mme 2010 metallurgical thermodynamics ii

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MME 2010 METALLURGICAL THERMODYNAMICS II Chemical Reaction Equilibria

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MME 2010

METALLURGICAL THERMODYNAMICS II

Chemical Reaction Equilibria

Chemical reactions take place in production of steel from liquid iron

Impurities in liquid iron are subjected to a reaction with gaseous oxygen

Steel production takes place in a blast furnace that is aimed to collect liquid iron, slag and

flue gases formed as a result of reaction with C and CO

The liquid phases iron and slag in the blast furnace consist of solutions of Fe, C, Si, Mn, P

and SiO2, Al2O3, CaO, FeO respectively

Flue gases typically contain CO, CO2 and N2 as main components

Mathematical relationships of extensive thermodynamic properties, particularly G, H and

S need to be considered for each solution in order to estimate the equilibrium condition

parameters for maximum efficiency

Consider a general equilibrium:

π‘Žπ΄ + 𝑏𝐡 𝑐𝐢 + 𝑑𝐷

The general criterion for equilibrium under constant T and P is βˆ†πΊ = 0

βˆ†πΊ = πΊπ‘π‘Ÿπ‘œπ‘‘π‘’π‘π‘‘π‘  βˆ’ πΊπ‘Ÿπ‘’π‘Žπ‘π‘‘π‘Žπ‘›π‘‘π‘ 

= 𝑐𝐺𝐢 + 𝑑𝐺𝐷 βˆ’ π‘ŽπΊπ΄ βˆ’ 𝑏𝐺𝐡

Recall that the complete differential of G is

Consider the reaction in a mixture of ideal gases at constant composition and

temperature (𝑑𝑛𝑖 = 𝑑𝑇 =0)

The change in Gibbs free energy of each component as a function of its pressure is given

as

πœ•πΊπ‘–

πœ•π‘ƒπ‘–= 𝑉

πœ•πΊπ‘– =𝑅𝑇𝑑𝑃𝑖

𝑃𝑖

𝑑 𝑛𝐺 = 𝑛𝑉 𝑑𝑃 βˆ’ 𝑛𝑆 𝑑𝑇 + πœ‡π‘– 𝑑𝑛𝑖

πœ•πΊπ‘– = 𝑅𝑇𝑑𝑃𝑖

𝑃𝑖

𝐺𝑖 = πΊπ‘–π‘œ + 𝑅𝑇 ln

𝑃𝑖

π‘ƒπ‘–π‘œ = 𝐺𝑖

π‘œ + 𝑅𝑇 ln𝑃𝑖 βˆ’ 0

Since pressure of gases at standard conditions is assigned a value of 1 atm

The change in free energy of the system at constant temperature is

𝑛𝐺 = 𝑛𝑖𝐺𝑖

Since mole number and pressure of ideal gases are proportional, ni /Pi is constant

and since the total pressure of the system is constant, 𝑑𝑃𝑖 = 0

𝑑 𝑛𝐺 = 𝑛𝑖 𝑑𝐺𝑖 + 𝐺𝑖 𝑑𝑛𝑖

βˆ† 𝑛𝐺 = 𝑅𝑇𝑛𝑖

𝑃𝑖𝑑𝑃𝑖 + 𝐺𝑖 𝑑𝑛𝑖

βˆ†πΊ = 𝐺𝑖 𝑑𝑛𝑖

In the case of system equilibrium

If the number of molecules of each component in the ideal gas mixture is relatively high,

their coefficients a, b, c, d can be used to represent 𝑑𝑛𝑖:

