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Chemical Reaction Equilibria

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  • 5/26/2018 Chapter 4 Chemical Reaction Equilibria

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    CHEMIC L RE CTIONEQUILIBRI

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    PURPOSE

    OF THIS CHAPTER

    To determine the effect of of temperature, pressure and initial composition on the

    equilibrium conversions of chemical reaction.

    Example

    The rate of oxidation of sulfur dioxide to sulfur trioxide catalyzed by vanadium pentoxide

    increases at higher temperature.

    However, the equilibrium conversion falls as temperature rises, decreasing from 90% at

    520oC to 50% at 680oC

    These values represent maximum possible conversion regardless of catalyst or reaction

    rate.

    CONCLUSION

    Both the equilibrium and rate must be considered in the exploitation of chemical

    reactions for commercial purposes.

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    Reaction is from where Chemical Engineers getDerived ChemicalsfromFeed Stock (rawmaterial)

    Examples of reactions:

    Why is chemical reaction so important tochemical engineers ?

    1. Production of Methanolfrom Carbon Monoxideand Hydrogen

    CO (g) + 2H2 (g) = CH3OH (g)

    2. Fischer Tropsch Synthesis

    x CO (g) + y H2 (g) = Hydrocarbons

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    Chemical Reaction

    Kinetics - reaction rate Equilibria - extent of reaction

    Composition

    Catalyst

    Temperature Pressure

    we will focus here !

    parameters

    The difference between chemical reaction kinetics and the

    chemical reaction equilibrium

    To sum it all .

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    Reaction Equilibrium

    A measure to indicate the extent of reaction

    especially for reversible reaction.

    Combining both concept (reaction kinetic and equlibrium).

    Indicate the speed of a reaction system achieving

    its equilibriumwhich will be the end state.

    It is worth looking at the thermodynamics of chemical equilibrium before

    moving over to look at its kinetics.

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    Forward Reaction

    Reverse Reaction

    CO (g) + H2O (g) CO2(g) + H2(g)

    On a macroscopic view, the reaction will be seemed as if it has

    achieved a final static condition.

    In actual fact, at microscopic level, the reaction still proceeds but theforward and the reverse reaction have balanced each other in term of

    the speed and therefore no net change could be viewed.

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    The reaction coordinate

    Consider the following reaction equation .

    ............ nNmMbBaA

    The equation can be written in general form as

    uaA + ub B + .. umM + unN +

    where is known as stoichiometric coefficient. It has a positive value for

    product but negative value for reactant.

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    Iu1I A1 + Iu2I A2 + Iu3I A3 + ..... -----> IunI An + Iun+1I A n+1+......

    Reactant Product

    Applied to a differential amount of reaction, the equation below is derived:

    dni = ui de

    ui- stoichiometry numbers

    An- chemical species

    +ve for products

    -ve for reactants

    dn1 = dn2 = dn3 = ......... = de

    Reaction coordinate-

    Characterizes extent or degree

    of reaction

    as a general form (the differential change dni with de;

    The general form of reaction structure could be written in the following equation;

    u1 u2 u3

    (i = 1,2,..N)

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    by integrating the equation,

    dn = ui de

    ni = nio + ui e (i = 1,2,3 ...., n)

    Summation over all species ;

    n = Sni = S nio + e Sui

    note : here e is expressed in mol

    ni

    nio

    e

    0

    i i i

    The mole fraction for each component at any time can be calculated using

    e

    e

    0

    0

    n

    n

    n

    nxory iiiii where

    i

    i

    No. of moles initially for

    component i

    FOR SINGLE REACTION

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    SEE EXAMPLE 13.1

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    Consider a fuel cell based on the direct conversion of methanol to form hydrogen:

    H2O(g) + CH3OH(g)CO2(g) + 3 H2(g)

    The reaction is carried out at 60 C and low pressure, with a feed of twice as

    much water as methanol. The equilibrium extent of reaction (e) is 0.87. How

    many moles of H2can be produced per mole of CH3OH in the feed. What is themole fraction of H2.

