The phase transition of a substance from liquid to solid state, as when magma cools to form rock.Solidification is the phase transition in which a liquid becomes a solid, typically by cooling below its freezing point. It is the process by which magma cools into igneous rock, water turns to ice in a stream, or molten metal takes a permanent shape in a mold. In physics and materials science, solidification is a rich field because it involves the interplay of thermodynamics, heat flow, and the microscopic arrangement of atoms or molecules as they lose kinetic energy and lock into a crystalline or amorphous structure.
The scientific study of solidification began in earnest in the 19th century with the development of thermodynamics, particularly through the work of Josiah Willard Gibbs, who formulated the theory of phase equilibria and nucleation in the 1870s.
As a liquid cools, its constituent particles lose thermal energy and move more slowly. When the temperature drops below the freezing point, small clusters of particles begin to form stable nuclei — a process called nucleation. Once a nucleus exists, additional particles attach to its surface, and the solid grows outward. The rate of growth and the final structure depend on how quickly heat is removed and on impurities present, which can act as nucleation sites. In many cases, solidification is not uniform: it can produce dendritic (tree-like) crystal patterns, as seen in snowflakes or metal castings, and can trap impurities or bubbles in the solid.
Solidification is central to metallurgy and casting, where controlling the cooling rate determines the strength and quality of metal parts, and to the formation of igneous rocks, which geologists study to understand planetary history.
The Moon's geochemical similarity to Earth is partly explained by the solidification of a global magma ocean early in its history, which produced a crust with a composition matching Earth's mantle.



