π‘πΊπΆπ‘œ + 𝑑𝐺𝐷

π‘œ βˆ’ π‘ŽπΊπ΄π‘œ βˆ’ 𝑏𝐺𝐡

π‘œ + 𝑅𝑇 ln𝑃𝐢𝑐 +𝑅𝑇 ln𝑃𝐷

𝑑 +𝑅𝑇 lnπ‘ƒπ΄βˆ’π‘Ž +𝑅𝑇 ln𝑃𝐡

βˆ’π‘ = 0

where βˆ†πΊπ‘œ = π‘πΊπΆπ‘œ + 𝑑𝐺𝐷

π‘œ βˆ’ π‘ŽπΊπ΄π‘œ βˆ’ 𝑏𝐺𝐡

π‘œ

Absolute Gibbs free energy is computed for condensed phases as:

𝐺𝑖 = πΊπ‘–π‘œ + 𝑅𝑇 ln π‘Žπ‘–

where a can be taken as unity for pure condensed phases

βˆ†πΊ = πΊπ‘–π‘œ 𝑑𝑛𝑖 + 𝑅𝑇 ln(𝑃𝑖) 𝑑𝑛𝑖 = 0

βˆ†πΊ = 𝐺𝑖 𝑑𝑛𝑖 = 0

βˆ†πΊπ‘œ + 𝑅𝑇 ln𝑃𝐢

𝑐𝑃𝐷𝑑

π‘ƒπ΄π‘Žπ‘ƒπ΅

𝑏 = 0

The equation can be written for condensed phases as

βˆ†πΊ = βˆ†πΊπ‘œ + 𝑅𝑇 lnπ‘ŽπΆ

π‘π‘Žπ·π‘‘

π‘Žπ΄π‘Žπ‘Žπ΅

𝑏= βˆ†πΊπ‘œ + 𝑅𝑇 ln𝑄

Q is called the reaction quotient

Q = K when βˆ†πΊ = 0

βˆ†πΊ = 0 = βˆ†πΊπ‘œ + 𝑅𝑇 ln𝐾

βˆ†πΊπ‘œ is readily given in literature for most compounds at STP

Since πœ•πΊπ‘œ

πœ•π‘‡ 𝑃= βˆ’π‘†,

βˆ†πΊπ‘œ = βˆ†π»π‘œ + π‘‡πœ•βˆ†πΊπ‘œ

πœ•π‘‡π‘ƒ

βˆ’π‘…π‘‡ ln𝐾 = βˆ†π»π‘œ βˆ’ π‘‡πœ• 𝑅𝑇 ln𝐾

πœ•π‘‡π‘ƒ

πœ• ln𝐾

πœ•π‘‡=

βˆ†π»π‘œ

𝑅𝑇2

πœ• ln𝐾

πœ• 1 𝑇

= βˆ’βˆ†π»π‘œ

𝑅Van’t Hoff equation

Equilibrium constant K of condensed phases

π‘Žπ΄ 𝑠 + 𝑏𝐡 𝑠 𝑐𝐢 𝑠 + 𝑑𝐷 𝑠 βˆ†πΊ1π‘œ

The standard state equilibrium free energy of the above reaction can be expressed in terms of

the partial pressures of the gas phase of the components

At equilibrium

For all components the equilibrium equations are

π‘Žπ΄ 𝑠 + 𝑏𝐡 𝑠 = 𝑐𝐢 𝑠 + 𝑑𝐷 𝑠 βˆ†πΊ1π‘œ

π‘Žπ΄ 𝑔, π‘ƒπ΄π‘œ = π‘Žπ΄ 𝑠 βˆ†πΊ2 = 0

𝑏𝐡 𝑔, π‘ƒπ΅π‘œ = 𝑏𝐡 𝑠 βˆ†πΊ3 = 0

𝑐𝐢 𝑔, π‘ƒπΆπ‘œ = 𝑐𝐢 𝑠 βˆ†πΊ4 = 0

𝑑𝐷 𝑔, π‘ƒπ·π‘œ = 𝑑𝐷 𝑠 βˆ†πΊ5 = 0

π‘Žπ΄ 𝑔, π‘ƒπ΄π‘œ + 𝑏𝐡 𝑔, 𝑃𝐡

π‘œ = 𝑐𝐢 𝑔, π‘ƒπΆπ‘œ + 𝑑𝐷 𝑔, 𝑃𝐷

π‘œ βˆ†πΊ6 = βˆ†πΊ1π‘œ

Reaction free energy is the same if the reaction between gas phases that are in equilibrium

with the condensed phases is taken into consideration

However the reaction between gas phases is not in equilibrium state since βˆ†πΊ6 β‰  0