    Taking a basis of 1 mole CH3OH, the initial composition can be written as:

    n 0CH3OH = 1 and n0H2O = 2 with the number of moles of product = 0

    Using the equation: ni = nio + ui en (CH3OH) = 1 - e

    n (H2O) = 2 - e

    n (CO2) = e

    n (H2) = 3e

    n (total) = 3 + 2e

    Example

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    For a given e= 0.87,

    n (H2) could be calculated i.e.,

    n(H2) = 0.87 X 3 = 2.61 moles

    The others can be calculated as well,

    n(CH3OH) = 1 - 0.87 = 0.13 moles

    n(H2O) = 2 - 0.87 = 1.13 molesn(CO2) = 0.87 X 1 = 0.87 moles

    The mole fraction of H2is calculated by ;

    y (H2) = 2.61 / (3 + 2(0.87))

    = 0.55

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    FOR MULTIPLE REACTION

    See Example 13.3

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    dG = 0T,P

    Similar to physical equilibrium, the criteria for chemical reaction equilibrium from

    thermodynamics point of view;

    G

    eee

    dG = 0T,P

    The total Gibbs Free Energy is at minimum

    possible value at equilibrium condition

    d(nG) = nV dP - nS dT + S m i dnii

    Now, for physical equilibrium we can write ;

    d(nG) = nV dP - nS dT + S vi mi dei

    [ dG T,P / de]S v m = 0iii

    = 0 at const. T,P

    Equilibrium Criteria for Chemical Reaction

    i

    Similarly, for chemical reaction, the equation can be written as;

    At equilibrium

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    i

    ii

    PT

    G0

    ,

    me

    At equilibrium, we can write

    Substituting for chemical potential,

    0

    0ln

    i

    iii

    f

    fRTmm

    i i

    iii

    PT f

    fRT

    G0)ln(

    0

    0

    ,

    me

    We know that:

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    Simplify;

    i

    i

    vi

    i

    iiif

    fRTG 0ln 00

    RT

    Gv

    f

    fo

    ii

    i

    vi

    i

    i

    0

    ln

    Where signifies the product over all species i.

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    Go= standard Gibbs-energy change of reaction

    - fixed for a given reaction once the temperature is established and is

    independent of the equilibrium pressure and composition.

    K= equilibrium constant

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    EFFECT OF TEMPER TURE ON THEEQUILIBRIUM CONST NT

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    Relation of K and enthalpy of reaction (DhR)

    From the following equation,

    Equilibrium Constant

    -RT ln K(T) = Svi mio= DgR

    o

    We can derive,

    dT

    RTgd

    dT

    Kd R )/(ln 0D

    2

    0001)/(

    RT

    g

    dT

    gd

    RTdT

    RTgd RRR DD

    D

    Since,

    2

    00

    1lnRT

    gdT

    gdRTdT

    Kd RR D

    D

    Therefore,

    From earlier developed relation,

    0

    0

    RP

    R sT

    gD

    D

    Recall,

    dG = (dG/dT)PdT + (dG/dP)TdP

    = - s dT + v dP

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    Equilibrium Constant

    From the definition;000

    RRR sThg DDD

    2

    001ln

    RT

    g

    dT

    gd

    RTdT

    Kd RR DD

    00

    r

    P

    r sT

    gD

    D

    We will obtain;

    2

    0ln

    RT

    h

    dT

    KdR

    D

    And the enthalpy of reaction can be calculated in similar manner to the Gibbs Free

    energy for reaction but enthalpy of formation for the individual component is used.

    Svi hio= Svi (Dhf

    o)i= DhRo

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    Effect of Temperature on Equilibrium Constant

    From the following equation,

    we can develop the relation that give the temperature dependence

    of the equilibrium constant by integrating the above relation.

    Equilibrium Constant

    2

    0ln

    RT

    h

    dT

    Kd RD

    =

    If Ho is independent of T

    (constant)

    If Ho is varies with T(dependent on T)

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    See example 13.4

    Problem 13.3 and 13.11

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    Consider the following reaction equation,

    Find the equilibrium constant at room temperature.

