Spontaneous processes Chapter 19 We have a general idea of what we consider spontaneous to mean: Spontaneous Change: Entropy and Free Energy A spontaneous process WILL OCCUR in a system WITHOUT any outside action being performed on the system. Dr. Peter Warburton [email protected] http://www.chem.mun.ca/zcourses/1051.php 2 Spontaneous processes Spontaneous processes Ice will melt above zero Celcius. We don’t have to DO anything! Objects will fall to earth. We don’t have to DO anything! Ice melting above zero Celcius is spontatneous Object falling to earth is spontaneous 3 4 1 Spontaneous processes Non-spontaneous processes We have a general idea of what we consider non-spontaneous to mean: Since we DON’T have to DO anything for these spontaneous processes to occur it APPEARS that an overall energy change from potential energy to kinetic energy IS SPONTANEOUS A non-spontaneous process WILL NOT OCCUR in a system UNTIL an outside action is performed on the system. 5 Non-spontaneous processes Ice freezing above zero Celcius is non-spontatneous 6 Non-spontaneous processes We can make water freeze above zero Celcius by increasing the pressure. We can make an object rise from the earth by picking it up. Object rising from earth is non-spontaneous 7 8 2 Non-spontaneous processes Chemistry and spontaneity We know there are chemical processes that are spontaneous because we can put the chemical system together and reactants become products without us having to do anything. Since we DO have to ACT for these non-spontaneous processes to occur it APPEARS that an overall energy change from kinetic energy to potential energy IS NON-SPONTANEOUS H3O+ (aq) + OH- (aq) → 2 H2O (l) 9 Chemistry and non-spontaneity 10 Spontaneous vs. non-spontaneous It is obvious by the examples we’ve looked at that the opposite of every spontaneous process is a non-spontaneous process. We know there are chemical processes that are non-spontaneous because we can put the chemical system together and reactants DO NOT become products. In chemical systems we’ve seen that if we put a chemical system together a reaction occurs until the system reaches equilibrium. The system we put together stays like it is UNTIL WE CHANGE SOMETHING! Whether the forward reaction or the reverse reaction dominates depends on which of the two reactions is spontaneous at those conditions! 2 H2O (l) → 2 H2 (g) + O2 (g) 11 12 3 Spontaneity and energy In our examples it APPEARED that the spontaneous process ALWAYS takes a system to a lower potential energy. Equilibrium and spontaneity are related! 13 Spontaneity and energy 14 Recall the First Law The First Law of thermodynamics stated that the energy of an ISOLATED system is constant. What’s the largest ISOLATED system we can think of? If this were true all exothermic processes would be spontaneous and all endothermic processes would be nonspontaneous. THIS ISN’T TRUE! NH4NO3 (s) → NH4+ (aq) + NO3- (aq) is spontaneous even though It’s the UNIVERSE! The energy of the universe is constant! H2O ∆H = +25.7 kJ 15 16 4 Recall the First Law Further proof lower energy isn’t enough If an ideal gas expands into a vacuum at a constant temperature, then On the universal scale, there is no overall change in energy, and so lower energy CANNOT be the only requirement for spontaneity. no work is done There must be something else as well! and no heat is transferred 17 Further proof lower energy isn’t enough 18 Further proof lower energy isn’t enough No work done and no heat transferred means This spontaneous process has no overall change in energy! NO OVERALL CHANGE in energy of the system 19 20 5 Entropy Entropy Entropy (from Greek, meaning “in transformation”) is a thermodynamic property that