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Chapter 16
Spontaneity, Entropy
and Free Energy
DE Chemistry
Dr. Walker
Thermodynamics: the study of energy and
its transformations
Thermochemistry: the sub discipline involving
chemical reactions and
energy changes
Laws Of Thermodynamics
• The first law of thermodynamics is a
statement of the law of conservation of
energy:
– Energy can be neither created nor destroyed. In
other words, the energy of the universe is
constant.
Energy in Chemical Reactions
• The potential energy is broken in chemical
bonds in compounds A and B
• The potential energy is the chemical bonds of
C and D is lower
– The excess has been given off (energy) as thermal
energy, or heat, which is kinetic energy transferred
to the surroundings
A + B C + D + Energy
In endothermic processes, heat is _________ by
the system.
absorbed
melting
boiling
sublimation
released
freezing
condensation
deposition
In exothermic processes, heat is ________ by
the system.
• Exothermic process is any process that gives off heat –
The energy will be listed as a product.
2H2 (g) + O2 (g) 2H2O (l) + energy
H2O (g) H2O (l) + energy
Endothermic process is any process in which heat is
required by the system. The energy is listed as a reactant.
energy + 2HgO (s) 2Hg (l) + O2 (g)
energy + H2O (s) H2O (l)
ΔH = Hproducts – Hreactants
When ΔH is +, the system... has gained heat.
When ΔH is –, the system... has lost heat.
(ENDO)
(EXO)
Enthalpy is used to measure the heat that is
either gained or lost by a system that is at
constant pressure.
• Enthalpy is an extensive property, meaning that…the amount
of material affects its value
Enthalpy (H)
H2O (s) H2O (l) ΔH = 6.01 kJ/mol ΔH = 6.01 kJ
Thermochemical Equations
If you reverse a reaction, the sign of ΔH changes
H2O (l) H2O (s) ΔH =- 6.01 kJ
Spontaneity
• Spontaneous Processes
• Processes that occur without outside
intervention
• Spontaneous processes may be fast or
slow
–Many forms of combustion are fast
–Conversion of graphite to diamond is
slow
–Kinetics is concerned with speed,
thermodynamics with the initial and
final state
Spontaneous or Non-spontaneous?
Entropy (S)
• A measure of the randomness or disorder
• The driving force for a spontaneous process is an increase in
the entropy of the universe (one of the laws of
thermodynamics!)
– The universe favors chaos!!
• Entropy is a thermodynamic function describing the number
of arrangements that are available to a system
• Nature proceeds towards the states that have the highest
probabilities of existing
Second Law of Thermodynamics
 "In any spontaneous process there is
always an increase in the entropy of the
universe"
 "The entropy of the universe is
increasing"
 For a given change to be spontaneous,
Suniverse must be positive
Suniv = Ssys + Ssurr
Positional Entropy
 The probability of occurrence of a particular
state depends on the number of ways
(microstates) in which that arrangement can
be achieved
Ssolid < Sliquid << Sgas
Entropy and Temperature
• Entropy changes in the surrounding are
primarily determined by heat flow
• The magnitude of entropy is dependent on
the temperature
• The lower the temperature, the higher the
impact to the surroundings of the transfer of
energy
Suniv = Ssys + Ssurr
Entropy and Exothermic Processes
• Entropy and a process being exothermic are
related, but a process doesn’t have to be both
• Exothermic process
– Ssurr = positive, exothermic = more disorder in
surroundings
• Endothermic process
– Ssurr = negative, endothermic = less disorder in
surroudings
– ssystem must increease to obey 2nd Law of
Thermodynamics
More on Entropy
• Why is the sign different?
–The enthalpy (H) concerns the system
–Our entropy here concerns the
surroundings
–As usual, temperatures must be in Kelvin
Example
Example
• 1st reaction
• H = -125 kJ, 25 oC + 273 = 298 K
• Ssurr = -125 kJ/298 K = 419 J/K
• Remember 125 kJ = 125000 J
• ssurr is positive, calculation refers
to system!
