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CHEM 160 General Chemistry II Lecture Presentation Chemical Thermodynamics Chapter 19 November 19, 2018 Chapter 19.

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Presentation on theme: "CHEM 160 General Chemistry II Lecture Presentation Chemical Thermodynamics Chapter 19 November 19, 2018 Chapter 19."— Presentation transcript:

1 CHEM 160 General Chemistry II Lecture Presentation Chemical Thermodynamics
Chapter 19 November 19, 2018 Chapter 19

2 Thermodynamics Thermodynamics
study of energy and its transformations heat and energy flow Helps determine natural direction of reactions Allows us to predict if a chemical process will occur under a given set of conditions Organized around three fundamental laws of nature 1st law of thermodynamics 2nd law of thermodynamics 3rd law of thermodynamics November 19, 2018 Chapter 19

3 First Law of Thermodynamics
Energy can be neither created nor destroyed Energy of the universe is constant Important concepts from thermochemistry Enthalpy Hess’s law Purpose of 1st Law Energy bookkeeping How much energy? Exothermic or endothernic? What type of energy? November 19, 2018 Chapter 19

4 Spontaneous vs Nonspontaneous
Spontaneous process Occurs without outside assistance in the form of energy (occurs naturally) Product-favored at equilibrium May be fast or slow May be influenced by temperature Nonspontaneous process Does not occur without outside assistance Reactant-favored at equilibrium All processes which are spontaneous in one direction cannot be spontaneous in the reverse direction Spontaneous processes have a definite direction Spontaneous processes are irreversible November 19, 2018 Chapter 19

5 Spontaneous vs. Nonspontaneous
Spontaneous Processes Gases expand into larger volumes H2O(s) melts above 0C H2O(l) freezes below 0C NH4NO3 dissolves spontaneously in H2O Steel (iron) rusts in presence of O2 and H2O Wood burns to form CO2 and H2O CH4 gas burns to form CO2 and H2O Reverse processes are not spontaneous! nonspontaneous November 19, 2018 Chapter 19

6 Spontaneous vs. Nonspontaneous
Spontaneous Processes H2O(s) melts above 0C (endothermic) NH4NO3 dissolves spontaneously in H2O (endothermic) Steel (iron) rusts in presence of O2 and H2O (exothermic) Wood burns to form CO2 and H2O (exothermic) CH4 gas burns to form CO2 and H2O (exothermic) Heat change alone is not enough to predict spontaneity because energy is conserved Many, but not all, spontaneous processes are exothermic November 19, 2018 Chapter 19

7 Factors That Favor Spontaneity
Two thermodynamic properties of a system are considered when determining spontaneity: Enthalpy, H Many, but not all, spontaneous processes tend to be exothermic as already noted Entropy, S (J/K) Measure of the disorder of a system Many, but not all, spontaneous processes tend to increase disorder of the system November 19, 2018 Chapter 19

8 Entropy Entropy, S (J/K)
describes # of ways the particles in a system can be arranged in a given state More arrangements = greater entropy S = heat change/T = q/T S = Sfinal - Sinitial  S > 0 represents increased randomness or disorder November 19, 2018 Chapter 19

9 Patterns of Entropy Change
For the same or similar substances: Ssolid < Sliquid < Sgas solid vapor November 19, 2018 Chapter 19 liquid

10 Patterns of Entropy Change
Particles farther apart, occupy larger volume of space; even more positions available to particles Rigidly held particles; few positions available to particles Particles free to flow; more positions available for particles solid vapor November 19, 2018 Chapter 19 liquid

11 Patterns of Entropy Change
least ordered less ordered most ordered solid vapor November 19, 2018 Chapter 19 liquid

12 Patterns of Entropy Change
Solution formation usually leads to increased entropy particles more disordered solvent solute solution November 19, 2018 Chapter 19

13 Patterns of Entropy Change
Chemical Reactions If more gas molecules produced than consumed, S increases. (Srxn > 0) If only solids, ions and/or liquids involved, S increases if total # particles increases. November 19, 2018 Chapter 19

14 fewer arrangements possible so lower entropy
more arrangements possible so higher entropy November 19, 2018 Chapter 19

15 Patterns of Entropy Change
Increasing temperature increases entropy System at T1 (S1) System at T2 (T2 > T1) (S2 > S1) November 19, 2018 Chapter 19

