Detailed Summary of Chemical Equilibria
Chemical equilibrium represents a state where the forward and reverse reactions occur at equal rates, leading to constant concentrations of reactants and products. This is a dynamic process, often exemplified by reactions involving volatile liquids or gases. For example, when water evaporates in a closed container, molecules with higher kinetic energy transition into the vapor phase until equilibrium is established, characterized by a constant vapor pressure.
Equilibrium can also be established in chemical reactions where changes in reactant concentration or pressure will shift the balance, adhering to Le Chatelier's principle. The equilibrium constant (Kc) provides a quantitative measure of the concentrations of reactants and products at equilibrium, reflecting the reaction's favorability based on stoichiometric coefficients.
Important factors influencing this equilibrium state include temperature, concentration, and pressure. The section outlines the importance of ionic equilibrium within solutions, where acids and bases dissolve and ionize, emphasizing the Arrhenius, Brönsted-Lowry, and Lewis definitions of acids and bases. Additionally, the pH scale is introduced, which quantifies the acidity or basicity of a solution, and specific examples illustrate concepts like solubility product constant (Ksp) for sparingly soluble salts. The properties and behavior of buffer solutions, which resist changes in pH, are also discussed, establishing their essential role in maintaining biochemical stability. Finally, the section includes various exercises and applications to strengthen understanding of chemical equilibria.