Example
• 2nd reaction
• H = 778 kJ, 25 oC + 273 = 298 K
• S = 778 kJ/298 K = -2.61 kJ/K
• Remember 778 kJ = 778000 J
Free Energy, G
• Typically defined as the energy available to
perform work
• G determines whether a process is spontaneous
or not (G = negative = spontaneous)
– Takes into account enthalpy, entropy, and
temperature
– Symbol honors Josiah Gibbs (sometimes called Gibbs
Free Energy or Gibbs energy), a physics professor at
Yale during the late 1800’s who was important in
developing much of modern thermodynamics
G = H - TS
Energy Diagrams
• Left – A spontaneous reaction
– The products have a lower free energy (G) than the
reactants (G < 0)
• Right – A nonspontaneous reaction
– The reactants have a higher free energy than the products
(G > 0)
What If?
• G = 0?
– The reaction is at equilibrium
• As a result
G < 0 The reaction is spontaneous.
G > 0 The reaction is nonspontaneous.
G = 0 The reaction mixture is at equilibrium.
-It’s not moving forward or reverse overall – mult
processes, same speed
Dependence on Temperature
• Notice there are two terms in the equation
– Spontaneity can change when the temperature
changes.
– Temperature and spontaneity are not necessarily
correlated.
• A reaction with a negative entropy (loss of
randomness) would be LESS spontaneous at higher
temperatures – it doesn’t want to happen, but is
pushed by the extra heat.
G = H - TS
Reaction Rates
• Free energy (G) values tell us if reactions will
occur
• They do not tell us how fast reactions will
occur.
• During a reaction
– Reactant particles must physically collide
– They must collide with enough energy to break
the bonds in the reactant
• Some reactions require the addition of heat energy.
This gives the reactants the extra energy needed (more
collisions, harder collisions) for this process to occur.
H, S, G and Spontaneity
Value of
H
Value of
TS
Value of
G
Spontaneity
Negative Positive Negativ
e
Spontaneous
Positive Negative Positive Nonspontaneous
Negative Negative ??? Spontaneous if the absolute
value of H is greater than
the absolute value of TS
(low temperature)
Positive Positive ??? Spontaneous if the absolute
value of TS is greater than
the absolute value of H
(high temperature)
G = H - TS
H is enthalpy, T is Kelvin temperature
Example of Gibbs Energy
• For the reaction at 298 K, the values of H and
S are 58.03 kJ and 176.6 J/K, respectively.
What is the value of G at 298 K?
Example of Gibbs Energy
• For the reaction at 298 K, the values of H and
S are 58.03 kJ and 176.6 J/K, respectively.
What is the value of G at 298 K?
G = H - TS
G = 58.03 kJ – (298 K)(176.6 J/K)
G = 5.40 kJ Not spontaneous at
this temperature
Second Example
Calculate the standard free-energy change at 25 oC
for the Haber synthesis of ammonia using the given
values for the standard enthalpy and standard
entropy changes:
So = 198.7 J/K
2NH3(g)
N2(g) + 3H2(g) Ho = 92.2 kJ
Second Example
Calculate the standard free-energy change at 25 oC
for the Haber synthesis of ammonia using the given
values for the standard enthalpy and standard
entropy changes:
So = 198.7 J/K
2NH3(g)
N2(g) + 3H2(g) Ho = 92.2 kJ
G = H  TS
G = 92.2 kJ  (298 K)(-198.7 J/K)(1 kJ/1000 J)
= -33.0 kJ
Third Example
• Iron metal can be produced by reducing
iron(III) oxide with hydrogen:
• Fe2O3(s) + 3 H2(g)  2 Fe(s) + 3 H2O(g)
H = +98.8 kJ; S = +141.5 J/K
• (a) Is this reaction spontaneous under
standard-state conditions at 25 °C?
• (b) At what temperature will the reaction
become spontaneous?
Third Example
• To determine whether the reaction is spontaneous
at 25 °C, we need to determine the sign of G =
H  TS. At 25 C (298 K), G for the reaction is
• G = H  TS = (98.8 kJ)  (298 K)(0.1415 kJ/K)
• = (98.8 kJ)  (42.2 kJ)
• = 56.6 k
• Reaction is NOT spontaneous!
Third Example
• At temperatures above 698 K, the TS term
becomes larger than H, making the Gibbs
energy negative and the process spontaneous
• Why is this postive this time?
– Remember, here we’re dealing with the system,
not the surroundings!
At what temperature does this become spontaenous?
