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Chapter 19: Spontaneous Change: Entropy and Gibbs Energy
Chemistry 140 Fall 2002 General Chemistry Principles and Modern Applications Petrucci • Harwood • Herring 8th Edition Chapter 19: Spontaneous Change: Entropy and Gibbs Energy Philip Dutton University of Windsor, Canada N9B 3P4 Prentice-Hall © 2002
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General Chemistry: Chapter 20
Chemistry 140 Fall 2002 Contents 19-1 Spontaneity: The Meaning of Spontaneous Change 19-2 The Concept of Entropy 19-3 Evaluating Entropy and Entropy Changes 19-4 Criteria for Spontaneous Change: The Second Law of Thermodynamics 19-5 Standard Gibbs Energy Change, ΔG° 19-6 Gibbs Energy Change and Equilibrium 19-7 ΔG° and Keq as Functions of Temperature 19-8 Coupled Reactions Focus On Coupled Reactions in Biological Systems Prentice-Hall © 2002 General Chemistry: Chapter 20
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19-1 Spontaneity: The Meaning of Spontaneous Change
Prentice-Hall © 2002 General Chemistry: Chapter 20
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General Chemistry: Chapter 20
Spontaneous Process A process that occurs in a system left to itself. Once started, no external actions is necessary to make the process continue. A non-spontaneous process will not occur without external action continuously applied. 4 Fe(s) + 3 O2(g) → 2 Fe2O3(s) H2O(s) H2O(l) 2 Fe2O3(s) → 4 Fe(s) + 3 O2(g) Prentice-Hall © 2002 General Chemistry: Chapter 20
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General Chemistry: Chapter 20
Spontaneous Process Potential energy decreases. For chemical systems the internal energy U is equivalent to potential energy. Berthelot and Thomsen 1870’s Spontaneous change occurs in the direction in which the enthalpy of a system decreases. Mainly true but there are exceptions. Prentice-Hall © 2002 General Chemistry: Chapter 20
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19-2 The Concept of Entropy
Entropy, S. The greater the number of configurations of the microscopic particles among the energy levels in a particular system, the greater the entropy of the system. ΔS > 0 spontaneous ΔU = ΔH = 0 Prentice-Hall © 2002 General Chemistry: Chapter 20
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The Boltzmann Equation for Entropy
Chemistry 140 Fall 2002 The Boltzmann Equation for Entropy S = k lnW S is the entropy k = R/NA: Boltzmann constant W = number of microstates. The particular way in which particles are distributed amongst the microscopic energy levels called states available in a system with the same total energy. Ludwig Boltzmann. Associated the number of energy levels in a system with the number of ways of arranging the particles in these levels. General Chemistry: Chapter 20
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Boltzmann Distribution FIG. 19-3
Chemistry 140 Fall 2002 Boltzmann Distribution FIG. 19-3 FIGURE 19-3 Energy levels for a particle in a one-dimensional box (a) The energy levels of a particle in a box become more numerous and closer together as the length of the box increases. The range of thermally accessible levels is indicated by the tinted band. The solid circles signify a system consisting of 15 particles. Each drawing represents a single microstate of the system. Can you see that as the box length increases there are many more microstates available to the particles for a given amount of thermal energy? As the number of possible microstates for a given total energy increases, so does the entropy. (b) More energy levels become accessible in a box of fixed length as the temperature is raised. Because the average energy of the particles also increases, the internal energy and entropy both increase as the temperature is raised. Prentice-Hall © 2002 General Chemistry: Chapter 20
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General Chemistry: Chapter 20