16 Patterns of Entropy Change
more energetic molecular motions less energetic molecular motions System at T1 (S1) System at T2 (T2 > T1) (S2 > S1) November 19, 2018 Chapter 19

17 Third Law of Thermodynamics
If increasing T increases S, then the opposite should be true also. Is it possible to decrease T to the point that S is zero? At what T does S = 0? If entropy is zero, what does that mean? November 19, 2018 Chapter 19

18 Third Law of Thermodynamics
Entropy of a perfect crystalline substance at 0 K is zero No entropy = highest order possible Why? Purpose of 3rd Law Allows S to be measured for substances S = 0 at 0 K S = heat change/temperature = q/T S = standard molar entropy November 19, 2018 Chapter 19

19 Standard entropy, S° (J/K)
50 40 Standard entropy, S° (J/K) 30 20 10 50 100 150 200 250 300 November 19, 2018 Temperature (K) Chapter 19

20 Gas Liquid Solid Standard entropy, S° (J/K) Temperature (K) 50 40 30
20 Solid 10 50 100 150 200 250 300 November 19, 2018 Temperature (K) Chapter 19

21 Standard Molar Entropies of Selected Substances at 298 K
S (J/K) H2O(l) 69.9 NaCl(s) 72.3 H2O(g) 188.8 NaCl(aq) 115.5 I2(s) 116.7 Na2CO3(s) 136.0 I2(g) 260.6 CH4(g) 186.3 Na(s) 51.5 C2H6(g) 229.5 K(s) 64.7 C3H8(g) 269.9 Cs(s) 85.2 C4H10(g) 310.0 November 19, 2018 Chapter 19

22 Entropy versus Probability
Systems tend to move spontaneously towards increased entropy. Why? Entropy is related to probability Disordered states are more probable than ordered states S = k(lnW) k (Boltzman’s constant) = 1.38 x J/K W = # possible arrangements in system November 19, 2018 Chapter 19

23 Consider why gases tend to isothermally expand into larger volumes.
Isothermal Gas Expansion Consider why gases tend to isothermally expand into larger volumes. Gas Container = two bulbed flask Ordered State Gas Molecules November 19, 2018 Chapter 19

24 Isothermal Gas Expansion
Gas Container Ordered State S = k(ln 1) = (1.38 x J/K)(0) = 0 J/K November 19, 2018 Chapter 19

25 November 19, 2018 Chapter 19

26 November 19, 2018 Chapter 19

27 November 19, 2018 Chapter 19

28 November 19, 2018 Chapter 19

29 November 19, 2018 Chapter 19

30 Disordered States November 19, 2018 Chapter 19

31 Disordered States November 19, 2018 Chapter 19

32 Disordered States More probable that the gas molecules will disperse between two halves than remain on one side November 19, 2018 Chapter 19

33 Disordered States Driving force for expansion is entropy (probability); gas molecules have a tendency to spread out November 19, 2018 Chapter 19

34 Disordered States S = k(ln 7) = (1.38 x J/K)(1.95) = 2.7 x J/K November 19, 2018 Chapter 19

35 Total Arrangements Stotal = k(ln 23) = k(ln 8) = (1.38 x J/K)(1.79) = x J/K November 19, 2018 Chapter 19

36 2nd Law of Thermodynamics
The entropy of the universe increases in any spontaneous process (Suniv > 0) Increased disorder in the universe is the driving force for spontaneity November 19, 2018 Chapter 19

37 2nd Law of Thermodynamics
Suniv = Ssysyem + Ssurroundings Suniv > 0, process is spontaneous Suniv = 0, process at equilibrium Suniv < 0, process is nonspontaneous Process is spontaneous in reverse direction November 19, 2018 Chapter 19

38 2nd Law of Thermodynamics
Spontaneous Processes H2O(s) melts above 0C (endothermic) Steel (iron) rusts in presence of O2 and H2O (exothermic) 4Fe(s) + 3O2(g)  2Fe2O3(s) CH4 gas burns to form CO2 and H2O (exothermic) CH4(g) + 2O2(g)  CO2(g) + 2H2O(g) Each process increases Suniverse. November 19, 2018 Chapter 19