Entropy Changes in Chemical
Reactions
• Constant Temperature and Pressure
–Reactions involving gaseous molecules
• The change in positional entropy is dominated
by the relative numbers of molecules of
gaseous reactants and products
Typically, more moles of gas, more entropy
Third Law of Thermodynamics
• "The entropy of a perfect crystal at O K is
zero" (NO disorder, since everything is in
perfect position)
–No movement = 0 K
–No disorder = no entropy (S = 0)
Standard State Conditions
• We’ve seen that quantities such as entropy
(S), enthalpy (H), and free energy (G) are
dependent upon the conditions present
• Standard State
– One set of conditions at which quantities can be
compared
• Pure solids/liquids/gases at 1 atm pressure
• Solutes at 1 M concentration
• Typically @ 25 oC (298 K)
• Designated by o sign (similar to degree sign)
Calculating Entropy Change in a
Reaction
0 0 o
reaction products reactants
p r
S n S n S
  
 
 Calculates standard entropy of a reaction,
uses standard entropies of compounds
 Entropy is an extensive property (a function
of the number of moles)
 Generally, the more complex the molecule, the
higher the standard entropy value
Calculating Standard Entropy -
Example
Calculating Standard Entropy -
Example
• 2 (28 J/Kmol) + 3 (189 J/Kmol) – 51 J/K mole – 3
(131 J/Kmol) = 179 J/K
• System gained entropy – water more complex
than hydrogen!
0 0 o
reaction products reactants
p r
S n S n S
  
 
Second Example
• Evaluate the entropy change for the reaction:
CO + 3 H2 -> CH4 + H2O
in which all reactants and products are gaseous.
So values: CO 198 J/Kmol
H2 131 J/Kmol
CH4 186 J/Kmol
H2O 189 J/Kmol
Second Example
• Evaluate the entropy change for the reaction:
CO + 3 H2 -> CH4 + H2O
in which all reactants and products are gaseous.
So values: CO 198 J/Kmol
H2 131 J/Kmol
CH4 186 J/Kmol
H2O 189 J/Kmol
s
oreaction = [186 + 189] – [198 + 3(131)] = 216 J/Kmol
Standard Free Energy Change
• G0 is the change in free energy that will occur
if the reactants in their standard states are
converted to the products in their standard
states
– G0 cannot be measured directly
– The more negative the value for G0, the farther to
the right the reaction will proceed in order to
achieve equilibrium
– Equilibrium is the lowest possible free energy
position for a reaction
Calculating Free Energy of Formation
Using standard free energy of formation (Gf
0):
0 0 0
(products) (reactants)
p f r f
G n G n G
    
 
Gf
0 of an element in its standard state is zero!
Calculating Free Energy of Formation -
Example
Calculating Free Energy of Formation -
Example
• 2 (-394kJ/mol) + 4 (-229 kJ/mol) – 2 (-163
kJ/mol) – 3 (0) = - 1378 kJ
0 0 0
(products) (reactants)
p f r f
G n G n G
    
 
Second Example
• Calculate the standard free energy for the
reaction below and determine whether it is
spontaneous at standard conditions.
Fe2O3(s) + 3 CO (g) 2 Fe (s) + 3 CO2(g)
Go = -742.2 -137.2 0 -394.4
Second Example
• Calculate the standard free energy for the
reaction below and determine whether it is
spontaneous at standard conditions.
Fe2O3(s) + 3 CO (g) 2 Fe (s) + 3 CO2(g)
Go (kJ/mol)= -742.2 -137.2 0 -394.4
Go = [0 + (3 x -394.4)] – [-742.2 + (3 x -137.2)] =
-29.4 kJ/mol
Additional Note on Energies of
Formation
• Examples on enthalpy are not shown, but
could be calculated the same way.
