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MI- Based Module:
THERMODYNAMICS
Prepared by:
NOROLAYN K. SAID
Presented to:
DR. THELMA A. ANTONIO
CONTENTS
 Introduction
 Objectives
 Pre-Test
 First Law of Thermodynamics
 Some Thermodynamic Terms
 Enthalpy Changes
 Calorimetry
 Thermochemical Equation03/06/17 Presented to DR. THELMA A. ANTONIO 2
 Standard States and Standard Enthalpy Chan
 Standard Molar Enthalpy of Formation
 Hess’s Law
 Bond Energies
 Changes in Internal Energy
 Relationship of Enthalpy and Internal
Energy
03/06/17 Presented to DR. THELMA A. ANTONIO 3
 Spontaneity of Physical and Chemical
Changes
 Two Aspects of Spontaneity
 Second Law of Thermodynamics
 Entropy
 Free Energy Change and Spontaneity
 Temperature Dependence of Spontaneity
 Post-Test
 References
03/06/17 Presented to DR. THELMA A. ANTONIO 4
Hi students! Welcome to
the world of Thermodynamics!
In this module, you will be
learning important concepts on
heat changes and
thermochemistry and the
spontaneity of physical and
chemical changes.
5
INTRODUCTION
03/06/17 Presented to DR. THELMA A. ANTONIO
OBJECTIVES
After accomplishing the module, you are
expected to:
1.Distinguish between exothermic and
endothermic reactions;
2.Explain what is meant by enthalpy and
enthalpy change;
3.Define standard enthalpy change and explain
how it is used;
03/06/17 Presented to DR. THELMA A. ANTONIO 6
4. Describe how calorimeter determines
heats of reactions;
5. State Hess’s Law;
6. Apply Hess’s Law to determine ∆H for a
reaction;
7. Explain what is meant by spontaneous
process;
8. Relate enthalpy change to spontaneity;
03/06/17 Presented to DR. THELMA A. ANTONIO 7
9. Define entropy;
10. State the entropy criterion for a
spontaneous process;
11. State the criterion for reaction
spontaneity in terms of its free energy;
12. Compare the three Laws of
Thermodynamics;
03/06/17 Presented to DR. THELMA A. ANTONIO 8
13. Perform problem-solving on
thermodynamic problems; and
14. Perform activities using multiple
intelligences.
03/06/17 Presented to DR. THELMA A. ANTONIO 9
PRE-TEST
Oopps! Before you proceed,
check yourself first with the pre-
test for an evaluation. Don’t worry
this will not affect your grade.
This will only measure your pre-
knowledge on the concepts and
problems on Thermodynamics.
Good Luck!
03/06/17 Presented to DR. THELMA A. ANTONIO 10
Answer to the Pre-Test
03/06/17 Presented to DR. THELMA A. ANTONIO 11
RoundRobin
In three to four members in a
group, share to the team one
physical and one chemical change
that take place at home before you
went to school. And try to identify
them as releasing heat or absorbing
heat. Do this one-at-a-time with
your group-mates.
03/06/17 Presented to DR. THELMA A. ANTONIO 12
13
The First Law of
Thermodynamics
 Thermodynamics is the study of the changes in
energy and transfers of energy that accompany
chemical and physical processes.
 You will address 3 fundamental questions.
1. Will two (or more) substances react when they are
mixed under specified conditions?
2. If they do react, what energy changes and transfers
are associated with their reaction?
3. If a reaction occurs, to what extent does it occur?
03/06/17 Presented to DR. THELMA A. ANTONIO
14
 Exothermic reactions release energy in the form of heat.
 For example, the combustion of propane is exothermic.
 The combustion of n-butane is also exothermic.
kJ102.22O4HCO3O5HC 3
)(22(g)2(g)(g)83 ×++→+ 
kJ105.78OH10CO8O13HC2 3
)(22(g)2(g)10(g)4 ×++→+ 
03/06/17 Presented to DR. THELMA A. ANTONIO
15
 Exothermic
reactions generate
specific amounts
of heat.
 This is because the
potential energies
of the products are
lower than the
potential energies
of the reactants.
03/06/17 Presented to DR. THELMA A. ANTONIO
16
 There are two basic ideas of importance for
thermodynamic systems.
1. Chemical systems tend toward a state of minimum
potential energy.
 Some examples of this include:
 H2O flows downhill.
 Objects fall when dropped.
 The energy change for these two examples is:
 Epotential = mgh
 ∆Epotential = mg(∆h)03/06/17 Presented to DR. THELMA A. ANTONIO
17
2. Chemical systems tend toward a state of
maximum disorder.
 Common examples of this are:
 A mirror shatters when dropped and does not
reform.
 It is easy to scramble an egg and difficult to
unscramble it.
 Food dye when dropped into water disperses.
03/06/17 Presented to DR. THELMA A. ANTONIO
18
 This law can be stated as, “The combined
amount of energy in the universe is constant.”
 The first law is also known as the Law of
Conservation of Energy.
 Energy is neither created nor destroyed in
chemical reactions and physical changes.
03/06/17 Presented to DR. THELMA A. ANTONIO
19
Some Thermodynamic Terms
 The substances involved in the chemical and
physical changes under investigation are called the
system.
 In chemistry lab, the system is the chemicals inside the
beaker.
 The environment around the system is called the
surroundings.
 The surroundings are outside the beaker.
 The system plus the surroundings is called the
universe.
03/06/17 Presented to DR. THELMA A. ANTONIO
20
 The set of conditions that specify all of the
properties of the system is called the
thermodynamic state of a system.
 For example the thermodynamic state could include:
 The number of moles and identity of each substance.
 The physical states of each substance.
 The temperature of the system.
 The pressure of the system.
03/06/17 Presented to DR. THELMA A. ANTONIO
21
 The properties of a system that depend only on the state of
the system are called state functions.
 State functions are always written using capital letters.
 The value of a state function is independent of pathway.
 An analog to a state function is the energy required to climb a
mountain taking two different paths.
 E1 = energy at the bottom of the mountain
 E1 = mgh1
 E2 = energy at the top of the mountain
 E2 = mgh2
 ∆E = E2-E1 = mgh2 – mgh1 = mg(∆h)
03/06/17 Presented to DR. THELMA A. ANTONIO
22
 Notice that the energy change in moving from the
top to the bottom is independent of pathway but
the work required may not be!
 Some examples of state functions are:
 T, P, V, ∆E, ∆H, and S
 Examples of non-state functions are:
 n, q, w
03/06/17 Presented to DR. THELMA A. ANTONIO
23
 In thermodynamics we are often interested in
changes in functions.
 We will define the change of any function X as:
 ∆X = Xfinal – Xinitial
 If X increases ∆X > 0
 If X decreases ∆X < 0.
03/06/17 Presented to DR. THELMA A. ANTONIO
Team Chant
Create a Chem. Jingle by group using
familiar tunes and the following
thermodynamic terms in the lyrics such as
system
surroundings
universe
thermodynamic state of a system
state functions
03/06/17 Presented to DR. THELMA A. ANTONIO 24
25
Enthalpy Change
 Chemistry is commonly done in open beakers
on a desk top at atmospheric pressure.
 Because atmospheric pressure only changes by
small increments, this is almost at constant
pressure.
 The enthalpy change, ∆H, is the change in
heat content at constant pressure.
 ∆H = qp
03/06/17 Presented to DR. THELMA A. ANTONIO
26
Enthalpy Change
 ∆Hrxn is the heat of reaction.
 This quantity will tell us if the reaction produces
or consumes heat.
 If ∆Hrxn < 0 the reaction is exothermic.
 If ∆Hrxn > 0 the reaction is endothermic.
 ∆Hrxn = Hproducts - Hreactants
 ∆Hrxn = Hsubstances produced - Hsubstances consumed
 Notice that this is ∆Hrxn = Hfinal – Hinitial
03/06/17 Presented to DR. THELMA A. ANTONIO
Word Hunt
03/06/17 Presented to DR. THELMA A. ANTONIO 27
28
Calorimetry
 A coffee-cup
calorimeter is used to
measure the amount of
heat produced (or
absorbed) in a reaction
at constant P
 This is one method to
measure qP for reactions
in solution.
03/06/17 Presented to DR. THELMA A. ANTONIO
29
Calorimetry
 If an exothermic reaction is performed in a
calorimeter, the heat evolved by the reaction is
determined from the temperature rise of the solution.
 This requires a two part calculation.
 Amount of heat gained by calorimeter is called the heat
capacity of the calorimeter or calorimeter constant.
 The value of the calorimeter constant is determined by adding a
specific amount of heat to calorimeter and measuring the temperature
rise.






+





=





solutionbyabsorbed
heatofAmount
rcalorimetebyabsorbed
heatofAmount
reactionbyreleased
heatofAmount
03/06/17 Presented to DR. THELMA A. ANTONIO
30
Calorimetry
 Example 1: When 3.425 kJ of heat is added to
a calorimeter containing 50.00 g of water the
temperature rises from 24.00o
C to 36.54o
C.
Calculate the heat capacity of the calorimeter
in J/o
C. The specific heat of water is 4.184 J/g
o
C.
 This is a four part calculation.
03/06/17 Presented to DR. THELMA A. ANTONIO
31
Calorimetry
1. Find the temperature change.
2. Find the heat absorbed by the water in going from
24.000
C to 36.540
C.
( )∆T = 36.54- 24.00 C = 12.54 C00
( )( )( )
q mC T
= 50.00 g C
J 2623 J
P
J
g C0
=
= ≈
∆
4184 1254
262337
0
. .
.03/06/17 Presented to DR. THELMA A. ANTONIO
32
Calorimetry
3. Find the heat absorbed by the calorimeter.
 Take the total amount of heat added to calorimeter and
subtract the heat absorbed by the water.
4. Find the heat capacity of the calorimeter.
 (heat absorbed by the calorimeter)/(temperature change)
( )
3425. kJ = 3425 J
3425 J - 2623 J = 802 J
03/06/17 Presented to DR. THELMA A. ANTONIO
33
Calorimetry
 Example 2: A coffee-cup calorimeter is used
to determine the heat of reaction for the acid-
base neutralization
CH3COOH(aq) + NaOH(aq) → NaCH3COO(aq) + H2O()
When we add 25.00 mL of 0.500 M NaOH at
23.000o
C to 25.00 mL of 0.600 M CH3COOH
already in the calorimeter at the same
temperature, the resulting temperature is
observed to be 25.947o
C.03/06/17 Presented to DR. THELMA A. ANTONIO
34
Calorimetry
The heat capacity of the calorimeter has
previously been determined to be 27.8 J/0
C.
Assume that the specific heat of the mixture is the
same as that of water, 4.18 J/g0
C and that the
density of the mixture is 1.02 g/mL.
03/06/17 Presented to DR. THELMA A. ANTONIO
35
Calorimetry
 This is a three part calculation.
1. Calculate the amount of heat given off in the reaction.
( )
temperature change
T = 25.947 - 23.000 C = 2.947 C∆ 0 0
( )
( )( )
temperature change
T = 25.947 - 23.000 C = 2.947 C
heat absorbed by calorimeter
q = 2.947 C JJ
C0
∆ 0 0
0
278 819. .=
( )
( )( )
( )
temperature change
T = 25.947 - 23.000 C = 2.947 C
heat absorbed by calorimeter
q = 2.947 C J
mass of solution in calorimeter
25.00 mL + 25.00 mL
g
mL
g
J
C0
∆ 0 0
0
27 8 819
102
510
. .
.
.
=
=
03/06/17 Presented to DR. THELMA A. ANTONIO
36
Calorimetry
( )( )( )
heat absorbed by solution
q = mC T
q = 51.0 g 2.947 C J
total amount of heat produced by reaction
q = 81.9 J + 628 J = 709.9 J
J
g C
∆
418 6280
0
. =( )( )( )
heat absorbed by solution
q = mC T
q = 51.0 g 2.947 C JJ
g C
∆
418 6280
0
. =
03/06/17 Presented to DR. THELMA A. ANTONIO
37
Calorimetry
2. Determine ∆H for the reaction under the conditions of the
experiment.
 We must determine the number of moles of reactants consumed
which requires a limiting reactant calculation.
( ) ( ) ( ) ( )
( )
CH COOH + NaOH NaCH COO + H O
mL NaOH
mmol NaOH
1 mL NaOH
mmol NaCH COO
1 mmol NaOH
mmol NaCH COO
3 aq aq 3 aq 2
3
3
→





 ×





 =
l
2500
0500
1
12 5
.
.
.
( ) ( ) ( ) ( )
( )
( )
CH COOH + NaOH NaCH COO + H O
mL NaOH
mmol NaOH
1 mL NaOH
mmol NaCH COO
1 mmol NaOH
mmol NaCH COO
mL CH COOH
mmol CH COOH
1 mL CH COOH
mmol NaCH COO
1 mmol CH COOH
mmol NaCH COO
3 aq aq 3 aq 2
3
3
3
3
3
3
3
3
→





