Chapter 17 Free Energy and Thermodynamics Lesson 1.

Slides:



Advertisements
Similar presentations
Spontaneity, Entropy, and Free Energy
Advertisements

Chapter 17 Free Energy and Thermodynamics
Spontaneous Processes
Entropy, Free Energy, and Equilibrium
Entropy and Free Energy How to predict if a reaction can occur, given enough time? THERMODYNAMICS How to predict if a reaction can occur at a reasonable.
Chapter 16 Thermodynamics: Entropy, Free Energy, and Equilibrium
The entropy, S, of a system quantifies the degree of disorder or randomness in the system; larger the number of arrangements available to the system, larger.
Thermodynamics Chapter 19 Liquid benzene Production of quicklime Solid benzene ⇅ CaCO 3 (s) ⇌ CaO + CO 2.
Thermodynamics: Spontaneity, Entropy and Free Energy.
Chapter 18 Entropy, Free Energy and Equilibrium
Chemical Thermodynamics: Entropy, Free Energy and Equilibrium Chapter
Copyright McGraw-Hill 2009 Chapter 18 Entropy, Free Energy and Equilibrium.
Entropy and the 2nd Law of Thermodynamics
Chemical Thermodynamics Chapter 19 (except 19.7!).
Chemical Thermodynamics BLB 12 th Chapter 19. Chemical Reactions 1. Will the reaction occur, i.e. is it spontaneous? Ch. 5, How fast will the reaction.
CHEM 163 Chapter 20 Spring minute exercise Is each of the following a spontaneous change? Water evaporates from a puddle A small amount of sugar.
Chemical Thermodynamics. Spontaneous Processes First Law of Thermodynamics Energy is Conserved – ΔE = q + w Need value other than ΔE to determine if a.
Chapter 20 Thermodynamics: Entropy, Free Energy and the Direction of Chemical Reactions.
Thermodynamics: Entropy, Free Energy Direction of Chemical Reactions Chapter 20 Entropy and Free Energy - Spontaneity of Reaction 1. The Second Law of.
Spontaneity, Entropy, & Free Energy Chapter 16. 1st Law of Thermodynamics The first law of thermodynamics is a statement of the law of conservation of.
Chemical Thermodynamics
Chapter 19 – Principles of Reactivity: Entropy and Free Energy Objectives: 1)Describe terms: entropy and spontaneity. 2)Predict whether a process will.
First Law of Thermodynamics-The total amount of energy in the universe is constant. Second Law of Thermodynamics- All real processes occur spontaneously.
Chapter 20: Thermodynamics
A.P. Chemistry Spontaneity, Entropy, and Free Energy.
Chapter 6. = the capacity to do work or to produce heat Kinetic energy = the energy due to motion depends on mass & velocity Potential Energy = energy.
11 Entropy and Free Energy How to predict if a reaction can occur, given enough time? THERMODYNAMICS How to predict if a reaction can occur at a reasonable.
1 Entropy & Gibbs Free Energy Chapter The heat tax No matter what the process, heat always lost to surroundings No matter what the process, heat.
Chapter 17 Lecture © 2014 Pearson Education, Inc. Sherril Soman Grand Valley State University Lecture Presentation Chapter 17 Free Energy and Thermodynamics.
Chapter 17 Free Energy and Thermodynamics. Goals Entropy (S,  S) and spontaneity Free energy;  G,  G o  G, K, product- or reactant-favored Review:
First Law of Thermodynamics – Basically the law of conservation of energy energy can be neither created nor destroyed i.e., the energy of the universe.
Spontaneity, Entropy and Free Energy. Spontaneous Processes and Entropy  First Law “Energy can neither be created nor destroyed" The energy of the universe.
AP Chapter 19.  Energy can not be created nor destroyed, only transferred between a system and the surroundings.  The energy in the universe is constant.
11 © 2006 Brooks/Cole - Thomson Chemistry and Chemical Reactivity 6th Edition John C. Kotz Paul M. Treichel Gabriela C. Weaver CHAPTER 19 Principles of.