• There are numerous other possibilities for
calculating these
– Another type of problem could be where Ho and
So values are given --- you find Ho
reaction and
So
reaction, then plug in to get Go
reaction
The Dependence of Free Energy on Pressure
Enthalpy, H, is not pressure dependent
Entropy, S
 entropy depends on volume, so it also depends
on pressure
Slarge volume > Ssmall volume
Slow pressure > Shigh pressure
Free Energy and Equilibrium
• R = Universal gas constant = 8.314 J/K mol
• T = Temperature in Kelvin
• K = Equilibrium constant = [Pproducts]/[Preactants]
• System is at equilbrium (no net movement)
when Go = 0 (K = 1)
• If the system is NOT at equilibrium, use Q
instead of K
G = Go + RTln(Q)
Go = -RTln(K) at equilibrium
Example
• For the synthesis of ammonia where Go =
-33.3 kJ/mole, determine whether the reaction is
spontaneous at 25 C with the following pressures:
PN2 = 1.0 atm, PH2 = 3.0 atm, PNH3 = 0.020 atm
Example
• For the synthesis of ammonia where Go =
-33.3 kJ/mole, determine whether the reaction is
spontaneous at 25 C with the following pressures:
PN2 = 1.0 atm, PH2 = 3.0 atm, PNH3 = 0.020 atm
G = Go + RTln(Q)
G = -33.3 kJ/mole + (8.314 J/K mol)(298 K) ln( [0.02 atm]2 )
___________________
[1.0 atm][3.0 atm]3
G = -33.3 kJ/mole + (8.314 J/K mol)(298 K) ln(1.5 x 10-5)
G = -60.5 kJ/mol
Example
• The synthesis of methanol from carbon
dioxide and hydrogen has a Go = -25.1
kJ/mol. What is the value of the equilibrium
constant at 25 oC?
Example
• The synthesis of methanol from carbon
dioxide and hydrogen has a Go = -25.1
kJ/mol. What is the value of the equilibrium
constant at 25 oC?
G = Go + RTln(K)
Go = - RTln(K)
-25.1 kJ/mol = -(8.314 J/molK)(298)lnK
Solve for ln K = 10.1, K = 2 x 104
Example
• At 298 K, Go = -5.40 kJ/mole. Give the
equilibrium K for this process.
Example
• At 298 K, Go = -5.40 kJ/mole. Give the
equilibrium constant K for this process.
• Go = -RTln(K)
• -5.40 kJ/mole = -(8.31 J/K mol)(298 K)ln K
• 2.18 = ln K
• 8.85 = K
Free Energy and Work
• The maximum possible useful work obtainable
from a process at constant temperature and
pressure is equal to the change in free energy
• The amount of work obtained is always less the
maximum
– Work is changed to heat in surroudings – You lose
efficiency, but the Ssurr increases (favorable!)
• Henry’s Bent’s First Two Laws of Thermodynamics
– 1st Law: You can’t win, you can only break even
– 2nd Law: You can’t break even

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entropy-and-gibbs-free-energy.ppt

  • 1. Chapter 16 Spontaneity, Entropy and Free Energy DE Chemistry Dr. Walker
  • 2. Thermodynamics: the study of energy and its transformations Thermochemistry: the sub discipline involving chemical reactions and energy changes
  • 3. Laws Of Thermodynamics • The first law of thermodynamics is a statement of the law of conservation of energy: – Energy can be neither created nor destroyed. In other words, the energy of the universe is constant.
  • 4. Energy in Chemical Reactions • The potential energy is broken in chemical bonds in compounds A and B • The potential energy is the chemical bonds of C and D is lower – The excess has been given off (energy) as thermal energy, or heat, which is kinetic energy transferred to the surroundings A + B C + D + Energy
  • 5. In endothermic processes, heat is _________ by the system. absorbed melting boiling sublimation released freezing condensation deposition In exothermic processes, heat is ________ by the system.
  • 6. • Exothermic process is any process that gives off heat – The energy will be listed as a product. 2H2 (g) + O2 (g) 2H2O (l) + energy H2O (g) H2O (l) + energy Endothermic process is any process in which heat is required by the system. The energy is listed as a reactant. energy + 2HgO (s) 2Hg (l) + O2 (g) energy + H2O (s) H2O (l)
  • 7.
  • 8.