 ×





 =





 ×





 =
l
25 00
0 500
1
12 5
25 00
0 600
1
15 0
.
.
.
.
.
.03/06/17 Presented to DR. THELMA A. ANTONIO
38
Calorimetry
3. Finally, calculate the ∆Hrxn based on the limiting reactant
calculation.
125
7099
56792
.
.
mmol = 0.0125 mol
H
J
0.0125 mol
J / mol 56.8 kJ / molrxn∆ = = ≈
03/06/17 Presented to DR. THELMA A. ANTONIO
Hands-on Learning
(Laboratory)
03/06/17 Presented to DR. THELMA A. ANTONIO 39
40
Thermochemical Equations
 Thermochemical equations are a balanced chemical
reaction plus the ∆H value for the reaction.
 For example, this is a thermochemical equation.
 The stoichiometric coefficients in thermochemical
equations must be interpreted as numbers of moles.
 1 mol of C5H12 reacts with 8 mol of O2 to produce 5 mol
of CO2, 6 mol of H2O, and releasing 3523 kJ is
referred to as one mole of reactions.
moles6moles5moles8mole1
kJ3523OH6CO5O8HC )(22(g)2(g))12(5 ++→+ 
03/06/17 Presented to DR. THELMA A. ANTONIO
41
 This is an equivalent method of writing thermochemical
equations.
 ∆H < 0 designates an exothermic reaction.
 ∆H > 0 designates an endothermic reaction
kJ3523-HOH6CO5O8HC o
rxn)(22(g)2(g))12(5 =∆+→+ 
03/06/17 Presented to DR. THELMA A. ANTONIO
42
 Example 3: Write the thermochemical
equation for the reaction in Example 2.
You do it!
( ) ( ) ( ) ( )CH COOH + NaOH NaCH COO + H O H = -56.8 kJ / mol3 aq aq 3 aq 2→ l ∆
03/06/17 Presented to DR. THELMA A. ANTONIO
Timed Pair Share
Answer the following problem in 2
minutes. And share it with a partner.
“A sample of aluminum metal absorbs 9.86
J of heat, upon which the temperature of the
sample increases from 23.2 °C to 30.5 °C.
Since the specific heat capacity of aluminum
is 0.90 J/g-K, the mass of the sample is
__________ g.”
03/06/17 Presented to DR. THELMA A. ANTONIO 43
44
Standard States and Standard
Enthalpy Changes
 Thermochemical standard state conditions
 The thermochemical standard T = 298.15 K.
 The thermochemical standard P = 1.0000 atm.
 Be careful not to confuse these values with STP.
 Thermochemical standard states of matter
 For pure substances in their liquid or solid phase the standard
state is the pure liquid or solid.
 For gases the standard state is the gas at 1.00 atm of pressure.
 For gaseous mixtures the partial pressure must be 1.00 atm.
 For aqueous solutions the standard state is 1.00 M
concentration.03/06/17 Presented to DR. THELMA A. ANTONIO
45
Standard Molar Enthalpies of
Formation, ∆Hf
o
 The standard molar enthalpy of formation is defined as
the enthalpy for the reaction in which one mole of a
substance is formed from its constituent elements.
 The symbol for standard molar enthalpy of formation is ∆Hf
o
.
 The standard molar enthalpy of formation for MgCl2 is:
( ) ( ) ( )
( )
Mg Cl MgCl kJ
H kJ / mol
s 2 g 2 s
f MgCl
o
2 s
+ → +
= −
6418
6418
.
.∆
03/06/17 Presented to DR. THELMA A. ANTONIO
46
 Standard molar enthalpies of formation have been
determined for many substances.
 Standard molar enthalpies of elements in their most stable
forms at 298.15 K and 1.000 atm are zero.
 Example 4: The standard molar enthalpy of formation for phosphoric
acid is -1281 kJ/mol. Write the equation for the reaction for
which ∆Ho
rxn = -1281 kJ.
P in standard state is P4
Phosphoric acid in standard state is H3PO4(s)
You do it!
03/06/17 Presented to DR. THELMA A. ANTONIO
47
( ) ( ) ( ) ( )
( )
3
2
1
42 1281
1281
H O P H PO kJ
H kJ / mol
2 g 2 g 4 s 3 4 s
f H PO
o
3 4 s
+ + → +
= −∆
03/06/17 Presented to DR. THELMA A. ANTONIO
48
 Example 5: Calculate the enthalpy change for the
reaction of one mole of H2(g) with one mole of F2(g) to
form two moles of HF(g) at 25o
C and one atmosphere.
( ) ( ) ( )
( )( )
H F HF
std. state std. state std. state
for this rxn. H H
from Appendix K, H kJ / mol
H 2 mol kJ / mol kJ
2 g 2 g g
298
o
f
o
f
o
298
o
+ →
=
= −
= − = −
2
2
271
271 542
∆ ∆
∆
∆
03/06/17 Presented to DR. THELMA A. ANTONIO
49
 Example 6: Calculate the enthalpy change for
the reaction in which 15.0 g of aluminum
reacts with oxygen to form Al2O3 at 25o
C and
one atmosphere.
You do it!You do it!
03/06/17 Presented to DR. THELMA A. ANTONIO
50
( ) ( ) ( )4 Al + 3 O 2 Al O
from Appendix K, H kJ / mol
? kJ = 15.0 g Al
1 mol Al
27.0 g Al
mol Al O
4 mol Al
kJ
mol Al O
kJ
s 2 g 2 3 s
f Al O
o
2 3
2 3
2 3
→
= −
× × ×
−
= −
∆ 1676
2
1676
1
466
03/06/17 Presented to DR. THELMA A. ANTONIO
Blackboard Share
The class are grouped into five
teams with four to five members. One
representative from the team will pick
one problem randomly. You will
answer by team and one will share
(and discuss) the answer to the class
on the blackboard.
03/06/17 Presented to DR. THELMA A. ANTONIO 51
Problems:
03/06/17 Presented to DR. THELMA A. ANTONIO 52
The value of for the reaction below is -72 kJ. __________ kJ of heat are released when 1.0
mol of HBr is formed in this reaction.
The value of for the reaction below is -126 kJ. __________ kj are released when 2.00 mol
of NaOH is formed in the reaction?
03/06/17 Presented to DR. THELMA A. ANTONIO 53
The value of for the reaction below is -790 kJ. The enthalpy change accompanying the
reaction of 0.95 g of S is __________ kJ.
The value of for the reaction below is -6535 kJ. __________ kJ of heat are released in the
combustion of 16.0 g of ?
The value of for the reaction below is -336 kJ. Calculate the heat (kJ) released to the
surroundings when 23.0 g of HCl is formed.
54
Hess’s Law
 Hess’s Law of Heat Summation states that the enthalpy
change for a reaction is the same whether it occurs by
one step or by any (hypothetical) series of steps.
 Hess’s Law is true because ∆H is a state function.
 If we know the following ∆Ho
’s
[ ]
[ ]
[ ] kJ1648HOFe2O3Fe43
kJ454HFeO2OFe22
kJ560HOFe2OFeO41
o
3(s)22(g)(s)
o
(g)2(g)(s)
o
(s)322(g)(s)
−=∆→+
−=∆→+
−=∆→+
03/06/17 Presented to DR. THELMA A. ANTONIO
55
Hess’s Law
 For example, we can calculate the ∆Ho
for reaction [1] by properly adding
(or subtracting) the ∆Ho
’s for reactions [2] and [3].
 Notice that reaction [1] has FeO and O2 as reactants and Fe2O3 as a product.
 Arrange reactions [2] and [3] so that they also have FeO and O2 as reactants
and Fe2O3 as a product.
 Each reaction can be doubled, tripled, or multiplied by half, etc.
 The ∆Ho
values are also doubled, tripled, etc.
 If a reaction is reversed the sign of the ∆Ho
is changed.
( ) ( ) ( )
[ ] ( ) ( ) ( )
[ ] ( ) ( )
H
2(2 FeO Fe O kJ
3 4 Fe O Fe O kJ
4 FeO O Fe O kJ
0
s s 2 g
s 2 g 2 3 s
s 2 g 2 3
∆
2 2 2 2 544
3 2 1648
1 2 560
x [ ] ) ( )− → + +
+ → −
+ → −
03/06/17 Presented to DR. THELMA A. ANTONIO
56
Hess’s Law
 Example 7: Given the following equations
and ∆Ho
values
calculate ∆Ho
for the reaction below.
( )
( ) ( ) ( )
( ) ( ) ( )
( ) ( ) ( )
H kJ
2 N O N O 164.1
[2] N + O NO 180.5
[3] N + 2 O NO 66.4
o
2 g 2 g 2 g
2 g 2 g g
2 g 2 g 2 g
∆
[ ]1 2
2
2
+ →
→
→
( ) ( ) ( )
You do it!
?HNO3NO+ON o
gg2g2 =∆→
03/06/17 Presented to DR. THELMA A. ANTONIO
57
Hess’s Law
 Use a little algebra and Hess’s Law to get the
appropriate ∆Ho
values
[ ] ( ) ( ) ( )
[ ] ( ) ( ) ( )
H (kJ)
N O N + O -82.05
N + O 3 NO 270.75
o
2 g 2 g
1
2 2 g
3
2
3
2 2 g
3
2 2 g g
∆
1
2 1
2
× − →
× →
[ ] ( ) ( ) ( )
H (kJ)
N O N + O -82.05
o
2 g 2 g
1
2 2 g
∆
1
2 1× − →[ ] ( ) ( ) ( )
[ ] ( ) ( ) ( )
[ ] ( ) ( ) ( )
( ) ( ) ( )
H (kJ)
N O N + O -82.05
N + O 3 NO 270.75
NO N + O -33.2
N O NO 3 NO 155.5
o
2 g 2 g
1
2 2 g
3
2
3
2 2 g
3
2 2 g g
2 g 2 g 2 g
2 g 2 g g
∆
1
2
1
2
1
2
1
2
3
× − →
× →
× − →
+ →
03/06/17 Presented to DR. THELMA A. ANTONIO
58
Hess’s Law
 The + sign of the ∆Ho
value tells us that the reaction is
endothermic.
 The reverse reaction is exothermic, i.e.,
( ) ( ) ( )3 NO N O + NO H = -155.5 kJg 2 g 2 g
o
→ ∆
03/06/17 Presented to DR. THELMA A. ANTONIO
59
Hess’s Law
 Hess’s Law in a more useful form.
 For any chemical reaction at standard conditions, the
standard enthalpy change is the sum of the standard molar
enthalpies of formation of the products (each multiplied
by its coefficient in the balanced chemical equation)
minus the corresponding sum for the reactants.
tscoefficientricstoichiomen
HnHnH 0
reactantsf
0
productsf
0
rxn
=
∆−∆=∆ ∑∑ nn
03/06/17 Presented to DR. THELMA A. ANTONIO
60
Hess’s Law
 Example 8: Calculate the ∆H o
298 forthe following
reaction from data in the reference.
)(22(g)2(g)8(g)3 OH4CO3O5HC +→+
03/06/17 Presented to DR. THELMA A. ANTONIO
61
Hess’s Law
 Example 8: Calculate ∆Ho
298 for the following reaction
from data in reference.
( ) ( ) ( ) ( )
( ) ( )[ ] ( ) ( )[ ]
[ ] [ ]{ }
C H + 5 O CO + 4 H O
H H H H H
kJ
3 8 g 2 g 2 g 2
298
o
f CO
o
f H O
o
f C H
o
f O g
o
2 g 2 3 8 g 2
→
= + − +
= − + − − − +
3
3 4 5
3 3935 4 2858 1038 5 0
l
l∆ ∆ ∆ ∆ ∆
( . ) ( . ) ( . ) ( )
( ) ( ) ( ) ( )
( ) ( )[ ] ( ) ( )[ ]
C H + 5 O CO + 4 H O
H H H H H
3 8 g 2 g 2 g 2
298
o
f CO
o
f H O
o
f C H
o
f O g
o
2 g 2 3 8 g 2
→
= + − +
3
3 4 5
l
l∆ ∆ ∆ ∆ ∆
( ) ( ) ( ) ( )
( ) ( )[ ] ( ) ( )[ ]
[ ] [ ]{ }
C H + 5 O CO + 4 H O
H H H H H
kJ
= -2211.9 kJ
H kJ, and so the reaction is exothermic.
3 8 g 2 g 2 g 2
298
o
f CO
o
f H O
o
f C H
o
f O g
o
298
o
2 g 2 3 8 g 2
→
= + − +
= − + − − − +
= −
3
3 4 5
3 3935 4 2858 1038 5 0
22119
l
l∆ ∆ ∆ ∆ ∆
∆
( . ) ( . ) ( . ) ( )
.
03/06/17 Presented to DR. THELMA A. ANTONIO
62
Hess’s Law
 Application of Hess’s Law and more algebra allows us to
calculate the ∆Hf
o
for a substance participating in a reaction
for which we know ∆Hrxn
o
, if we also know ∆Hf
o
for all other
substances in the reaction.
 Example 9: Given the following information, calculate ∆Hf
o
for H2S(g).
( ) ( ) ( ) ( )2 H S + 3 O 2 SO + 2 H O H = -1124 kJ
H ? 0 - 296.8 - 285.8
(kJ / mol)
2 g 2 g 2 g 2 298
o
f
o
→ l ∆
∆
You do it!You do it!
03/06/17 Presented to DR. THELMA A. ANTONIO
63
Hess’s Law
( ) ( )[ ] ( ) ( )[ ]
[ ] ( )[ ]{ }
( )
( )
( )
∆ ∆ ∆ ∆ ∆
∆
∆
∆
∆
H H H H H
kJ H kJ
now we solve for H
H kJ
H kJ
298
o
f SO
o
f H O
o
f H S
o
f O
o
f H S
o
f H S
o
f H S
o
f H S
o
2 g 2 2 g 2 g
2 g
2 g
2 g
2 g
= + − +
− = − + − − +
= −
= −
2 2 2 3
1124 2 2968 2 2858 2 3 0
2 412
20 6
l
( . ) ( . ( )
.
.
03/06/17 Presented to DR. THELMA A. ANTONIO
Numbered Heads Together
The class will form groups
with four members. You will get a
problem from the teacher.
Afterwards, you are to answer and
discuss with the group. Your teacher
then will call randomly one
representative from the group and
discuss it with her/him in a corner.
03/06/17 Presented to DR. THELMA A. ANTONIO 64
Possible Problems:
03/06/17 Presented to DR. THELMA A. ANTONIO 65
ΔH for the reaction
is __________ kJ, give the data below.
ΔH = -390 kJ
ΔH = -745 kJ
03/06/17 Presented to DR. THELMA A. ANTONIO 66
Given the following reactions:
ΔH = -790 kJ
ΔH = -297 kJ
the enthalpy of the reaction in which sulfur dioxide is oxidized to sulfur trioxide
is __________ kJ.
03/06/17 Presented to DR. THELMA A. ANTONIO 67
Given the following reactions
ΔH = 178.1 kJ
ΔH = -393.5 kJ
the enthalpy of the reaction
is __________ kJ.
03/06/17 Presented to DR. THELMA A. ANTONIO 68
Given the following reactions
ΔH = +180.7 kJ
ΔH = -163.2 kJ
the enthalpy of reaction for
is __________ kJ.
69
Bond Energies
 Bond energy is the amount of energy required to
break the bond and separate the atoms in the gas
phase.
 To break a bond always requires an absorption of energy!
( ) ( ) ( )
( ) ( ) ( )
A - B bond energy A + B
H - Cl H + Cl
g g g
g
kJ
mol g g
+ →
+ →432
03/06/17 Presented to DR. THELMA A. ANTONIO
70
Bond Energies
 Table of average bond energies
 Molecule Bond Energy (kJ/mol)
 F2 159
 Cl2 243
 Br2 192
 O2 (double bond) 498
 N2 (triple bond) 946
03/06/17 Presented to DR. THELMA A. ANTONIO
71
Bond Energies
 Bond energies can be calculated from other ∆Ho
298 values.
03/06/17 Presented to DR. THELMA A. ANTONIO
72
Bond Energies
 Bond energies can be calculated from other ∆Ho
298 values
 Example 9: Calculate the bond energy for hydrogen
fluoride, HF.
( ) ( ) ( )
( ) ( ) ( )
( ) ( )[ ] ( )[ ]
H - F BE H F atoms NOT ions
H - F H F H BE
H H H H
g HF g g
g g g 298
o
HF
298
o
f H
o
f F
o
f HF
o
g g g
+ → +
→ + =
= + −
or
∆
∆ ∆ ∆ ∆
( ) ( ) ( )
( ) ( ) ( )
H - F BE H F atoms NOT ions
H - F H F H BE
g HF g g
g g g 298
o
HF
+ → +
→ + =
or
∆
( ) ( ) ( )
( ) ( ) ( )
( ) ( )[ ] ( )[ ]
[ ] [ ]
H - F BE H F atoms NOT ions
H - F H F H BE
H H H H
H kJ + 78.99 kJ kJ
H kJ BE for HF
g HF g g
g g g 298
o
HF
298
o
f H
o
f F
o
f HF
o
298
o
298
o
g g g
+ → +
→ + =
= + −
= − −
= ←
or
∆
∆ ∆ ∆ ∆
∆
∆
218 0 271
568 0
.
.
03/06/17 Presented to DR. THELMA A. ANTONIO
73
Bond Energies
 Example 10: Calculate the average N-H bond
energy in ammonia, NH3.
You do it!You do it!
03/06/17 Presented to DR. THELMA A. ANTONIO
74
Bond Energies
( ) ( ) ( )
( ) ( )
[ ] ( )
[ ]
[ ] [ ]{ }
bondsH-Nmol
kJ
H-N
o
298
o
298
o
NHf
o
Hf
o
Nf
o
298
H-N
o
298ggg3
391
3
kJ1173
BEaverage
kJ1173H
kJ11.46)218(3)7.472(H
HH3HH
BE3HH3+NNH
g3gg
==
=∆
−−+=∆
∆−∆+∆=∆
=∆→
03/06/17 Presented to DR. THELMA A. ANTONIO
75
Bond Energies
 In gas phase reactions ∆Ho
values may be
related to bond energies of all species in the
reaction.
∆H BE BE298
o
reactants products= ∑ − ∑
03/06/17 Presented to DR. THELMA A. ANTONIO
76
Bond Energies
 Example 11: Use the bond energies listed in
the reference to estimate the heat of reaction
at 25o
C for the reaction below.
]BE4BE[2-]BE2BE[4H
OH2COO2CH
H-OOCOOH-C
o
298
(g)22(g)2(g)4(g)
++=∆
+→+
==
03/06/17 Presented to DR. THELMA A. ANTONIO
77
Bond Energies
{ }
kJ686-H
kJ(464)]4741)([2-498)](2(414)[4H
]BE4BE[2-]BE2BE[4H
OH2COO2CH
o
298
o
298
H-OOCOOH-C
o
298
(g)22(g)2(g)4(g)
=∆
++=∆
++=∆
+→+
==
03/06/17 Presented to DR. THELMA A. ANTONIO
Pairs Check
By pair (pairing prepared by
your teacher), one coaches
his/her partner to answer the
problems given by the teacher.
03/06/17 Presented to DR. THELMA A. ANTONIO 78
Possible Problems:
03/06/17 Presented to DR. THELMA A. ANTONIO 79
G iven: H -H bond energy = 435 kJ, C l-C l bond energy = 243 kJ, and the standard heat of
form ation of H C l(g) is –92 kJ/m ol, calculate the H -C l bond energy.
The H0f for gaseous acetylene (shown below), is 227 kJ/mol. What is the bond
energy? The bond energies are 423 kJ/mol for C–H and 436 kJ/mol for H–H. The heat of
sublimation for carbon is 717 kJ/mol.
80
Changes in Internal Energy, ∆E
 The internal energy, E, is all of the energy
contained within a substance.
 This function includes all forms of energy such as
kinetic, potential, gravitational, electromagnetic,
etc.
 The First Law of Thermodynamics states that the
change in internal energy, ∆E, is determined by
the heat flow, q, and the work, w.
03/06/17 Presented to DR. THELMA A. ANTONIO
81
Changes in Internal Energy, ∆E
system.by theabsorbedisheatif0q
system.by theabsorbedisheatif0q
wqE
EEE reactantsproducts
<
>
+=∆
−=∆∆
∆
E = E E
E = q + w
products reactants−
gs.surroundinon theworkdoessystemtheif0w
system.on theworkdogssurroundintheif0w
system.by theabsorbedisheatif0q
system.by theabsorbedisheatif0q
wqE
EEE reactantsproducts
<
>
<
>
+=∆
−=∆
03/06/17 Presented to DR. THELMA A. ANTONIO
82
Changes in Internal Energy, ∆E
 ∆E is negative when energy is released by a system
undergoing a chemical or physical change.
 Energy can be written as a product of the process.
kJ103.516-E
kJ103.516OH6CO5O8HC
3
3
)(22(g)2(g))(125
×=∆
×++→+ 
03/06/17 Presented to DR. THELMA A. ANTONIO
83
Changes in Internal Energy, ∆E
 ∆E is positive when energy is absorbed by a system
undergoing a chemical or physical change.
 Energy can be written as a reactant of the process.
kJ103.516E
O8HCkJ103.516OH6CO5
3
2(g))(125
3
)(22(g)
×+=∆
+→×++ 
03/06/17 Presented to DR. THELMA A. ANTONIO
84
Changes in Internal Energy, ∆E
 Example 12: If 1200 joules of heat are added to a
system in energy state E1, and the system does 800
joules of work on the surroundings, what is the :
1. energy change for the system, ∆Esys?
∆
∆
∆
∆
E = E - E = q + w
E = 1200 J + (-800 J)
E = 400 J
E = + 400 J
2 1
sys03/06/17 Presented to DR. THELMA A. ANTONIO
85
Changes in Internal Energy, ∆E
2. energy change of the surroundings, ∆Esurr?
You do it!
∆E Jsurr = −400
03/06/17 Presented to DR. THELMA A. ANTONIO
86
Changes in Internal Energy, ∆E
3. energy of the system in the new state, E2?
∆
∆
E E - E
E E E
E J
sys 2 1
2 1 sys
1
=
= +
= + 400
03/06/17 Presented to DR. THELMA A. ANTONIO
87
Changes in Internal Energy, ∆E
 In most chemical and physical changes, the
only kind of work is pressure-volume work.
 Pressure is force per unit area.
P =
force
area
F
d2
=
03/06/17 Presented to DR. THELMA A. ANTONIO
88
Changes in Internal Energy, ∆E
 Volume is distance cubed.
 P∆V is a work term, i.e., the same units are used for
energy and work.
V = d3
( )P V =
F
d
d F d which is work2
3
∆ 




