| Ideal
Gas
Equation of State |
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Boyle: Using the definition of pressure as a force (created by the change in a gas molecule's momentum on striking the wall) per unit area, we saw that doubling all the dimensions of a container quadruples its area (reducing pressure to ¼) and halves wall collision frequencies (reducing pressure another ½). This yields an overall pressure reduction by a factor of 8, precisely the volume's change. So PV is fixed for fixed n,T, and Boyle was right in 1660. (Fixed T means fixed velocityRMS.) |
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Charles:
If we quadruple T, we double the RMS (root mean squared) velocities, which,
in a fixed container, doubles both momenta and wall collision
frequencies, quadrupling pressure. If we wanted pressure to remain the
same, Boyle tells us we must quadruple the volume of the container to bring
P back down to its original value. Hence quadrupling T at fixed P (and
n), quadruples V. Or V/T is fixed
for fixed n,P. So Charles and Gay-Lussac
were right in 1787.
The added bonus to Charles' Law is that a plot of V vs. T for an ideal gas (or a real gas a really low pressures) shows its origin at T = - 273.16°C which we conveniently relabel as 0.00 K. And the very linearity of that plot means that an ideal gas makes a first principles thermometer! |
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Avogadro:
If we double the number of molecules at fixed V and T, they will collide
twice as often with the walls, doubling P. If instead, we insist that P
remain fixed, we will be obliged to double the volume to return pressure
to its original value. Hence at fixed P,T, Avogadro (1811) was right to
assert that V/n is fixed.
The bonus to Avogadro's Law is that we get to measure number of molecules (in moles) by measuring volume! And since we can weigh known volumes of gas, we can weigh molecules (well, OK, only gaseous molecules, but it's a start). |
| PV=nRT | (the golden rule; how appropriate) Of course all
three rules can only be true if PV/nT
is fixed. And the constant, R, that is that ratio
is called the gas constant. It's numeric value depends on your choice
of units for P and V. You don't have a choice for n and T; they
are mol and K (the absolute temperature), respectively.
So if you insist on SI units, P is in Pascals (N/m2 = Nm/m3 = J/m3 = kg m-1 s-2) and V is in m3. That's instructive since it makes PV in J! We'll soon see that PV is work; it's nice to know it has the units for it. So a little algebra shows R's units to be J mol-1 K-1. And experimental measurements with ideal gases give its value as R = 8.3145 J mol-1 K-1. If you're sane, on the other hand, you'll probably be measuring P in atmospheres and V in Liters which renders R = 0.082058 atm L mol-1 K-1. And, using that value, you can show that at Standard Temperature and Pressure (0°C and 1 atm), the molar volume of an (ideal) gas is 22.414 L or 22,414 cm3. For water, that's some 1244 times its volume as a liquid (18.016 cm3 at the slightly higher 25°C)! Contemporary practice is to standardize pressure as the
bar defined as 100 kPa. It's sort of convenient since 1 atm = 101.325
kPa. So 1 bar = 0.98692 atm, and you can convert at leisure.
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Yet another pressure unit is in wide use. It celebrates Galileo's secretary
and also inventor (1643) of the barometer, Evangelista
Torricelli. At 1 atm pressure, 760 mm of Hg is supported in an evacuated
tube. The pressure of 1 mm of Hg is called a torr.
Not surprisingly, it is useful for lower pressure measurements.
Note that since pressure is a force per unit area measurement,
the cross-section and even the shape of the mercury tube is irrelevant!
Bigger ones certainly weigh more, but the force is spread out over the
larger area. Bulgy ones weigh more too, but the extra force is distributed
over the non-vertical glass (which might break if it's not really sturdy!);
so their pressures are still only a function of the height of the Hg.
|
MS Encarta 99
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Vapor pressures about liquids are often quoted in torr. And since Hg
is a liquid, it must have a vapor pressure! Oops. If it's significant,
it will make a barometer read underpressure by the pressure of the
Hg vapor trapped up there where there should be only vacuum! From my prized
1936 edition of the HCP (Handbook of Chemistry and Physics), at
25°C, Hg has a vapor pressure of 1.85×10-3 torr which
means (whew) that the barometer's pressure is good
to nearly 6 significant figures.