  • 9. ΔH = Hproducts – Hreactants When ΔH is +, the system... has gained heat. When ΔH is –, the system... has lost heat. (ENDO) (EXO) Enthalpy is used to measure the heat that is either gained or lost by a system that is at constant pressure. • Enthalpy is an extensive property, meaning that…the amount of material affects its value
  • 11. H2O (s) H2O (l) ΔH = 6.01 kJ/mol ΔH = 6.01 kJ Thermochemical Equations If you reverse a reaction, the sign of ΔH changes H2O (l) H2O (s) ΔH =- 6.01 kJ
  • 12. Spontaneity • Spontaneous Processes • Processes that occur without outside intervention • Spontaneous processes may be fast or slow –Many forms of combustion are fast –Conversion of graphite to diamond is slow –Kinetics is concerned with speed, thermodynamics with the initial and final state
  • 14. Entropy (S) • A measure of the randomness or disorder • The driving force for a spontaneous process is an increase in the entropy of the universe (one of the laws of thermodynamics!) – The universe favors chaos!! • Entropy is a thermodynamic function describing the number of arrangements that are available to a system • Nature proceeds towards the states that have the highest probabilities of existing
  • 15. Second Law of Thermodynamics  "In any spontaneous process there is always an increase in the entropy of the universe"  "The entropy of the universe is increasing"  For a given change to be spontaneous, Suniverse must be positive Suniv = Ssys + Ssurr
  • 16. Positional Entropy  The probability of occurrence of a particular state depends on the number of ways (microstates) in which that arrangement can be achieved Ssolid < Sliquid << Sgas
  • 17. Entropy and Temperature • Entropy changes in the surrounding are primarily determined by heat flow • The magnitude of entropy is dependent on the temperature • The lower the temperature, the higher the impact to the surroundings of the transfer of energy Suniv = Ssys + Ssurr
  • 18. Entropy and Exothermic Processes • Entropy and a process being exothermic are related, but a process doesn’t have to be both • Exothermic process – Ssurr = positive, exothermic = more disorder in surroundings • Endothermic process – Ssurr = negative, endothermic = less disorder in surroudings – ssystem must increease to obey 2nd Law of Thermodynamics
  • 19. More on Entropy • Why is the sign different? –The enthalpy (H) concerns the system –Our entropy here concerns the surroundings –As usual, temperatures must be in Kelvin
  • 21. Example • 1st reaction • H = -125 kJ, 25 oC + 273 = 298 K • Ssurr = -125 kJ/298 K = 419 J/K • Remember 125 kJ = 125000 J • ssurr is positive, calculation refers to system!
  • 22. Example • 2nd reaction • H = 778 kJ, 25 oC + 273 = 298 K • S = 778 kJ/298 K = -2.61 kJ/K • Remember 778 kJ = 778000 J
  • 23. Free Energy, G • Typically defined as the energy available to perform work • G determines whether a process is spontaneous or not (G = negative = spontaneous) – Takes into account enthalpy, entropy, and temperature – Symbol honors Josiah Gibbs (sometimes called Gibbs Free Energy or Gibbs energy), a physics professor at Yale during the late 1800’s who was important in developing much of modern thermodynamics G = H - TS
  • 24. Energy Diagrams • Left – A spontaneous reaction – The products have a lower free energy (G) than the reactants (G < 0) • Right – A nonspontaneous reaction – The reactants have a higher free energy than the products (G > 0)
  • 25. What If? • G = 0? – The reaction is at equilibrium • As a result G < 0 The reaction is spontaneous. G > 0 The reaction is nonspontaneous. G = 0 The reaction mixture is at equilibrium. -It’s not moving forward or reverse overall – mult processes, same speed
  • 26. Dependence on Temperature • Notice there are two terms in the equation – Spontaneity can change when the temperature changes. – Temperature and spontaneity are not necessarily correlated. • A reaction with a negative entropy (loss of randomness) would be LESS spontaneous at higher temperatures – it doesn’t want to happen, but is pushed by the extra heat. G = H - TS
  • 27. Reaction Rates • Free energy (G) values tell us if reactions will occur • They do not tell us how fast reactions will occur. • During a reaction – Reactant particles must physically collide – They must collide with enough energy to break the bonds in the reactant • Some reactions require the addition of heat energy. This gives the reactants the extra energy needed (more collisions, harder collisions) for this process to occur.
  • 28. H, S, G and Spontaneity Value of H Value of TS Value of G Spontaneity Negative Positive Negativ e Spontaneous Positive Negative Positive Nonspontaneous Negative Negative ??? Spontaneous if the absolute value of H is greater than the absolute value of TS (low temperature) Positive Positive ??? Spontaneous if the absolute value of TS is greater than the absolute value of H (high temperature) G = H - TS H is enthalpy, T is Kelvin temperature
  • 29. Example of Gibbs Energy • For the reaction at 298 K, the values of H and S are 58.03 kJ and 176.6 J/K, respectively. What is the value of G at 298 K?