 = × ←
03/06/17 Presented to DR. THELMA A. ANTONIO
89
Changes in Internal Energy, ∆E
 Using the ideal gas law PV = nRT, we can look at
volume changes of ideal gases at constant T and P
due to changes in the number of moles of gas
present, ∆ngas.
 ∆ngas = (number of moles of gaseous products) - (number of
moles of gaseous reactants)
( ) ( )
PV = nRT
P V n RTgas∆ ∆=
03/06/17 Presented to DR. THELMA A. ANTONIO
90
Changes in Internal Energy, ∆E
 Work is defined as a force acting through a specified
distance.
 Consequently, there are three possibilities for volume
changes:
( )
( )
P.andTconstantat
RTn-that wseecanweThus
RTn-V-PdFw
gas
gas
∆=
∆=∆=×=
03/06/17 Presented to DR. THELMA A. ANTONIO
91
Changes in Internal Energy, ∆E
When Then Examples
1. V2 = V1 P∆V = 0
∆ngas = 0
    
gasmol2
2(g)(g)2
gasmol2
(g)2(g) COHOHCO +→+
3. V2 < V1 P∆V < 0
∆ngas < 0
2. V2 > V1 P∆V > 0
∆ngas > 0
    
gasmol1
2(g)2(aq)
gasmol0
(aq)(s) HZnClHCl2Zn +→+
  
gasmol2
3(g)
gasmol4
2(g)2(g) NH2H3N →+
03/06/17 Presented to DR. THELMA A. ANTONIO
92
Changes in Internal Energy, ∆E
 Consider the following gas phase reaction at
constant pressure at 200o
C.
( ) ( ) ( )2 NO + O 2 NOg 2 g
3 mol gas
2 g
2 mol gas
     
→
gs.surroundinbysystemondoneisWork
0.VP-wly,Consequent
0.VPand0VthusVV 12
>∆=
<∆<∆<
03/06/17 Presented to DR. THELMA A. ANTONIO
93
Changes in Internal Energy, ∆E
 Consider the following gas phase reaction at
constant pressure at 1000o
C.
( ) ( ) ( )
  
gasmol2
g2g3
gasmol1
g5 ClPClPCl +→
gs.surroundinon thesystemby thedoneisWork
0.VP-wly,Consequent
0.VPand0VthusVV 12
<∆=
>∆>∆>
03/06/17 Presented to DR. THELMA A. ANTONIO
94
Relationship of ∆H and ∆E
 The total amount of heat energy that a system
can provide to its surroundings at constant
temperature and pressure is given by
∆H= ∆E + P ∆V
 which is the relationship between ∆H and ∆E.
 ∆H = change in enthalpy of system
 ∆E = change in internal energy of system
 P∆V = work done by system
03/06/17 Presented to DR. THELMA A. ANTONIO
95
Relationship of ∆H and ∆E
 At the start we defined
∆H = qP.
 Here we define ∆H = ∆E + P∆V.
 Are these two definitions compatible?
 Remember ∆E = q + w.
 We have also defined w = -P∆V .
 Thus ∆E = q + w = q -P∆V
 Consequently, ∆H = q- P∆V + P∆V = q
 At constant pressure ∆H = qP.
03/06/17 Presented to DR. THELMA A. ANTONIO
96
Relationship of ∆H and ∆E
 For reactions in which the volume change is
very small or equal to zero.
E.H
change,volumenoFor
E.H
thenVPEHSince
0.VPand0V
changes,volumesmallFor
∆=∆
∆≈∆
∆+∆=∆
≈∆≈∆
03/06/17 Presented to DR. THELMA A. ANTONIO
97
Relationship of ∆H and ∆E
 Change in enthalpy, ∆H, or heat of reaction is amount of heat
absorbed or released when a reaction occurs at constant
pressure.
 The change in energy, ∆E, is the amount of heat absorbed or
released when a reaction occurs at constant volume.
 How much do the ∆H and ∆E for a reaction differ?
 The difference depends on the amount of work performed by the
system or the surroundings.
03/06/17 Presented to DR. THELMA A. ANTONIO
98
Relationship of ∆H and ∆E
 Example 13: Noted that ∆Ho
= -3523 kJ/mol
for the combustion of n-pentane, n-C5H12.
Combustion of one mol of n-pentane at
constant pressure releases 3523 kJ of heat.
What are the values of the work term and ∆E
for this reaction?
)(22(g)2(g))12(5 OH6CO5O8HC  +→+
03/06/17 Presented to DR. THELMA A. ANTONIO
99
Relationship of ∆H and ∆E
 Determine the work done by this reaction.
You do it!You do it!
kJ7.433J7433K)298)(mol)(8.314-(-3w
mol3-mol85n
RT)n(-VP-w
K.298TthatknowwekJ/mol,3523-HSince
OH6CO5O8HC
Kmol
J
gas
gas
o
gasmol5
)(22(g)
gasmol8
2(g))12(5
===
=−=∆
∆=∆=
==∆
+→+
     
