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The solution to homework 4 in the physical chemistry i course offered by the chemistry program at the richard stockton college of new jersey. The solution covers the calculation of enthalpy changes and temperature transitions during a chemical reaction, involving the phase transformations of iron oxide (fe2o3) and iron (fe).
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Chemistry Program, School of Natural Sciences and Mathematics PO Box 195, Pomoma, NJ
Fe 2 O 3 + 2 Al → 2 Fe + Al 2 O 3 The enthalpy change for this reaction at 298 K can be calculated using standard enthalpies of formation of the products and reactants:
∆H rxn◦ =
∆H f◦ (Al 2 O 3 ) + 2∆H f◦ (F e)
∆H f◦ (F e 2 O 3 ) + 2∆H f◦ (Al)
The standard enthalpies of formation of elements are zero, so using available thermochemical data: ∆H rxn◦ = − 851 .5 kJ/mole
(b) To answer this part of the question, you needed more information. From the heat capacity, you could calculate the heat necessary to heat the iron from room temperature to its melting point. However, I neglected to give you the enthalpy of melting of iron, nor did I give you data on the solid-solid phase transformation that occurs below the melting point (see the latest batch of in-class problems).
q = n
298
Cpα dT = 2
298
mole · K
dT = (2)(21.6159)(993 − 298) = 30046 J
We have a total of 100698 J of heat available. Therefore we have enough to raise the temperature to the first transition (from α to β) and have 100698 − 30046 = 70652 J of heat remaining. ii. Now do we have enough heat available to complete the transition from the α to the β phase: ∆Htransα→β = (2 moles)(2010 J/mole) = 4020 J We have 70652 J remaining from (i), so we can completely transform to the β phase, leaving 70652 − 4020 = 66632 J of heat remaining. iii. Now can we raise the temperature from 993 K to the transition temperature for β to γ at 1373K?
q = n
993
Cpβ dT = 2
993
mole · K
dT = (2)(34.9028)(1373−993) = 26526 J
Yes we can! This leaves us with 66632 − 26526 = 40106 J leftover. So we can continue! iv. Now do we have enough heat available to complete the transition from the β to the γ phase: ∆Htransβ→γ = (2 moles)(2300 J/mole) = 4600 J This leaves us 40106 − 4600 = 35506 J leftover.
v. Now can we raise the temperature from 1373 K to the transition temperature for γ to δ at 1409?
q = n
1373
Cpγ dT = 2
1373
mole · K
dT = (2)(44.8)(1409 − 1373) = 3226 J
Yes we can! This leaves us with 35506 − 3226 = 32280 J leftover. So we can continue! vi. Now do we have enough heat available to complete the transition from the γ to the δ phase: ∆Htransγ→δ = (2 moles)(1800 J/mole) = 3600 J This leaves us 32280 − 3600 = 28680 J leftover. vii. Now that we are in the delta phase, no additional phase transitions are possible (according to our data). Therefore, the remaining heat coming into the system will go into raising the temperature of the δ phase. We can then solve for the final T knowing how much heat is leftover from the previous steps:
∫ (^) Tf inal
1409
nCpδ dT = (2)(47.3)(Tf inal − 1409)
Solving for Tf inal we find: Tf inal = 1712 K
(b) Since we are working at constant pressure, qp = ∆H, therefore:
∆H = 100698 J (c) To find the entropy change, we need to take into consideration each of our heating steps and phase transformations from part (a). For the heating steps, the change in entropy can be written as: ∆S =
T 1
∂qrev T
T 1
nCpdT T
= nCp ln
ensuring that for each different phase we use the correct value for Cp. Note that we have assumed that the heat capacities are independent of temperature since we are given not data to contradict this. For the phase transformations, the entropy change is just:
∆Strans =
∆Htrans Ttrans
Putting this together:
∆S = (2 moles)
Cpα ln
∆Hαtrans→β 993 K
∆Htransβ→γ 1373 K
∆Htransγ→δ 1409 K
∆S = (2 moles) [26.0177 + 2.0242 + 11.3093 + 1.6752 + 1.1595 + 1.2775 + 9.2132]
mole · K
(d) As we found in part (a), at the final temperature we are completely in the δ phase.