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Enthalpy & Temperature Changes in Chemical Reactions: Physical Chemistry I Homework 4 - Pr, Assignments of Physical Chemistry

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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Uploaded on 08/08/2009

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The Richard Stockton College of New Jersey
Chemistry Program, School of Natural Sciences and Mathematics
PO Box 195, Pomoma, NJ
CHEM 3410: Physical Chemistry I Fall 2008
Homework 4— Solutions
1. (a) The balanced chemical reaction would look like this:
Fe2O3+ 2 Al 2 Fe + Al2O3
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(Al2O3) + 2∆H
f(F e)H
f(F e2O3) + 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).
2. (a) To find the final temperature, we need to find out how much heat is required to raise the
temperature in each phase and each phase temperature. The best way to do this is in steps.
i. First ask if there is enough heat coming into the system to raise the temperature from
the initial temperature (298 K) to the first transition temperature (αβ, 993 K). The
heat required to raise the temperature this much is:
q=nZ992
298
Cα
pdT = 2 Z992
298 21.6159 J
mole ·KdT = (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 αto β) and have 100698 30046 = 70652 J of
heat remaining.
ii. Now do we have enough heat available to complete the transition from the αto the β
phase:
Hαβ
trans = (2 moles)(2010 J /mole) = 4020 J
We have 70652 J remaining from (i), so we can completely transform to the βphase,
leaving 70652 4020 = 66632 J of heat remaining.
iii. Now can we raise the temperature from 993 K to the transition temperature for βto γ
at 1373K?
q=nZ1373
993
Cβ
pdT = 2 Z1373
993 34.9028 J
mole ·KdT = (2)(34.9028)(1373993) = 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 βto the γ
phase:
Hβγ
trans = (2 moles)(2300 J /mole) = 4600 J
This leaves us 40106 4600 = 35506 J leftover.
pf2

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Download Enthalpy & Temperature Changes in Chemical Reactions: Physical Chemistry I Homework 4 - Pr and more Assignments Physical Chemistry in PDF only on Docsity!

The Richard Stockton College of New Jersey

Chemistry Program, School of Natural Sciences and Mathematics PO Box 195, Pomoma, NJ

CHEM 3410: Physical Chemistry I — Fall 2008

Homework 4— Solutions

  1. (a) The balanced chemical reaction would look like this:

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).

  1. (a) To find the final temperature, we need to find out how much heat is required to raise the temperature in each phase and each phase temperature. The best way to do this is in steps. i. First ask if there is enough heat coming into the system to raise the temperature from the initial temperature (298 K) to the first transition temperature (α → β, 993 K). The heat required to raise the temperature this much is:

q = n

298

Cpα dT = 2

298

J

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

J

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

J

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:

28680 J =

∫ (^) 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 2

T 1

∂qrev T

∫ T 2

T 1

nCpdT T

= nCp ln

T 2

T 1

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

  • Cpβ ln

∆Htransβ→γ 1373 K

  • Cpγ ln

∆Htransγ→δ 1409 K

  • Cpδ ln

]

∆S = (2 moles) [26.0177 + 2.0242 + 11.3093 + 1.6752 + 1.1595 + 1.2775 + 9.2132]

J

mole · K

∆S = 105.4 J/K

(d) As we found in part (a), at the final temperature we are completely in the δ phase.