03/06/17 Presented to DR. THELMA A. ANTONIO
100
Relationship of ∆H and ∆E
 Now calculate the ∆E for this reaction from the
values of ∆H and w that we have determined.
You do it!You do it!
∆ ∆ ∆ ∆ ∆ ∆
∆
∆
∆
H E + P V E = H - P V
since w = - P V = 7.433 kJ
then P V = - 7.433 kJ
E = - 3523 kJ - (-7.433 kJ) = -3516 kJ
= ∴
03/06/17 Presented to DR. THELMA A. ANTONIO
Journal Reflection
In your journal, try to reflect
whether the following is spontaneous
or not and justify your answer. And go
back to your journal after tackling the
next topic on spontaneity of physical
and chemical changes.
Spreading of the fragrance of
perfume throughout the room
03/06/17 Presented to DR. THELMA A. ANTONIO 101
 Separation of nitrogen and oxygen molecules
in air
 Fixing of a broken watch
 Extraction of salt from seawater
03/06/17 Presented to DR. THELMA A. ANTONIO 102
103
Spontaneity of Physical and
Chemical Changes
 Spontaneous changes happen without any continuing
outside influences.
 A spontaneous change has a natural direction.
 For example the rusting of iron occurs
spontaneously.
 Have you ever seen rust turn into iron metal without man
made interference?
 The melting of ice at room temperature occurs
spontaneously.
 Will water spontaneously freeze at room temperature?03/06/17 Presented to DR. THELMA A. ANTONIO
104
The Two Aspects of Spontaneity
 An exothermic reaction does not ensure
spontaneity.
 For example, the freezing of water is exothermic
but spontaneous only below 0o
C.
 An increase in disorder of the system also
does not insure spontaneity.
 It is a proper combination of exothermicity
and disorder that determines spontaneity.
03/06/17 Presented to DR. THELMA A. ANTONIO
105
The Second Law of Thermodynamics
 The second law of thermodynamics states, “In
spontaneous changes the universe tends towards a
state of greater disorder.”
 Spontaneous processes have two requirements:
1. The free energy change of the system must be negative.
2. The entropy of universe must increase.
 Fundamentally, the system must be capable of doing useful work
on surroundings for a spontaneous process to occur.
03/06/17 Presented to DR. THELMA A. ANTONIO
Draw-it
By group of three members, make a
poster on the following scenario.
Afterwards, determine if its “disorder”
increases or decreases.
A football stadium empties after a game
A baby develops into an adult
Paper, plastics, and aluminum are
separated and recycled
03/06/17 Presented to DR. THELMA A. ANTONIO 106
107
Entropy, S
 Entropy is a measure of the disorder or
randomness of a system.
 As with ∆H, entropies have been measured and
tabulated in Appendix K as So
298.
 When:
 ∆S > 0 disorder increases (which favors
spontaneity).
 ∆S < 0 disorder decreases (does not favor
spontaneity).
03/06/17 Presented to DR. THELMA A. ANTONIO
108
Entropy, S
 From the Second Law of Thermodynamics, for a
spontaneous process to occur:
 In general for a substance in its three states of
matter:
Sgas> Sliquid > Ssolid
0SSS gssurroundinsystemuniverse >∆+∆=∆
03/06/17 Presented to DR. THELMA A. ANTONIO
109
Entropy, S
 The Third Law of Thermodynamics states, “The
entropy of a pure, perfect, crystalline solid at 0 K is
zero.”
 This law permits us to measure the absolute values
of the entropy for substances.
 To get the actual value of S, cool a substance to 0 K, or as
close as possible, then measure the entropy increase as the
substance heats from 0 to higher temperatures.
03/06/17 Presented to DR. THELMA A. ANTONIO
110
Entropy, S
 Entropy changes for reactions can be determined
similarly to ∆H for reactions.
o
reactants
n
o
products
n
o
298 SnSnS ∑∑ −=∆
03/06/17 Presented to DR. THELMA A. ANTONIO
111
Entropy, S
 Example 14: Calculate the entropy change for
the following reaction at 25o
C.
You do it!
←→
4(g)22(g) ONNO2
03/06/17 Presented to DR. THELMA A. ANTONIO
112
Entropy, S
Kmol
kJ
Kmol
J
Kmol
J
Kmol
J
o
NO
o
ON
o
reactants
n
o
products
n
o
rxn
4(g)22(g)
0.1758-or8.175
)0.240(2)2.304(
S2S
SnSnS
ONNO2
2(g)4(g)2
−=
−=
−=
−=∆
←→
∑∑
 The negative sign of ∆S indicates that the system is
more ordered.
 If the reaction is reversed the sign of ∆S changes.
 For the reverse reaction ∆So
298= +0.1758 kJ/K
 The + sign indicates the system is more disordered.03/06/17 Presented to DR. THELMA A. ANTONIO
113
Entropy, S
 Example 15: Calculate ∆So
298 for the reaction
below.
( ) ( ) ( )
You do it!
← +→
g2g2g NOONNO3
03/06/17 Presented to DR. THELMA A. ANTONIO
114
Entropy, S
( ) ( ) ( )
( ) ( ) ( )
( )[ ]
Kmol
kJ
Kmol
J
Kmol
J
0
NO
0
NO
0
ON
0
298
g2g2g
0.1724-or4.172
210.43-240.07.219
S3SSS
NOONNO3
gg2g2
−=
+=
−+=∆
← +→
 Changes in ∆S are usually quite small compared to
∆E and ∆H.
 Notice that ∆S has units of only a fraction of a kJ while
∆E and ∆H values are much larger numbers of kJ.03/06/17 Presented to DR. THELMA A. ANTONIO
Hands-on Learning
(Laboratory)
03/06/17 Presented to DR. THELMA A. ANTONIO 115
116
Free Energy Change, ∆G,
and Spontaneity
 In the mid 1800’s J. Willard Gibbs determined the
relationship of enthalpy, H, and entropy, S, that best
describes the maximum useful energy obtainable in
the form of work from a process at constant
temperature and pressure.
 The relationship also describes the spontaneity of a
system.
 The relationship is a new state function, ∆G, the
Gibbs Free Energy.
∆ ∆ ∆G = H - T S (at constant T & P)03/06/17 Presented to DR. THELMA A. ANTONIO
117
Free Energy Change, ∆G,
and Spontaneity
 The change in the Gibbs Free Energy, ∆G, is a
reliable indicator of spontaneity of a physical
process or chemical reaction.
 ∆G does not tell us how quickly the process occurs.
 Chemical kinetics, the subject of Chapter 16, indicates the rate of
a reaction.
 Sign conventions for ∆G.
 ∆G > 0 reaction is nonspontaneous
 ∆G = 0 system is at equilibrium
 ∆G < 0 reaction is spontaneous
03/06/17 Presented to DR. THELMA A. ANTONIO
118
Free Energy Change, ∆G,
and Spontaneity
 Changes in free energy obey the same type of
relationship we have described for enthalpy,
∆H, and entropy, ∆S, changes.
0
reactants
n
0
products
n
0
298 GnGnG ∆−∆=∆ ∑∑
03/06/17 Presented to DR. THELMA A. ANTONIO
119
Free Energy Change, ∆G,
and Spontaneity
 Example16: Calculate ∆Go
298 for the reaction in
Example 8.
You do it!
)(22(g)2(g))8(3 OH4CO3O5HC  +→+
03/06/17 Presented to DR. THELMA A. ANTONIO
120
Free Energy Change, ∆G,
and Spontaneity
 ∆Go
298< 0, so the reaction is spontaneous at
standard state conditions.
 If the reaction is reversed:
 ∆Go
298> 0, and the reaction is nonspontaneous at
standard state conditions.
mol
kJ
mol
kJ
o
Of
o
HCf
o
OHf
o
COf
o
rxn
)(22(g)2(g)8(g)3
5.2108
)]}0(5)49.23[()3.237(4)4.394(3{[
]G5G[]G4G3[G
OH4CO3O5HC
2(g)(g)83)(22(g)
−=
+−−−+−=
∆+∆−∆+∆=∆
+→+


03/06/17 Presented to DR. THELMA A. ANTONIO
Impersonation
By team, one member
impersonates the life and works
of J. Willard Gibbs. Other
members may act as support
characters. Then, present it to
the class.
03/06/17 Presented to DR. THELMA A. ANTONIO 121
122
The Temperature
Dependence of Spontaneity
 Free energy has the relationship ∆G = ∆H -T∆S.
 Because 0 ≤ ∆H ≥ 0 and 0 ≤ ∆S ≥ 0, there are four
possibilities for ∆G.
∆H ∆S ∆G Forward reaction spontaneity
< 0 > 0 < 0 Spontaneous at all T’s.
< 0 < 0 T dependent Spontaneous at low T’s.
> 0 > 0 T dependent Spontaneous at high T’s.
> 0 < 0 > 0 Nonspontaneous at all T’s.
03/06/17 Presented to DR. THELMA A. ANTONIO
123
The Temperature
Dependence of Spontaneity
03/06/17 Presented to DR. THELMA A. ANTONIO
124
The Temperature
Dependence of Spontaneity
 Example 17: Calculate ∆So
298 for the following reaction. In
example 8, we found that ∆Ho
298= -2219.9 kJ, and in Example
16 we found that ∆Go
298= -2108.5 kJ.
o
oo
ooo
ooo
)(22(g)2(g))12(5
S
T
GH
STGH
STHG
OH6CO5O8HC
∆=
∆−∆
∆=∆−∆
∆−∆=∆
+→+ 
( )[ ]
K
J-374
K
kJ374.0S
K298
kJ5.21089.2219
S
o
o
=−=∆
−−−
=∆
03/06/17 Presented to DR. THELMA A. ANTONIO
125
The Temperature
Dependence of Spontaneity
 ∆So
298= -374 J/K which indicates that the
disorder of the system decreases .
 For the reverse reaction,
3 CO2(g) + 4 H2O(g)→ C3H8(g) + 5 O2(g)
 ∆So
298= +374 J/K which indicates that the
disorder of the system increases .
03/06/17 Presented to DR. THELMA A. ANTONIO
126
The Temperature
Dependence of Spontaneity
 Example 18: Use thermodynamic data to estimate
the normal boiling point of water.
S
H
TandSTHThus
0.GprocessequlibriumanisthisBecause
OHOH (g)2)(2
∆
∆
=∆=∆
=∆
←→

03/06/17 Presented to DR. THELMA A. ANTONIO
127
The Temperature
Dependence of Spontaneity
[ ]
assume H@BP H
H H H
H
H kJ@25 C
298
o
o
H O
o
H O
o
o J
K
o o
2 (g) 2 ( )
∆ ∆
∆ ∆ ∆
∆
∆
≈
= −
= − − −
= +
l
2418 2858
44 0
. ( . )
.03/06/17 Presented to DR. THELMA A. ANTONIO
128
The Temperature
Dependence of Spontaneity
( ) ( )
[ ]
K
kJ
K
J0
rxn
K
J0
rxn
0
OH
0
OH
0
rxn
0
rxn
0.1188or8.118S
91.697.188S
SSS
SBP@Sassume
2g2
=∆
−=∆
−=∆
∆≈∆