We'd be in lots worse trouble if we tried to substitute water (density 1.0 g/cm3) for Hg (13.6 g/cm3) because (a) we'd have a barometer 0.760×13.6=10.3 m high (we'd need a 3-story building) and (b) the vapor pressure of water at room temperature is about 24 torr, giving a water barometer over 3% error! Nevertheless, trees have to give it a go as they siphon water up their trunks to survive. But wait! Some trees exceed 10.3 m in height (Pacific Coast Redwoods have reached 112 m!) and still water gets pulled up to their leaves. So since straws can't work over (0.97)×10.3 m, trees have to be more clever. We'll find out how later. |
| Kinetic
Theory |
Our reliance on instinct to rationalize Boyle's (etc.) Law at
the top of this web page presumed that chemists have an instinct for Kinetic
Theory. We presumed that you accepted prenatally that
|
| Equipartition
Theorem |
Whoa! Where'd that come from? My genes code that specifically
for instinctive knowledge?
Actually, it's a consequence of statistical mechanics that you won't see until Physical Chemistry, but it is consistent with the instinctive notion that higher temperatures ought to correlate with higher energies. And, in particular, for a gas, the interesting energies are the translational ones (which permit the molecules to run into the walls) as opposed, say, to the rotational ones, although the latter also scale with T. |
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Since that molecular kinetic energy, ½mv2, really
represents the average over however many moles of gas you got, it's not
hard to see that the important average is v2 and not v itself.
So when we argue about the effects of velocity on momentum, p=mv, it's
the vRMS = <v2>½ that's important.
If you want to see how a Newtonian (classical mechanical) analysis gets from ½mv2=3(½)kT to PV=nRT, jump with this link (using your BACK key to return). It's nice to know that one part of the connection is that R=kNAv. |
| Diffusion
and Effusion |
If the frequency with which molecules strike the wall is (in part)
dependent upon their velocity, and we prick a tiny hole in that wall, the
faster moving ones leave most quickly. Surprise surprise. Curiously, that
means that if the container didn't efficiently equilibrate the gas pressure,
the molecules left behind would be the slower (colder)
ones.
But we fixate on a different effect of this effusion of gas out of a small hole. Suppose two different gases were inside. Since they must share the same T (another piece of intuition...if they didn't initially, the colder one would warm up, the hotter cool down, until they had the same T), that equipartition theorem insists they share the same average kinetic energy. So if one is 4x the molecular weight of the other, it must be going only ½ as fast on average so that ½mv2 is the same for both! |
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The general form for this is v1/v2
= (m2/m1)½ where
it's understood that those v are really vRMS. This is known
as Graham's
Law.
So we can use relative leak rates (what a weird concept) to compare gases of unknown molecular weight to those of known molecular weights in effusion experiments. But gaseous diffusion (spreading) depends on velocities in the same way; heavier ones diffuse slower than lighter ones. And that's not even taking into consideration gases so heavy that they "settle out." |
| Gas Density | "Settle out?" I mean like the effect that killed all of those
unfortunate villagers in Cameroon when a thermal inversion overturned their
lake (Nyos)
filling the valley with carbon dioxide from the lake's bottom.
Being heavier than air, it displaced the lighter N2 and even
O2. CO2's greater density was the killer.
Why is it more dense? Density r = M/V and M = n(MW) so r = (MW)n/V = (MW)P/RT by the ideal gas law, and gas density is directly proportional to MW, molecular weight! So since equal volumes (of different gases) contain the same number of moles (for fixed P,T), the weights of those volumes are in direct proportion to their molecular weights. And we have another method for "weighing" molecules. |
| Physics
of the Atmosphere |
So if r = MW (P/RT), gas should be less
dense and rise if it's hotter than the surrounding gas. That's the
principle of hot-air balloons: P, R, and even <MW> are fixed, but if
T increases, r decreases, and up she goes. (Why
are balloons "she?") It's not precisely that simple, of course.
The density difference (between the hot and the outside air) times the
balloon's volume (now a mass difference) must be enough to counter the
weight of the balloon, its gondola (basket), fuel, burner, and pilot. That's
why balloons are so big; you need a massive V to get Dm
large enough given the rather small changes in r.
