acceptor) | 2e (L-type) | Ubiquitous in carbonyl complexes.[3] |
| PR₃ (phosphine) | 2e (neutral σ-donor) | 2e (L-type) | Variable cone angle affects sterics.[3] |
| Halide (X, e.g., Cl) | 1e (neutral radical X•) | 2e (X-type, X⁻) | Common in early transition metal complexes.[6] |
| Allyl (C₃H₅) | 3e (neutral η³-allyl radical) | 2e (allyl⁻, X-type) or 4e (η³-allyl⁻ as L) | Depends on hapticity and charge.[6] |
| Cyclopentadienyl (Cp) | 5e (neutral Cp•) | 6e (Cp⁻, L-type) | Often η⁵-bound in sandwich compounds.[3] |