Igneous rocks form from solidified magma; cooling rate determines crystal size and rock texture. Fractional crystallization—the preferential crystallization of certain minerals—creates compositionally diverse igneous rocks from a single parental magma. This process explains variation from basalt to granite.
Examine hand samples of coarse-grained (plutonic) and fine-grained (volcanic) rocks of similar composition. Conduct melting experiments or study phase diagrams showing how temperature and pressure influence crystallization. Compare mineralogy across a basalt-dolerite-gabbro sequence.
Magma and lava are chemically distinct. All igneous rocks cool slowly underground. Crystal size depends only on composition, not cooling rate. Fractional crystallization requires manual separation—it occurs naturally due to density differences and settling.
From your study of mineral crystal systems, you know that minerals have specific chemical compositions and crystal structures determined by the conditions under which they form. Igneous rocks are the direct product of magma cooling and crystallizing — and the central insight of igneous petrology is that cooling rate and chemical differentiation together explain the enormous variety of igneous rock types found on Earth.
Start with cooling rate, because it controls texture. When magma cools slowly deep underground (forming plutonic or intrusive rocks), atoms have time to migrate through the melt and attach to growing crystal faces. The result is coarse-grained rock like granite, where individual mineral crystals are easily visible to the naked eye. When magma erupts at the surface as lava and cools rapidly (forming volcanic or extrusive rocks), crystals have little time to grow, producing fine-grained rock like basalt. Cool it fast enough — as when lava hits water — and you get glass (obsidian), where atoms freeze in place before crystals can form at all. The same magma composition can produce very different-looking rocks depending solely on where and how fast it solidifies. Gabbro and basalt, for instance, are chemically identical but texturally opposite: one cooled over thousands of years underground, the other in hours or days at the surface.
Now consider chemical differentiation, which explains how a single parent magma can produce rocks ranging from dark, iron-rich basalt to light, silica-rich granite. The key process is fractional crystallization. As magma cools, minerals do not all crystallize simultaneously — they crystallize in a predictable sequence determined by their melting points, as described by phase diagrams. High-temperature minerals like olivine and pyroxene crystallize first, locking iron and magnesium into solid crystals. If these dense, early-formed crystals settle to the bottom of the magma chamber (a process called crystal settling), they are physically removed from the remaining liquid. The residual melt is now depleted in iron and magnesium but enriched in silica, aluminum, sodium, and potassium — the ingredients of minerals like feldspar and quartz. Continued crystallization and removal progressively shifts the melt composition from mafic (basaltic) toward felsic (granitic).
This is why igneous rocks form a compositional spectrum. A single large magma chamber beneath a volcanic arc can produce basaltic rocks from early crystallization, intermediate rocks (andesite/diorite) as differentiation proceeds, and eventually granitic rocks from the last, most silica-rich residual melt. The process is not hypothetical — it has been directly observed in layered intrusions like the Bushveld Complex in South Africa, where you can walk across exposed magma chamber floors and see the cumulate layers of early-crystallizing minerals grading upward into progressively more evolved compositions. Understanding this connection between phase diagrams, crystallization sequence, and melt evolution is what allows geologists to read the history of a magma chamber from the rocks it left behind.