| Chem 110 |
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Fall 2003 |
| Lecture Notes::Lec 7_10 September |
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| PREVIOUS |
We must consider the system and its surroundings to determine the overall change in entropy and thus the spontaneity of a given process. In most cases we need only analyze the local surroundings to understand what is happening, though ultimately it is the entire Universe which determines spontaneity.
To make things even more complex, the net entropy change, and therefore spontaneity of a reaction depends also on the temperature. To understand the temperature dependence, consider the vaporization of water as an example:
Why should such a change occur with temperature? At either side of 100°C DH will be about the same as will DS, within the system.
Apparently the change must be due to changes in the surroundings. Let's look at an exothermic process because its a bit easier to follow. Essentially, the fractional change in entropy in the surroundings due to enthalpy will be greater at low temperatures. Generally we can therefore say:
Thus DSsur depends on heat/temperature (with temperature in Kelvins):
At constant pressure we use DH for heat exchange. We also generally look at the enthalpy and entropy of the system, so an exothermic process, for which the DH of the surroundings is +, the DH of the system is -, and for endothermic DH is +. Thus
Note that the (-) sign occurs because we are looking at the surroundings, but DH is defined for the system:
-DHsys = +DHsur
We can now begin to see why the vaporization of water changes in spontaneity with T:
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Note that this represents a continuum - that is the % liquid vs. vapor changes continuously as the vapor pressure increases, until at 100°C the vapor pressure = atmospheric pressure and all of the water evaporates.
Summarizing overall:
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To predict whether a process is spontaneous then, we need to determine the DS of the Universe. This is not always convenient however, so another expression is more often used in chemistry and the life sciences, the "free energy" = G, defined as:
The free energy is particularly useful because it tells us the energy from a process available to do useful work at constant pressure - often an important consideration in life!
For a process occurring at constant pressure then,
Thus a negative DG must correspond to to an increase in the entropy of the Universe. This can be seen if we divide both sides of the free energy expression by T:
but we showed earlier that:
substituting:
So
Thus a process with a negative DG is spontaneous!
Discussion of DG vs. negative and positive values of DH and DS.
First let's review some important aspects of free energy.
As an example of picking conditions to solve a problem let's look at a variation of the example on p 805 in your text.
Find the entropy of vaporization of Br2 given the enthalpy of vaporization, DH, and a table of vapor pressure versus T. DH = 3.1 x 104J/mol. So how do we approach this problem?
- Write the equation:
DG = DH -TDS - rearranging
-TDS = DG - DH TDS = DH - DG DS = (DH - DG)/T
We know DH and T, but what about DG? Let's think about the process. Remember that DG tells us about spontaneity. Is there a condition where the system has no net tendency to either vaporize or condense? If the system doesn't tend either direction then DG must be 0! This occurs in any system at equilibrium. An obvious equilibrium position is at the boiling point where the vapor pressure = atmospheric pressure. So all we need to do is look up the boiling point and set our calculations to the appropriate temperature! T = 333K. - We can now place values into our equation:
DS = (DH - DG)/T = (3.1 x 104J/mol - 0)/333K DS = 93.0 JK-1mol-1
Free Energy and Chemical Reactions We very frequently want to find DG for a chemical process. Last semester we saw that we can determine the values for DH for chemical reactions using tabulated heats (enthalpies) of formation (DH°). Similarly we can find DS from tabulations of Standard Molar Entropy values, DS°.
Example: Calculate DS for the complete combustion of ethane (C2H6) with oxygen (O2).
First we need to write the chemical equation:
C2H6 + O2 Æ CO2 + H2O Balancing by inspection:
C2H6 + 7/2 O2 Æ 2 CO2 + 3 H2O (Notice that we left the coefficients in fractional form. This is acceptable for thermo problems because we are attempting to find the molar values of DH, DS, DG, etc. and giving whole number coefficients will add another step and thus another chance for error.) We'll finish this example next time!
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© R A Paselk
Last modified 12 September 2003