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Crystallisation is the process through which a liquid is solidified into a highly structured solid, where a solvent is typically evaporated to leave the crystallised solid. One area where crystallisation is used is in the process of manufacturing sugar crystals, where a thick syrup is fed into a crystallisation chamber and evaporated until a desired sugar crystal size is achieved.

Equilibria and Binary Mixtures

The process of crystallisation focuses on the solid to liquid transition, where a single substance can crystallise into as many as 7 different forms, resulting in different lattice arrangements and therefore different properties. A polymorphic substance can form multiple crystal forms, where the rate of cooling during the crystallisation process may dictate the resulting form.

Figure 1 shows a plot of temperature against the mass fraction of two substances, ‘A’ and ‘B’. A eutectic binary mixture consists of two substances which may have different freezing points, where the eutectic point, shown as ‘e’ on the diagram, is where both substances are crystallised at the lowest possible temperature.

Figure 1. Plot of Temperature against Composition for a eutectic binary mixture of two compounds.

Supersaturation is one of three states, alongside saturated and unsaturated systems, where the concentration of a mix is at its highest and the system is beyond equilibrium, and is necessary for crystallisation to occur. Equation 1 shows the equation for the degree of supersaturation (), with Equation 2 showing the equation for the supersaturation ratio (\(S\)) and Equation 3 showing the equation for the relative supersaturation (\(\phi\)).

\(\Delta c = c - c^*\)

Equation 1. Equation for the degree of supersaturation, where is the degree supersaturation, \(c\) is the concentration in the super saturated solution, and \(c^*\) is the concentration of equilibrium saturated solution, all with units of kg solvent/kg solution.

\(S = \frac{c}{c^*}\)

Equation 2. Equation for the supersaturation ratio, \(S\) (no units), where \(c\) is the concentration in the super saturated solution, and \(c^*\) is the concentration of equilibrium saturated solution, both with units of kg solvent/kg solution.

\(\phi = \frac{\Delta c}{c^*} = S-1\)

Equation 3. Equation for the relative supersaturation, \(\phi\) (no units), where is the degree supersaturation and \(c^*\) is the concentration of equilibrium saturated solution, both with units of kg solvent/kg solution. \(S\) is the supersaturation ratio (no units).

This state of supersaturation required for crystallisation can be achieved in three main ways:

  • Cooling: Used in systems where the stability decreases with temperature
  • Solvent removal: Used in systems where the stability is not affected by temperature and so the solvent is normally removed by evaporation
  • Additional components: Used if neither cooling nor evaporation can be used, where the this additional compound might react to form an insoluble substance with the original solute via a precipitation reaction

The spontaneous nucleation of crystals as a result of supersaturation can be predicted using a solubility-supersolubility diagram, such as the one shown in Figure 2. The three regions are as follows:

  • Stable: Crystallisation impossible here
  • Metastable region: Spontaneous nucleation improbable
  • Labile region: Spontaneous nucleation probable but not inevitable
Figure 2. Concentration-Temperature plot showing the three regions of the solubility-supersolubility diagram.

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