Chemical Bonding & Molecular Structure
Why atoms bond, how electrons rearrange to form ions and shared pairs, and why a molecule takes the exact three-dimensional shape it does. This is one of the highest-yield physical chemistry chapters in NEET, so you can expect 2 to 3 direct questions almost every year.
Kössel–Lewis Approach to Bonding
Atoms bond to attain the stable noble gas electronic configuration.
The Octet Rule
Atoms combine by losing, gaining, or sharing electrons so that each atom acquires eight electrons in its outermost shell to achieve the stable configuration of the nearest noble gas. Hydrogen and helium are exceptions, as they only need 2 electrons (the duplet rule).
Lewis Symbols & Structures
A Lewis (dot) symbol shows the valence electrons of an atom as dots around its symbol. Follow these rules for drawing a Lewis structure of a molecule or ion:
- Count the total valence electrons of all atoms (add the charge magnitude for anions, and subtract it for cations).
- Identify the central atom. This is usually the least electronegative, non-hydrogen atom.
- Connect atoms with single bonds (2 electrons each) to form the skeleton.
- Distribute the remaining electrons as lone pairs to satisfy the octets of the outer atoms first.
- If the central atom lacks an octet, convert the lone pairs on the outer atoms into additional bonds (multiple bonds).
Formal Charge
Formal charge helps you choose the most reasonable Lewis structure among several possibilities:
The structure with formal charges closest to zero, and a negative formal charge placed on the more electronegative atom, is the more stable (and preferred) representation.
Ionic (Electrovalent) Bond
Complete transfer of electrons from a metal to a non-metal, held together by electrostatic attraction.
Factors Favouring Ionic Bond Formation
- Low ionization enthalpy of the metal atom (the cation forms easily).
- High (negative) electron gain enthalpy of the non-metal atom (the anion forms easily).
- High lattice enthalpy of the resulting crystal. The more exothermic this process is, the more stable the ionic compound becomes.
Lattice Enthalpy & Born–Landé Equation
Lattice enthalpy is the energy required to completely separate one mole of a solid ionic compound into its gaseous ions. It is estimated using this formula:
where \(N_A\) = Avogadro constant, \(M\) = Madelung constant, \(z^+, z^-\) = ionic charges, \(r_0\) = inter-ionic distance, \(n\) = Born exponent.
Born–Haber Cycle
This is an indirect route to calculate lattice enthalpy via Hess's Law. You can sum the sublimation, ionization, dissociation, electron gain, and formation enthalpies to equal the lattice enthalpy step.
Covalent Bond & Lewis Structures
A shared pair of electrons holds two atoms together. Langmuir named this interaction the covalent bond.
One shared electron pair, e.g. H–H, Cl–Cl. The bond order is 1.
A double bond has 2 shared pairs (O=O), and a triple bond has 3 shared pairs (N≡N). As the bond order increases, the bond strength increases and the bond length decreases.
Coordinate (Dative) Bond
Both shared electrons are donated by a single atom (the donor) to another (the acceptor), such as in \(\text{NH}_4^+\) and \(\text{H}_3\text{O}^+\). Once formed, a coordinate bond behaves identically to a normal covalent bond.
Bond Parameters
The measurable fingerprints of a bond: length, angle, enthalpy, and order.
| Parameter | Definition | Trend / Note |
|---|---|---|
| Bond length | Equilibrium distance between nuclei of two bonded atoms | ↓ as bond order ↑; ↑ down a group |
| Bond angle | Angle between orbitals containing bonding electron pairs around a central atom | Distorted by lone pairs (lp–lp > lp–bp > bp–bp repulsion) |
| Bond enthalpy | Energy needed to break one mole of bonds in gaseous state | ↑ as bond order ↑ (triple > double > single) |
| Bond order | Number of bonds between two atoms | Higher order means a shorter, stronger bond |
\(N_b\) = electrons in bonding molecular orbitals, \(N_a\) = electrons in antibonding molecular orbitals.
Resonance & Bond Polarity
When one Lewis structure isn't enough, and when a shared pair isn't shared equally.
Resonance
Some molecules (like \(\text{O}_3\), \(\text{CO}_3^{2-}\), and benzene) cannot be represented by a single Lewis structure. The actual molecule is a weighted hybrid of two or more contributing structures (canonical forms) that differ only in electron placement, not atomic position. The resonance hybrid is always more stable than any single contributing structure.
Polarity of Covalent Bonds
Unequal sharing of the bonding pair, which happens because of a difference in electronegativity, creates a polar covalent bond with partial charges \(\delta^+\) and \(\delta^-\).
Dipole moment \(\mu\) is measured in Debye (D); \(1\ \text{D} = 3.33564 \times 10^{-30}\ \text{C m}\). It is a vector quantity, pointing from the positive to the negative end.
VSEPR Theory
Valence Shell Electron Pair Repulsion dictates that electron pairs arrange to minimize mutual repulsion.
Postulates
- The shape of a molecule depends on the number of valence shell electron pairs (bonding and lone) around the central atom.