  • 30. Example of Gibbs Energy • For the reaction at 298 K, the values of H and S are 58.03 kJ and 176.6 J/K, respectively. What is the value of G at 298 K? G = H - TS G = 58.03 kJ – (298 K)(176.6 J/K) G = 5.40 kJ Not spontaneous at this temperature
  • 31. Second Example Calculate the standard free-energy change at 25 oC for the Haber synthesis of ammonia using the given values for the standard enthalpy and standard entropy changes: So = 198.7 J/K 2NH3(g) N2(g) + 3H2(g) Ho = 92.2 kJ
  • 32. Second Example Calculate the standard free-energy change at 25 oC for the Haber synthesis of ammonia using the given values for the standard enthalpy and standard entropy changes: So = 198.7 J/K 2NH3(g) N2(g) + 3H2(g) Ho = 92.2 kJ G = H  TS G = 92.2 kJ  (298 K)(-198.7 J/K)(1 kJ/1000 J) = -33.0 kJ
  • 33. Third Example • Iron metal can be produced by reducing iron(III) oxide with hydrogen: • Fe2O3(s) + 3 H2(g)  2 Fe(s) + 3 H2O(g) H = +98.8 kJ; S = +141.5 J/K • (a) Is this reaction spontaneous under standard-state conditions at 25 °C? • (b) At what temperature will the reaction become spontaneous?
  • 34. Third Example • To determine whether the reaction is spontaneous at 25 °C, we need to determine the sign of G = H  TS. At 25 C (298 K), G for the reaction is • G = H  TS = (98.8 kJ)  (298 K)(0.1415 kJ/K) • = (98.8 kJ)  (42.2 kJ) • = 56.6 k • Reaction is NOT spontaneous!
  • 35. Third Example • At temperatures above 698 K, the TS term becomes larger than H, making the Gibbs energy negative and the process spontaneous • Why is this postive this time? – Remember, here we’re dealing with the system, not the surroundings! At what temperature does this become spontaenous?
  • 36. Entropy Changes in Chemical Reactions • Constant Temperature and Pressure –Reactions involving gaseous molecules • The change in positional entropy is dominated by the relative numbers of molecules of gaseous reactants and products Typically, more moles of gas, more entropy
  • 37. Third Law of Thermodynamics • "The entropy of a perfect crystal at O K is zero" (NO disorder, since everything is in perfect position) –No movement = 0 K –No disorder = no entropy (S = 0)
  • 38. Standard State Conditions • We’ve seen that quantities such as entropy (S), enthalpy (H), and free energy (G) are dependent upon the conditions present • Standard State – One set of conditions at which quantities can be compared • Pure solids/liquids/gases at 1 atm pressure • Solutes at 1 M concentration • Typically @ 25 oC (298 K) • Designated by o sign (similar to degree sign)
  • 39. Calculating Entropy Change in a Reaction 0 0 o reaction products reactants p r S n S n S       Calculates standard entropy of a reaction, uses standard entropies of compounds  Entropy is an extensive property (a function of the number of moles)  Generally, the more complex the molecule, the higher the standard entropy value
  • 41. Calculating Standard Entropy - Example • 2 (28 J/Kmol) + 3 (189 J/Kmol) – 51 J/K mole – 3 (131 J/Kmol) = 179 J/K • System gained entropy – water more complex than hydrogen! 0 0 o reaction products reactants p r S n S n S     
  • 42. Second Example • Evaluate the entropy change for the reaction: CO + 3 H2 -> CH4 + H2O in which all reactants and products are gaseous. So values: CO 198 J/Kmol H2 131 J/Kmol CH4 186 J/Kmol H2O 189 J/Kmol
  • 43. Second Example • Evaluate the entropy change for the reaction: CO + 3 H2 -> CH4 + H2O in which all reactants and products are gaseous. So values: CO 198 J/Kmol H2 131 J/Kmol CH4 186 J/Kmol H2O 189 J/Kmol s oreaction = [186 + 189] – [198 + 3(131)] = 216 J/Kmol
  • 44. Standard Free Energy Change • G0 is the change in free energy that will occur if the reactants in their standard states are converted to the products in their standard states – G0 cannot be measured directly – The more negative the value for G0, the farther to the right the reaction will proceed in order to achieve equilibrium – Equilibrium is the lowest possible free energy position for a reaction
  • 45. Calculating Free Energy of Formation Using standard free energy of formation (Gf 0): 0 0 0 (products) (reactants) p f r f G n G n G        Gf 0 of an element in its standard state is zero!
