State |
The "state" of the system is all those parameters needed to describe the system such that it is identifiably the same if they are all returned to their original values after having been changed in any way. Among them are intensive variables like temperature and pressure and extensive variables like energy and number of moles of component compounds. |
The important point about the conservation of state variables is that processes which change and then return a system to a given state can only take place with ZERO CHANGE in the original state variables. That lets us imagine multiple ways to play around with a system and even stop short of returning to our starting point! Then by the difference of the state variable in the endpoint of the truncated path vs. the starting point (the original state of the system), tells us immediately how the state variables must change (that difference exactly) along any path from where we quit back to the original state! | |
Non-State |
This is not to say that any variable must be a state variable. Only a few are so privileged. As a counter-example, consider the work done in climbing straight up a hill vs. zig-zagging back and forth on convenient "switchbacks." Although you'd arrive at the same altitude (a state variable) either way, you'd find vastly different work done trodding the different paths. So work is not a state variable. |
Energy, E |
Energy is a state variable, and so is chemical potential. So we can take advantage of them being so when trying to determine the energy ebb and flow as chemical reactions take place. |
We'll need to measure or predict such energies since all systems tend to try to find their most stable (lowest energy) condition, knowing the chemical potential of several possible outcomes of chemical reactions may help us identify the most likely of them! It will turn out that stability is more complex than just knowing the lowest energy. That'll be a necessary but not quite sufficient condition, but for the moment we'll imagine it to be an important touchstone. | |
The physicists have already copyrighted E as energy, so us chemists need another symbol. So why don't we make it a form of energy most useful to bench chemists, eh? And one of the hallmarks of "bench" chemistry is that it is done under atmospheric pressure! | |
"So what?", you ask. So consider a chemical reaction which produces
a gas such as: CaCO3(s) + Heat CaO(s) + CO2(g) | |
Enthalpy |
And from where comes the energy the CO2 requires to
do that work? From the energy supplied to the process. So we'd
actually have to supply more heat to expand the CO2
against the atmosphere than we would have had to if the decomposition
had been carried out in a closed container. The chemist's energy
that incorporates that added work is called Enthalpy,
and it carries the symbol, H. It's a real convenience
that tables of H don't have to be corrected for gas expansion
(or compression...we could have reactions like |
Reaction |
Now we're all set to assign ethalpy consequences to chemical reactions. These will enable us to predict the heat consumed or evolved by chemical processes. Bear in mind that these heat transfers are not the consequence of temperature differences between the System (the reaction vessel of interest) and its Surroundings (the rest of the Universe). Indeed, the tables that enable us to look up enthalpies assume that both System and Surroundings are at the same temperature, viz., a standard 25°C (a temperature accessible to any terrestrial chemist). |
Instead, these enthalpies result from heat (evolved or consumed) as a consequence of the products having different chemical potentials from the reactants. Since energy is neither created nor destroyed, that difference has to show up as heat transfer between the System and its Surroundings. | |
Exo- Endo- thermic |
Chemists have special names to distinguish reactions which produce heat (exothermic) from those which require it (endothermic). More Greek; exo- means outside of as in "crabs have an exoskeleton" while endo- is its opposite inside of as in "people have endoskeletons; where does that leave crabby people?" And which is which is designated by the sign of H. Exothermic reactions transfer heat to their surroundings, losing enthalpy in the process; so their change in enthalpy, D H < 0; so reactions with large negative enthalpies should be treated with great respect...they're probably fireworks. On the other hand, a D H > 0 implies that the System's enthalpy has risen by the amount of heat transferred in; expect to have to heat them. |
But what if D H = 0 ? Not surprisingly, chemists call those thermoneutral. | |
Using |
Enthalpies like energies are extensive properties; the more stuff
that reacts, the more heat is transferred. Duhhh. However, they are
tied to specific reaction stoichiometries as well as the reactions
themselves! So if we replicate the Hindenberg Disaster in the lab via |
But you probably wouldn't have balanced the reaction that way; that
½ stoichiometric factor, although OK, would've annoyed. Instead,
you're likely to have written | |
Reverse Reactions |
If instead we electrolyze water, i.e., run DC current through it
to attract the few OH -(aq) to the anode and the few
H3O +(aq) to the cathode, we can decompose the
water back into its elements! (The primary reaction of a "Hydrogen
Economy," if we can ever wean ourselves of fossil fuels.) |
Chemical |
Now comes the neat part. Because we can treat chemical reactions and their enthalpies just like algebraic equations, we can add and subtract them (subtraction means "reverse the reaction before adding") to our hearts content. And the exercise is not idle! It is the cornerstone of obtaining the enthalpies of reactions we haven't run from others involving their compounds which we have run or found in tables of enthalpies! |
Standard |
The trick here is to agreeing upon some standard state for all of the atoms which go to make up all of the chemical compounds and then assigning a standard enthalpy to those atoms. The standard state of any atom in the Periodic Table is taken to be that allotrope (alternate form of the element like graphite vs. diamond vs. C60 for carbon) which is the most stable (OK, graphite) at a temperature of 25°C and a pressure of 1 atmosphere. And since we can set an arbitrary scale for enthalpies only once (differences not absolute values being all we can ever measure anyway), let's say the Enthalpy of every element is zero at standard state. |
Of course, we have to make sure we're talking about the phase of the element that's stable at standard state too. Thus, the versions of the 3 following halogens are all the ones which get awarded zero enthalpy: Cl2(gas), Br2(liquid), I2(solid). For sulfur, it'd be S8(s). And so on. | |
Enthalpies |
Then with this ground floor of elements, we can refer enthalpies of all compounds to their component elements be using Enthalpies of Formation, DH f° , (from elements, of course) for all compounds. (The ° means "at standard state.") This is going to work because we can treat chemical equations like algebraic ones; enthalpies of formation add and subtract along with their compounds. So we can imagine, as did Hess, that making products from reactants involves mentally decomposing the reactants to their elements and then using those as tinkertoy parts to reconstruct the product compounds. That first mental step, decomposition of reactant molecules, is going to necessitate subtracting DH f° for the reactants since we're un-forming them but adding DH f° for the products since we are forming them! |
As an example, let's look at the key step in the production of
sulfuric acid, oxidation of SO2 to SO3 in the
presence of a catalyst [V2O5 which we'll ignore
...also, it's accepted practice to use S(s) in place of S8(s)] SO2(g) S(s) + O2(g) , D H = - D H f°(SO2) = + 296.9 kJ/mol | |
add & cancel |
|
Tables of D H f° are found on page 209 and pages A40-A47 in your book. More are in the Handbook of Chemistry and Physics, various National Bureau of Standards publications, and Stull, Westrum, and Sinke, The Chemical Thermodynamics of Organic Compounds. | |
So the general rule for using those tables is that the enthalpy of any reaction will be the sum of the enthalpies of formation of the products (each scaled by its stoichiometric coefficient, of course) minus the sum of the enthalpies of formation of the reactants (also so scaled). And skip all elements in their most stable form since their enthalpy is zero by choice. Dead simple. |