03/06/17 Presented to DR. THELMA A. ANTONIO
129
The Temperature
Dependence of Spontaneity
T =
H
S
H
S
.0 kJ
0.1188
K
370 K -273 K = 97 C
o
o kJ
K
o
∆
∆
∆
∆
≈ = =
44
370
03/06/17 Presented to DR. THELMA A. ANTONIO
Act-Like-a-Teacher
Review the problems
given in the next slides. If
you are confident with your
answer in any of the given,
volunteer to the class and
discuss it like a teacher.
03/06/17 Presented to DR. THELMA A. ANTONIO 130
Problems
03/06/17 Presented to DR. THELMA A. ANTONIO 131
For w hich set of values of ∆ H and ∆ S w ill a reaction be spontaneous (product-favored) at
all temperatures?
(a) ∆ H = +10 kJ, ∆ S = –5 J/K (b) ∆ H = –10 kJ, ∆ S = –5 J/K
(c) ∆ H = –10 kJ, ∆ S = +5 J/K (d) ∆ H = +10 kJ, ∆ S = +5 J/K
(e) no such values exist
03/06/17 Presented to DR. THELMA A. ANTONIO 132
Joseph Priestley prepared oxygen by heating mercury(II) oxide. The compound H gO is stable
at room temperature but decomposes into its elements (H g and O 2) at high temperatures. W hat
conclusio ns can be draw n concerning ∆ H and ∆ S for this decompositio n reaction?
(a) ∆ H is negative and ∆ S is positive.
(b) ∆ H is negative and ∆ S is negative.
(c) ∆ H is positive and ∆ S is positive.
(d) ∆ H is positive and ∆ S is negative.
(e) ∆ H becomes negative at high temperatures.
03/06/17 Presented to DR. THELMA A. ANTONIO 133
The follow ing reaction is spontaneous only below 5000 K . W hat conclusio ns can be draw n
regarding this reaction? A + B  A B
(a) ∆ H is negative and ∆ S is positive.
(b) ∆ H is negative and ∆ S is negative.
(c) ∆ H is positive and ∆ S is positive.
(d) ∆ H is positive and ∆ S is negative.
(e) C an’t conclude anything.
03/06/17 Presented to DR. THELMA A. ANTONIO 134
For a certain process at 127°C , ∆ G = –16.20 kJ and ∆ H = –17.0 kJ. W hat is the entropy
change for this process at this temperature? Express your answ er in the form,
∆ S = _______________ J/K .
(a) –6.3 J/K (b) +6.3 J/K (c) –2.0 J/K (d) +2.0 J/K (e) –8.1 J/K
03/06/17 Presented to DR. THELMA A. ANTONIO 135
For the follow ing reaction, ∆ H o
= -104.9 kJ/mol. If this reaction is spontaneous at all
temperatures below 361 K , w hat is the value of ∆ So
?
(a) -165 J/mol•K (b) –0.291 J/mol•K (c) 3.44 J/mol•K
(d) -291 J/mol•K (e) 3.44 kJ
03/06/17 Presented to DR. THELMA A. ANTONIO 136
Estim ate the tem perature above w hich this reaction is spontaneous. ∆ S0 = 16.1 J/K .
C H 4(g) + N 2(g) + 163.8 kJ → H C N (g) + N H 3(g)
(a) 9.91°C (b) 1045 K (c) 9.90 x 103°C (d) 10.7 K (e) 10.1°C
03/06/17 Presented to DR. THELMA A. ANTONIO 137
Fora particular reaction at25 o
C,∆Ho
= -297 kJ/mol, and ∆So
= -113.3 J/mol•K . Atwhich ofthe
follow ing temperatures would the reaction spontaneous?
(a)2750 K (b)3250 K (c) 2450 K (d) 10500 K (e) 3750 K
Synthesis
Finally, after dealing with the
concepts on the heat changes and
thermochemistry and the spontaneity of
physical and chemical changes, create
an MI project mode by group according
to your MI profile. On the other side,
prior to that, read in the class the
following free verse poem as starter.
03/06/17 Presented to DR. THELMA A. ANTONIO 138
POST-TEST
Congratulations! You finished
the module tapping your multiple
intelligences. This time, check yourself
again on your mastery on the
Thermodynamics concepts and
problems. God bless you!
03/06/17 Presented to DR. THELMA A. ANTONIO 139
Answer to the Post-Test
03/06/17 Presented to DR. THELMA A. ANTONIO 140
REFERENCES
 Antero, ES., et al. Conceptual and Functional
Chemistry. 2010. Vibal Publishing House,
1253 G. Araneta Ave., Quezon City
 LeMAy, H.E., et al. Chemistry: Connection
to our Changing World. 2002. Prentice-Hall,
Inc. New Jersey
03/06/17 Presented to DR. THELMA A. ANTONIO 141
 White, David P. Chemistry: The Central
Science. 9th ed. 2003. Prentice-Hall, Inc.
New Jersey
03/06/17 Presented to DR. THELMA A. ANTONIO 142

