First Law of Thermodynamics Enthalpy -  H, HfHf Second Law Third Law Entropy  S, Free Energy GG Spontaneity n Chap 18. Thermodynamics and Equilibrium.

Slides:



Advertisements
Similar presentations
Entropy and Free Energy Chapter 19. Laws of Thermodynamics First Law – Energy is conserved in chemical processes neither created nor destroyed converted.
Advertisements

Thermodynamics:Entropy, Free Energy, and Equilibrium
Chapter 17 Spontaneity, Entropy, and Free Energy The goal of this chapter is to answer a basic question: will a given reaction occur “by itself” at a particular.
AP CHEMISTRY CHAPTER 6 NOTES THERMOCHEMISTRY
Entropy, Free Energy, and Equilibrium
1 Entropy, Free Energy, and Equilibrium Chapter 18 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
THERMODYNAMICS. IMPORTANT DEFINITIONS System: the object or collection of objects being studied. Surroundings: everything outside the system that can.
CHEMISTRY 161 Chapter 6. Energy an Chemical Change 1.Forms of Energy 2.SI Unit of Energy 3.Energy in Atoms and Molecules 4.Thermodynamics 5.Calculation.
Thermodynamics B. Thermodynamics –Deals with the interconversion of heat an other forms of energy First Law: Energy can be converted from one form to.
System. surroundings. universe.
Chapter 16 Spontaneity, Entropy and Free energy. Contents l Spontaneous Process and Entropy l Entropy and the second law of thermodynamics l The effect.
Chemical Thermodynamics: Entropy, Free Energy and Equilibrium Chapter
Entropy and the 2nd Law of Thermodynamics
Heat Capacity Amount of energy required to raise the temperature of a substance by 1C (extensive property) For 1 mol of substance: molar heat capacity.
Chemical Thermodynamics. Spontaneous Processes First Law of Thermodynamics Energy is Conserved – ΔE = q + w Need value other than ΔE to determine if a.
Energy Changes in Chemical Reactions -- Chapter First Law of Thermodynamics (Conservation of energy)  E = q + w where, q = heat absorbed by system.
Daniel L. Reger Scott R. Goode David W. Ball Chapter 17 Chemical Thermodynamics.
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
Ch. 19: Chemical Thermodynamics (Thermochemistry II) Chemical thermodynamics is concerned with energy relationships in chemical reactions. - We consider.
Chapter 20: Thermodynamics
In general, the more atoms in its molecules, the greater is the entropy of a substance Entropy is a function of temperature.
Instructor: Dr. Upali Siriwardane Office: CTH 311 Phone Office Hours: M,W, 8:00-9:00 & 11:00-12:00 a.m.; Tu,Th,F.
Thermodynamics Chapter 19. First Law of Thermodynamics You will recall from Chapter 5 that energy cannot be created or destroyed. Therefore, the total.
A.P. Chemistry Spontaneity, Entropy, and Free Energy.
http:\\asadipour.kmu.ac.ir...46 slides. Thermodynamics http:\\asadipour.kmu.ac.ir...46 slides.
18-1 CHEM 102, Fall LA TECH Instructor: Dr. Upali Siriwardane Office: CTH 311 Phone Office Hours: M,W 8:00-9:00.
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.
Ch. 16: Spontaneity, Entropy, and Free Energy 16.1 Spontaneous Processes and Entropy.
Entropy, Free Energy, and Equilibrium Chapter 18 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Entropy, Free Energy, and Equilibrium Chapter 19 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
18-1 CHEM 102, Spring 2012 LA TECH CTH :00-11:15 am Instructor: Dr. Upali Siriwardane Office: CTH 311 Phone Office.
Chapter 19 Chemical Thermodynamics Lecture Presentation John D. Bookstaver St. Charles Community College Cottleville, MO © 2012 Pearson Education, Inc.
Chemical Thermodynamics Chapter 17 Chemical Thermodynamics.
Chapter 17 Spontaneity, entropy and free energy. Spontaneous l A reaction that will occur without outside intervention. l We need both thermodynamics.
http:\\asadipour.kmu.ac.ir...43 slides. Thermodynamics http:\\asadipour.kmu.ac.ir...43 slides.
Spontaneity, Entropy and Free Energy. Spontaneous Processes and Entropy  First Law “Energy can neither be created nor destroyed" The energy of the universe.
Chapter 17. Thermodynamics: Spontaniety, Entropy and Free Energy
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.
Chapter 19 Spontaneity, entropy and free energy (rev. 11/09/08)
18-1 CHEM 102, Spring 2012 LA TECH CTH :00-11:15 am Instructor: Dr. Upali Siriwardane Office: CTH 311 Phone Office.
Chemistry 100 Chapter 19 Spontaneity of Chemical and Physical Processes: Thermodynamics.
Chapter 15 Energy and Chemical Change Energy Energy can change for and flow, but it is always conserved.
Thermodynamics. study of energy changes that accompany physical and chemical processes. Thermochemistry is one component of thermodynamics which focuses.
A science that includes the study of energy transformations and the relationships among the physical properties of substances which are affected by.
Energy The ability to do work or produce heat The ability to do work or produce heat Potential- Stored energy Potential- Stored energy Energy stored in.
Thermodynamics Chapter 15. Part I Measuring Energy Changes.
Unit 11 Thermodynamics Chapter 16. Thermodynamics Definition Definition A study of heat transfer that accompanies chemical changes A study of heat transfer.
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.
J Villamil, Franklin Magnet HS1 Spontaneous Processes and Entropy Thermodynamics lets us predict whether a process will occur but gives no information.
17-1 CHEM 102, Fall 2015 LA TECH Instructor: Dr. Upali Siriwardane Office: CTH 311 Phone Office Hours: M.W &F, 8:00-9:00.
Free energy and Thermodynamics suroviec Spring 2014
The study of energy and the changes it undergoes.
A science that includes the study of energy transformations and the relationships among the physical properties of substances which are affected by.
Entropy (S) is a measure of the randomness or disorder of a system. orderS disorder S  S = S f - S i If the change from initial to final results in an.
Entropy, Free Energy, and Equilibrium Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
1 Entropy, Free Energy, and Equilibrium Chapter 18 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chemical Thermodynamics First Law of Thermodynamics You will recall from earlier this year that energy cannot be created nor destroyed. Therefore, the.
Energy Changes in Chemical Reactions -- Chapter First Law of Thermodynamics (Conservation of energy)  E = q + w where, q = heat absorbed by system.
Thermochemistry Energy and Chemical Change. Energy Energy can change for and flow, but it is always conserved.
A science that includes the study of energy transformations and the relationships among the physical properties of substances which are affected by.
Chapter 15 Energy and Chemical Change Section 15.1 Energy Section 15.2Heat Section 15.3Thermochemical Equations Section 15.4 Calculating Enthalpy Change.
17-1 CHEM 102, Fall 2014 LA TECH Instructor: Dr. Upali Siriwardane Office: CTH 311 Phone Office Hours: M,W 8:00-9:00.
http:\\academicstaff.kmu.ac.ir\alia sadipour...43 slides.
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.
Presentation transcript:

First Law of Thermodynamics Enthalpy -  H, HfHf Second Law Third Law Entropy  S, Free Energy GG Spontaneity n Chap 18. Thermodynamics and Equilibrium

Thermochemistry n Heat changes during chemical reactions Thermochemical equation. eg. H 2 (g) + O 2 (g) ---> 2H 2 O(l)  H =- 256 kJ;  is called the enthalpy of reaction. if  H is + reaction is called endothermic if  H is - reaction is called exothermic

Why is it necessary to divide Universe into System and Surrounding n Universe = System + Surrounding

Why is it necessary to divide Universe into System and Surrounding Universe = System + Surrounding

What is the internal energy change (  U) (  U) of a system?  U is associated with changes in atoms, molecules and subatomic particles E total = E ke + E pe +  U  U = heat (q) + w (work)  U = q + w  U = q -P  V; w =- P  V

What forms of energy are found in the Universe? n mechanical n thermal n electrical n nuclear n mass: E = mc 2 n others yet to discover

What is 1 st Law of Thermodynamics n Eenergy is conserved in the universe n All forms of energy are inter-convertible and conserved n Energy is neither created nor destroyed.

What exactly is  H? n Heat measured at constant pressure q p n Chemical reactions exposed to atmosphere and are held at a constant pressure. Volume of materials or gases produced can change. ie: work = -P  V  U = q p + w;  U = q p -P  V q p =  U + P  V;w = -P  V  H =  U + P  V;q p =  H(enthalpy )

How do you measure  U? Heat measured at constant volume q v Chemical reactions take place inside a bomb. Volume of materials or gases produced can not change. ie: work = -P  V= 0  U = q v + w q v =  U + o;w = 0  U = q v =  U(internal energy )

What is Hess's Law of Summation of Heat? n To heat of reaction for new reactions. n Two methods? 1st method: new  H is calculated by adding  Hs of other reactions. 2nd method: Where  H f (  H of formation) of reactants and products are used to calculate  H of a reaction.

