Table 1 Summary of key findings of thermodynamic observations
Factor | Effect on carbonate precipitation | Key observations |
|---|---|---|
CO₂ Pressure (50–500 atm) | Higher pressure increases CO₂ solubility, leading to more bicarbonate (HCO₃⁻) formation and CaCO₃ precipitation | Precipitation rate increases significantly at 500 atm |
Temperature (274–298 K) | Higher temperatures promote aragonite formation due to the slightly lower stability of calcite at elevated temperatures. | Aragonite is more likely to form above 298 K |
Salinity (TDS up to 19,000 ppm) | Higher salinity reduces CO₂ solubility but increases solution alkalinity, promoting CaCO₃ precipitation. | Seawater enhances precipitation more than NaCl solutions |
pH (6.5–8.5) | Optimal pH range for CaCO₃ precipitation. Extreme pH changes may lead to impurity formation (e.g., dolomite, huntite) | pH above 8.5 favours CaCO₃ formation but may reduce purity |
Mg²⁺ and SO₄²⁻ Ions | Mg²⁺ can incorporate into carbonate structures, forming dolomite/huntite; SO₄²⁻ can lead to gypsum precipitation | Control of Mg²⁺/Ca²⁺ ratios is essential for purity. |
Supersaturation Index (S) | Higher saturation levels accelerate precipitation, but excessive supersaturation can lead to secondary mineral formation. | Maintaining moderate saturation prevents impurity formation. |