♨️Thermodynamics of Fluids Unit 12 – Chemical Reaction Equilibria
Chemical reaction equilibria is a fundamental concept in thermodynamics, describing the balance between reactants and products in reversible reactions. This unit explores the principles governing equilibrium, including the equilibrium constant, factors affecting equilibrium, and Le Chatelier's principle.
Understanding chemical equilibria is crucial for predicting reaction outcomes and optimizing industrial processes. The unit covers thermodynamic foundations, types of equilibria, and practical applications, providing essential knowledge for analyzing and manipulating chemical systems in various fields.
Chemical equilibrium occurs when the rates of forward and reverse reactions are equal, resulting in no net change in concentrations of reactants and products over time
Dynamic equilibrium maintains constant concentrations of reactants and products, but reactions continue to occur in both directions
Equilibrium constant (K) quantifies the relationship between reactant and product concentrations at equilibrium, indicating the extent of a reaction
For a general reaction aA+bB⇌cC+dD, K=[A]a[B]b[C]c[D]d
Homogeneous equilibria involve reactants and products in the same phase (gas or liquid)
Heterogeneous equilibria involve reactants and products in different phases (solid, liquid, or gas)
Law of mass action states that the rate of a chemical reaction is directly proportional to the product of the concentrations of the reactants, each raised to a power equal to its stoichiometric coefficient
Equilibrium position refers to the relative amounts of reactants and products at equilibrium, which can be shifted by changing conditions (temperature, pressure, or concentration)
Thermodynamic Foundations
Gibbs free energy (ΔG) determines the spontaneity of a reaction at constant temperature and pressure
ΔG<0: reaction is spontaneous and proceeds in the forward direction
ΔG>0: reaction is non-spontaneous and proceeds in the reverse direction
ΔG=0: system is at equilibrium
Standard Gibbs free energy change (ΔG∘) relates to the equilibrium constant (K) through the equation ΔG∘=−RTlnK
R is the universal gas constant (8.314 J/mol·K)
T is the absolute temperature in Kelvin
Entropy (S) is a measure of the disorder or randomness of a system, influencing the spontaneity of a reaction
Enthalpy (H) represents the heat content of a system and determines whether a reaction is exothermic (releases heat) or endothermic (absorbs heat)
Van 't Hoff equation describes the temperature dependence of the equilibrium constant: lnK1K2=R−ΔH∘(T21−T11)
K1 and K2 are equilibrium constants at temperatures T1 and T2, respectively
ΔH∘ is the standard enthalpy change of the reaction
Types of Chemical Equilibria
Acid-base equilibria involve the transfer of protons (H⁺) between species in solution
Acid dissociation constant (Ka) quantifies the strength of an acid
Base dissociation constant (Kb) quantifies the strength of a base
Solubility equilibria occur when a solid substance dissolves in a solvent to form a saturated solution
Solubility product constant (Ksp) represents the equilibrium between a solid and its dissolved ions
Complex ion equilibria involve the formation of complex ions from metal cations and ligands (Lewis bases)
Formation constant (Kf) measures the stability of a complex ion
Redox equilibria involve the transfer of electrons between species, resulting in changes in oxidation states
Nernst equation relates the reduction potential of a half-reaction to its standard reduction potential and the concentrations of the oxidized and reduced species
Gas-phase equilibria occur when gaseous reactants and products reach a state of dynamic equilibrium
Equilibrium partial pressures of gases are used instead of concentrations in the equilibrium constant expression
Equilibrium Constants and Their Significance
Equilibrium constant (K) is a dimensionless quantity that represents the ratio of product concentrations to reactant concentrations at equilibrium, each raised to their stoichiometric coefficients
K is specific to a particular reaction at a given temperature
Magnitude of K indicates the extent of a reaction at equilibrium
K>1: products are favored at equilibrium
K<1: reactants are favored at equilibrium
K≈1: reactants and products are present in similar amounts at equilibrium
Equilibrium constant expressions differ for homogeneous and heterogeneous equilibria
For homogeneous equilibria, all reactants and products are included in the expression
For heterogeneous equilibria, only gaseous and aqueous species are included; pure solids and liquids are omitted
Reaction quotient (Q) has the same form as the equilibrium constant expression but uses instantaneous concentrations instead of equilibrium concentrations
Comparing Q to K predicts the direction of a reaction to reach equilibrium