Do it yourself: if the outside air is 298 K and the inside is, say, 373
K, the relative change in (1/T) is a piddling -20%; that's the relative
amount by which the density is lowered. If gases don't weigh much
You can witness them first-hand locally at the Plano Annual Balloon
Festival in Bob Woodruff Park.
|
| So here's how the atmosphere works: on buoyancy.
The sun warms the equator more than it does the poles. That's because cos(0°) = 1 at the equator indicating the sun's rays are fully perpendicular to the ground, but cos(90°) = 0 at the poles with the sun's rays only tangential. However, Nature abhors a non-uniformity like that, and She does whatever it takes to transport heat from the equator to the poles. Most of it goes oceanic; that is, warm waters circulate up eastern coasts (in our hemisphere anyway), deposit their heat in northern latitudes, and circulate back down again on western coasts. (Means you want to swim on an eastern seaboard.) |
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| The atmosphere does this to a lesser degree but with a big, big difference. The warmest water is at the top (surface), and it's lower density means it won't sink, but the warmest air is at the bottom of the atmosphere, and it must rise! So air circulations are decidedly more 3-d than oceanic ones. Hence our weather as follows: | |
MS Encarta 99
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Hot, damp, equatorial air rises (less dense), expanding as it
does so as the pressure falls with altitude. That expansion actually pushes
atmosphere out of the way of the rising gas, in other words, it does
work. Where comes the energy to perform that work? You might think
this rising parcel would just borrow a tad of heat from a neighbor, but
the neighbor's in the same fix and won't give it up. So the rising parcels
have no choice but to cool off, trading thermal energy for expansion work.
(We'll see the details later.)
Since it was damp (near 100% humidity in the tropics), the temperature soon falls enough to condense the water vapor into clouds which coalesce into raindrops and give us spectacular tropical thunderstorms. But for our purposes, the important feature is what the condensation does for that rising parcel: it took energy from the sun to evaporate that water in the first place, and the water vapor gives that energy back when it condenses! So while the rain in forming, the parcel can't cool off, and it's density difference becomes impressive. That means it rises faster, and the storm cloud grows higher. |
| But not forever. And that's strange since you'd expect the buoyancy to continue to let the parcel rise, but it stops dead at 8-15 km (depending on the latitude) because the air above that altitude is not cooler but warmer than the parcel. That seemingly impenetrable layer is called the "tropopause" which divides the "troposphere" below (in which we live) from the "stratosphere" above. You've even seen the tropopause whenever you've looked at a flatiron thundercloud. The altitude where it flattens out (no choice) is the tropopause. | |
| Stratospheric
Ozone |
So what makes the stratosphere special?
Oops, the margin gave it away. We have to sneak a little atmospheric chemistry in here (early) to answer the question. And it has to do with the sun's germicidal ultraviolet (shorter wavelength) rays. They'd kill off life right quick (as we say here in Texas) if they reached the surface (where life lives). And they used to do so! Life hid in the ocean (about a fathom down, 6' landlubber, is sufficient shielding). And as Life did its photosynthetic thing, it cast off O2(g) which bubbled out of the sea. After it had oxidized all the surface metals, it started to accumulate in the atmosphere. And set up its own UV shield as follows: O2 + hvhard UV ®
O: + O:
And that latter absorption converts light, hv, into heat that keeps the stratosphere (where these reactions occur) warm. These reactions make the stratosphere! They keep hvUV off our doorsteps until we interfere. |
| CFCs
|
When we release freon from air-conditioners, CCl2F2,
a non-toxic, water-insoluble molecule with nothing much but mischief to
do gets lose. Since it's not water soluble, it doesn't rain out
of the atmosphere. It accumulates. Has accumulated. Is accumulating. And
heading everywhere including the stratosphere where it meets UV and:
CCl2F2 + hvUV
®
·CClF2 + ·Cl
Net result: ·Cl kills off ozone catalytically, reducing the "ozone shield" and increasing UV at Earth's surface. Estimates are that for every 1% increase in UV, there's a 2% increase in skin cancers, but that's only the sensationalism. What's truly disturbing is the way UV will interfere with the "Green Revolution" (efficient food production) upon which nations have come to depend. It's no surprise that the nations of the world are banning these chlorofluorocarbons. Those polar ozone "holes" are working their way equatorward. |
| Hadley
Cell
|
So that's why tropical thunderstorms can only get so high, but if the
tropopause halts them, and the parcels below are still rising, where is
the air to go?