Chemistry 140 Fall 2002 Entropy Change FIG. 19-4 ΔS = qrev T FIGURE 19-4 Three processes in which entropy increases Each of the processes pictured (a) the melting of a solid, (b) the evaporation of a liquid, and (c) the dissolving of a solute results in an increase in entropy. For part (c), the generalization works best for nonelectrolyte solutions, in which ion dipole forces do not exist. Prentice-Hall © 2002 General Chemistry: Chapter 20
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19-3 Evaluating Entropy and Entropy Changes
Chemistry 140 Fall 2002 19-3 Evaluating Entropy and Entropy Changes Phase transitions. Exchange of heat can be carried out reversibly. ΔS = ΔH Ttr H2O(s, 1 atm) H2O(l, 1 atm) ΔHfus° = 6.02 kJ at K ΔSfus = ΔHfus Ttr = 6.02 kJ mol-1 K = 22 J mol-1 K-1 Prentice-Hall © 2002 General Chemistry: Chapter 20
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General Chemistry: Chapter 20
Chemistry 140 Fall 2002 Trouton’s Rule The molar boiling entropy changes are similar for many materials (e.g. toluene, 87.3, benzene, 89.5, chloroform, 87.9,…): ΔS = ΔHvap Tbp = 87 kJ mol-1 K-1 Failures of this rule are understandable: Water and hydrogen bonding. Sliquid is lower than expected so ΔS is larger than 87. Prentice-Hall © 2002 General Chemistry: Chapter 20
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General Chemistry: Chapter 20
Chemistry 140 Fall 2002 Absolute Entropies Third law of thermodynamics. The entropy of a pure perfect crystal at 0 K is zero. Standard molar entropy. Tabulated in Table 17. Extensive state function, entropy can be summed in a multistep reaction ΔS = [ ∑pS°(products) - ∑rS°(reactants)] are the stoichiometric coefficients. General Chemistry: Chapter 20
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Molar entropies for the standard conditions
Compound Smo, J K-1mol-1 Solids C (diamond) 2.38 C (graphite) 5.74 Na 51.2 K 64.2 Rb 69.5 Cs 85.2 NaCl 72.1 KCl 82.6 I2 116.1 General Chemistry: Chapter 20
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Molar entropies for the standard conditions
Compound Smo, J K-1mol-1 Liquids Hg 76.0 Br2 152.2 H2O 69.9 CH3OH 126.8 C2H5OH 160.7 C6H6 172.8 Prentice-Hall © 2002 General Chemistry: Chapter 20
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Molar entropies for the standard conditions
Compound Smo, J K-1mol-1 Triatomic Gases H2O 188.8 NO2 240.1 H2S 205.8 CO2 213.7 SO2 248.2 Prentice-Hall © 2002 General Chemistry: Chapter 20
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Calculate DSº for the complete combustion of ethane (C2H6) with oxygen (O2).
Equation: C2H6 + 7/2 O2 → 2 CO2 + 3 H2O Vapor S°, JK-1mol-1 C2H6 229.6 O2 205.1 CO2 213.7 H2O 188.8 DSº= [2(213.7) + 3(188.8)] - [ /2(205.1)] = JK-1mol-1 Prentice-Hall © 2002 General Chemistry: Chapter 20
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Entropy as a Function of Temperature
Prentice-Hall © 2002 General Chemistry: Chapter 20
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Vibrational Energy and Entropy
Prentice-Hall © 2002 General Chemistry: Chapter 20
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General Chemistry: Chapter 20
19-4 Criteria for Spontaneous Change: The Second Law of Thermodynamics. ΔStotal = ΔSuniverse = ΔSsystem + ΔSsurroundings The Second Law of Thermodynamics (Clausius): ΔSuniverse = ΔSsystem + ΔSsurroundings > 0 All spontaneous processes produce an increase in the entropy of the universe. (Macroscopic, non equilibrium, isolated systems – spontaneous process: the entropy increases; it is maximal in the equilibrium.) Prentice-Hall © 2002 General Chemistry: Chapter 20
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Gibbs Energy and Gibbs Energy Change
Chemistry 140 Fall 2002 Gibbs Energy and Gibbs Energy Change Hypothetical process: only pressure-volume work, at constant T and P. qsurroundings = -qp = -ΔHsys Make the enthalpy change reversible. large surroundings, infinitesimal change in temperature. Under these conditions we can calculate entropy. Want to evaluate the system only, not the surroundings. Prentice-Hall © 2002 General Chemistry: Chapter 20
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Ice Melting Tsys= 273 K < Tsurr= 298 K and qsys = DHsys>0.