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Thermodynamics

  • 1. MI- Based Module: THERMODYNAMICS Prepared by: NOROLAYN K. SAID Presented to: DR. THELMA A. ANTONIO
  • 2. CONTENTS  Introduction  Objectives  Pre-Test  First Law of Thermodynamics  Some Thermodynamic Terms  Enthalpy Changes  Calorimetry  Thermochemical Equation03/06/17 Presented to DR. THELMA A. ANTONIO 2
  • 3.  Standard States and Standard Enthalpy Chan  Standard Molar Enthalpy of Formation  Hess’s Law  Bond Energies  Changes in Internal Energy  Relationship of Enthalpy and Internal Energy 03/06/17 Presented to DR. THELMA A. ANTONIO 3
  • 4.  Spontaneity of Physical and Chemical Changes  Two Aspects of Spontaneity  Second Law of Thermodynamics  Entropy  Free Energy Change and Spontaneity  Temperature Dependence of Spontaneity  Post-Test  References 03/06/17 Presented to DR. THELMA A. ANTONIO 4
  • 5. Hi students! Welcome to the world of Thermodynamics! In this module, you will be learning important concepts on heat changes and thermochemistry and the spontaneity of physical and chemical changes. 5 INTRODUCTION 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 6. OBJECTIVES After accomplishing the module, you are expected to: 1.Distinguish between exothermic and endothermic reactions; 2.Explain what is meant by enthalpy and enthalpy change; 3.Define standard enthalpy change and explain how it is used; 03/06/17 Presented to DR. THELMA A. ANTONIO 6
  • 7. 4. Describe how calorimeter determines heats of reactions; 5. State Hess’s Law; 6. Apply Hess’s Law to determine ∆H for a reaction; 7. Explain what is meant by spontaneous process; 8. Relate enthalpy change to spontaneity; 03/06/17 Presented to DR. THELMA A. ANTONIO 7
  • 8. 9. Define entropy; 10. State the entropy criterion for a spontaneous process; 11. State the criterion for reaction spontaneity in terms of its free energy; 12. Compare the three Laws of Thermodynamics; 03/06/17 Presented to DR. THELMA A. ANTONIO 8
  • 9. 13. Perform problem-solving on thermodynamic problems; and 14. Perform activities using multiple intelligences. 03/06/17 Presented to DR. THELMA A. ANTONIO 9
  • 10. PRE-TEST Oopps! Before you proceed, check yourself first with the pre- test for an evaluation. Don’t worry this will not affect your grade. This will only measure your pre- knowledge on the concepts and problems on Thermodynamics. Good Luck! 03/06/17 Presented to DR. THELMA A. ANTONIO 10
  • 11. Answer to the Pre-Test 03/06/17 Presented to DR. THELMA A. ANTONIO 11
  • 12. RoundRobin In three to four members in a group, share to the team one physical and one chemical change that take place at home before you went to school. And try to identify them as releasing heat or absorbing heat. Do this one-at-a-time with your group-mates. 03/06/17 Presented to DR. THELMA A. ANTONIO 12
  • 13. 13 The First Law of Thermodynamics  Thermodynamics is the study of the changes in energy and transfers of energy that accompany chemical and physical processes.  You will address 3 fundamental questions. 1. Will two (or more) substances react when they are mixed under specified conditions? 2. If they do react, what energy changes and transfers are associated with their reaction? 3. If a reaction occurs, to what extent does it occur? 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 14. 14  Exothermic reactions release energy in the form of heat.  For example, the combustion of propane is exothermic.  The combustion of n-butane is also exothermic. kJ102.22O4HCO3O5HC 3 )(22(g)2(g)(g)83 ×++→+  kJ105.78OH10CO8O13HC2 3 )(22(g)2(g)10(g)4 ×++→+  03/06/17 Presented to DR. THELMA A. ANTONIO
  • 15. 15  Exothermic reactions generate specific amounts of heat.  This is because the potential energies of the products are lower than the potential energies of the reactants. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 16. 16  There are two basic ideas of importance for thermodynamic systems. 1. Chemical systems tend toward a state of minimum potential energy.  Some examples of this include:  H2O flows downhill.  Objects fall when dropped.  The energy change for these two examples is:  Epotential = mgh  ∆Epotential = mg(∆h)03/06/17 Presented to DR. THELMA A. ANTONIO
  • 17. 17 2. Chemical systems tend toward a state of maximum disorder.  Common examples of this are:  A mirror shatters when dropped and does not reform.  It is easy to scramble an egg and difficult to unscramble it.  Food dye when dropped into water disperses. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 18. 18  This law can be stated as, “The combined amount of energy in the universe is constant.”  The first law is also known as the Law of Conservation of Energy.  Energy is neither created nor destroyed in chemical reactions and physical changes. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 19. 19 Some Thermodynamic Terms  The substances involved in the chemical and physical changes under investigation are called the system.  In chemistry lab, the system is the chemicals inside the beaker.  The environment around the system is called the surroundings.  The surroundings are outside the beaker.  The system plus the surroundings is called the universe. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 20. 20  The set of conditions that specify all of the properties of the system is called the thermodynamic state of a system.  For example the thermodynamic state could include:  The number of moles and identity of each substance.  The physical states of each substance.  The temperature of the system.  The pressure of the system. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 21. 21  The properties of a system that depend only on the state of the system are called state functions.  State functions are always written using capital letters.  The value of a state function is independent of pathway.  An analog to a state function is the energy required to climb a mountain taking two different paths.  E1 = energy at the bottom of the mountain  E1 = mgh1  E2 = energy at the top of the mountain  E2 = mgh2  ∆E = E2-E1 = mgh2 – mgh1 = mg(∆h) 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 22. 22  Notice that the energy change in moving from the top to the bottom is independent of pathway but the work required may not be!  Some examples of state functions are:  T, P, V, ∆E, ∆H, and S  Examples of non-state functions are:  n, q, w 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 23. 23  In thermodynamics we are often interested in changes in functions.  We will define the change of any function X as:  ∆X = Xfinal – Xinitial  If X increases ∆X > 0  If X decreases ∆X < 0. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 24. Team Chant Create a Chem. Jingle by group using familiar tunes and the following thermodynamic terms in the lyrics such as system surroundings universe thermodynamic state of a system state functions 03/06/17 Presented to DR. THELMA A. ANTONIO 24
  • 25. 25 Enthalpy Change  Chemistry is commonly done in open beakers on a desk top at atmospheric pressure.  Because atmospheric pressure only changes by small increments, this is almost at constant pressure.  The enthalpy change, ∆H, is the change in heat content at constant pressure.  ∆H = qp 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 26. 26 Enthalpy Change  ∆Hrxn is the heat of reaction.  This quantity will tell us if the reaction produces or consumes heat.  If ∆Hrxn < 0 the reaction is exothermic.  If ∆Hrxn > 0 the reaction is endothermic.  ∆Hrxn = Hproducts - Hreactants  ∆Hrxn = Hsubstances produced - Hsubstances consumed  Notice that this is ∆Hrxn = Hfinal – Hinitial 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 27. Word Hunt 03/06/17 Presented to DR. THELMA A. ANTONIO 27
  • 28. 28 Calorimetry  A coffee-cup calorimeter is used to measure the amount of heat produced (or absorbed) in a reaction at constant P  This is one method to measure qP for reactions in solution. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 29. 29 Calorimetry  If an exothermic reaction is performed in a calorimeter, the heat evolved by the reaction is determined from the temperature rise of the solution.  This requires a two part calculation.  Amount of heat gained by calorimeter is called the heat capacity of the calorimeter or calorimeter constant.  The value of the calorimeter constant is determined by adding a specific amount of heat to calorimeter and measuring the temperature rise.       +      =      solutionbyabsorbed heatofAmount rcalorimetebyabsorbed heatofAmount reactionbyreleased heatofAmount 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 30. 30 Calorimetry  Example 1: When 3.425 kJ of heat is added to a calorimeter containing 50.00 g of water the temperature rises from 24.00o C to 36.54o C. Calculate the heat capacity of the calorimeter in J/o C. The specific heat of water is 4.184 J/g o C.  This is a four part calculation. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 31. 31 Calorimetry 1. Find the temperature change. 2. Find the heat absorbed by the water in going from 24.000 C to 36.540 C. ( )∆T = 36.54- 24.00 C = 12.54 C00 ( )( )( ) q mC T = 50.00 g C J 2623 J P J g C0 = = ≈ ∆ 4184 1254 262337 0 . . .03/06/17 Presented to DR. THELMA A. ANTONIO
  • 32. 32 Calorimetry 3. Find the heat absorbed by the calorimeter.  Take the total amount of heat added to calorimeter and subtract the heat absorbed by the water. 4. Find the heat capacity of the calorimeter.  (heat absorbed by the calorimeter)/(temperature change) ( ) 3425. kJ = 3425 J 3425 J - 2623 J = 802 J 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 33. 33 Calorimetry  Example 2: A coffee-cup calorimeter is used to determine the heat of reaction for the acid- base neutralization CH3COOH(aq) + NaOH(aq) → NaCH3COO(aq) + H2O() When we add 25.00 mL of 0.500 M NaOH at 23.000o C to 25.00 mL of 0.600 M CH3COOH already in the calorimeter at the same temperature, the resulting temperature is observed to be 25.947o C.03/06/17 Presented to DR. THELMA A. ANTONIO
  • 34. 34 Calorimetry The heat capacity of the calorimeter has previously been determined to be 27.8 J/0 C. Assume that the specific heat of the mixture is the same as that of water, 4.18 J/g0 C and that the density of the mixture is 1.02 g/mL. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 35. 35 Calorimetry  This is a three part calculation. 1. Calculate the amount of heat given off in the reaction. ( ) temperature change T = 25.947 - 23.000 C = 2.947 C∆ 0 0 ( ) ( )( ) temperature change T = 25.947 - 23.000 C = 2.947 C heat absorbed by calorimeter q = 2.947 C JJ C0 ∆ 0 0 0 278 819. .= ( ) ( )( ) ( ) temperature change T = 25.947 - 23.000 C = 2.947 C heat absorbed by calorimeter q = 2.947 C J mass of solution in calorimeter 25.00 mL + 25.00 mL g mL g J C0 ∆ 0 0 0 27 8 819 102 510 . . . . = = 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 36. 36 Calorimetry ( )( )( ) heat absorbed by solution q = mC T q = 51.0 g 2.947 C J total amount of heat produced by reaction q = 81.9 J + 628 J = 709.9 J J g C ∆ 418 6280 0 . =( )( )( ) heat absorbed by solution q = mC T q = 51.0 g 2.947 C JJ g C ∆ 418 6280 0 . = 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 37. 37 Calorimetry 2. Determine ∆H for the reaction under the conditions of the experiment.  We must determine the number of moles of reactants consumed which requires a limiting reactant calculation. ( ) ( ) ( ) ( ) ( ) CH COOH + NaOH NaCH COO + H O mL NaOH mmol NaOH 1 mL NaOH mmol NaCH COO 1 mmol NaOH mmol NaCH COO 3 aq aq 3 aq 2 3 3 →       ×       = l 2500 0500 1 12 5 . . . ( ) ( ) ( ) ( ) ( ) ( ) CH COOH + NaOH NaCH COO + H O mL NaOH mmol NaOH 1 mL NaOH mmol NaCH COO 1 mmol NaOH mmol NaCH COO mL CH COOH mmol CH COOH 1 mL CH COOH mmol NaCH COO 1 mmol CH COOH mmol NaCH COO 3 aq aq 3 aq 2 3 3 3 3 3 3 3 3 →       ×       =       ×       = l 25 00 0 500 1 12 5 25 00 0 600 1 15 0 . . . . . .03/06/17 Presented to DR. THELMA A. ANTONIO
  • 38. 38 Calorimetry 3. Finally, calculate the ∆Hrxn based on the limiting reactant calculation. 125 7099 56792 . . mmol = 0.0125 mol H J 0.0125 mol J / mol 56.8 kJ / molrxn∆ = = ≈ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 40. 40 Thermochemical Equations  Thermochemical equations are a balanced chemical reaction plus the ∆H value for the reaction.  For example, this is a thermochemical equation.  The stoichiometric coefficients in thermochemical equations must be interpreted as numbers of moles.  1 mol of C5H12 reacts with 8 mol of O2 to produce 5 mol of CO2, 6 mol of H2O, and releasing 3523 kJ is referred to as one mole of reactions. moles6moles5moles8mole1 kJ3523OH6CO5O8HC )(22(g)2(g))12(5 ++→+  03/06/17 Presented to DR. THELMA A. ANTONIO
  • 41. 41  This is an equivalent method of writing thermochemical equations.  ∆H < 0 designates an exothermic reaction.  ∆H > 0 designates an endothermic reaction kJ3523-HOH6CO5O8HC o rxn)(22(g)2(g))12(5 =∆+→+  03/06/17 Presented to DR. THELMA A. ANTONIO
  • 42. 42  Example 3: Write the thermochemical equation for the reaction in Example 2. You do it! ( ) ( ) ( ) ( )CH COOH + NaOH NaCH COO + H O H = -56.8 kJ / mol3 aq aq 3 aq 2→ l ∆ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 43. Timed Pair Share Answer the following problem in 2 minutes. And share it with a partner. “A sample of aluminum metal absorbs 9.86 J of heat, upon which the temperature of the sample increases from 23.2 °C to 30.5 °C. Since the specific heat capacity of aluminum is 0.90 J/g-K, the mass of the sample is __________ g.” 03/06/17 Presented to DR. THELMA A. ANTONIO 43
  • 44. 44 Standard States and Standard Enthalpy Changes  Thermochemical standard state conditions  The thermochemical standard T = 298.15 K.  The thermochemical standard P = 1.0000 atm.  Be careful not to confuse these values with STP.  Thermochemical standard states of matter  For pure substances in their liquid or solid phase the standard state is the pure liquid or solid.  For gases the standard state is the gas at 1.00 atm of pressure.  For gaseous mixtures the partial pressure must be 1.00 atm.  For aqueous solutions the standard state is 1.00 M concentration.03/06/17 Presented to DR. THELMA A. ANTONIO