The equilibirum reaction between gas phases should include actual partial pressures rather

than pure pressures of the components:

π‘Žπ΄ 𝑔, 𝑃𝐴 + 𝑏𝐡 𝑔, 𝑃𝐡 = 𝑐𝐢 𝑔, 𝑃𝐢 + 𝑑𝐷 𝑔, 𝑃𝐷 βˆ†πΊ7 = 0

π‘Žπ΄ 𝑔, π‘ƒπ΄π‘œ = π‘Žπ΄ 𝑠 βˆ†πΊ = 0

The change in reaction free energy due to the altered partial pressures can be calculated as

𝑑𝐺𝑖 = 𝑅𝑇𝑑 ln𝑃𝑖 π‘œπ‘Ÿ βˆ†πΊ = 𝑅𝑇 ln𝑃𝑖

π‘ƒπ‘œ

π‘Žπ΄ 𝑔, π‘ƒπ΄π‘œ + 𝑏𝐡 𝑔, 𝑃𝐡

π‘œ = 𝑐𝐢 𝑔, π‘ƒπΆπ‘œ + 𝑑𝐷 𝑔, 𝑃𝐷

π‘œ βˆ†πΊ6π‘œ = βˆ†πΊ1

π‘œ

π‘Žπ΄ 𝑔, 𝑃𝐴 = π‘Žπ΄ 𝑔, π‘ƒπ΄π‘œ βˆ†πΊ8

π‘œ = 𝑅𝑇 lnπ‘ƒπ‘œ

𝑃𝐴

π‘Ž

𝑏𝐡 𝑔, 𝑃𝐡 = 𝑏𝐡 𝑔, π‘ƒπ΅π‘œ βˆ†πΊ9

π‘œ = 𝑅𝑇 lnπ‘ƒπ‘œ

𝑃𝐡

𝑏

𝑐𝐢 𝑔, 𝑃𝐢 = 𝑐𝐢 𝑔, π‘ƒπΆπ‘œ βˆ†πΊ10

π‘œ = 𝑅𝑇 lnπ‘ƒπ‘œ

𝑃𝐢

𝑐

𝑑𝐷 𝑔, π‘ƒπ·π‘œ = 𝑑𝐷 𝑔, 𝑃𝐷

π‘œ βˆ†πΊ11π‘œ = 𝑅𝑇 ln

π‘ƒπ‘œ

𝑃𝐷

𝑑

π‘Žπ΄ 𝑔, 𝑃𝐴 + 𝑏𝐡 𝑔, π‘ƒπ΅π‘œ = 𝑐𝐢 𝑔, 𝑃𝐢

π‘œ + 𝑑𝐷 𝑔, π‘ƒπ·π‘œ βˆ†πΊ7 = 0

βˆ†πΊ7 = βˆ†πΊ1π‘œ + βˆ†πΊπ‘– = 0

0 = βˆ†πΊ1π‘œ + 𝑅𝑇 ln

π‘ƒπΆπ‘ƒπ‘œ

𝑐 π‘ƒπ·π‘ƒπ‘œ

𝑑

π‘ƒπ΄π‘ƒπ‘œ

π‘Ž π‘ƒπ΅π‘ƒπ‘œ

𝑏 = βˆ†πΊ1π‘œ + 𝑅𝑇 ln𝐾

βˆ†πΊ π‘œ = 𝑅𝑇 ln K

Fugacity

The equations used to calculate the free energy change of mixtures comprised of ideal gases

like 𝑑𝐺𝑖 = 𝑅𝑇𝑑 ln𝑃𝑖 can be modified by the fugacity concept for use with non-ideal gases:

𝑑𝐺𝑖 = 𝑅𝑇𝑑 ln 𝑓𝑖

For an ideal gas 𝑓𝑖 = 𝑃𝑖

If the free energy of a substance corresponding to the standard state fugacity is denoted as

βˆ†πΊπ‘–π‘œ,

βˆ†πΊ1 βˆ’ βˆ†πΊ1π‘œ = 𝑅𝑇 ln

𝑓𝑖

π‘“π‘–π‘œ

As pressure approaches 0, 𝑓𝑖 approaches 𝑃𝑖

Activity rather than fugacity is used to relate ideal mixtures to condensed phase mixtures

π‘Žπ‘– =𝑓𝑖

π‘“π‘–π‘œ

βˆ†πΊπ‘œ can be calculated for any temperature since βˆ†πΊπ‘œ = βˆ†π»π‘œ βˆ’ π‘‡βˆ†π‘†π‘œ,

βˆ†πΊπ‘œ = βˆ†π»π‘œ298 +

298

𝑇

βˆ†πΆπ‘ƒπ‘‘π‘‡ βˆ’ 𝑇 βˆ†π‘†π‘œ298 +

298

𝑇 βˆ†πΆπ‘ƒπ‘‘π‘‡

𝑇

where 𝐢𝑃 = π‘Ž + 𝑏𝑇 +𝑐

𝑇2

and βˆ†πΆπ‘ƒ= βˆ†π‘Ž + βˆ†π‘π‘‡ +𝑐

𝑇2 where βˆ†π‘Ž, 𝑏, 𝑐 = βˆ†π‘Ž, 𝑏, π‘π‘π‘Ÿπ‘œπ‘‘π‘’π‘π‘‘π‘  βˆ’ βˆ†π‘Ž, 𝑏, π‘π‘Ÿπ‘’π‘Žπ‘π‘‘π‘Žπ‘›π‘‘π‘ 

βˆ†πΊπ‘œ = βˆ†π»π‘œ298 +

298

𝑇

βˆ†π‘Ž + βˆ†π‘π‘‡ + βˆ†π‘π‘‡2 𝑑𝑇 βˆ’ 𝑇 βˆ†π‘†π‘œ

298 + 298

𝑇 βˆ†π‘Ž + βˆ†π‘π‘‡ + βˆ†π‘π‘‡2 𝑑𝑇

𝑇

βˆ†πΊπ‘œ = βˆ†π»π‘œ298 + βˆ†π‘Žπ‘‡ +

βˆ†π‘π‘‡2

2βˆ’ βˆ†π‘

𝑇 βˆ’ 𝑇 βˆ†π‘†π‘œ298 + βˆ†π‘Ž ln𝑇 + βˆ†π‘π‘‡ βˆ’ βˆ†π‘

2𝑇2

Replacement of the upper and the lower limits yields

βˆ†πΊπ‘œ = πΌπ‘œ + 𝐼1𝑇 βˆ’ βˆ†π‘Žπ‘‡ ln𝑇 βˆ’βˆ†π‘

2𝑇2 βˆ’

βˆ†π‘

2𝑇

where πΌπ‘œ = βˆ†π»π‘œ298 βˆ’ βˆ†π‘Ž298 +

βˆ†π‘2982

2βˆ’ βˆ†π‘

298

𝐼1 = βˆ†π‘Ž βˆ’ βˆ†π‘†π‘œ298 + βˆ†π‘Ž ln 298 + βˆ†π‘298 βˆ’ βˆ†π‘

2βˆ—2982

T

298

T

298

Example - One important equilibrium between condensed phases such as metals and

oxides and a gaseous phase such as oxygen is oxidation of metals

Consider the oxidation of copper

4Cu 𝑠 + O2 𝑔 = 2Cu2O(𝑠)