Equilibrium constants can be combined for multiple reactions using multiplication or division, depending on how the reactions are added or subtracted
Factors Affecting Chemical Equilibria
Temperature changes affect the equilibrium position according to the Le Chatelier's principle
Increasing temperature shifts the equilibrium in the endothermic direction (absorbs heat)
Decreasing temperature shifts the equilibrium in the exothermic direction (releases heat)
Pressure changes affect gaseous equilibria by altering the partial pressures of the gases involved
Increasing pressure shifts the equilibrium towards the side with fewer moles of gas
Decreasing pressure shifts the equilibrium towards the side with more moles of gas
Concentration changes of reactants or products shift the equilibrium position to counteract the change
Adding reactants or removing products shifts the equilibrium towards the products
Removing reactants or adding products shifts the equilibrium towards the reactants
Catalysts accelerate the rates of both forward and reverse reactions equally, reaching equilibrium faster without changing the equilibrium position
Inert gases (non-reactive) added at constant volume do not affect the equilibrium position, as they do not change the partial pressures of the reactants or products
Le Chatelier's Principle and Its Applications
Le Chatelier's principle states that when a system at equilibrium is subjected to a disturbance, the equilibrium shifts in the direction that minimizes the disturbance
Applying Le Chatelier's principle helps predict the direction of equilibrium shift in response to changes in temperature, pressure, or concentration
Temperature changes
Exothermic reactions (release heat): increasing temperature shifts equilibrium towards reactants; decreasing temperature shifts equilibrium towards products
Endothermic reactions (absorb heat): increasing temperature shifts equilibrium towards products; decreasing temperature shifts equilibrium towards reactants
Pressure changes (gaseous equilibria)
Increasing pressure shifts equilibrium towards the side with fewer moles of gas
Decreasing pressure shifts equilibrium towards the side with more moles of gas
Concentration changes
Adding reactants or removing products shifts equilibrium towards products
Removing reactants or adding products shifts equilibrium towards reactants
Le Chatelier's principle has practical applications in industrial processes (Haber-Bosch process for ammonia synthesis) and biological systems (hemoglobin-oxygen binding in blood)
Calculating Equilibrium Compositions
ICE tables (Initial, Change, Equilibrium) are used to organize information and solve for equilibrium concentrations or partial pressures
Initial: concentrations or partial pressures before the reaction starts
Change: changes in concentrations or partial pressures as the reaction proceeds to equilibrium
Equilibrium: final concentrations or partial pressures at equilibrium
Equilibrium concentrations or partial pressures are calculated using the equilibrium constant expression and the ICE table
For reactions with small equilibrium constants (K<<1), the assumption of x << [initial] can simplify calculations
For reactions with large equilibrium constants (K>>1), the assumption of [initial] ≈ x can simplify calculations
Quadratic equations may be necessary to solve for equilibrium concentrations in more complex cases
pH calculations for acid-base equilibria involve using the acid dissociation constant (Ka) or the base dissociation constant (Kb)
Solubility calculations for slightly soluble salts involve using the solubility product constant (Ksp)
Real-World Applications and Case Studies
Haber-Bosch process for ammonia synthesis
\ceN2(g)+3H2(g)<=>2NH3(g), ΔH∘=−92.4 kJ/mol
High pressure (200-300 atm) and moderate temperature (400-500°C) favor product formation
Iron catalyst accelerates the reaction
Synthesis of methanol from syngas (CO and H₂)
\ceCO(g)+2H2(g)<=>CH3OH(g), ΔH∘=−90.6 kJ/mol
High pressure (50-100 atm) and moderate temperature (250-300°C) favor product formation
Copper-zinc oxide catalyst accelerates the reaction
Boudouard reaction in the production of carbon monoxide
\ce2CO(g)<=>CO2(g)+C(s), ΔH∘=−172.4 kJ/mol
High temperature (above 700°C) favors the reverse reaction, producing CO
Hemoglobin-oxygen binding in blood
Hemoglobin (Hb) binds oxygen (O₂) in the lungs and releases it in the tissues
Oxygen binding exhibits cooperative behavior due to the quaternary structure of hemoglobin
Factors such as pH, CO₂ concentration, and 2,3-bisphosphoglycerate (BPG) levels affect the oxygen affinity of hemoglobin
Calcium carbonate (CaCO₃) dissolution in ocean acidification
\ceCaCO3(s)<=>Ca2+(aq)+CO32−(aq), Ksp=3.36×10−9 at 25°C
Increasing atmospheric CO₂ levels lead to ocean acidification, shifting the equilibrium towards the dissolution of calcium carbonate
Impacts marine organisms that rely on calcium carbonate for their shells or skeletons (corals, mollusks, and some plankton)