P=const. Tsys= 273 K < Tsurr= 298 K and qsys = DHsys>0. Egyensúly
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Ice Melting: Entalpy and Entropy
The entropy change of the surroundings and system: The ice melts because the total entropy change is positive: the entropy of the universe increases. Egyensúly
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Gibbs Energy and Energy Change
For the universe (P and Tsurr = const.) reversible: Tsurr ΔSuniv. = Tsurr ΔSsys – ΔHsys = -(ΔHsys – TsurrΔSsys) -TΔSuniv. = ΔHsys – TΔSsys For the system (P and T = const.): G = H - TS ΔG = ΔH - TΔS ΔGsys = - TΔSuniverse General Chemistry: Chapter 20
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Criteria for Spontaneous Change
ΔGsys < 0 (negative), the process is spontaneous. ΔGsys = 0 (zero), the process is at equilibrium. ΔGsys > 0 (positive), the process is non-spontaneous. Prentice-Hall © 2002 General Chemistry: Chapter 20
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19-5 Standard Gibbs Energy Change, ΔG°
The standard Gibbs energy of formation, ΔfG°. The Gibbs energy change for a reaction in which a substance in its standard state is formed from its elements in reference forms in their standard states. The standard Gibbs energy of reaction, ΔG°. where i s are the stoichiometric factors ΔG° = [ ∑p ΔfG°(products) - ∑r ΔfG°(reactants)] Prentice-Hall © 2002 General Chemistry: Chapter 20
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Standard changes of extensive quantities
Reaction Gibbs energy: ΔG° = [ ∑p ΔfG°(products) - ∑r ΔfG°(reactants)] Reaction entropy change: ΔS° = [ ∑p S°(products) - ∑r S°(reactants)] Reaction enthalpy change: ΔH° = [ ∑p ΔfH°(products) - ∑r ΔfH°(reactants)] where i s are the stoichiometric factors. General Chemistry: Chapter 20
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Általános Kémia, 2008 tavasz
Termodinamic table P = 1 atm, T =298 K DfH° S° DfG° kJ mol-1 J mol-1 K-1 H2O(l) -285.8 69.9 -237.1 H2O(g) -241.8 188.8 -228.6 H2O(l) → H2O(g) 44.0 118.9 8.5 The enthalpy change is positive, endothermic. DG° positive, the reaction is non spontaneous at atmospheric pressure DG° = 0 if P = mmHg - equilibrium. Equilibrium
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Gibbs Energy Change and Equilibrium
Prentice-Hall © 2002 General Chemistry: Chapter 20
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19-6 Gibbs Energy Change and Equilibrium
DG(T) = DH –TDS DS negative General Chemistry: Chapter 20
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Temperature dependence of the Gibbs free energy
DH and DS are constant for K. At the boiling point: (DG = 0) 𝑇= Δ𝐻 Δ𝑆 Tboil = /118.9 = 370 K ( 373 K) Above this temperature the DG < 0, and the water boils, evaporates completely. Δ𝐺=Δ𝐻−𝑇⋅Δ𝑆 0=Δ𝐻−𝑇⋅Δ𝑆 Egyensúly
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Water boiling, P = 1 atm Egyensúly
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+ Spontneous reactions DG(T) = DH –TDS DH DS DG(T) Examples -
H2O(l) → H2O(g) High T helps H2O(g) → H2O(l) Low T helps 4Fe(s) +3O2(g) →2Fe2O3(s) always 2Fe2O3(s)→ 4Fe(s) +3O2(g) never T T 32 11/18/2018 Professor Gabor I. Csonka
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Relationship of ΔG° to ΔG for Nonstandard Conditions
N2(g) + 3 H2(g) 2 NH3(g) ΔG = ΔH - TΔS ΔG° = ΔH° - TΔS° For ideal gases ΔH = ΔH° ΔG = ΔH° - TΔS Prentice-Hall © 2002 General Chemistry: Chapter 20
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Relationship Between S and S°
Vf qrev = -w = RT ln Vi ΔS = qrev T = R ln Vf Vi ΔS = Sf – Si = R ln Vf Vi Pi Pf = -R ln S = S° - R ln P P° = S° 1 = S° - R ln P Prentice-Hall © 2002 General Chemistry: Chapter 20
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N2(g) + 3 H2(g) 2 NH3(g) SN2 = S°N2 – R·ln PN2 SH2 = S°H2 – R·ln PH2
SNH3 = S°NH3 – R·ln PNH3 ΔSrxn = 2·(S°NH3 – R·ln PNH3) – (S°N2 – R·ln PN2) – 3· (S°H2 – R·ln PH2) PN2PH2 3 ΔSrxn = 2 S°NH3 –S°N2 –3S°H2+ R·ln PNH3 2 PN2PH2 3 ΔSrxn = ΔS°rxn + R·ln PNH3 2 Prentice-Hall © 2002 General Chemistry: Chapter 20