Polarward. |
| It moves parallel to the Earth at 8 to 15 km suffering a surprising fate. Formed at the equator, equatorial storms have equatorial rotational speeds. The equator is 24,000 miles long and goes around the Earth once in 24 hours; so equatorial speed is 1,000 mph! The parcels don't lose that momentum when they're migrating north, but the ground does. After all, polar rotation speed is zero. So if your latitude is q, your eastern speed (see that spinning globe) is 1000 cos(q) mph. | |
| At about q = 30° north and south,
the speed difference between the ground air and the rushing air aloft is
too great to sustain "laminar" (smooth) flow. The parcel air becomes turbulent,
forms a sinuous tube of 100+ mph (eastward) jet stream, and cascades down
to Earth, dry as a bone since it lost its moisture on the rise in the tropics.
Check out a map. Many of Earth's deserts lie around 30° latitudes...our
Sonoran Desert, for example.
The complete circuit (after all, the parcel has to head south along the ground to be uplifted again in the tropics) is called a Hadley Cell. If you want to know (much) more about atmospheric circulation, there's an entire course on it in progress at Columbia University; the topic we've touched on here is on Monday of Week 5 of their Climatology course. |
|
| Chemistry
of the Atmosphere |
We had to sneak a little ozone chemistry into the physics above in
order to explain why weather stops at the tropopause. There's no
weather any higher in the atmosphere. But there's certainly chemistry below
the tropopause as well as above it.
Some of it is trivial acid-base chemistry. The partial pressure of CO2 is currently PCO2 = 3.3×10-4 atm. At that concentration, atmospheric CO2(g) is in equilibrium with CO2(aq) which is the anhydride of H2CO3, a weak acid. The 1st acid dissociation constant, 4.3×10-7 and [CO2(aq)] conspire to render atmospheric water at a pH of 5.6, as one text likes to put it, "the acidity of flat beer." Weak as it is, that carbonic acid is sufficient to dissolve mountains (over geologic time, mind you), releasing, among other ions, Ca2+ from limestone, the most easily attacked material: H2CO3(aq) + CaCO3(s) ® Ca2+(aq) + 2 HCO3-(aq) which flows to the ocean, reacting to its pH 8 by redepositting CaCO3 not only on the ocean floor but also in the shells of much marine life. The ocean is a vast resevoir of hydrogen carbonate ion, but while it's
a very large sink, it isn't a very quick sink. So mankind's extensive use
of fossil fuels for combustion is steadily increasing the CO2(g)
in the atmosphere faster than the ocean can get rid of it. That's good
news to plants since photosynthesis proceeds even better with a more abundant
supply of CO2(g). And, if fact, life as we know it demands a
supply of a gas with CO2's light absorption properties!
|
| Global
Warming |
Yes, I know: carbon dioxide is a colorless gas. But that's only true
in visible light. It doesn't absorb visible light; it absorbs in the infrared
region of the spectrum we can't see with our unaided eyes. That's necessary
because it keeps the entire Earth warm. CO2 is our infrared
blanket (along with H2O, CH4, NOX, and
others). It works like this. Visible light from the sun passes easily through
the (transparent) atmosphere and 67% gets to the ground (the other 33%,
called "albedo," is reflected back to space as visible light by
clouds, ice, etc. The 67% striking the Earth is absorbed and reradiated
as infrared light back into space. The balance between the incoming and
outgoing radiation must be perfect or the extra energy would cause the
Earth to grow hotter. Hot objects are good infrared radiators (which is
why we said in class, "Hot glass looks like cold glass"). And one
can determine the temperature for the Earth's energy balance; it's 20°C
below freezing!