39 2nd Law of Thermodynamics
To determine Suniv for a process, both Ssystem and Ssurroundings need to be known: Ssysyem related to matter dispersal in system Ssurroundings determined by heat exchange between system and surroundings and T at which it occurs Sign of Ssurroundings depends on whether process in system is endothermic or exothermic Why? Magnitude of Ssurroundings depends on T Ssurroundings = -Hsystem/T November 19, 2018 Chapter 19

40 Entropy Changes in a System
For any reaction: S°rxn = nS°(products) - mS°(reactants) Where n and m are stoichiometric coefficients November 19, 2018 Chapter 19

41 Example 1 (1 on Example Problem Handout)
Using standard molar entropies, calculate S°rxn for the following reaction at 25°C: 2SO2(g) + O2(g) --> 2SO3(g) S° = (J · K-1mol-1) (Ans.: J/K) November 19, 2018 Chapter 19

42 Gibbs Free Energy, G 2nd law: Suniv = Ssys + Ssurr = Ssys - Hsys/T
Rearrange (multiply by -T) -TSuniv = -TSsys + Hsys = Hsys - TSsys -TSuniv = G (-TSuniv = G) G = Gibbs free energy (J or kJ) G = H - TS and G = Hsys - TSsys G° = H°sys - TS°sy (if at standard state) November 19, 2018 Chapter 19

43 Gibbs Free Energy Summary of Conditions for Spontaneity G < 0
November 19, 2018 Chapter 19

44 Gibbs Free Energy Summary of Conditions for Spontaneity G < 0
reaction is spontaneous in the forward direction (Suniv > 0) G > 0 G = 0 November 19, 2018 Chapter 19

45 Gibbs Free Energy Summary of Conditions for Spontaneity G < 0
reaction is spontaneous in the forward direction (Suniv > 0) G > 0 reaction is nonspontaneous in the forward direction (Suniv < 0) G = 0 November 19, 2018 Chapter 19

46 Gibbs Free Energy Summary of Conditions for Spontaneity G < 0
reaction is spontaneous in the forward direction (Suniv > 0) G > 0 reaction is nonspontaneous in the forward direction (Suniv < 0) G = 0 system is at equilibrium (Suniv = 0) November 19, 2018 Chapter 19

47 Example 2 (2 in Example Problem Handout)
For a particular reaction, Hrxn = 53 kJ and Srxn = 115 J/K. Is this process spontaneous a) at 25°C, and b) at 250°C? (c) At what temperature does Grxn = 0? (ans.: a) G = 18.7 kJ, nonspontaneous; b) –7.1 kJ, spontaneous; c) K or 188C) November 19, 2018 Chapter 19

48 Gibbs Free Energy and Temperature
G = H - TS S > 0 H < 0 Spontaneous at all T S < 0 H > 0 Not spontaneous at any T S > 0 H > 0 Spontaneous at high T; nonspontaneous at low T S < 0 H < 0 Spontaneous at low T; nonspontaneous at high T November 19, 2018 Chapter 19

49 Gibbs Free Energy and Temperature
Spontaneous Processes H2O(s) melts above 0C (endothermic) H > 0, S > 0 Steel (iron) rusts in presence of O2 and H2O at 25 C (exothermic) 4Fe(s) + 3O2(g)  2Fe2O3(s) H < 0, S < 0 G < 0 for each process T determines sign of G: G = H -TS November 19, 2018 Chapter 19

50 Calculating Free Energy Changes
For any reaction: G°rxn = Gf°(products) - mGf°(reactants) Where n and m are stoichiometric coefficients and Gf° = standard free energy of formation November 19, 2018 Chapter 19

51 Example 3 (3 on Example Problem Handout)
Calculate the standard free energy change for the reaction at 25°C: CH4(g) + 2O2(g)  CO2(g) + 2H2O(l) G°f = (kJ/mol) November 19, 2018 Chapter 19

52 Gibbs Free Energy What does Gibbs free energy represent?
For a spontaneous process: Maximum amount of energy released by the system that can do useful work on the surroundings Energy available from spontaneous process that can be used to drive nonspontaneous process For a nonspontaneous process: Minimum amount of work that must be done to force the process to occur In actuality, Gspont > Gnonspont November 19, 2018 Chapter 19

53 Gibbs Free Energy Conversion of rust to iron
2Fe2O3  4Fe + 3O2 G = 1487 kJ (NS) To convert iron to rust, G must be provided from spontaneous rxn 6CO + 3O2  6CO2 G = kJ (S) November 19, 2018 Chapter 19