βˆ†π»π‘œ298 = βˆ’334400 J

βˆ†π‘†π‘œ298 = βˆ’152.07 J/K

βˆ†πΆπ‘ƒ = 4.18 + 0.01839𝑇 +1.67 βˆ— 105

𝑇2 J/K

πΌπ‘œ = βˆ’334400 βˆ’ 1500𝐼1 = 4.18 + 152.07 + 28.35

Using the above thermochemical data

βˆ†πΊπ‘œ = βˆ’335900 + 184.59𝑇 βˆ’ 4.18𝑇 ln𝑇 βˆ’ 0.0092𝑇2 βˆ’0.84 βˆ— 105

𝑇J

Alternatively the standard free energy for formation of pure Cu2O from pure Cu and oxygen

is

βˆ†πΊπ‘œ = 𝑅𝑇 ln𝑃𝑂2(π‘’π‘žπ‘š)

Experimental variation of βˆ†πΊπ‘œwith T can be calculated from the measured oxygen partial

pressure 𝑃𝑂2(π‘’π‘žπ‘š) that is in equilibrium with Cu and Cu2O

When experimental βˆ†πΊπ‘œ vs T is fit to

βˆ†πΊπ‘œ = 𝐴 + 𝐡𝑇 log𝑇 + πΆπ‘‡βˆ†πΊπ‘œ = βˆ’338580 βˆ’ 32.77𝑇 log𝑇 + 246.62𝑇 J

If a 2-term fit is used

βˆ†πΊπ‘œ = 𝐴 + π΅π‘‡βˆ†πΊπ‘œ = βˆ’328580 + 137.94𝑇 J

The comparison of βˆ†πΊπ‘œ calculated from the thermochemical data and experimental data is

made, the difference in temperature range 400 to 1200 K is seen between 293 to 794 J

The comparison of βˆ†πΊπ‘œ calculated from the experimental data and 2-term fit shows that

the difference in the 400 to 1200 K temperature range is even less, between 286 to 788 J

T (K) Thermochemical Experimental 2-term fit a-b b-c a-c

400 -273748 -274041 -273324 293 -717 -424

600 -244655 -245241 -245736 586 495 1081

800 -216566 -217360 -218148 794 7881582

1000 -189480 -190274 -190560 794 286 1080

1200 -163270 -163689 -162972 419 -717 -298

Table shows that overall difference between βˆ†πΊπ‘œ calculated from the thermochemical data

and 2-term fit in the temperature range is at most 1.6 kJ which is within the experimental

error for most of the βˆ†πΊπ‘œmeasurements

Therefore the variation of βˆ†πΊπ‘œwith temperature for oxidation and sulfidation reactions can

be approximated to linear forms

This observation lead to representation of the reaction free energies as Ellingham

diagram:

Ellingham plotted the experimentally determined βˆ†πΊπ‘œ values as a function of T for the

oxidation and sulfidation of a series of metals

The general form of the relationships approximated to straight lines over temperature

ranges in which no change in physical state occurred

The complex terms TlnT, T2 and 1/T does not affect the linearity of the curves for the

considered range

βˆ†πΊπ‘œ = βˆ†π»π‘œ βˆ’ π‘‡βˆ†π‘†π‘œ

βˆ†πΊπ‘œ = 𝐴 + 𝐡𝑇

A, which is the intercept at 0 K, is the temperature independent βˆ†π»π‘œ

B, the slope, βˆ’βˆ†π‘†π‘œ

These approximations imply that Ξ”CPβ‰ˆ 0 for oxidation reactions

Another important characteristic of Ellingham diagram is that; all the lines represent

reactions involving one mole of oxygen:

2π‘₯

𝑦M + O2

2

𝑦MxOy

Therefore, the ordinate βˆ†πΊπ‘œ of all the oxidation reactions become 𝑅𝑇 ln𝑃𝑂2(π‘’π‘žπ‘š)