Thermodynamics. study of energy changes that accompany physical and chemical processes. Thermochemistry is one component of thermodynamics which focuses.
Thermodynamics The universe is in a state of constant change, the only invariant is Energy.
A science that includes the study of energy transformations and the relationships among the physical properties of substances which are affected by.
Entropy and Free Energy (Kotz Ch 20) - Lecture #2
Entropy, Free Energy, and Equilibrium
Spontaneity, Entropy, & Free Energy Chapter 16. 1st Law of Thermodynamics The first law of thermodynamics is a statement of the law of conservation of.
CHE 116 No. 1 Chapter Nineteen Copyright © Tyna L. Meeks All Rights Reserved.
Chapter 19 Lecture presentation
Spontaneous Processes and Entropy First Law “Energy can neither be created nor destroyed“. The energy of the universe is constant. Spontaneous Processes.
11 Entropy and Free Energy How to predict if a reaction can occur, given enough time? THERMODYNAMICS How to predict if a reaction can occur at a reasonable.
Chapter 17 Free Energy and Thermodynamics Chemistry II.
Free energy and Thermodynamics suroviec Spring 2014
Chemical Thermodynamics BLB 11 th Chapter 19. Chemical Reactions 1. How fast will the reaction occur? Ch How far toward completion will the reaction.
Thermodynamics: Spontaneity, Entropy and Free Energy.
A science that includes the study of energy transformations and the relationships among the physical properties of substances which are affected by.
Prentice Hall © 2003Chapter 19 Chapter 19 Chemical Thermodynamics CHEMISTRY The Central Science 9th Edition David P. White.
Entropy, Free Energy, and Equilibrium Chapter 18 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Entropy, Free Energy, and Equilibrium Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 17 Spontaneity, Entropy, and Free Energy.
20-1 Due: CH 20 Connect - Take out Notes/POGIL Today: Solving Problems for Thermodynamics HW: Test on Wednesday Potluck Thursday.
Chapter 19: Thermodynamics First Law of Thermodynamics: energy cannot be created or destroyed -total energy of the universe cannot change -you can transfer.
Chemical Thermodynamics First Law of Thermodynamics You will recall from earlier this year that energy cannot be created nor destroyed. Therefore, the.
THERMODYNAMICS – ENTROPY AND FREE ENERGY 3A-1 (of 14) Thermodynamics studies the energy of a system, how much work a system could produce, and how to predict.
Energy Changes in Chemical Reactions -- Chapter First Law of Thermodynamics (Conservation of energy)  E = q + w where, q = heat absorbed by system.
A science that includes the study of energy transformations and the relationships among the physical properties of substances which are affected by.
Thermodynamics The universe is in a state of constant change, the only invariant is Energy.
Chapter 17 Free Energy and Thermodynamics 2008, Prentice Hall Chemistry: A Molecular Approach, 1 st Ed. Nivaldo Tro Roy Kennedy Massachusetts Bay Community.
Chapter 19 Spontaneity, entropy and free energy (rev. 11/09/08)
Thermodynamics Chander Gupta and Matt Hagopian. Introduction into Thermo Thermodynamics is the study of energy and its transformations Thermochemistry.
Ch. 19: Spontaneity (“Thermodynamically Favored”), Entropy and Free Energy.
Thermodynamics: Spontaneity, Entropy and Free Energy
Chapter 17: Free Energy & Thermodynamics
Chapter 17 Free Energy and Thermodynamics
Chapter 17 Free Energy and Thermodynamics
Thermodynamics: Spontaneity, Entropy and Free Energy
Presentation transcript:

Chapter 17 Free Energy and Thermodynamics Lesson 1

2 First Law of Thermodynamics First Law of Thermodynamics: Energy cannot be created or destroyed the total energy of the universe cannot change it can be transfered from one place to another   E universe = 0 =  E system +  surroundings system = reactants & products surroundings = everything else (the transfer of energy from one to the other does not change the energy of the universe)

3 First Law of Thermodynamics For an exothermic reaction, heat from the system goes into the surroundings two ways energy can be “lost” from a system, converted to heat, q used to do work, w Energy conservation requires that the energy change in the system = heat exchanged + work done on the system.  E = q + w (  E = internal energy change)  E =  H – P  V (at const. P, q p =  H, enthalpy change)

4 Enthalpy, H related to (includes) the internal energy  H generally kJ/mol stronger bonds = more stable molecules if products more stable than reactants, energy released; exothermic  H = negative if reactants more stable than products, energy absorbed; endothermic  H = positive The enthalpy is favorable for exothermic reactions and unfavorable for endothermic reactions. Hess’ Law:  H° rxn =  (  H f ° prod ) -  (  H f ° react )

5 Thermodynamics and Spontaneity thermodynamics predicts whether a process will proceed (occur) under the given conditions spontaneous process  nonspontaneous process does not occur under specific conditions. spontaneity is determined by comparing the free energy (G) 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 (rate); this is kinetics

6 Spontaneous Nonspontaneous ice 25 o C water 25 o C 2Na(s) + 2H 2 O(l)  H 2 (g) + 2NaOH(aq)  H 2 (g) + 2NaOH(aq) 2Na(s) + 2H 2 O(l) ball rolls downhill ball rolls uphill water -10 o C ice -10 o C

Copyright McGraw- Hill 2009 Entropy Changes in a System Qualitative S solid < S liquid

Copyright McGraw- Hill 2009 Entropy Changes in a System Qualitative S liquid < S vapor

Copyright McGraw- Hill 2009 Entropy Changes in a System Qualitative S pure < S aqueous

Copyright McGraw- Hill 2009 Entropy Changes in a System Qualitative S lower temp < S higher temp

11 Diamond → Graphite Graphite is thermodynamically more stable than diamond, so the conversion of diamond into graphite is spontaneous – but it’s kinetically too slow (inert) it will never happen in many, many generations. kinetics Spontaneity: direction & extent kinetics: how fast

12 Factors Affecting Whether a Reaction Is Spontaneous The two factors that determine the thermodynamic favorability are the enthalpy and the entropy. The enthalpy is a comparison of the bond energy of the reactants to the products. bond energy = amount needed to break a bond.  H The entropy factors relate to the randomness/orderliness of a system  S The enthalpy factor is generally more important than the entropy factor

14 Entropy, S Entropy is a thermodynamic function that increases as the number of energetically equivalent ways of arranging the components increases.  S generally in J/K (joules/K) S = k lnW k = Boltzmann Constant (R/N A ) = 1.38  J/K W is the number of energetically equivalent ways, (microstates). It is unitless. Entropy is usually described as a measure of the randomness or disorder; the greater the disorder of a system, the greater its S. The greater the order  the smaller its S.

15 Entropy & Microstates, W Energetically Equivalent States for the Expansion of a Gas (4 gas molecules) 1 microstate 6 microstates (most probable distribution) S = k ln W  S = k ln W f - k ln W i if W f > W i,  S > 0 & entropy increases.

16 Changes in Entropy,  S entropy change is favorable when the result is a more random system (State C: higher entropy ).  S is positive (  S > 0) Some changes that increase the entropy are: rxns where products are in a more disordered state. (solid > liquid > gas) less order (solid< liquid < gas)  larger S (disorder) reactions which have larger numbers of product molecules than reactant molecules. increase in temperature (more movement) solids dissociating into ions upon dissolving

Copyright McGraw- Hill 2009 Entropy Changes in a System Qualitative S fewer moles < S more moles

18 Changes in Entropy in a System (melting) Particles fixed in space Particles can occupy many positions

19 Changes in Entropy in a System (vaporization) Particles occupy more space (larger volume)

20 Changes in Entropy in a System (solution process) Structure of solute and solvent disrupted (also more solute particles)

Strategy To determine the entropy change in each case, we examine whether the number of microstates of the system increases or decreases. The sign of ΔS will be positive if there is an increase in the number of microstates and negative if the number of microstates decreases. Solution (a)Upon freezing, the ethanol molecules are held rigid in position. This phase transition reduces the number of microstates and therefore the entropy decreases; that is, ΔS < 0.