relates the distribution of the total energy of the system to the available energy levels of the particles. A general way to envision entropy is “differing ways to move” Consider mountain climbers on a mountain. Two factors affect the distribution of mountain climbers on a mountain: Total energy of all the climbers and how many places can you stop on the mountain 21 Consider hungry mountain climbers 22 Consider well fed mountain climbers Hungry mountain climbers have little total energy amongst themselves to climb a mountain, so most of them are near the bottom, while some are distributed on the lower parts of the mountain. Well-fed mountain climbers have more total energy amongst themselves to climb a mountain, so the climbers will be more spread out on the whole mountain. Few energy levels can be reached! More energy levels can be reached! 23 24 6 Temperature and total energy Higher mountain means more places to stop The total energy shared by molecules is related to the temperature. A given number of molecules at a low temperature (less total energy) have less “differing ways to move” than the same number of molecules at a high temperature (more total energy). If a well-fed mountain climber tries to climb Signal Hill, they will most likely reach the top. They have only a few places to stop (levels) because Signal Hill is a small mountain. The same well-fed mountain climber on Mount Everest has a greater number of places to stop (levels) because it is a larger mountain. 25 Volume and energy levels 26 Entropy The number of levels of energy distribution of molecules is related to the volume. A given number of molecules in a small volume have less “differing ways to move” than the same number of molecules in a larger volume. The greater the number of “differing ways to move” molecules can take amongst the available energy levels of a system of a given state (defined by temperature and volume, and number of molecules), the greater the entropy of the system. 27 28 7 Expansion into vacuum Expansion into vacuum A gas expands into a vacuum because the increased volume allows for a greater number of “differing ways to move” for the molecules, even if the temperature is the same. That is, the entropy increases when the gas is allowed to expand into a vacuum. Entropy increase plays a role in spontaneity! 29 Entropy is a state function 30 Boltzmann equation and entropy Entropy, S, is a state function like enthalpy or internal energy. The entropy of a system DEPENDS ONLY on the current state (n, T, V, etc.) of the system, and NOT how the system GOT TO BE in that state. 31 More available energy levels when the size of a box increases – like expanding a gas into a vacuum – ENTROPY INCREASES! More energy levels are accessible when the temperature increases – ENTROPY INCREASES! 32 8 Hess’s Law Change in entropy is a state function Recall Hess’s Law – as long as we get from the same initial state to the same final state then ∆H will be the same regardless of the steps we add together. Because entropy is a state function, then change in entropy ∆S is ALSO a state function. The difference in entropy between two states ONLY depends on the entropy of the initial and final states, and NOT the path taken to get there. Change in entropy ∆S will work exactly the same way! As long as we get from the same initial state to the same final state then ∆S will be the same regardless of the steps we add together. 