    CH4O (g) H2CO (g)+ H2(g)

    DgRo= S viDgf

    o298= - (-162.0 kJ/mol) + (-110 kJ/mol) + (0 kJ/mol)

    mio

    = 52 kJ/molRefer to appendix data

    K298 = exp ( - Dgfo

    298/ RT ) = exp ( - 52,000 / 8.314 . 298.15)

    K298

    = 7.64 X 10-10

    Equilibrium Constant

    formaldehyde

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    To demonstrate the effect of temperature on K, consider the reaction system ;

    H2O(g)+ CH3OH(g)CO2(g)+ 3 H2(g) Given K298(25 C)= 4.69

    Similarly to Gibbs Free Energy, the enthalpy of reaction could be determined from

    the enthalpy of formation,

    Dh0rxn= S vi(Dh0f)i = 1 (Dh0f)CO2+ 3 (Dh0f)H2- 1 (Dh0f)H2O - 1 (Dh0f)CH3OH

    Dh0rxn= (-393.51) + 3 (0)(-241.82)(- 200.66) = 48.97 (kJ/mol)

    ln (K2/K1) = - ( DhR/ R ) [ 1/T2- 1/T1]From equation :

    ln (K333/K298) = - ( DhR/ R ) [ 1/333 - 1/298 ]

    ln (K333/4.69) = - ( DhR/ 8.314 ) [ 1/333 - 1/298 ]

    K333= 37.44

    Find the K value at 60 oC

    Equilibrium Constant

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    and Cpi= [ai+ biT + ciT2 + diT

    -2]R

    Therefore, enthalpy of reaction at temp T is ;

    integrate the above relation and substitute in the equation below,

    In actual fact, the heat capacity is a function of temperature.

    yielding the eqn. in the next slide

    Equilibrium Constant

    iP

    P

    i CdT

    dh

    DD

    T

    T

    PiT

    T dTCvhh

    i0

    0

    00

    D

    D T

    T

    T

    T

    dT

    T

    Th

    RRT

    gd

    00

    2

    00)(1

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    the constants ai, biand ciare determined from Appendix 2,

    Text Chem. Eng. Thermo. by J. Winnick.

    Equilibrium Constant

    2

    0

    2

    2

    0

    2

    0

    00

    0

    11

    262

    ln11

    TT

    dvTT

    cvTT

    bv

    T

    Tav

    TT

    F iiiiii

    ii

    D ii

    iiii

    iiT dv

    T

    cvT

    bvTavT

    R

    hF

    0

    3

    0

    2

    000

    1

    32

    0and

    This will give )lnln( 00

    00

    TTTT KK

    RT

    g

    RT

    g

    D

    D

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    Equilibrium Constant

    Example : We wish to produce formaldehyde, CH2O by the gas phase pyrolysis of

    methanol, CH3OH according to;

    CH3OH(g)

    CH2O(g)+ H2(g)

    a. What is the equilibrium constant at room temperature? Would you expect

    an appreciable amount of product?

    b. Consider the reaction at 600 C and 1 bar. What is the equilibrium

    constant?

    i. Assuming enthalpy of reaction is constant

    ii. If enthalpy of reaction varies with temperature

    Data : CH3OH CH2O H2

    Gibbs Free Energy at 298 -162 -110 0

    (Formation)

    Enthalpy of Formation at 298 -200.7 -116 0

    Vi -1 1 1

    ai 2.211 2.264 3.249

    bi 1.222X10-2 7.022X10-3 0.422X10-3

    ci -3.450X10-6 -1.877X10-6 -di - - 0.083X10

    5

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    Equilibrium Constant

    a. The equilibrium constant can be calculated from the Gibbs Free Energy of Reaction

    DgRo= S viDgf

    o298 = 1 ( -110) + 1 (0)1 (-162.0) = 52 kJ/mol

    -RT ln K(T) = Svi mio= DgR

    o

    ln K = - 52,000 / RT = -52,000 / (8.314 X 298.15) = 7.64 X 10-10

    too small !

    b. (i) To calculate K at 600 C, we need the enthalpy of reaction.

    DhRo= S viDhf

    o298 = 1 ( -116) + 1 (0)1 (-200.7) = 84.7 kJ/mol

    D

    12

    0

    1

    2 11lnTTR

    h

    K

    K R

    K at 873 K = 4.63 produce noticeable amount of product

    K = 2.07 x 10 -7

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    Equilibrium Constant

    b. (ii) To calculate K at 600 C while accounting for changes in enthalpy of reaction.

    2

    0

    2

    2

    0

    2

    0

    00

    0

    11

    262ln

    11

    TT

    dvTT

    cvTT

    bv

    T

    Tav

    TTF

    iiiiii

    ii

    D ii

    iiii

    iiT dv

    T

    cvT

    bvTavT

    R

    hF

    0

    3

    0

    2

    000

    1

    32

    0

    and

    Substitute all the value for the constants and taking T0= 298 and T = 873, the valueof - ln K at 873 could be obtained

    )lnln( 00

    00

    TTTT KK

    RT

    g

    RT

    g

    D

    D

    K (873 K) = 8.67

    The assumption of constant enthalpy has caused significant error !