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ΔG Under Non-standard Conditions
PN2PH2 3 ΔG = ΔH° - TΔS ΔSrxn = ΔS°rxn + Rln PNH3 2 PN2PH2 3 ΔG = ΔH° - TΔS°rxn – TR ln PNH3 2 PNH3 2 ΔG = ΔG° + RT ln PN2PH2 3 ΔG = ΔG° + RT ln Q Q reaction quotient Prentice-Hall © 2002 General Chemistry: Chapter 20
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ΔG and the Equilibrium Constant Keq
ΔG = ΔG° + RT ln Q ΔG = ΔG° + RT ln Keq= 0 If the reaction is at equilibrium then: ΔG° = -RT ln Keq Prentice-Hall © 2002 General Chemistry: Chapter 20
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Criteria for Spontaneous Change
Every chemical reaction consists of both a forward and a reverse reaction. The direction of spontaneous change is the direction in which the Gibbs energy decreases. Prentice-Hall © 2002 General Chemistry: Chapter 20
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Significance of the Magnitude of ΔG0
Prentice-Hall © 2002 General Chemistry: Chapter 20
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The Thermodynamic Equilibrium Constant: Activities
Chemistry 140 Fall 2002 The Thermodynamic Equilibrium Constant: Activities For ideal gases at 1.0 bar: S = S° - R ln P P° = S° 1 PV=nRT or P=(n/V)RT, pressure is an effective concentration Therefore, in solution: S = S° - R ln c c° = S° - R ln a Activity is the effective concentration divided by the effective concentration in the standard state. The effective concentration in the standard state for an ideal solution is c° = 1 M. Prentice-Hall © 2002 General Chemistry: Chapter 20
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General Chemistry: Chapter 20
Activities For pure solids and liquids: a = 1 For ideal gases: a = P (in bars, 1 bar = atm) For ideal solutes in aqueous solution: a = c (in mol L-1) Prentice-Hall © 2002 General Chemistry: Chapter 20
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The Thermodynamic Equilibrium Constant, Keq
A dimensionless equilibrium constant expressed in terms of activities. Often Keq = Kc Must be used to determine ΔG. ΔG = ΔG° + RT ln agah… aaab… Prentice-Hall © 2002 General Chemistry: Chapter 20
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19-7 ΔG° and Keq as Functions of Temperature
ΔG° = ΔH° -TΔS° ΔG° = -RT ln Keq ln Keq = -ΔG° RT = -ΔH° TΔS° + ln Keq = -ΔH° RT ΔS° R + ln = -ΔH° RT2 ΔS° R + RT1 - = 1 T2 T1 Keq1 Keq2 Prentice-Hall © 2002 General Chemistry: Chapter 20
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Temperature Dependence of Keq
ln Keq = -ΔH° RT ΔS° R + slope = -ΔH° R -ΔH° = R · slope = J mol-1 K-1 · 2.2·104 K = -1.8·102 kJ mol-1 Prentice-Hall © 2002 General Chemistry: Chapter 20
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General Chemistry: Chapter 20
19-8 Coupled Reactions In order to drive a non-spontaneous reactions we changed the conditions (i.e. temperature or electrolysis) Another method is to couple two reactions. One with a positive ΔG and one with a negative ΔG. Overall spontaneous process. Prentice-Hall © 2002 General Chemistry: Chapter 20
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General Chemistry: Chapter 20
Smelting Copper Ore Cu2O(s) → 2 Cu(s) + ½ O2(g) ΔG°673K = +125 kJ Δ Cu2O(s) → 2 Cu(s) + ½ O2(g) Non-spontaneous reaction: +125 kJ C(s) + ½ O2(g) → CO(g) Spontaneous reaction: -175 kJ Cu2O(s) + C(s) → 2 Cu(s) + CO(g) -50 kJ Spontaneous reaction! Prentice-Hall © 2002 General Chemistry: Chapter 20
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Focus On Coupled Reactions in Biological Systems
ADP3- + HPO42- + H+ → ATP4- + H2O ΔG° = -9.2 kJ mol-1 ΔG = ΔG° + RT ln aATPaH2O aADPaPiaH3O+ But [H3O+] = 10-7 M not 1.0 M. ΔG = -9.2 kJ mol kJ mol-1 = kJ mol-1 = ΔG°' The biological standard state: Prentice-Hall © 2002 General Chemistry: Chapter 20
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Focus On Coupled Reactions in Biological Systems
Glucose → 2 lactate + 2 H+ -218 kJ 2 ADP HPO H+ → 2 ATP H2O +64 kJ 2 ADP HPO42- + glucose → 2 ATP H2O + 2 lactate -153 kJ Prentice-Hall © 2002 General Chemistry: Chapter 20
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