33 Boltzmann equation and entropy 34 Playing cards Say we have a deck of 52 playing cards. Choosing one playing card is a state. n, T, V help define the number of states (number of available energy levels) the system can have. The many “different ways to move” of molecules in a particular state are called microstates. Hopefully it makes sense that more total states should automatically mean more total microstates. If we choose the first card out of the pack, there are 52 microstates for this first state. The second card (second state) we choose has 51 microstates, and so on. The number of microstates is often symbolized by W. 35 36 9 Playing cards Playing cards and coin flips If we flip 52 coins (a coin is one state), with two possible microstates (heads or tails) each, there are Overall there are W = 52! ≈ 8 x 1067 possible distributions (total microstates) for 52 playing cards! W = 252 = 4.5 x 1015 possible distributions. (total microstates) A deck of 52 playing cards has greater entropy than 52 coins! 37 Boltzmann equation and entropy 38 Boltzmann equation and entropy S = k ln W where k = R / NA Ludwig Boltzmann formulated the relationship between the number of microstates (W) and the entropy (S). S = k ln W The constant k is the Boltzmann constant which has a value equal to the gas constant R divided by Avagadro’s number NA k = (8.3145 J⋅K-1⋅mol-1) / (6.022 x 1023 mol-1) k = 1.381 x 10-23 J⋅K-1 We can see the units for entropy will be Joules per Kelvin (J⋅K-1) 39 40 10 Measuring entropy change Measuring entropy change From the units for entropy (J⋅K-1) we get an idea of how we might measure entropy change ∆S ∆S = qrev / T The change in entropy is the heat involved in a reversible process at a constant temperature. It must involve some sort of energy change relative to the temperature change! 41 Heat IS NOT a state function 42 Reversible processes Since heat IS NOT a state function we need a reversible process to make it ACT LIKE a state function. 43 In a reversible process a change in one direction is exactly equal and opposite to the change we see if we do the change in the reverse direction. In reality it is impossible to make a reversible process without making an infinite number of infinitesimally small changes. 44 11 Reversible processes Endothermic increases in entropy We can however imagine the process is done reversibly and calculate the heat involved in it, so we can calculate the reversible entropy change that could be involved in a process. In these three processes the molecules gain greater “differing ability to move.” The molecules occupy more available microstates at the given temperature, and so the entropy increases in all three processes! ∆Srev = qrev / T 45 46 Problem Generally entropy increases when… …we go from solid to liquid. …we go from solid or liquid to gas. …we increase the amount of gas in a reaction. …we increase the temperature. …we allow gas to expand against a vacuum. …we mix gases, liquids, or otherwise make solutions of most types. Predict whether entropy increases, decreases, or we’re uncertain for the following processes or reactions: a) 2 H 2 S (g) + SO 2 (g) ⎯ ⎯→ 3 S (s) + 2 H 2 O (g) b) 2 HgO (s) ⎯ ⎯→ 2 Hg (l) + O 2 (g) c) Zn (s) + 2 Ag 2 O (s) ⎯ ⎯→ ZnO (s) + 2 Ag (s) is d) 2 Cl - (aq) + 2 H 2 O (l) ⎯electrolys ⎯ ⎯⎯ → 2 OH - (aq) + H 2 (g) + Cl 2 (g) Answers: a) decreases b) increases c) uncertain d) increases 47 48 12 Evaluating entropy and entropy changes Evaluating entropy and entropy changes Phase transitions – In phase transitions the heat change does occur reversibly, so we can use the formula Phase transitions – For water going from ice (solid) to liquid, ∆H°fus = 6.02 kJ⋅mol-1 at the melting point (transition temp.) of 273.15 K (0 °C) ∆Srev = qrev / T ∆S°fus = ∆H°fus / Tmp ∆S°fus = 6.02 kJ⋅mol-1 / 273.15 K ∆S°fus = 22.0 J⋅K-1⋅mol-1 to calculate the entropy change. In this case the heat is the enthalpy of the phase transition and the temperature is the transition temperature ∆S = ∆Htr / Ttr 49 50 