Depletion-driven self-assembly in binary colloidal mixtures is studied via the time evolution of the cluster-size distribution and structure factor as the mixtures equilibrate after shear melting. The data suggest a two-stage crystallization process governed by an initial collapse into an amorphous metastable state, the growth kinetics of which are interpreted within the context of reversible aggregation and early-stage phase separation. [S0031-9007(98)07565-6] PACS numbers: 82.70.Dd, 64.60.My, 64.75. + gThe segregation of a binary fluid and the crystallization of a simple liquid are familiar examples of first order phase transitions [1,2]. In mixtures whose components interact through excluded volume, these two phenomena can be driven simultaneously via a depletion force [3][4][5]. The phase-ordering dynamics of such systems have just begun to be investigated, and the underlying physics may have relevance to such things as the crystallization of globular proteins and nematic ordering of rodlike particles in the presence of a nonadsorbing polymer [6,7]. Beyond their broad commercial significance, colloidal suspensions serve as useful models for a variety of condensed matter systems, from crystals [8,9] and glasses [10] to critical fluids [11] and fractal networks [12]. In this Letter, video microscopy is used to study depletion driven selfassembly in confined binary suspensions of nearly hardsphere colloids. The results suggest that crystallization in these mixtures is a two-stage process governed by an initial collapse into an amorphous metastable state, and the kinetics of cluster formation are interpreted within the context of both reversible colloidal aggregation and entropically driven phase separation.The mixtures consist of monodisperse polystyrene spheres of diameter 2R L 2.9 mm and 2R S 213 nm (stabilized with a charged polymer surfactant) in aqueous suspensions containing enough salt (0.01 M) to screen the electrostatic repulsion to short range. The large-sphere volume fraction is fixed at f L 0.025 for small-sphere volume fractions 0 # f S # 0.4. Rapid gravitational settling of the large spheres restricts their motion to a plane [13], leading to two-dimensional trajectories in the bulk free-energy landscape. This facilitates tracking of the large spheres and has potential relevance to microscale lithography and lubrication. A shell of excluded volume around each large sphere means that when two come into contact the effective value of f S decreases, lowering the entropic free energy by an amount D [3]. If D͞k B T is big enough, the large spheres aggregate into clusters. For the geometry in question, a close-packed triangular lattice yields the greatest reduction in excluded volume, and hence the greatest decrease in free energy. Phase separation was observed only for f S $ 0.20, in agreement with the bulk phase diagram of a comparable system [4].The value of f L is below the percolation threshold, and slightly lower values yield smaller clusters, while slightly higher values yield clusters that are per...