(b) Evaporating bromine increases the number of microstates because the Br 2 molecules can occupy many more positions in nearly empty space. Therefore, ΔS > 0. (c) Glucose is a nonelectrolyte. The solution process leads to a greater dispersal of matter due to the mixing of glucose and water molecules so we expect ΔS > 0. (d) The cooling process decreases various molecular motions. This leads to a decrease in microstates and so ΔS < 0.

23 The 2nd Law of Thermodynamics The entropy of the universe increases in a spontaneous process.  S universe =  S system +  S surroundings > 0  S universe =  S system +  S surroundings = 0 (equilibrium) If  S system >> 0,  S surroundings 0! If  S system > 0 for  S universe > 0! the increase in  S surroundings often comes from the heat released in an exothermic reaction,  system < 0.

24 Entropy Changes in the Surroundings (  S surr ) Exothermic Process  S surr > 0 Endothermic Process  S surr < 0

25 The 3 rd Law of Thermodynamics S = k ln W S = k ln W = k ln 1 = 0  S = S f – S i ; where S i = 0 K the absolute entropy of a substance is always (+) positive at the new T - allows determination of entropy of substances. (W = 1, there is only one way to arrange the particles to form a perfect crystal) the 3rd Law states that for a perfect crystal at absolute zero, the absolute entropy = 0 J/mol∙K

26 Third Law of Thermodynamics The entropy of a perfect crystalline substance is zero at the absolute zero of temperature. S = k ln W W = 1 S = 0

27 Standard Entropies S° entropies for 1 mole at 298 K for a particular state, a particular allotrope, particular molecular complexity, a particular molar mass, and a particular degree of dissolution Values can be used to calculate the standard entropy change for a reaction,  S o rxn (=  S o sys )

29 Trends: Standard Entropies Molar Mass For monatomic species, the larger the molar mass, the larger the entropy available energy states more closely spaced, allowing more dispersal of energy through the states

30 Trends: Standard Entropies States the standard entropy of a substance in the gas phase is greater than the standard entropy of the same substance in the solid or liquid phase at a particular temperature Substance S°, (J/mol∙K) H 2 O (l)70.0 H 2 O (g)188.8

31 Trends: Standard Entropies Allotropes the more highly ordered form has the smaller entropy -different forms of an element

32 Trends: Standard Entropies Molecular Complexity (inc # of atoms) larger, more complex molecules generally have larger entropy more available energy states, allowing more dispersal of energy through the states Substance Molar Mass S°, (J/mol∙K) Ar (g) NO (g)

33 Trends: Standard Entropies Dissolution dissolved solids generally have larger entropy distributing particles throughout the mixture Substance S°, (J/mol∙K) KClO 3 (s)143.1 KClO 3 (aq)265.7

34 Q. Arrange the following in order of increasing 25 o C! (lowest to highest) Ne(g), SO 2 (g), Na(s), NaCl(s) and H 2 (g) Na(s) < NaCl(s) < H 2 (g) < Ne(g) < SO 2 (g)

Calculate  S  for the reaction 4 NH 3(g) + 5 O 2(g)  4 NO (g) + 6 H 2 O (g)  S is +, as you would expect for a reaction with more gas product molecules than reactant molecules standard entropies from Appendix IIB  S, J/K Check: Solution: Concept Plan: Relationships: Given: Find: SS S  NH3, S  O2, S  NO, S  H2O, Substance S , J/mol  K NH 3 (g)192.8 O2(g)O2(g)205.2 NO(g)210.8 H 2 O(g)188.8