Problem Evaluating entropy and entropy changes Phase transitions – For water going from liquid to gas, ∆H°vap = 40.7 kJ⋅mol-1 at the boiling point (transition temp.) of 373.15 K (100 °C) What is the standard molar entropy of vapourisation ∆S°vap for CCl2F2 if its boiling point is -29.79 °C and ∆H°vap = 20.2 kJ⋅mol-1? ∆S°vap = ∆H°vap / Tbp ∆S°vap = 40.7 kJ⋅mol-1 / 373.15 K ∆S°vap = 109 J⋅K-1⋅mol-1 Answer: ∆S°vap = 83.0 J⋅K-1⋅mol-1 51 52 13 Problem Absolute entropies The entropy change for the transition from solid rhombic sulphur to solid monoclinic sulphur at 95.5 °C is ∆S°tr = 1.09 J⋅K-1⋅mol-1. What is the standard molar enthalpy change ∆H°tr for this transition? Answer: ∆H°tr = 402 J⋅mol-1 Say we imagine a system of molecules that has no total energy. At this zeropoint energy there can ONLY be ONE possible distribution of microstates, as no molecule has the energy to occupy a higher energy level. The entropy CAN NEVER get smaller than its value in this situation, so we define the entropy S of this situation as ZERO. 53 54 Absolute entropies This kind of imagining is the Third Law of Thermodynamics which states that The entropy of a pure perfect crystal at 0K is zero. Methyl chloride entropy as a function of temperature At conditions other than at absolute zero, our entropy is that of the perfect system (zero) PLUS any entropy changes that come changing temperature and/or volume. These are absolute entropies! 55 56 14 Standard molar entropies Standard molar entropies One mole of a substance in its standard state will have an absolute entropy that we often call the standard molar entropy S°. ∆S° = [ΣνpS°(products) - ΣνrS°(reactants)] Hopefully this looks somewhat familiar! We have seen a special treatment of Hess’s Law in Chem 1050 where These are usually tabulated at 298.15 K In a chemical process we can then use these standard molar entropies to calculate the entropy change in the process. ∆H° = [Σνp∆Hf°(products) - Σνr∆Hf°(reactants)] We can do something similar with ANY thermodynamic property that IS A STATE FUNCTION! 57 Standard molar entropies 58 Problem ∆S° = [ΣνpS°(products) – ΣνrS°(reactants)] ∆H° = [Σνp∆Hf°(products) – Σνr∆Hf°(reactants)] Enthalpies of formation ARE NOT absolute! Use the data given to calculate the standard molar entropy change for the synthesis of ammonia from its elements. N2 (g) + 3 H2 (g) → 2 NH3 (g) S°298 for N2 = 191.6 J⋅K-1⋅mol-1 S°298 for H2 = 130.7 J⋅K-1⋅mol-1 S°298 for NH3 = 192.5 J⋅K-1⋅mol-1 Answer: -198.7 J⋅K-1 ⋅ mol-1 (per mole of rxn) 59 60 15 Problem The second law of thermodynamics We’ve seen that entropy MUST play a role in spontaneity, because the total energy of the universe doesn’t change. We could say that an entropy increase leads to spontaneity, but we have to be careful. N2O3 is an unstable oxide that readily decomposes. The decomposition of 1.00 mol N2O3 to nitrogen monoxide and nitrogen dioxide at 25 °C is accompanied by the entropy change ∆S° = 138.5 J⋅K-1⋅mol-1. What is the standard molar entropy of N2O3 (g) at 25 °C? S°298 for NO (g) = 210.8 J⋅K-1⋅mol-1 S°298 for NO2 (g) = 240.1 J⋅K-1⋅mol-1 Answer: 312.4 J⋅K-1 ⋅mol-1 61 The second law of thermodynamics 62 The second law of thermodynamics Ice freezing below 0 Celcius is spontaneous, but the entropy of the water decreases in the process! The water is ONLY the system. The rest of the universe (the surroundings) must experience an opposite heat change as it takes the heat the freezing water gave off (a +ve ∆H for the surroundings), which means the entropy of the REST OF THE UNIVERSE INCREASES in the process of water freezing! ∆S°freeze = -∆H°fus / Tmp Since ∆H°fus and Tmp are +ve, then ∆S°freeze is –ve! -ve since “freezing” is the reverse of “fusion” (like we do in Hess’s Law) 63 64 16 The second law of thermodynamics The second law of thermodynamics The total entropy change in any process is the entropy change for the system PLUS the entropy change for the surroundings In any spontaneous process the entropy of the universe INCREASES. ∆Suniverse = ∆Ssys + ∆Ssurr > ∆Suniverse = ∆Stotal = ∆Ssys + ∆Ssurr Now we can connect entropy and spontaneity! 