  • 45. 45 Standard Molar Enthalpies of Formation, ∆Hf o  The standard molar enthalpy of formation is defined as the enthalpy for the reaction in which one mole of a substance is formed from its constituent elements.  The symbol for standard molar enthalpy of formation is ∆Hf o .  The standard molar enthalpy of formation for MgCl2 is: ( ) ( ) ( ) ( ) Mg Cl MgCl kJ H kJ / mol s 2 g 2 s f MgCl o 2 s + → + = − 6418 6418 . .∆ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 46. 46  Standard molar enthalpies of formation have been determined for many substances.  Standard molar enthalpies of elements in their most stable forms at 298.15 K and 1.000 atm are zero.  Example 4: The standard molar enthalpy of formation for phosphoric acid is -1281 kJ/mol. Write the equation for the reaction for which ∆Ho rxn = -1281 kJ. P in standard state is P4 Phosphoric acid in standard state is H3PO4(s) You do it! 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 47. 47 ( ) ( ) ( ) ( ) ( ) 3 2 1 42 1281 1281 H O P H PO kJ H kJ / mol 2 g 2 g 4 s 3 4 s f H PO o 3 4 s + + → + = −∆ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 48. 48  Example 5: Calculate the enthalpy change for the reaction of one mole of H2(g) with one mole of F2(g) to form two moles of HF(g) at 25o C and one atmosphere. ( ) ( ) ( ) ( )( ) H F HF std. state std. state std. state for this rxn. H H from Appendix K, H kJ / mol H 2 mol kJ / mol kJ 2 g 2 g g 298 o f o f o 298 o + → = = − = − = − 2 2 271 271 542 ∆ ∆ ∆ ∆ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 49. 49  Example 6: Calculate the enthalpy change for the reaction in which 15.0 g of aluminum reacts with oxygen to form Al2O3 at 25o C and one atmosphere. You do it!You do it! 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 50. 50 ( ) ( ) ( )4 Al + 3 O 2 Al O from Appendix K, H kJ / mol ? kJ = 15.0 g Al 1 mol Al 27.0 g Al mol Al O 4 mol Al kJ mol Al O kJ s 2 g 2 3 s f Al O o 2 3 2 3 2 3 → = − × × × − = − ∆ 1676 2 1676 1 466 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 51. Blackboard Share The class are grouped into five teams with four to five members. One representative from the team will pick one problem randomly. You will answer by team and one will share (and discuss) the answer to the class on the blackboard. 03/06/17 Presented to DR. THELMA A. ANTONIO 51
  • 52. Problems: 03/06/17 Presented to DR. THELMA A. ANTONIO 52 The value of for the reaction below is -72 kJ. __________ kJ of heat are released when 1.0 mol of HBr is formed in this reaction. The value of for the reaction below is -126 kJ. __________ kj are released when 2.00 mol of NaOH is formed in the reaction?
  • 53. 03/06/17 Presented to DR. THELMA A. ANTONIO 53 The value of for the reaction below is -790 kJ. The enthalpy change accompanying the reaction of 0.95 g of S is __________ kJ. The value of for the reaction below is -6535 kJ. __________ kJ of heat are released in the combustion of 16.0 g of ? The value of for the reaction below is -336 kJ. Calculate the heat (kJ) released to the surroundings when 23.0 g of HCl is formed.
  • 54. 54 Hess’s Law  Hess’s Law of Heat Summation states that the enthalpy change for a reaction is the same whether it occurs by one step or by any (hypothetical) series of steps.  Hess’s Law is true because ∆H is a state function.  If we know the following ∆Ho ’s [ ] [ ] [ ] kJ1648HOFe2O3Fe43 kJ454HFeO2OFe22 kJ560HOFe2OFeO41 o 3(s)22(g)(s) o (g)2(g)(s) o (s)322(g)(s) −=∆→+ −=∆→+ −=∆→+ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 55. 55 Hess’s Law  For example, we can calculate the ∆Ho for reaction [1] by properly adding (or subtracting) the ∆Ho ’s for reactions [2] and [3].  Notice that reaction [1] has FeO and O2 as reactants and Fe2O3 as a product.  Arrange reactions [2] and [3] so that they also have FeO and O2 as reactants and Fe2O3 as a product.  Each reaction can be doubled, tripled, or multiplied by half, etc.  The ∆Ho values are also doubled, tripled, etc.  If a reaction is reversed the sign of the ∆Ho is changed. ( ) ( ) ( ) [ ] ( ) ( ) ( ) [ ] ( ) ( ) H 2(2 FeO Fe O kJ 3 4 Fe O Fe O kJ 4 FeO O Fe O kJ 0 s s 2 g s 2 g 2 3 s s 2 g 2 3 ∆ 2 2 2 2 544 3 2 1648 1 2 560 x [ ] ) ( )− → + + + → − + → − 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 56. 56 Hess’s Law  Example 7: Given the following equations and ∆Ho values calculate ∆Ho for the reaction below. ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) H kJ 2 N O N O 164.1 [2] N + O NO 180.5 [3] N + 2 O NO 66.4 o 2 g 2 g 2 g 2 g 2 g g 2 g 2 g 2 g ∆ [ ]1 2 2 2 + → → → ( ) ( ) ( ) You do it! ?HNO3NO+ON o gg2g2 =∆→ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 57. 57 Hess’s Law  Use a little algebra and Hess’s Law to get the appropriate ∆Ho values [ ] ( ) ( ) ( ) [ ] ( ) ( ) ( ) H (kJ) N O N + O -82.05 N + O 3 NO 270.75 o 2 g 2 g 1 2 2 g 3 2 3 2 2 g 3 2 2 g g ∆ 1 2 1 2 × − → × → [ ] ( ) ( ) ( ) H (kJ) N O N + O -82.05 o 2 g 2 g 1 2 2 g ∆ 1 2 1× − →[ ] ( ) ( ) ( ) [ ] ( ) ( ) ( ) [ ] ( ) ( ) ( ) ( ) ( ) ( ) H (kJ) N O N + O -82.05 N + O 3 NO 270.75 NO N + O -33.2 N O NO 3 NO 155.5 o 2 g 2 g 1 2 2 g 3 2 3 2 2 g 3 2 2 g g 2 g 2 g 2 g 2 g 2 g g ∆ 1 2 1 2 1 2 1 2 3 × − → × → × − → + → 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 58. 58 Hess’s Law  The + sign of the ∆Ho value tells us that the reaction is endothermic.  The reverse reaction is exothermic, i.e., ( ) ( ) ( )3 NO N O + NO H = -155.5 kJg 2 g 2 g o → ∆ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 59. 59 Hess’s Law  Hess’s Law in a more useful form.  For any chemical reaction at standard conditions, the standard enthalpy change is the sum of the standard molar enthalpies of formation of the products (each multiplied by its coefficient in the balanced chemical equation) minus the corresponding sum for the reactants. tscoefficientricstoichiomen HnHnH 0 reactantsf 0 productsf 0 rxn = ∆−∆=∆ ∑∑ nn 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 60. 60 Hess’s Law  Example 8: Calculate the ∆H o 298 forthe following reaction from data in the reference. )(22(g)2(g)8(g)3 OH4CO3O5HC +→+ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 61. 61 Hess’s Law  Example 8: Calculate ∆Ho 298 for the following reaction from data in reference. ( ) ( ) ( ) ( ) ( ) ( )[ ] ( ) ( )[ ] [ ] [ ]{ } C H + 5 O CO + 4 H O H H H H H kJ 3 8 g 2 g 2 g 2 298 o f CO o f H O o f C H o f O g o 2 g 2 3 8 g 2 → = + − + = − + − − − + 3 3 4 5 3 3935 4 2858 1038 5 0 l l∆ ∆ ∆ ∆ ∆ ( . ) ( . ) ( . ) ( ) ( ) ( ) ( ) ( ) ( ) ( )[ ] ( ) ( )[ ] C H + 5 O CO + 4 H O H H H H H 3 8 g 2 g 2 g 2 298 o f CO o f H O o f C H o f O g o 2 g 2 3 8 g 2 → = + − + 3 3 4 5 l l∆ ∆ ∆ ∆ ∆ ( ) ( ) ( ) ( ) ( ) ( )[ ] ( ) ( )[ ] [ ] [ ]{ } C H + 5 O CO + 4 H O H H H H H kJ = -2211.9 kJ H kJ, and so the reaction is exothermic. 3 8 g 2 g 2 g 2 298 o f CO o f H O o f C H o f O g o 298 o 2 g 2 3 8 g 2 → = + − + = − + − − − + = − 3 3 4 5 3 3935 4 2858 1038 5 0 22119 l l∆ ∆ ∆ ∆ ∆ ∆ ( . ) ( . ) ( . ) ( ) . 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 62. 62 Hess’s Law  Application of Hess’s Law and more algebra allows us to calculate the ∆Hf o for a substance participating in a reaction for which we know ∆Hrxn o , if we also know ∆Hf o for all other substances in the reaction.  Example 9: Given the following information, calculate ∆Hf o for H2S(g). ( ) ( ) ( ) ( )2 H S + 3 O 2 SO + 2 H O H = -1124 kJ H ? 0 - 296.8 - 285.8 (kJ / mol) 2 g 2 g 2 g 2 298 o f o → l ∆ ∆ You do it!You do it! 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 63. 63 Hess’s Law ( ) ( )[ ] ( ) ( )[ ] [ ] ( )[ ]{ } ( ) ( ) ( ) ∆ ∆ ∆ ∆ ∆ ∆ ∆ ∆ ∆ H H H H H kJ H kJ now we solve for H H kJ H kJ 298 o f SO o f H O o f H S o f O o f H S o f H S o f H S o f H S o 2 g 2 2 g 2 g 2 g 2 g 2 g 2 g = + − + − = − + − − + = − = − 2 2 2 3 1124 2 2968 2 2858 2 3 0 2 412 20 6 l ( . ) ( . ( ) . . 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 64. Numbered Heads Together The class will form groups with four members. You will get a problem from the teacher. Afterwards, you are to answer and discuss with the group. Your teacher then will call randomly one representative from the group and discuss it with her/him in a corner. 03/06/17 Presented to DR. THELMA A. ANTONIO 64
  • 65. Possible Problems: 03/06/17 Presented to DR. THELMA A. ANTONIO 65 ΔH for the reaction is __________ kJ, give the data below. ΔH = -390 kJ ΔH = -745 kJ
  • 66. 03/06/17 Presented to DR. THELMA A. ANTONIO 66 Given the following reactions: ΔH = -790 kJ ΔH = -297 kJ the enthalpy of the reaction in which sulfur dioxide is oxidized to sulfur trioxide is __________ kJ.
  • 67. 03/06/17 Presented to DR. THELMA A. ANTONIO 67 Given the following reactions ΔH = 178.1 kJ ΔH = -393.5 kJ the enthalpy of the reaction is __________ kJ.
  • 68. 03/06/17 Presented to DR. THELMA A. ANTONIO 68 Given the following reactions ΔH = +180.7 kJ ΔH = -163.2 kJ the enthalpy of reaction for is __________ kJ.
  • 69. 69 Bond Energies  Bond energy is the amount of energy required to break the bond and separate the atoms in the gas phase.  To break a bond always requires an absorption of energy! ( ) ( ) ( ) ( ) ( ) ( ) A - B bond energy A + B H - Cl H + Cl g g g g kJ mol g g + → + →432 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 70. 70 Bond Energies  Table of average bond energies  Molecule Bond Energy (kJ/mol)  F2 159  Cl2 243  Br2 192  O2 (double bond) 498  N2 (triple bond) 946 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 71. 71 Bond Energies  Bond energies can be calculated from other ∆Ho 298 values. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 72. 72 Bond Energies  Bond energies can be calculated from other ∆Ho 298 values  Example 9: Calculate the bond energy for hydrogen fluoride, HF. ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( )[ ] ( )[ ] H - F BE H F atoms NOT ions H - F H F H BE H H H H g HF g g g g g 298 o HF 298 o f H o f F o f HF o g g g + → + → + = = + − or ∆ ∆ ∆ ∆ ∆ ( ) ( ) ( ) ( ) ( ) ( ) H - F BE H F atoms NOT ions H - F H F H BE g HF g g g g g 298 o HF + → + → + = or ∆ ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( )[ ] ( )[ ] [ ] [ ] H - F BE H F atoms NOT ions H - F H F H BE H H H H H kJ + 78.99 kJ kJ H kJ BE for HF g HF g g g g g 298 o HF 298 o f H o f F o f HF o 298 o 298 o g g g + → + → + = = + − = − − = ← or ∆ ∆ ∆ ∆ ∆ ∆ ∆ 218 0 271 568 0 . . 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 73. 73 Bond Energies  Example 10: Calculate the average N-H bond energy in ammonia, NH3. You do it!You do it! 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 74. 74 Bond Energies ( ) ( ) ( ) ( ) ( ) [ ] ( ) [ ] [ ] [ ]{ } bondsH-Nmol kJ H-N o 298 o 298 o NHf o Hf o Nf o 298 H-N o 298ggg3 391 3 kJ1173 BEaverage kJ1173H kJ11.46)218(3)7.472(H HH3HH BE3HH3+NNH g3gg == =∆ −−+=∆ ∆−∆+∆=∆ =∆→ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 75. 75 Bond Energies  In gas phase reactions ∆Ho values may be related to bond energies of all species in the reaction. ∆H BE BE298 o reactants products= ∑ − ∑ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 76. 76 Bond Energies  Example 11: Use the bond energies listed in the reference to estimate the heat of reaction at 25o C for the reaction below. ]BE4BE[2-]BE2BE[4H OH2COO2CH H-OOCOOH-C o 298 (g)22(g)2(g)4(g) ++=∆ +→+ == 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 78. Pairs Check By pair (pairing prepared by your teacher), one coaches his/her partner to answer the problems given by the teacher. 03/06/17 Presented to DR. THELMA A. ANTONIO 78
  • 79. Possible Problems: 03/06/17 Presented to DR. THELMA A. ANTONIO 79 G iven: H -H bond energy = 435 kJ, C l-C l bond energy = 243 kJ, and the standard heat of form ation of H C l(g) is –92 kJ/m ol, calculate the H -C l bond energy. The H0f for gaseous acetylene (shown below), is 227 kJ/mol. What is the bond energy? The bond energies are 423 kJ/mol for C–H and 436 kJ/mol for H–H. The heat of sublimation for carbon is 717 kJ/mol.
  • 80. 80 Changes in Internal Energy, ∆E  The internal energy, E, is all of the energy contained within a substance.  This function includes all forms of energy such as kinetic, potential, gravitational, electromagnetic, etc.  The First Law of Thermodynamics states that the change in internal energy, ∆E, is determined by the heat flow, q, and the work, w. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 81. 81 Changes in Internal Energy, ∆E system.by theabsorbedisheatif0q system.by theabsorbedisheatif0q wqE EEE reactantsproducts < > +=∆ −=∆∆ ∆ E = E E E = q + w products reactants− gs.surroundinon theworkdoessystemtheif0w system.on theworkdogssurroundintheif0w system.by theabsorbedisheatif0q system.by theabsorbedisheatif0q wqE EEE reactantsproducts < > < > +=∆ −=∆ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 82. 82 Changes in Internal Energy, ∆E  ∆E is negative when energy is released by a system undergoing a chemical or physical change.  Energy can be written as a product of the process. kJ103.516-E kJ103.516OH6CO5O8HC 3 3 )(22(g)2(g))(125 ×=∆ ×++→+  03/06/17 Presented to DR. THELMA A. ANTONIO
  • 83. 83 Changes in Internal Energy, ∆E  ∆E is positive when energy is absorbed by a system undergoing a chemical or physical change.  Energy can be written as a reactant of the process. kJ103.516E O8HCkJ103.516OH6CO5 3 2(g))(125 3 )(22(g) ×+=∆ +→×++  03/06/17 Presented to DR. THELMA A. ANTONIO
  • 84. 84 Changes in Internal Energy, ∆E  Example 12: If 1200 joules of heat are added to a system in energy state E1, and the system does 800 joules of work on the surroundings, what is the : 1. energy change for the system, ∆Esys? ∆ ∆ ∆ ∆ E = E - E = q + w E = 1200 J + (-800 J) E = 400 J E = + 400 J 2 1 sys03/06/17 Presented to DR. THELMA A. ANTONIO
  • 85. 85 Changes in Internal Energy, ∆E 2. energy change of the surroundings, ∆Esurr? You do it! ∆E Jsurr = −400 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 86. 86 Changes in Internal Energy, ∆E 3. energy of the system in the new state, E2? ∆ ∆ E E - E E E E E J sys 2 1 2 1 sys 1 = = + = + 400 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 87. 87 Changes in Internal Energy, ∆E  In most chemical and physical changes, the only kind of work is pressure-volume work.  Pressure is force per unit area. P = force area F d2 = 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 88. 88 Changes in Internal Energy, ∆E  Volume is distance cubed.  P∆V is a work term, i.e., the same units are used for energy and work. V = d3 ( )P V = F d d F d which is work2 3 ∆       = × ← 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 89. 89 Changes in Internal Energy, ∆E  Using the ideal gas law PV = nRT, we can look at volume changes of ideal gases at constant T and P due to changes in the number of moles of gas present, ∆ngas.  ∆ngas = (number of moles of gaseous products) - (number of moles of gaseous reactants) ( ) ( ) PV = nRT P V n RTgas∆ ∆= 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 90. 90 Changes in Internal Energy, ∆E  Work is defined as a force acting through a specified distance.  Consequently, there are three possibilities for volume changes: ( ) ( ) P.andTconstantat RTn-that wseecanweThus RTn-V-PdFw gas gas ∆= ∆=∆=×= 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 91. 91 Changes in Internal Energy, ∆E When Then Examples 1. V2 = V1 P∆V = 0 ∆ngas = 0      gasmol2 2(g)(g)2 gasmol2 (g)2(g) COHOHCO +→+ 3. V2 < V1 P∆V < 0 ∆ngas < 0 2. V2 > V1 P∆V > 0 ∆ngas > 0      gasmol1 2(g)2(aq) gasmol0 (aq)(s) HZnClHCl2Zn +→+    gasmol2 3(g) gasmol4 2(g)2(g) NH2H3N →+ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 92. 92 Changes in Internal Energy, ∆E  Consider the following gas phase reaction at constant pressure at 200o C. ( ) ( ) ( )2 NO + O 2 NOg 2 g 3 mol gas 2 g 2 mol gas       → gs.surroundinbysystemondoneisWork 0.VP-wly,Consequent 0.VPand0VthusVV 12 >∆= <∆<∆< 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 93. 93 Changes in Internal Energy, ∆E  Consider the following gas phase reaction at constant pressure at 1000o C. ( ) ( ) ( )    gasmol2 g2g3 gasmol1 g5 ClPClPCl +→ gs.surroundinon thesystemby thedoneisWork 0.VP-wly,Consequent 0.VPand0VthusVV 12 <∆= >∆>∆> 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 94. 94 Relationship of ∆H and ∆E  The total amount of heat energy that a system can provide to its surroundings at constant temperature and pressure is given by ∆H= ∆E + P ∆V  which is the relationship between ∆H and ∆E.  ∆H = change in enthalpy of system  ∆E = change in internal energy of system  P∆V = work done by system 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 95. 95 Relationship of ∆H and ∆E  At the start we defined ∆H = qP.  Here we define ∆H = ∆E + P∆V.  Are these two definitions compatible?  Remember ∆E = q + w.  We have also defined w = -P∆V .  Thus ∆E = q + w = q -P∆V  Consequently, ∆H = q- P∆V + P∆V = q  At constant pressure ∆H = qP. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 96. 96 Relationship of ∆H and ∆E  For reactions in which the volume change is very small or equal to zero. E.H change,volumenoFor E.H thenVPEHSince 0.VPand0V changes,volumesmallFor ∆=∆ ∆≈∆ ∆+∆=∆ ≈∆≈∆ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 97. 97 Relationship of ∆H and ∆E  Change in enthalpy, ∆H, or heat of reaction is amount of heat absorbed or released when a reaction occurs at constant pressure.  The change in energy, ∆E, is the amount of heat absorbed or released when a reaction occurs at constant volume.  How much do the ∆H and ∆E for a reaction differ?  The difference depends on the amount of work performed by the system or the surroundings. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 98. 98 Relationship of ∆H and ∆E  Example 13: Noted that ∆Ho = -3523 kJ/mol for the combustion of n-pentane, n-C5H12. Combustion of one mol of n-pentane at constant pressure releases 3523 kJ of heat. What are the values of the work term and ∆E for this reaction? )(22(g)2(g))12(5 OH6CO5O8HC  +→+ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 99. 99 Relationship of ∆H and ∆E  Determine the work done by this reaction. You do it!You do it! kJ7.433J7433K)298)(mol)(8.314-(-3w mol3-mol85n RT)n(-VP-w K.298TthatknowwekJ/mol,3523-HSince OH6CO5O8HC Kmol J gas gas o gasmol5 )(22(g) gasmol8 2(g))12(5 === =−=∆ ∆=∆= ==∆ +→+       03/06/17 Presented to DR. THELMA A. ANTONIO