    D

    DRT

    g

    RT

    g TT000

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    REL TION OF EQUILIBRIUM CONST NTS TO COMPOSITION

    Gas-phase Reactions

    The standard state for the gas is ideal gas state of the pure gas at the standard-state pressure

    (Po) of 1 bar. Since

    For ideal solution,

    Each for a pure species can be evaluated from a generalized correlation once the equilibrium T and P

    are specified .

    For pressures sufficiently low or temperatures sufficiently high, the equilibrium mixture behaves essentially

    as an ideal gas. In this case, = 1, so above equation becomes;

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    EXAMPLES

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    LIQUID-PHASE REACTIONS

    Where, is the fugacity of pure liquid i at the temperature of system and at 1 bar.

    The fugacity ratio can be expressed as:

    By using equation 13.29 and 13.30, equation 13.10 can be written as;

    At high pressure, the equation is reduced to;

    If the equilibrium mixture is an ideal solution, = 1, therefore,

    =

    =

    Equilibrium for Non Ideal Gases Reaction System

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    Some reactions of industrial importance are carried out at high pressure therefore

    the impact causing from the non ideality behaviour becomes more apparent.

    P ( ai)vi = exp [ - S vi mi O / RT ] = K (T)

    Recall the equation

    The modification required here is to account for the fterm.

    ai= yi fiP instead of = yiP as used previously

    Therefore,

    K = P yi fi Pvi vi v

    In order to determine fi, use method as given in earlier section on real gas.

    = (z - 1)/P dP

    P

    ln fP*

    For high density region, use generalised compressibility chart

    For low density region, use virial equation of lowest order

    Equilibrium for Non-Ideal Gases Reaction System

    ii

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    For our earlier example

    in mol

    fractionx/(2x+1) 2x/(2x+1) (1-x)/(2x+1)

    CO(g) + 2H2(g) CH3OH(g)

    Equilibrium composition x 2x 1-x

    will now become

    Pyy

    yK

    HCO

    OHCH

    2

    2

    3

    2

    2

    22

    33 Pyy

    yK

    HHCOCO

    OHCHOHCH

    ff

    f

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    Example : Consider reaction to produce ammonia as below;

    N2 + 3 H2 2 NH3 High pressure reaction and exothermic

    ii vii

    v

    i PyaK f

    2

    3

    2

    2222

    33

    Pyy

    y

    KHHNN

    NHNH

    ff

    f

    Using the free energy data, calculation on equilibrium constant give K = 8.93 X 10-6

    Knowing K value then the composition could be calculated. However for non ideal

    gas case the fugacity coefficient (f) has to be additionally determined.

    One way of doing so is by calculating it based on pure component basis (Lewis

    and Randall Rule)

    RTBP

    i ef

    B = BRRTc/ Pc

    BR= B0

    + wB1

    ffor ammonia calculated is 0.975

    ffor other components nearly 1

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    To calculate the equilibrium concentrations,

    N2 + 3 H2

    2 NH3

    At equilibrium x 3x 2(1-x) N total = 2 + 2x

    2

    3

    2

    2222

    33

    P

    yy

    yK

    HHNN

    NHNH

    ff

    fSubstitute in

    2

    23

    2

    2

    23

    2

    1.31.

    975.0).22(

    .3.

    ).22(

    22

    3

    P

    nxx

    xP

    nxx

    xK

    TTHN

    NH

    ff

    f

    2

    23

    2

    6

    1.31.

    975.0).22(1093.8

    P

    nxx

    x

    Ty (NH3)= 0.144

    y(H2)

    = 0.642

    y (N2) = 0.214

    Answer :

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    EQUILIBRIUM CONVERSIONS FOR

    SINGLE REACTIONS

    SINGLE-PHASE REACTIONS

    For homogeneous system, and K is known, the calculation for phase composition at equilibrium is straightforward if the gas ph ase is assumed an ideal gas and liquid mixture is ideal solution.

    For non-ideal solution, activity coefficient must be determined first.

    See example 13.5 to 13.9.