Almost all the βˆ†πΊπ‘œ lines have positive slopes since βˆ†π‘†π‘œ < 0:

M(s) + O2(𝑔) MO2(𝑠)

βˆ†π‘†π‘œ = βˆ†π‘†π‘œπ‘€π‘‚2 βˆ’ βˆ†π‘†π‘œ

𝑀 βˆ’ βˆ†π‘†π‘œπ‘‚2

π‘†π‘œπ‘‚2 is generally dominant in the temperature range where M and MO2 are solid

So βˆ†π‘†π‘œ β‰ˆ βˆ’π‘†π‘œπ‘‚2

The slopes are approximately equal in the temperature range where metal and oxide are

solid

Therefore almost all the lines are parallel to each other in this temperature range

Examples

2Ni 𝑠 + O2 𝑔 2NiO 𝑠

π‘†π‘œπ‘‚2 = 205.11

𝐽

π‘šπ‘œπ‘™. 𝐾

π‘†π‘œπ‘π‘–(𝑠) = 29.8

𝐽

π‘šπ‘œπ‘™. 𝐾

π‘†π‘œπ‘π‘–π‘‚(𝑠) = 38.09

𝐽

π‘šπ‘œπ‘™. 𝐾

βˆ†π‘†π‘œ = βˆ’188.53 J/K

Sn s + O2 𝑔 SnO2 𝑠

π‘†π‘œπ‘†π‘›(𝑠) = 51.49

𝐽

π‘šπ‘œπ‘™. 𝐾

π‘†π‘œπ‘†π‘›π‘‚2(𝑠) = 48.59

𝐽

π‘šπ‘œπ‘™. 𝐾

βˆ†π‘†π‘œ = βˆ’208.04 J/K

Standard entropies at 298 K

Standard entropies at 298 K

The exceptions to the general trends in oxidation lines are

C 𝑠 + O2 𝑔 CO2 𝑔 βˆ†π‘†π‘œ β‰ˆ 0

and

2C 𝑠 + O2 𝑔 2CO 𝑔 βˆ†π‘†π‘œ > 0

Lines on Ellingham diagrams often have sharp breaks in them which are caused by phase

transformations

The straight line representation of βˆ†πΊπ‘œ vs T relationships are valid if there is no physical

change taking place for any one of the components taking part in the reaction equilibrium

Consider the transformation of M(s) to M(l) at Tm

M 𝑠 + O2 𝑔 MO2 𝑔

M 𝑙 + O2 𝑔 MO2 𝑔 1

2

T

βˆ†π»π‘œ

Tm

T

βˆ†π‘†π‘œ

Tm

βˆ†π»π‘œ1> βˆ†π»π‘œ

2

βˆ†π‘†π‘œ1> βˆ†π‘†π‘œ

2

The net effect of phase transformation of a reactant from a low temperature to a high

temperature phase is an increase in slope

T

βˆ’π‘‡βˆ†π‘†π‘œ

Tm

M(s)

M(l)

T

βˆ†πΊπ‘œ

Tm

M(s)

M(l)

Consider the transformation of product MO2(s) to MO2(l) at Tm

M 𝑠 + O2 𝑔 MO2 𝑠

M 𝑠 + O2 𝑔 MO2 𝑙

1

2

TTm

T

βˆ†π‘†π‘œ

βˆ†π»π‘œ1< βˆ†π»π‘œ

2

βˆ†π‘†π‘œ1< βˆ†π‘†π‘œ

2

βˆ†π»π‘œ

Tm

The net effect of phase transformation of a product from a low temperature to a high

temperature phase is a decrease in slope

T

βˆ’π‘‡βˆ†π‘†π‘œ

Tm

MO2 (s)MO2 (l)

T

βˆ†πΊπ‘œ

Tm

M(s)

M(l)

Effect of evaporation on βˆ†πΊπ‘œ vs T plots is similar to melting, but more pronounced since

