Point defects—missing atoms (vacancies) and extra atoms in interstitial positions—form during solidification and at elevated temperatures. The equilibrium concentration of defects follows the Boltzmann distribution and increases exponentially with absolute temperature. Vacancies enable atomic diffusion and interstitials strengthen materials; both strongly influence mechanical, electrical, and thermal properties.
The idealized crystal you learned in crystal structure basics — every atom sitting exactly on its lattice site, perfectly periodic — never exists in reality, even in the most carefully grown single crystal. At any finite temperature, thermal fluctuations continuously create and destroy point defects: localized disruptions to the perfect lattice involving just one or a few atomic sites. The two most important are vacancies (empty lattice sites where an atom is missing) and interstitials (extra atoms squeezed into the gaps between normal lattice sites). These defects are not impurities — they can occur in a perfectly pure material. They are an unavoidable consequence of thermodynamics.
Why must point defects exist? Creating a vacancy costs energy — you break bonds removing an atom from the interior to the surface. But it also increases the configurational entropy of the crystal: there are an enormous number of ways to arrange n vacancies among N lattice sites. The competition between energy cost and entropy gain determines the equilibrium vacancy concentration: n_v/N = exp(−Q_v/kT), where Q_v is the vacancy formation energy, k is Boltzmann's constant, and T is absolute temperature. At room temperature this fraction is tiny — perhaps one vacancy per billion sites in a typical metal. Near the melting point it can reach one in a thousand. Crucially, this equilibrium concentration is set by temperature alone and cannot be driven to zero by any processing technique; vacancies are thermodynamically inevitable. Rapidly quenching a metal from high temperature "freezes in" a supersaturation of vacancies, which then slowly anneal out at room temperature — a process engineers exploit in age-hardening alloys.
Vacancies are the primary mechanism for solid-state diffusion. An atom adjacent to a vacancy can jump into the empty site — and this exchange, repeated billions of times per second across billions of sites, is how atoms migrate through a solid. The diffusion coefficient D = D₀ exp(−Q_d/kT) depends exponentially on temperature, because both the jump attempt frequency (governed by thermal vibrations) and the vacancy concentration have exponential temperature dependences. Without vacancies, atomic mobility in a crystal would be negligibly small: the direct exchange of adjacent atoms requires far more energy than vacancy-mediated jumps. Vacancy diffusion is what allows steel to be carburized, dopants to be thermally driven into semiconductors, and plastically deformed metals to recrystallize — all at practical temperatures.
Interstitials are geometrically strained defects: squeezing an extra atom into an interstitial site distorts the surrounding lattice elastically, so they carry more strain energy than vacancies and exist in lower equilibrium concentrations in pure metals. Their engineering importance comes as interstitial solutes — atoms of a small element (carbon, nitrogen, hydrogen) occupying interstitial sites in a host lattice. In iron, carbon atoms dissolved interstitially distort the BCC lattice into a tetragonal structure (martensite) and create elastic stress fields that interact strongly with gliding dislocations, raising the yield strength dramatically. This atomic-scale mechanism — small interstitial atoms locking dislocations in place — is the fundamental explanation for why adding 0.1–1% carbon by weight transforms soft iron into hard steel.