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Modern Engineering Thermodynamics

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15.6 Heat of Formation 605<br />

and<br />

H 2 O ! H 2 + ð1/2ÞðO 2 Þ + 285:8 MJ/kgmole H 2 O<br />

Then, the combustion equation for the compound C n H m can be written as<br />

C n H m + aðO 2 Þ!nðC + O 2 + 393:5Þ + ðm/2ÞðH 2 + ð1/2ÞO 2 + 285:8Þ+ HHV CnH m<br />

! nðCÞ + ðm/2ÞðH 2 Þ+ ðn + m/4ÞðO 2 Þ<br />

+ <br />

nð393:5Þ+ ðm/2Þð285:8Þ+ HHV Cn H m<br />

Now, an oxygen balance on the original compound combustion equation gives a = n + m/4, so the O 2 terms in<br />

the previous equation cancel, and again using Hess’s law to rearrange this equation, we get<br />

nðCÞ+ ðm/2ÞðH 2 Þ ! C n H m − <br />

nð393:5Þ+ ðm/2Þð285:8Þ+ HHV CnH m<br />

(15.4)<br />

! C n H m + q<br />

f<br />

C ° n H m<br />

where the HHV is in MJ/kgmole of compound. Consequently, the heat of formation in MJ/kgmole of the hydrocarbon<br />

fuel C n H m at the standard reference state is<br />

<br />

q<br />

f<br />

° = −½nð393:5Þ + ðm/2Þð285:5Þ + HHV CnH m<br />

Š in MJ/kgmole (15.5)<br />

C nH m<br />

The use of this relation is illustrated in the following example.<br />

EXAMPLE 15.6<br />

To prevent the Universe from collapsing in a deadly hypergeometric spiral, you must quickly determine the heat of formation<br />

of methane gas CH 4 (g) at the standard reference state. Normally, you would react carbon and hydrogen gas in your<br />

laboratory to form methane and measure its heat of formation during the reaction. Unfortunately, there is no known reaction<br />

by which you can form methane by reacting solid carbon with hydrogen gas. How will you save the Universe?<br />

Solution<br />

Even though we do not know how to form CH 4 (g) from a direct reaction of solid carbon and hydrogen gas, we can use<br />

Eqs. (15.4) and (15.5) with Tables 15.2 and 15.3 to calculate the heat of formation of CH 4 (g) at the standard reference<br />

state. Tables 15.2 and 15.3 give the higher heating value (HHV) of CH 4 as −890.4 MJ/kgmole. Then Eq. (15.5) gives<br />

ðq ° f Þ CH4<br />

= − ½nð393:5Þ + ðm/2Þð285:5Þ + HHV CnHm Š<br />

= − ½1ð393:5Þ + ð4/2Þð285:5Þ + HHV CH4 Š<br />

= − ½393:5 + 2ð285:8Þ + ð−890:4ÞŠ = −74:7 MJ/kgmole of CH 4<br />

and then Eq. (15.4) becomes<br />

CðsÞ + 2½H 2 ðgÞŠ ! CH 4 ðgÞ − 74:7 MJ/kgmole of CH 4<br />

In this example, we denote the physical state of the substances in parentheses as solid (s), liquid (l), or gas (g). Note that<br />

the negative sign on the HHV of methane indicates that the combustion of methane is an exothermic (heat-producing)<br />

reaction.<br />

Exercises<br />

16. The methane in Example 15.6 is replaced by acetylene gas. You must now determine the heat of formation of acetylene<br />

gas, C 2 H 2 (g), at the standard reference state to save the Universe. Answer: ðq<br />

f ° Þ acetylene<br />

=+227 MJ=kgmole.<br />

17. Oops, it is not methane or acetylene gas in Example 15.6, it is ethylene gas. So now, to save the Universe, you must<br />

determine the heat of formation of ethylene gas, C 2 H 4 (g), at the standard reference state. Answer:<br />

ðq<br />

f ° Þ ethylene = −52:4MJ=kgmole.<br />

18. Well, I bet you are surprised to find out that, at the last minute, it was ethane gas that was actually used to generate the<br />

deadly hypergeometric collapse of the Universe. To save all life in the Universe, you must now determine the heat of<br />

formation of ethane gas, C 2 H 6 (g), at the standard reference state. Answer: ðq ° f Þ ethane = −84:5MJ=kgmole:<br />

Notice that, in this example, we do not take into account the heat of formation of H 2 from atomic hydrogen H<br />

or O 2 from atomic oxygen O. This is because the elements used in the formation of a compound must be in<br />

their stable molecular forms at the standard reference state. In the case of methane, the elements are solid carbon<br />

(graphite), C, and diatomic hydrogen gas, H 2 .

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