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Chemistry, Julia Burdge, 2st Ed McGraw Hill Chapter 17 Free Energy and Thermodynamics Mr Truong Minh Chien ; losedtales@yahoo.com http://tailieu.vn/losedtales http://mba-programming.blogspot.com 2011, NKMB Co., Ltd Don’t get ahead of the game • There is a lot of theory in this chapter • Keep terms separate (5), and equations Universe, System, Surrounds, Enthalpy, and Entropy are all different, and you must know each • Memorize the Laws of Thermodynamics • You can break a California State Law but you can NOT break a Thermodynamic Law Chemistry, Julia Burdge, 2nd e., McGraw Hill First Law of Thermodynamics • you can’t win! • First Law of Thermodynamics: Energy cannot be Created or Destroyed the total energy of the universe cannot change though you can transfer it from one place to another • ∆Euniverse = = ∆Esystem + ∆Εsurroundings • Think of a match burning, crumbling paper, etc Chemistry, Julia Burdge, 2nd e., McGraw Hill First Law of Thermodynamics • Conservation of Energy • For an exothermic reaction, “lost” heat from the system • • • goes into the surroundings two ways energy “lost” from a system, converted to heat, q used to work, w Energy conservation requires that the energy change in the system equal the heat released + work done ∆E = q + w ∆E = ∆H + P∆V ∆E is a state function internal energy change independent of how done Chemistry, Julia Burdge, 2nd e., McGraw Hill Energy Tax • you can’t break even! • to recharge a battery with 100 kJ of • useful energy will require more than 100 kJ every energy transition results in a “loss” of energy conversion of energy to heat which is “lost” by heating up the surroundings ∆E = q + w ∆E = ∆H + P∆V Tro, Chemistry: A Molecular Approach Heat Tax fewer steps generally results in a lower total heat tax Tro, Chemistry: A Molecular Approach Thermodynamics and Spontaneity • thermodynamics predicts whether a process will proceed under the given conditions spontaneous process nonspontaneous processes require energy input to go • spontaneity is determined by comparing the free energy of the system before the reaction with the free energy of the system after reaction if the system after reaction has less free energy than before the reaction, the reaction is thermodynamically favorable • spontaneity ≠ fast or slow Tro, Chemistry: A Molecular Approach Comparing Potential Energy The direction of spontaneity can be determined by comparing the potential energy of the system at the start and the end Tro, Chemistry: A Molecular Approach Reversibility of Process • any spontaneous process is irreversible it will proceed in only one direction • a reversible process will proceed back and forth between the two end conditions equilibrium results in no change in free energy • if a process is spontaneous in one direction, it must be nonspontaneous in the opposite direction Tro, Chemistry: A Molecular Approach Thermodynamics vs Kinetics Tro, Chemistry: A Molecular Approach 10 Relative Standard Entropies Allotropes • the less constrained the structure of an allotrope is, the larger its entropy Tro, Chemistry: A Molecular Approach 41 Relative Standard Entropies Molecular Complexity • larger, more complex molecules generally have larger entropy • more available energy states, allowing more dispersal of energy through the states Tro, Chemistry: A Molecular Approach Molar S°, Substance Mass (J/mol∙K) Ar (g) 39.948 154.8 NO (g) 30.006 210.8 42 Relative Standard Entropies Dissolution • dissolved solids generally have larger entropy • distributing particles throughout the mixture Tro, Chemistry: A Molecular Approach Substance S°, (J/mol∙K) KClO3(s) 143.1 KClO3(aq) 265.7 43 Substance NH3(g) S°, J/mol⋅K 192.8 O2(g) 205.2 NO(g) 210.8 H2O(g) standard entropies from Appendix IIB 188.8 Ex 17.4 –Calculate ∆S° for the reaction NH3(g) + O2(g) → NO(g) + H2O(g) Given: Find: ∆S, J/K Concept Plan: Relationships: Solution: S°NH3, S°O2, S°NO, S°H2O, ( ( ) ( ∆S = Σn pSproducts − Σnr Sreactants ) ( ∆S = Σn pSproducts − ΣnrSreactants ) ) ∆S = [ 4(S NO( g ) ) + 6(SH O( g ) )] − [4(S NH ( g ) ) + 5(SO ( g ) )] J J J J = [ 4(210.8 K ) + 6(188.8 K )] − [4(192.8 K ) + 5(205.2 K )] J = 178.8 K Check: ∆S is +, as you would expect for a reaction with more gas product molecules than reactant molecules Calculating ∆G° • at 25°C: ∆Goreaction = ΣnGof(products) - ΣnGof(reactants) • at temperatures other than 25°C: assuming the change in ∆Horeaction and ∆Soreaction is negligible ∆G° reaction = ∆H° reaction – T∆S° reaction Tro, Chemistry: A Molecular Approach 45 ... determined by comparing the free energy of the system before the reaction with the free energy of the system after reaction if the system after reaction has less free energy than before the reaction,... Energy Tax • you can’t break even! • to recharge a battery with 100 kJ of • useful energy will require more than 100 kJ every energy transition results in a “loss” of energy conversion of energy. .. theory in this chapter • Keep terms separate (5), and equations Universe, System, Surrounds, Enthalpy, and Entropy are all different, and you must know each • Memorize the Laws of Thermodynamics