βˆ†π»π‘œπ‘£ is about 10 times greater than βˆ†π»π‘œ

π‘š

Slope changes for allotropic transformations will be less than that for melting

T

βˆ†πΊπ‘œ

Tm

M(s)

M(l)

M(g)

Tb

The Ellingham line for the M/MO2 equilibrium is shown in the figure

βˆ†πΊ = 0 all along the line and oxygen partial pressure is PO2(eqm)

Let the partial pressure of oxygen be PO2(actual) when a metal is exposed to an oxidizing

atmosphere

βˆ†πΊ = βˆ†πΊπ‘œ + 𝑅𝑇 ln1

𝑃𝑂2(π‘Žπ‘π‘‘π‘’π‘Žπ‘™), βˆ†πΊ = 𝑅𝑇 ln𝑃𝑂2 π‘’π‘žπ‘š βˆ’π‘…π‘‡ ln𝑃𝑂2 π‘Žπ‘π‘‘π‘’π‘Žπ‘™

At any point above the line, 𝑃𝑂2 π‘Žπ‘π‘‘π‘’π‘Žπ‘™ > 𝑃𝑂2 π‘’π‘žπ‘š , then βˆ†πΊ < 0This implies that MO2 formation is spontaneous and MO2 is stable above the line

At any point below the line, 𝑃𝑂2 π‘Žπ‘π‘‘π‘’π‘Žπ‘™ < 𝑃𝑂2 π‘’π‘žπ‘š , then βˆ†πΊ > 0This implies that MO2 formation is impossible and M is stable below the line

T

βˆ†πΊπ‘œ

M, O2

MO2, O2

Most of the lines on Ellingham diagram are almost parallel to each other

Consider the Ellingham lines for the M/MO2 and N/NO2 equilibria:

The oxide with the larger region of stability is more stable

It is evident from the figure that NO is relatively more stable than MO

The element with the more stable oxide is more reactive

The element of the less stable oxide is more stable in elemental form, M is more stable

than N

2MO 𝑠 2M 𝑠 + O2(𝑔)

2N 𝑠 + O2 𝑔 2NO(𝑠)

2MO 𝑠 + 2N 𝑠 2M 𝑠 + 2NO 𝑠 Net reaction

T

βˆ†πΊπ‘œ

M, NO2

MO2, NO2

M, N

Ellingham lines sometimes intercept each other

Consider the two lines for X/XO and Y/YO equilibria:

Relative stability of oxides changes with temperature in this case

Below the equilibrium temperature, YO2 is more stable, XO2 becomes more stable above TE

All the components X, Y, XO2, YO2 coexist at the equilibrium temperature

There is no stability region for Y and XO2 together below TE, and for X, YO2 together above

TE

If Y and XO2 are brought together at a temperature below TE, Y will be oxidized while XO2

will be reduced

T

βˆ†πΊπ‘œ

X, YO2

XO2, YO2

X, Y

XO2, Y

TE

Partial pressure grid lines

Ellingham diagram offers a simple and useful way to estimate equilibrium oxygen

pressures as a function of temperature

For constant 𝑃𝑂2 values, βˆ†πΊπ‘œ vs T is represented by straight lines with R ln𝑃𝑂2slope and

βˆ†πΊπ‘œ = 0 intercept

Constant oxygen partial pressures can be read from the oxygen partial pressure scale

when these lines are superimposed

The intersections of the constant oxygen partial pressure lines and the X-XO2equilibirum

line give the equilibrium oxygen partial pressures for this reaction at various temperatures

Oxygen partial pressure at 700 Β°C, in equilibrium with X and XO2 is 10-11atm

Oxide is stable if the oxide lines are under the partial pressure line at a temperature

T

βˆ†πΊπ‘œ

XO2, O2

X, O2

700 Β°C

0PO2

1 atm

10-11 atm

Oxide is stable if the

oxide lines are under

the partial pressure

line at a temperature