54 Gibbs Free Energy Conversion of rust to iron
2Fe2O3  4Fe + 3O2 G = 1487 kJ (NS) To convert iron to rust, G must be provided from spontaneous rxn 2Fe2O3  4Fe + 3O2 G = 1487 kJ (NS) 6CO + 3O2  6CO2 G = kJ (S) 2Fe2O3 + 6CO  4Fe + 6CO2  G = -56 kJ (S) Reactions are “coupled” November 19, 2018 Chapter 19

55 Gibbs Free Energy Many biological rxns essential for life are NS
Spontaeous rxns used to “drive” the NS biological rxns Example: photosynthesis 6CO2 + 6H2O  C6H12O6 + 6O2  G > 0 What spontaneous rxns drive photosynthesis? November 19, 2018 Chapter 19

56 proteins, cells etc., lower S amino acids, sugars, etc., higher S
sun big ball of G = G released high free energy DGsurr < 0 proteins, cells etc., lower S C6H12O6, O2 ATP NS Sp NS Sp NS CO2, H2O amino acids, sugars, etc., higher S ADP photosynthesis solar nuclear reactions low free energy November 19, 2018 Chapter 19

57 Free Energy and Equilibrium
G (Nonstandard State) G = G° + RTlnQ R = gas constant (8.314 J/K·mol) T = temperature (K) Q = reaction quotient November 19, 2018 Chapter 19

58 Example 4 (4 on Example Problem Handout)
Calculate Grxn for the reaction below: 2A(aq) + B(aq)  C(aq) + D(g) if G°rxn = 9.9 x 103 J/mol and (a) [A] = 0.8 M, [B] = 0.5 M, [C] = 0.05 M, and PD = 0.05 atm, and (b) [A] = 0.1 M, [B] = 1 M, [C] = 0.5 M, and PD = 0.5 atm. Is the reaction spontaneous under these conditions? (ans.: a) –2121 J, spontaneous; b) J, nonspontaneous) November 19, 2018 Chapter 19

59 Free Energy and Equilibrium
At equilibrium: Grxn = 0 and Q = K 0 = G°rxn + RTlnK G°rxn = -RTlnK November 19, 2018 Chapter 19

60 Example 5 (5 on Example Problem Handout)
Calculate G°rxn for the ionization of acetic acid, HC2H3O2 (Ka = 1.8 x 10-5) at 25°C. Is this reaction spontaneous under standard state conditions? (ans.: 27 kJ) November 19, 2018 Chapter 19

61 Example 6 (6 on Example Problem Handout)
Calculate G° for the neutralization of a strong acid with a strong base at 25°C. Is this process spontaneous under these conditions? For the reaction below, K = 1.0 x 1014. H+ + OH-  H2O (ans.: -80 kJ) November 19, 2018 Chapter 19

62 Example 7 Calculate Keq for a reaction at (a) 25°C and (b) 250°C if H°rxn = 42.0 kJ and S°rxn = 125 J/K. At which temperature is this process product favored? (ans.: a) 0.15; b) 216; 250C) November 19, 2018 Chapter 19

63 DGrxn < 0 Spontaneous Reaction equilibrium position Pure reactants
Pure products DGrxn < 0 Gproducts Greactants extent of reaction November 19, 2018 Chapter 19

64 Spontaneous Reaction At equilibrium, any change requires an uphill climb in energy, DGrxn > 0 Gproducts Greactants Pure reactants Pure products extent of reaction November 19, 2018 Chapter 19

65 Calculating G for Processes
G may be calculated in one of several ways depending on the information known about the process of interest G = H - TS; G° = H° - TS° G°rxn = Gf°(products) - mGf°(reactants) G = G° + RTlnQ G°rxn = -RTlnK November 19, 2018 Chapter 19

66 Entropy and Life Processes
If the 2nd law is valid, how is the existence of highly-ordered, sophisticated life forms possible? growth of a complex life form represents an increase in order (less randomness) lower entropy November 19, 2018 Chapter 19

67 Entropy and Life Processes
Organisms “pay” for their increased order by increasing Ssurr. Over lifetime, Suniv > 0. CO2 H2O heat November 19, 2018 Chapter 19


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