0 This is the Second Law of Thermodynamics! 65 Water freezing 66 Free energy So while water freezing below zero Celcius decreases the entropy of the system, the heat given off to the surroundings increases the entropy of the surroundings to a greater extent. We’ve seen entropy increases when molecules have more ways to distribute themselves amongst the energy levels. The total entropy change of the universe is positive and the process of water freezing below 0 Celcius is spontaneous! 67 68 17 Free energy Free energy ∆Suniverse = ∆Ssys + ∆Ssurr However, some of the energy a molecule uses to put itself at a higher energy level CAN NO LONGER be used to to do work because doing work would put the molecule back at a lower energy level, which would automatically decrease entropy. T∆Suniverse = T∆Ssys + T∆Ssurr T∆Suniverse = T∆Ssys + ∆Hsurr The energy is NOT free (or available) to be used! ∆S = ∆Hrev / T then Reversible since the rest of the universe is SO BIG T∆S = ∆H 69 Free energy 70 Free energy T∆Suniverse = T∆Ssys + ∆Hsurr T∆Suniverse = T∆Ssys - ∆Hsys T∆Suniverse = T∆Ssys – ∆Hsys -T∆Suniverse = ∆Hsys - T∆Ssys ∆G = ∆Hsys – T∆Ssys ∆G is the free energy (Gibbs free energy) Since ∆Hsys = -∆Hsurr 71 72 18 Free energy Free energy ∆G < 0 is spontaneous ∆G = -T∆Suniv For a spontaneous process ∆Suniv > 0, which means for a spontaneous process ∆G < 0! ∆G > 0 is non-spontaneous ∆G = 0 is at equilibrium 73 74 Problem Predict the spontaneity at low and high temperatures for: N2 (g) + 3 H2 (g) → 2 NH3 (g) ∆H° = -92.22 kJ 2 C (s) + 2 H2 (g) → C2H4 (g) ∆H° = 52.26 kJ 75 76 19 Standard free energy change ∆G° Problem Just like we can have a standard enthalpy change ∆H° for chemicals, we can also define the standard free energy change… ∆G° = ∆H° - T∆S° N2 (g) + 3 H2 (g) → 2 NH3 (g) ∆H° = -92.22 kJ Spontaneous @ low T and nonspontaneous @ high T 2 C (s) + 2 H2 (g) → C2H4 (g) ∆H° = 52.26 kJ Nonspontaneous @ all T 77 78 Problem Standard free energy of formation ∆Gf° Standard enthalpies of formation ∆Hf° of elements in their standard states are zero: ∆H°rxn = [Σνp ∆Hf°(products) – Σνr ∆Hf°(reactants)] Standard free energies of formation ∆Gf° of elements in their standard states are zero: ∆G° = [Σνp ∆Gf°(products) – Σνr ∆Gf°(reactants)] 79 Calculate ∆G° at 298.15 K for the reaction 4 Fe (s) + 3 O2 (g) → 2 Fe2O3 (s) by using the two following sets of data. Compare your answers. a) ∆H° = -1648 kJ ⋅mol-1 and ∆S° = -549.3 J⋅K-1 ⋅mol-1 b) ∆Gf° (Fe) = 0 kJ⋅mol-1 ∆Gf° (O2) = 0 kJ⋅mol-1 ∆Gf° (Fe2O3) = -742.2 kJ⋅mol-1 80 20 Problem answer Free energy and equilibrium a) ∆G° = -1484 kJ⋅mol-1 b) ∆G° = -1484.4 kJ⋅mol-1 The answers are the same because free energy is a state function. We’ve already seen that ∆G < 0 is spontaneous ∆G > 0 is non-spontaneous One process in a written reaction is spontaneous while the reverse is not, as long as ∆G ≠ 0. Therefore ∆G = 0 is at equilibrium 81 Water and steam 82 Water and steam H2O (l, 1 atm) ' H2O (g, 1 atm) ∆G°373.15 K = 0 kJ⋅mol-1 The system is at equilibrium at 1 atm (standard conditions) and at the boiling point temperature! 83 H2O (l, 1 atm) ' H2O (g, 1 atm) ∆G°298.15 K = 8.590 kJ⋅mol-1 The system is not at equilibrium at 1 atm (standard conditions) and at the room temperature! 