Consider 2 H 2 (g) + O 2 (g)  2 H 2 25 o C ∆S o = 2 S o (H 2 O) - [2 S o (H 2 ) + S o (O 2 )] ∆S o = 2 mol (69.9 J/Kmol) - [2 mol (130.6 J/Kmol) + 1 mol (205.0 J/Kmol)] ∆S o = J/K Note that there is a decrease in S because 3 mol of gas give 2 mol of liquid. Calculating ∆S o for a Reaction ∆S o =  S o (products) -  S o (reactants)

The more negative  H syst and the lower the temperature the higher (more positive)  S surr 37 Temperature Dependence of  S surroundings  system 0 )  system > 0 (endothermic), it takes heat from the surroundings, decreasing the entropy of the surroundings (  S surroundings < 0 )

The reaction C 3 H 8(g) + 5 O 2(g)  3 CO 2(g) + 4 H 2 O (g) has  H rxn = kJ at 25°C. Calculate the entropy change of the surroundings. combustion is largely exothermic, so the entropy of the surroundings should increase (inc in # gas mol)  H system = kJ, T = 298 K  S surroundings, J/K Check: Solution: Concept Plan: Relationships: Given: Find: SS T,  H

2 H 2 (g) + O 2 (g)  2 H 2 25 o C ∆S o system = J/K Calculating ∆S o for the surroundings ∆S o surroundings = J/K Can calculate ∆H o system = ∆H o rxn = kJ (2 mol H 2 0 (l) - 0) (2 mol H 2 0 (l) - 0)

2 H 2 (g) + O 2 (g)  2 H 2 25 o C ∆S o system = J/K ∆S o surroundings = J/K ∆S o universe = J/K The entropy of the universe is increasing, so the reaction is spontaneous ( product- favored).  S universe =  S system +  S surroundings Given S o surr, S o sys and T, determine S o univ and predict if the reaction will be spontaneous. Given  S o surr,  S o sys and T, determine  S o univ and predict if the reaction will be spontaneous.

Spontaneous or Not? originally: originally:  S universe =  S system +  S surroundingsbut but  S universe =  S system –  system /T  system  S system Spontaneous? Exothermic  H sys < 0 Less order  S sys > 0 Spontaneous under all conditions;  S univ > 0 Exothermic  H sys < 0 More order  S sys < 0 Favorable at low T Endothermic  H sys > 0 Less order  S sys > 0 Favorable at high T Endothermic  H sys > 0 More order  S sys < 0 Not spontaneous under any conditions  S univ < 0

42 Without doing any calculations, determine the sign of S sys and S surr for each reaction. Predict under what temperatures (all T, low T, or high T) the reaction will be spontaneous. 2CO(g) + O 2 (g)  2CO 2 (g)  rxn = kJ 2NO 2 (g)  O 2 (g) + 2NO(g)  rxn = kJ -/T)  S universe =  S system + ( -  sys /T)  S system = ( -); 3 mol gas form 2 mol gas  S surr = (+); low T  S system = (+); 2 mol gas form 3 mol gas  S surr = ( -) ; high T -/T)  S surr = ( -  sys /T)

43 Without doing any calculations, determine the sign of  S sys and  S surr for each reaction. Predict under what temperatures (all T, low T, or high T) the reaction will be spontaneous. 2H 2 (g) + O 2 (g)  2H 2 O(g)  rxn = kJ CO 2 (g)  C(s) + O 2 (g)  rxn = kJ -/T)  S universe =  S system + ( -  sys /T)  S system = ( -) ; 3 mol gas form 2 mol gas  S surr = (+) ; low T  S system = ( -) ; complicated gas forms a solid & gas  S surr = ( -) ; all T -/T)  S surr = ( -  sys /T)

44 At what temperature is the change in entropy for the reaction equal to the change in entropy for the surroundings, if  H o rxn = -127 kJ and  S o rxn = 314 J/K. Plan: set  S o rxn =  S o surr and solve for T; convert kJ to J rxn implies system!!! Ans: T = +404 K