Method 1: Calculate  H for the reaction: SO 2 (g) + 1/2 O 2 (g) + H 2 O(g) -----> H 2 SO 4 (l)  H = ? Other reactions: SO 2 (g) > S(s) + O 2 (g)  H = 297kJ H 2 SO 4 (l)------> H 2 (g) + S(s) + 2O 2 (g)  H = 814 kJ H 2 (g) +1/2O 2 (g) -----> H 2 O(g)  H = -242 kJ

SO 2 (g) > S(s) + O 2 (g);  H 1 = 297 kJ - 1 H 2 (g) + S(s) + 2O 2 (g) > H 2 SO 4 (l)  H 2 = -814 kJ - 2 H 2 O(g) ----->H 2 (g) + 1/2 O 2 (g)  H 3 = +242 kJ - 3 ______________________________________ SO 2 (g) + 1/2 O 2 (g) + H 2 O(g) -----> H 2 SO 4 (l) ª H =  H 1 +  H 2 +  H 3 ª H = ª H = -275 kJ

Calculate Heat (enthalpy) of Combustion: 2 nd method C 7 H 16 (l) + 11 O 2 (g) -----> 7 CO 2 (g) + 8 H 2 O(g) ;  H = ?  H f (C 7 H 16 ) = kJ/mol  H f (CO 2 ) = kJ/mol  H f (H 2 O) = kJ/mol  H f O 2 (g) = 0 (zero) n What method? n 2 nd method

ª H = [ 3 n ( ª H o f ) Products] - [ 3 n ( ª H o f ) reactants] ª H = [ 7( (-285.9)] - [ (0)] n = [ ] - [-198.8] n = n = kJ = 4843 kJ

Why is ª H o f of elements is zero? ª H o f, Heat formations are for compounds Note: ª H o f of elements is zero

What is 2 nd Law of Thermodynamics Entropy (  S) of the Universe increases during spontaneous process. n What is entropy Entropy (  S) : A measure of randomness or disorder of a system. n Spontaneous Process: A process that occurs without outside intervention.

Definitions n The Universe: The sum of all parts under consideration. n System: Part of the Universe we are interested in and a change is taking place. n Surrounding: Part of the Universe we are not interested in or can not observe.

Entropy  S  S univ = entropy of the Universe  S sys = entropy of the System  S surr = entropy of the Surrounding  S univ =  S sys +  S surr

 S univ  S sys  S surr n (  S sys >  S surr) (  S surr >  S sys)

Entropy Change Entropy (  S) normally increase (+) for the following changes: n i) Solid ---> liquid (melting) n ii) Liquid ---> gas n iii) Solid ----> gas n iv) Increase in temperature n v) Increasing in pressure n vi) Increase in volume ( at constant temperature and pressure)

What is  G ? n Free Energy  G = - T  S uni.  G =  H - T  S.

How do you get:  G =  H - T  S.  s univ =  s sys +  s surr  s surr = -  H sys /T)  S univ =  S sys -  H sys /T  S univ x T = T  S sys -  H sys : x T -  S univ x T = -T  S sys +  H sys : x -1 -  S univ x T =  H sys -T  S sys -  S univ x T =  G;  G =  H sys -T  S sys or  G =  H - T  S.

What  G means If  G is - for a change it will take place n spontaneously If  G is + for a change it will not take place If  G is 0 for a change it will be in equilibrium

Qualitative prediction of  S of Chemical Reactions n Look for (l) or (s) --> (g) n If all are gases: calculate  n = 3 n(gaseous prod.) - 3 n(gaseous reac.) n N 2 (g) + 3 H 2 (g) > 2 NH 3 (g)  n = = -2 If  n is -  S is negative (decrease in S) If  n is +  S is positive (increase in S)

Predict  S! n 2 C 2 H 6 (g) + 7 O 2 (g)--> 4 CO 2 (g) + 6H 2 0(g). n 2 CO(g) + O 2 (g)-->2 CO 2 (g). n HCl(g) + NH 3 (g)-->NH 4 Cl(s). n H 2 (g) + Br 2 (l) --> 2 HBr(g).

Calculating  S of reactions n Based on Hess’s Law second method:  S o = 3  S o (prod.) - 3  S o (react.)

How do you calculate  G There are two ways to calculate  G n for chemical reactions. i)  G =  H - T  S. ii)  G o = 3  G o f (products) - 3  G o f (reactants)

How do you calculate  G at different T and P  G =  G o + RT ln Q n Q = reaction quotient at equilibrium  G =   =  G o + RT ln K  G o = - RT ln K If you know  G o you could calculate K