84 21 Water and steam Water and steam H2O (l, 0.03126 atm) ' H2O (g, 0.03126 atm) H2O (l, 1 atm) ' H2O (g, 1 atm) ∆G°298.15 K = 8.590 kJ⋅mol-1 ∆G298.15 K = 0 kJ The system is at equilibrium at 0.03126 atm (non-standard conditions) and at the room temperature! The forward process is nonspontaneous (∆G° > 0) so the reverse process is spontaneous and condensation occurs. 85 Water and steam 86 Non-standard conditions H2O (l, 0.03126 atm) ' H2O (g, 0.03126 atm) ∆G298.15 K = 0 kJ⋅mol-1 Water CAN evaporate at room temperature, just not to give an equilibrium pressure of 1 atm! As we’ve seen with the previous water example, our interest in an equilibrium system is often at non-standard conditions, so knowing ∆G° is usually not as useful as knowing ∆G. 87 88 22 Non-standard conditions Non-standard free energy For an ideal gas ∆H does not change if pressure changes, so at all nonstandard conditions ∆H = ∆H°. Because of these facts, the nonstandard free energy change is For an ideal gas ∆S does change if pressure changes (expansion into vacuum shows us this!), so at all non-standard conditions ∆S ≠ ∆S°. But the standard free energy change is ∆G = ∆H° - T∆S ∆G° = ∆H° - T∆S° 89 Non-standard free energy 90 Boltzmann distribution The difference between standard and non-standard free energy is totally due to the difference in entropy change between the standard and non-standard conditions By the Boltzmann distribution S = R ln W for one mole of particles ∆G = ∆G° + T(R ln W - R ln W°) ∆G = ∆G° + T(R ln W / W°) We are comparing a real system with a standard one. We are dealing with activities! ∆G - ∆G° = - T(∆S-∆S°) ∆G = ∆G° + T(∆S°-∆S) 91 92 23 Boltzmann distribution Boltzmann distribution ∆G = ∆G° + RT ln Qeq In the comparison, we are looking at a reaction quotient! In other words, we are looking at how our non-standard system is different from the system we have at standard conditions! ∆G = ∆G° + RT ln Qeq If our system is at equilibrium then Qeq = Keq and ∆G = 0 93 Boltzmann distribution 94 Equilibrium constant ∆G = ∆G° + RT ln Keq = 0 which means The thermodynamic equilibrium constant for a reaction is directly related to the standard free energy change! ∆G° = -RT ln Keq ∆G° = -RT ln Keq Keq = e-∆G°/RT 95 96 24 Equilibrium constant ∆G° ≈ 0 Keq ≈ 1 ∆G° >> 0 then Keq is very small Equilibrium constant at 298 K ∆G° ∆G° << 0 then Keq is very large Keq Meaning Keq = e-∆G°/RT 97 Predicting reaction direction 98 Predicting reaction direction ∆G < 0 means the forward reaction is spontaneous at the given non-standard conditions ∆G = 0 means the system is at equilibrium at the given nonstandard conditions ∆G° < 0 means the forward reaction is spontaneous at standard conditions and so K > 1 ∆G° = 0 means the system is at equilibrium at standard conditions and so Keq = 1 which only occurs at one specific T! 99 100 25 Predicting reaction direction Predicting reaction direction ∆G = ∆G° ∆G > 0 means the forward reaction is non-spontaneous at the given non-standard conditions ∆G° > 0 means the forward reaction is non-spontaneous at standard conditions and so K < 1 ONLY at standard conditions! 101 Thermodynamic equilibrium constant Keq 102 Thermodynamic equilibrium constant Keq The thermodynamic equilibrium constant Keq is expressed in terms of activities, which are unitless quantities. Activities relate properties like concentration or pressure compared to a standard property value, like 1 M for concentration or 1 bar for pressure. aA+bB'cC+dD K eq (a C )c (a D )d = (a A )a (a B )b where ax = [X] / c0 (c0 is a standard concentration of 1 M) or ax = Px / P0 (P0 is a standard pressure of 1 atm) Note that ax = 1 for pure solids and liquids 103 104 26 Problem Free energy and equilibrium constants ∆G° = -RT ln Keq IS ALWAYS TRUE ∆G° = -RT ln Kc and ∆G° = -RT ln Kp DO NOT have to be