  • 46. Calculating Free Energy of Formation - Example
  • 47. Calculating Free Energy of Formation - Example • 2 (-394kJ/mol) + 4 (-229 kJ/mol) – 2 (-163 kJ/mol) – 3 (0) = - 1378 kJ 0 0 0 (products) (reactants) p f r f G n G n G       
  • 48. Second Example • Calculate the standard free energy for the reaction below and determine whether it is spontaneous at standard conditions. Fe2O3(s) + 3 CO (g) 2 Fe (s) + 3 CO2(g) Go = -742.2 -137.2 0 -394.4
  • 49. Second Example • Calculate the standard free energy for the reaction below and determine whether it is spontaneous at standard conditions. Fe2O3(s) + 3 CO (g) 2 Fe (s) + 3 CO2(g) Go (kJ/mol)= -742.2 -137.2 0 -394.4 Go = [0 + (3 x -394.4)] – [-742.2 + (3 x -137.2)] = -29.4 kJ/mol
  • 50. Additional Note on Energies of Formation • Examples on enthalpy are not shown, but could be calculated the same way. • There are numerous other possibilities for calculating these – Another type of problem could be where Ho and So values are given --- you find Ho reaction and So reaction, then plug in to get Go reaction
  • 51. The Dependence of Free Energy on Pressure Enthalpy, H, is not pressure dependent Entropy, S  entropy depends on volume, so it also depends on pressure Slarge volume > Ssmall volume Slow pressure > Shigh pressure
  • 52. Free Energy and Equilibrium • R = Universal gas constant = 8.314 J/K mol • T = Temperature in Kelvin • K = Equilibrium constant = [Pproducts]/[Preactants] • System is at equilbrium (no net movement) when Go = 0 (K = 1) • If the system is NOT at equilibrium, use Q instead of K G = Go + RTln(Q) Go = -RTln(K) at equilibrium
  • 53. Example • For the synthesis of ammonia where Go = -33.3 kJ/mole, determine whether the reaction is spontaneous at 25 C with the following pressures: PN2 = 1.0 atm, PH2 = 3.0 atm, PNH3 = 0.020 atm
  • 54. Example • For the synthesis of ammonia where Go = -33.3 kJ/mole, determine whether the reaction is spontaneous at 25 C with the following pressures: PN2 = 1.0 atm, PH2 = 3.0 atm, PNH3 = 0.020 atm G = Go + RTln(Q) G = -33.3 kJ/mole + (8.314 J/K mol)(298 K) ln( [0.02 atm]2 ) ___________________ [1.0 atm][3.0 atm]3 G = -33.3 kJ/mole + (8.314 J/K mol)(298 K) ln(1.5 x 10-5) G = -60.5 kJ/mol
  • 55. Example • The synthesis of methanol from carbon dioxide and hydrogen has a Go = -25.1 kJ/mol. What is the value of the equilibrium constant at 25 oC?
  • 56. Example • The synthesis of methanol from carbon dioxide and hydrogen has a Go = -25.1 kJ/mol. What is the value of the equilibrium constant at 25 oC? G = Go + RTln(K) Go = - RTln(K) -25.1 kJ/mol = -(8.314 J/molK)(298)lnK Solve for ln K = 10.1, K = 2 x 104
  • 57. Example • At 298 K, Go = -5.40 kJ/mole. Give the equilibrium K for this process.
  • 58. Example • At 298 K, Go = -5.40 kJ/mole. Give the equilibrium constant K for this process. • Go = -RTln(K) • -5.40 kJ/mole = -(8.31 J/K mol)(298 K)ln K • 2.18 = ln K • 8.85 = K
  • 59. Free Energy and Work • The maximum possible useful work obtainable from a process at constant temperature and pressure is equal to the change in free energy • The amount of work obtained is always less the maximum – Work is changed to heat in surroudings – You lose efficiency, but the Ssurr increases (favorable!) • Henry’s Bent’s First Two Laws of Thermodynamics – 1st Law: You can’t win, you can only break even – 2nd Law: You can’t break even