You're right; that's not the Earth's average temperature. So something else is happening to retain extra heat. Well, the Earth is slowly leaking heat from its interior (from radioactive decay), but not nearly enough to account for the actual average Earth temperature (a few degrees above freezing). Instead, it is due to our warm and fuzzy IR blanket, mostly powered by CO2. Those molecules intercept IR light on its way off Earth, and then they reradiate it again in the IR. Sounds like a wash, but that reradiation is down as often as it is up! So the Earth's surface gets to revisit about half the warming infrared each molecule nabs. And the more CO2, the warmer we get. We'll see that first at the poles. Last year the polar ice pack was
only 30% of its recent historical thickness, and only a small fraction
of that change can be attributed to El Niño. The rest is quite likely
to be our first unequivocal measurement of Global Warming. Now the trick
is to wean ourselves of fossil fuel combustion before we trick the Earth
into a new (and unpleasant simply because we're used to this one) climate
with the concomitant disruptions in the Earth's capacity for support (or
is that tolerance) of the human race.
|
| Acid
Rain
|
So CO2 is critically important for maintaining an Earth
with liquid water on it, but too much of a good thing gives rise to anxiety-provoking
changes in our lifestyles! Indeed, anxious times occur whenever we release
a new, reactive molecule into the environment or come anywhere near producing
the quantity of a familiar molecule Nature already cycles. The latter is
true with CO2. The former is true of freon, CCl2F2,
discussed above. But now, I want to concentrate on sulfur since we've been
exceeding Nature's production (by vulcanism) of that molecule for
many years now in smelters and especially power plants.
We pay for it when the SO2(g) gets oxidized to SO3(g), the thirsty anhydride of H2SO4. In one sense, we're lucky SO3(g) is so hydroscopic (water-loving) since it pulls water vapor out of the air to coalesce around SO3(g) molecules as the start of a sulfuric acid raindrop! True, that doesn't sound lucky, but it means that SO3(g) doesn't last long in the atmosphere. Unlucky, of course, is any plant, animal, lake, or stream that rain should drop on. While the pH of lakes ought to be 5.6 (if the lakebed itself has no acid-base character), but the lakes downwind of coal-burning factories (there's sulfur in cheap coal) have acid concentrations over 10 times higher. In those lakes, the fish have long since died. The Norwegians and Swedes are not at all happy at the coal-burning British, for example. Fortunately, it's a problem with an economical fix. The sulfur oxides can easily be captured by scrubbing the gases on their way out of the plant, and since H2SO4 is such a terrifically useful chemical (and the one in highest production in the world), this "pollutant" can be sold! But this fix only works for a centralized polluter. Decentralized pollution is the job of the internal combustion engine. No one is going to sell the nitrogen oxides, NOX (shorthand for NO, NO2, etc.), which are an almost inevitable product of using air to burn gasoline in our vehicles. Their oxidation from N2 to NO to NO2 to NO3 and the reactions: NO2 + NO3 ® N2O5 N2O5 + H2O ® 2 HNO3 demonstrate that nitric is also an acid rain acid. Here the fix is the same as that for Global Warming: change the combustion
of fossil fuels. The most promising possibility is the fuel cell
which oxidizes combustibles in a controlled manner in a battery cell. No
high temperature is involved to encourage NOX formation. And
if the combustibles aren't hydrocarbons, we could lose the excess CO2
as well. The best fuel bet is H2 which we could make by electrolysis
of seawater (using some cleaner energy source such as solar or fusion).
Instead of compressing the dihydrogen into dangerous cylinders of explosive
gas (remember the Hindenberg?), it may soon be possible to absorb H2
into metal sponges which will release it slowly and safely to the fuel
cell.
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| Smog
|
NOX has more fates than as HNO3. The NO2
might be photodecomposed (blown up by light) to NO and O: (the ":" means
an unshared pair of electrons; indeed, it's more like .O. ). Yeah, you're
right; something with two unsatisfied valence electrons (a double
radical) isn't likely to last long, probably reacting just about
anything, like
O: + H2O ® 2 ·OH Bear in mind that O: and ·OH aren't ions; they're neutral radicals. And although in very low concentration ( [·OH] ~ 105 molecules/cc ), they're of critical importance in smog formation and many of other atmospheric chemistry phenomena. . . . more later |
| Comments to Chris Parr | Return to CHM 1316 Topics Page | Last modified 25 January 2001. |