true! Write thermodynamic equilibrium constant expressions for each of the following reactions and relate them to Kc and Kp where appropriate: a) Si (s) + 2 Cl2 (g) ' SiCl4 (g) b) Cl2 (g) + H2O (l) ' HOCl (aq) + H+ (aq) + Cl- (aq) 105 Problem answer Problem a) Si (s) + 2 Cl2 (g) ' SiCl4 (g) K eq = (a SiCl 4 (a Si )(a Cl ) ⎛ PSiCl 4 ⎞ ⎜ ⎟ PSiCl 4 P° ⎠ = ⎝ = = Kp 2 2 PCl 2 ⎛ PCl 2 ⎞ (1)⎜ P ° ⎟ ⎝ ⎠ ( ) ( ) ) 2 2 b) Cl2 (g) + H2O (l) ' HOCl (aq) + H+ (aq) + Cl- (aq) K eq = (a HOCl )(a H )(a Cl + (a )(a ) Cl 2 H 2O ⎛ [HOCl] - ) = ⎜⎝ 106 + ⎞⎟⎛ [H ] ⎞⎛ [Cl ] ⎞ ⎜ ⎟⎜ ⎟ c ° ⎠⎝ c ° ⎠⎝ c ° ⎠ [HOCl][H + ][Cl - ] = PCl 2 ⎛ PCl 2 ⎞ ⎜ ° ⎟(1) P ⎠ ⎝ ( ) 107 Use the given data to determine if the following reaction is spontaneous at standard conditions at 298.15 K: N2O4 (g) ' 2 NO2 (g) ∆G°f (N2O4) = 97.89 kJ⋅mol-1 ∆G°f (NO2) = 51.31 kJ⋅mol-1 Answer: ∆G° = 4.73 kJ⋅mol-1, not spontaneous at standard conditions. 108 27 Problem Problem Determine the equilibrium constant at 298.15 K for the following reaction using the given data: AgI (s) ' Ag+ (aq) + I- (aq) Based on the problem of the previous slide, determine which direction the reaction will go in if 0.5 bar of each gas is placed in an evacuated container: N2O4 (g) ' 2 NO2 (g) ∆G°f (AgI) = -66.19 kJ⋅mol-1 ∆G°f (Ag+) = 77.11 kJ⋅mol-1 ∆G°f (I-) = -51.57 kJ⋅mol-1 Answer: Since ∆G° = 4.73 kJ⋅mol-1, then Keq = 0.15 = Kp. Since Qp = 0.5 the reaction should go from right to left. 109 110 ∆G° and Keq are functions of T Problem answer Since ∆G° = 91.73 kJ⋅mol-1, then Keq = 8.5 x 10-17 = Kc = Ksp. If we compare to the Ksp value in Table 18.1 (8.5 x 10-17) we see we are definitely in the right ballpark! 111 We’ve already seen that equilibrium constants change with temperature. Why? Keq = e-∆G°/RT and ∆G° = ∆H° - T∆S° 112 28 ∆G° and Keq are functions of T Problem ∆G° = -RT ln Keq = ∆H° - T∆S° ln Keq= -(∆H°/RT) + (∆S°/R) At what temperature will the following reaction have Kp = 1.50 x 102? 2 NO (g) + O2 (g) ' 2 NO2 (g) ∆H° = -114.1 kJ⋅mol-1 and ∆S° = -146.5 J ⋅K-1⋅mol-1 Answer: T = 606 K 113 ∆G° and Keq are functions of T 114 ∆G° and Keq are functions of T ∆G° = -RT ln Keq = ∆H° - T∆S° ln Keq= -(∆H°/RT) + (∆S°/R) If ∆H and ∆S are constant over a temperature range then 115 ln K1= -(∆H°/RT1) + (∆S°/R) minus ln K2= -(∆H°/RT2) + (∆S°/R) ln K1 - ln K2 = -(∆H°/RT1) - (-∆H°/RT2) 116 29 ∆G° and Keq are functions of T van’t Hoff equation ln K1 - ln K2 = [-∆H°/R] [(1/T1) - (1/T2)] OR ln [K1/K2] = [-∆H°/R] [(1/T1) - (1/T2)] The van’t Hoff equation relates equilibrium constants to temperatures ln [K1/K2] = [-∆H°/R] [(1/T1) - (1/T2)] It looks very similar to the Arrhenius equation and so a plot of ln K versus 1/T should give a straight line with a slope of [-∆H°/R] 117 118 Problem Plot of ln Kp versus 1/T for the reaction. 2 SO2 (g) + O2 (g) '2 SO3 (g) slope = -∆H° / R, so for this reaction The following equilibrium constant data have been determined for the reaction H2 (g) + I2 (g) ' 2 HI (g) Kp = 50.0 @ 448 °C Kp = 66.9 @ 350 °C Estimate ∆H° for the reaction. Answer: ∆H° = -11.1 kJ⋅mol-1. ∆H° = -180 kJ⋅mol-1 119 120 30 Coupled reactions Coupled reactions This should make sense because if we have two equilibria in one container, one with a small K (like Ksp) and one with a large K (like Kf for complex formation), then the coupled reaction that is the sum of the two reactions has a K value that is larger than Ksp! We have made the non-spontaneous reaction occur! If we have a non-spontaneous (∆G > 0) reaction with a product that appears as a reactant in a different reaction that is spontaneous (∆G < 0) then we can couple the two reactions (do them in the same container at the same time) to drive the non-spontaneous reaction! 121 122 31
© Copyright 2026 Paperzz