- Electron pairs orient themselves to minimize repulsion and maximize the distance between them.
- A multiple bond is treated as a single effective electron pair (electron density) for shape calculation purposes.
- The repulsion order is: lone pair–lone pair > lone pair–bond pair > bond pair–bond pair.
| BP + LP | Shape | Bond angle | Example |
|---|---|---|---|
| 2 + 0 | Linear | 180° | BeCl₂, CO₂ |
| 3 + 0 | Trigonal planar | 120° | BF₃, SO₃ |
| 2 + 1 | Bent / angular | <120° | SO₂ |
| 4 + 0 | Tetrahedral | 109.5° | CH₄, SO₄²⁻ |
| 3 + 1 | Trigonal pyramidal | ~107° | NH₃ |
| 2 + 2 | Bent / angular | ~104.5° | H₂O |
| 5 + 0 | Trigonal bipyramidal | 120° & 90° | PCl₅ |
| 4 + 1 | See-saw | ~173°, 120°, 90° | SF₄ |
| 3 + 2 | T-shaped | ~90° | ClF₃ |
| 2 + 3 | Linear | 180° | XeF₂, I₃⁻ |
| 6 + 0 | Octahedral | 90° | SF₆ |
| 5 + 1 | Square pyramidal | ~90° | BrF₅ |
| 4 + 2 | Square planar | 90° | XeF₄ |
Valence Bond Theory (VBT)
A covalent bond forms by the overlap of half-filled atomic orbitals of opposite spin.
Types of Overlap
This is a head-on (axial) overlap along the internuclear axis using s–s, s–p, or p–p orbitals. Free rotation is possible around a σ bond.
This is a sideways (lateral) overlap of parallel p-orbitals located above and below the internuclear axis. This restricts rotation and is weaker than a σ bond.
Strength of Overlap
Greater orbital overlap results in a stronger, shorter bond. The order of overlap strength is: s–s < s–p < p–p (σ) > p–p (π).
Hybridization
Mixing of atomic orbitals of similar energy on the same atom to form new, equivalent hybrid orbitals.
| Hybridization | Geometry | Examples |
|---|---|---|
| sp | Linear | BeCl₂, C₂H₂, CO₂ |
| sp² | Trigonal planar | BCl₃, C₂H₄, SO₃ |
| sp³ | Tetrahedral | CH₄, NH₃, H₂O |
| sp³d | Trigonal bipyramidal | PCl₅ |
| sp³d² | Octahedral | SF₆ |
| sp³d³ | Pentagonal bipyramidal | IF₇ |
Rules Governing Hybridization
- Only orbitals of comparable energy from the same atom can mix.
- The number of hybrid orbitals formed equals the number of atomic orbitals mixed.
- Hybrid orbitals are equivalent in energy and shape, and they point towards the corners of a definite geometric figure.
- They form only σ bonds or hold lone pairs, but they never form π bonds.
Molecular Orbital Theory (MOT)
Atomic orbitals combine using LCAO to give molecular orbitals delocalized over the whole molecule.
Formation of Molecular Orbitals
Using the Linear Combination of Atomic Orbitals (LCAO) method, constructive overlap (addition) gives a lower-energy bonding MO (σ, π). Destructive overlap (subtraction) gives a higher-energy antibonding MO (σ*, π*), which features a node between the nuclei.
1s
1s
σ1s
1s
1s
σ*1s
2pz
2pz
σ2pz
2pz
2pz
σ*2pz
2px
2px
π2px
2px
2px
π*2px
The order shown above applies to O₂, F₂, and Ne₂. For Li₂ through N₂, σ2p sits above π2p.
Energy Level Order
Bond Order & Key Examples
| Species | Electron config (valence) | Bond order | Nature |
|---|---|---|---|
| H₂ | σ1s² | 1 | Stable, diamagnetic |
| He₂ | σ1s² σ*1s² | 0 | Does not exist |
| N₂ | σ2s² σ*2s² π2p⁴ σ2p² | 3 | Very stable, diamagnetic |
| O₂ | σ2s² σ*2s² σ2p² π2p⁴ π*2p² | 2 | Paramagnetic (2 unpaired e⁻ in π*) |
Hydrogen Bonding
A special dipole–dipole attraction created when hydrogen sits between two highly electronegative atoms.
Condition for Formation
Hydrogen must be covalently bonded to a small, highly electronegative atom (specifically F, O, or N). This leaves the H nucleus exposed enough to attract a lone pair on a neighbouring electronegative atom.
This occurs between two different molecules, e.g. HF···HF, H₂O···H₂O. It raises the boiling point, viscosity, and surface tension significantly (leading to the anomalous behaviour of water, HF, and NH₃).
This occurs within the same molecule and forms a ring, e.g. o-nitrophenol. It tends to lower the boiling point compared to the para-isomer, because the hydrogen isn't available for intermolecular association.
Quick Revision Sheet
Every formula and rule from this chapter in one glance, perfectly suited for the night before your exam.