Covalent bonds form when atoms share electron pairs, typically between two nonmetals whose electronegativities are similar enough that complete electron transfer does not occur. Single, double, and triple bonds correspond to sharing one, two, or three electron pairs, respectively. Higher bond order produces shorter bond length and greater bond energy. The octet rule — most second-row atoms seek eight electrons in their valence shell — guides the distribution of shared and lone-pair electrons.
Start with simple homonuclear diatomics (H₂, O₂, N₂) and build up to heteronuclear molecules. Use bond energy data to connect the abstract concept of electron sharing to measurable quantities like reaction enthalpies estimated from bond breaking and forming.
You learned from periodic trends that electronegativity — an atom's ability to attract electrons — varies predictably across the periodic table. Covalent bonding arises directly from that property: when two atoms with similar electronegativities come close, neither can fully steal the other's electrons. Instead, they reach a compromise and share them. The shared electrons spend time between both nuclei, and their negative charge attracts both positively charged nuclei simultaneously, holding the atoms together. This is a covalent bond.
The number of pairs of electrons two atoms share determines the bond order. A single bond involves one shared pair, a double bond two, and a triple bond three. Bond order has two predictable consequences. First, more electron pairs pack the nuclei closer together: a triple bond is shorter than a double bond, which is shorter than a single bond. Second, more shared electrons make the bond harder to break: triple bonds have the highest bond energy, single bonds the lowest. You can see this clearly in the nitrogen family — N₂ (triple bond) is one of the strongest bonds in chemistry, which is why N₂ is so chemically unreactive.
The octet rule explains why atoms tend to form particular numbers of bonds. Most second-period atoms are most stable with 8 electrons in their valence shell — a complete outer shell matching the electron configuration of the nearest noble gas. Carbon has 4 valence electrons and needs 4 more, so it forms 4 bonds. Nitrogen has 5 and needs 3, so it forms 3 bonds (with one lone pair left over). Oxygen has 6 and needs 2, so it typically forms 2 bonds. These rules have exceptions — hydrogen obeys a duet rule (only needs 2), and heavier atoms like phosphorus and sulfur can hold more than 8 electrons in their valence shells — but the octet rule correctly predicts bonding patterns for most common molecules.
A critical nuance from the misconceptions: covalent bonding does not mean equal sharing. When two atoms with different electronegativities form a bond — say, H and Cl — the chlorine atom (more electronegative) pulls the shared electron pair closer to itself. The bond is still covalent (the electrons are shared, not transferred), but the electron density is unevenly distributed, creating a partial negative charge (δ−) on the Cl end and a partial positive charge (δ+) on the H end. This is a polar covalent bond, and it is the bridge between purely nonpolar covalent bonds (in homonuclear diatomics) and fully ionic bonds (where electron transfer is complete). The electronegativity difference between the bonded atoms determines where a bond falls on this continuum.