  • 100. 100 Relationship of ∆H and ∆E  Now calculate the ∆E for this reaction from the values of ∆H and w that we have determined. You do it!You do it! ∆ ∆ ∆ ∆ ∆ ∆ ∆ ∆ ∆ H E + P V E = H - P V since w = - P V = 7.433 kJ then P V = - 7.433 kJ E = - 3523 kJ - (-7.433 kJ) = -3516 kJ = ∴ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 101. Journal Reflection In your journal, try to reflect whether the following is spontaneous or not and justify your answer. And go back to your journal after tackling the next topic on spontaneity of physical and chemical changes. Spreading of the fragrance of perfume throughout the room 03/06/17 Presented to DR. THELMA A. ANTONIO 101
  • 102.  Separation of nitrogen and oxygen molecules in air  Fixing of a broken watch  Extraction of salt from seawater 03/06/17 Presented to DR. THELMA A. ANTONIO 102
  • 103. 103 Spontaneity of Physical and Chemical Changes  Spontaneous changes happen without any continuing outside influences.  A spontaneous change has a natural direction.  For example the rusting of iron occurs spontaneously.  Have you ever seen rust turn into iron metal without man made interference?  The melting of ice at room temperature occurs spontaneously.  Will water spontaneously freeze at room temperature?03/06/17 Presented to DR. THELMA A. ANTONIO
  • 104. 104 The Two Aspects of Spontaneity  An exothermic reaction does not ensure spontaneity.  For example, the freezing of water is exothermic but spontaneous only below 0o C.  An increase in disorder of the system also does not insure spontaneity.  It is a proper combination of exothermicity and disorder that determines spontaneity. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 105. 105 The Second Law of Thermodynamics  The second law of thermodynamics states, “In spontaneous changes the universe tends towards a state of greater disorder.”  Spontaneous processes have two requirements: 1. The free energy change of the system must be negative. 2. The entropy of universe must increase.  Fundamentally, the system must be capable of doing useful work on surroundings for a spontaneous process to occur. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 106. Draw-it By group of three members, make a poster on the following scenario. Afterwards, determine if its “disorder” increases or decreases. A football stadium empties after a game A baby develops into an adult Paper, plastics, and aluminum are separated and recycled 03/06/17 Presented to DR. THELMA A. ANTONIO 106
  • 107. 107 Entropy, S  Entropy is a measure of the disorder or randomness of a system.  As with ∆H, entropies have been measured and tabulated in Appendix K as So 298.  When:  ∆S > 0 disorder increases (which favors spontaneity).  ∆S < 0 disorder decreases (does not favor spontaneity). 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 108. 108 Entropy, S  From the Second Law of Thermodynamics, for a spontaneous process to occur:  In general for a substance in its three states of matter: Sgas> Sliquid > Ssolid 0SSS gssurroundinsystemuniverse >∆+∆=∆ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 109. 109 Entropy, S  The Third Law of Thermodynamics states, “The entropy of a pure, perfect, crystalline solid at 0 K is zero.”  This law permits us to measure the absolute values of the entropy for substances.  To get the actual value of S, cool a substance to 0 K, or as close as possible, then measure the entropy increase as the substance heats from 0 to higher temperatures. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 110. 110 Entropy, S  Entropy changes for reactions can be determined similarly to ∆H for reactions. o reactants n o products n o 298 SnSnS ∑∑ −=∆ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 111. 111 Entropy, S  Example 14: Calculate the entropy change for the following reaction at 25o C. You do it! ←→ 4(g)22(g) ONNO2 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 112. 112 Entropy, S Kmol kJ Kmol J Kmol J Kmol J o NO o ON o reactants n o products n o rxn 4(g)22(g) 0.1758-or8.175 )0.240(2)2.304( S2S SnSnS ONNO2 2(g)4(g)2 −= −= −= −=∆ ←→ ∑∑  The negative sign of ∆S indicates that the system is more ordered.  If the reaction is reversed the sign of ∆S changes.  For the reverse reaction ∆So 298= +0.1758 kJ/K  The + sign indicates the system is more disordered.03/06/17 Presented to DR. THELMA A. ANTONIO
  • 113. 113 Entropy, S  Example 15: Calculate ∆So 298 for the reaction below. ( ) ( ) ( ) You do it! ← +→ g2g2g NOONNO3 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 114. 114 Entropy, S ( ) ( ) ( ) ( ) ( ) ( ) ( )[ ] Kmol kJ Kmol J Kmol J 0 NO 0 NO 0 ON 0 298 g2g2g 0.1724-or4.172 210.43-240.07.219 S3SSS NOONNO3 gg2g2 −= += −+=∆ ← +→  Changes in ∆S are usually quite small compared to ∆E and ∆H.  Notice that ∆S has units of only a fraction of a kJ while ∆E and ∆H values are much larger numbers of kJ.03/06/17 Presented to DR. THELMA A. ANTONIO
  • 115. Hands-on Learning (Laboratory) 03/06/17 Presented to DR. THELMA A. ANTONIO 115
  • 116. 116 Free Energy Change, ∆G, and Spontaneity  In the mid 1800’s J. Willard Gibbs determined the relationship of enthalpy, H, and entropy, S, that best describes the maximum useful energy obtainable in the form of work from a process at constant temperature and pressure.  The relationship also describes the spontaneity of a system.  The relationship is a new state function, ∆G, the Gibbs Free Energy. ∆ ∆ ∆G = H - T S (at constant T & P)03/06/17 Presented to DR. THELMA A. ANTONIO
  • 117. 117 Free Energy Change, ∆G, and Spontaneity  The change in the Gibbs Free Energy, ∆G, is a reliable indicator of spontaneity of a physical process or chemical reaction.  ∆G does not tell us how quickly the process occurs.  Chemical kinetics, the subject of Chapter 16, indicates the rate of a reaction.  Sign conventions for ∆G.  ∆G > 0 reaction is nonspontaneous  ∆G = 0 system is at equilibrium  ∆G < 0 reaction is spontaneous 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 118. 118 Free Energy Change, ∆G, and Spontaneity  Changes in free energy obey the same type of relationship we have described for enthalpy, ∆H, and entropy, ∆S, changes. 0 reactants n 0 products n 0 298 GnGnG ∆−∆=∆ ∑∑ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 119. 119 Free Energy Change, ∆G, and Spontaneity  Example16: Calculate ∆Go 298 for the reaction in Example 8. You do it! )(22(g)2(g))8(3 OH4CO3O5HC  +→+ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 120. 120 Free Energy Change, ∆G, and Spontaneity  ∆Go 298< 0, so the reaction is spontaneous at standard state conditions.  If the reaction is reversed:  ∆Go 298> 0, and the reaction is nonspontaneous at standard state conditions. mol kJ mol kJ o Of o HCf o OHf o COf o rxn )(22(g)2(g)8(g)3 5.2108 )]}0(5)49.23[()3.237(4)4.394(3{[ ]G5G[]G4G3[G OH4CO3O5HC 2(g)(g)83)(22(g) −= +−−−+−= ∆+∆−∆+∆=∆ +→+   03/06/17 Presented to DR. THELMA A. ANTONIO
  • 121. Impersonation By team, one member impersonates the life and works of J. Willard Gibbs. Other members may act as support characters. Then, present it to the class. 03/06/17 Presented to DR. THELMA A. ANTONIO 121
  • 122. 122 The Temperature Dependence of Spontaneity  Free energy has the relationship ∆G = ∆H -T∆S.  Because 0 ≤ ∆H ≥ 0 and 0 ≤ ∆S ≥ 0, there are four possibilities for ∆G. ∆H ∆S ∆G Forward reaction spontaneity < 0 > 0 < 0 Spontaneous at all T’s. < 0 < 0 T dependent Spontaneous at low T’s. > 0 > 0 T dependent Spontaneous at high T’s. > 0 < 0 > 0 Nonspontaneous at all T’s. 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 123. 123 The Temperature Dependence of Spontaneity 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 124. 124 The Temperature Dependence of Spontaneity  Example 17: Calculate ∆So 298 for the following reaction. In example 8, we found that ∆Ho 298= -2219.9 kJ, and in Example 16 we found that ∆Go 298= -2108.5 kJ. o oo ooo ooo )(22(g)2(g))12(5 S T GH STGH STHG OH6CO5O8HC ∆= ∆−∆ ∆=∆−∆ ∆−∆=∆ +→+  ( )[ ] K J-374 K kJ374.0S K298 kJ5.21089.2219 S o o =−=∆ −−− =∆ 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 125. 125 The Temperature Dependence of Spontaneity  ∆So 298= -374 J/K which indicates that the disorder of the system decreases .  For the reverse reaction, 3 CO2(g) + 4 H2O(g)→ C3H8(g) + 5 O2(g)  ∆So 298= +374 J/K which indicates that the disorder of the system increases . 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 126. 126 The Temperature Dependence of Spontaneity  Example 18: Use thermodynamic data to estimate the normal boiling point of water. S H TandSTHThus 0.GprocessequlibriumanisthisBecause OHOH (g)2)(2 ∆ ∆ =∆=∆ =∆ ←→  03/06/17 Presented to DR. THELMA A. ANTONIO
  • 127. 127 The Temperature Dependence of Spontaneity [ ] assume H@BP H H H H H H kJ@25 C 298 o o H O o H O o o J K o o 2 (g) 2 ( ) ∆ ∆ ∆ ∆ ∆ ∆ ∆ ≈ = − = − − − = + l 2418 2858 44 0 . ( . ) .03/06/17 Presented to DR. THELMA A. ANTONIO
  • 128. 128 The Temperature Dependence of Spontaneity ( ) ( ) [ ] K kJ K J0 rxn K J0 rxn 0 OH 0 OH 0 rxn 0 rxn 0.1188or8.118S 91.697.188S SSS SBP@Sassume 2g2 =∆ −=∆ −=∆ ∆≈∆  03/06/17 Presented to DR. THELMA A. ANTONIO
  • 129. 129 The Temperature Dependence of Spontaneity T = H S H S .0 kJ 0.1188 K 370 K -273 K = 97 C o o kJ K o ∆ ∆ ∆ ∆ ≈ = = 44 370 03/06/17 Presented to DR. THELMA A. ANTONIO
  • 130. Act-Like-a-Teacher Review the problems given in the next slides. If you are confident with your answer in any of the given, volunteer to the class and discuss it like a teacher. 03/06/17 Presented to DR. THELMA A. ANTONIO 130
  • 131. Problems 03/06/17 Presented to DR. THELMA A. ANTONIO 131 For w hich set of values of ∆ H and ∆ S w ill a reaction be spontaneous (product-favored) at all temperatures? (a) ∆ H = +10 kJ, ∆ S = –5 J/K (b) ∆ H = –10 kJ, ∆ S = –5 J/K (c) ∆ H = –10 kJ, ∆ S = +5 J/K (d) ∆ H = +10 kJ, ∆ S = +5 J/K (e) no such values exist
  • 132. 03/06/17 Presented to DR. THELMA A. ANTONIO 132 Joseph Priestley prepared oxygen by heating mercury(II) oxide. The compound H gO is stable at room temperature but decomposes into its elements (H g and O 2) at high temperatures. W hat conclusio ns can be draw n concerning ∆ H and ∆ S for this decompositio n reaction? (a) ∆ H is negative and ∆ S is positive. (b) ∆ H is negative and ∆ S is negative. (c) ∆ H is positive and ∆ S is positive. (d) ∆ H is positive and ∆ S is negative. (e) ∆ H becomes negative at high temperatures.
  • 133. 03/06/17 Presented to DR. THELMA A. ANTONIO 133 The follow ing reaction is spontaneous only below 5000 K . W hat conclusio ns can be draw n regarding this reaction? A + B  A B (a) ∆ H is negative and ∆ S is positive. (b) ∆ H is negative and ∆ S is negative. (c) ∆ H is positive and ∆ S is positive. (d) ∆ H is positive and ∆ S is negative. (e) C an’t conclude anything.
  • 134. 03/06/17 Presented to DR. THELMA A. ANTONIO 134 For a certain process at 127°C , ∆ G = –16.20 kJ and ∆ H = –17.0 kJ. W hat is the entropy change for this process at this temperature? Express your answ er in the form, ∆ S = _______________ J/K . (a) –6.3 J/K (b) +6.3 J/K (c) –2.0 J/K (d) +2.0 J/K (e) –8.1 J/K
  • 135. 03/06/17 Presented to DR. THELMA A. ANTONIO 135 For the follow ing reaction, ∆ H o = -104.9 kJ/mol. If this reaction is spontaneous at all temperatures below 361 K , w hat is the value of ∆ So ? (a) -165 J/mol•K (b) –0.291 J/mol•K (c) 3.44 J/mol•K (d) -291 J/mol•K (e) 3.44 kJ
  • 136. 03/06/17 Presented to DR. THELMA A. ANTONIO 136 Estim ate the tem perature above w hich this reaction is spontaneous. ∆ S0 = 16.1 J/K . C H 4(g) + N 2(g) + 163.8 kJ → H C N (g) + N H 3(g) (a) 9.91°C (b) 1045 K (c) 9.90 x 103°C (d) 10.7 K (e) 10.1°C
  • 137. 03/06/17 Presented to DR. THELMA A. ANTONIO 137 Fora particular reaction at25 o C,∆Ho = -297 kJ/mol, and ∆So = -113.3 J/mol•K . Atwhich ofthe follow ing temperatures would the reaction spontaneous? (a)2750 K (b)3250 K (c) 2450 K (d) 10500 K (e) 3750 K
  • 138. Synthesis Finally, after dealing with the concepts on the heat changes and thermochemistry and the spontaneity of physical and chemical changes, create an MI project mode by group according to your MI profile. On the other side, prior to that, read in the class the following free verse poem as starter. 03/06/17 Presented to DR. THELMA A. ANTONIO 138
  • 139. POST-TEST Congratulations! You finished the module tapping your multiple intelligences. This time, check yourself again on your mastery on the Thermodynamics concepts and problems. God bless you! 03/06/17 Presented to DR. THELMA A. ANTONIO 139
  • 140. Answer to the Post-Test 03/06/17 Presented to DR. THELMA A. ANTONIO 140
  • 141. REFERENCES  Antero, ES., et al. Conceptual and Functional Chemistry. 2010. Vibal Publishing House, 1253 G. Araneta Ave., Quezon City  LeMAy, H.E., et al. Chemistry: Connection to our Changing World. 2002. Prentice-Hall, Inc. New Jersey 03/06/17 Presented to DR. THELMA A. ANTONIO 141
  • 142.  White, David P. Chemistry: The Central Science. 9th ed. 2003. Prentice-Hall, Inc. New Jersey 03/06/17 Presented to DR. THELMA A. ANTONIO 142