Lecture Notes from CHM 1341
12 June 1996
The Ideal Gas Law
Gases are one of the four common phases of matter.
Yes, there are four: solid, liquid, gas, and PLASMA.
Plasmas are fluids all right but they occur at such high temperatures
that the outer ("valence") electrons are stripped off, leaving them
as ions (charged atoms) in a sea of electrical currents.
You encounter plasmas daily in fluorescent lights.
You see them briefly during lightning strokes.
And they are of use in technology for etching surfaces.
While plasmas are spectacular, we'll dwell here on the other three.
Solids are molecules cheek-by-jowl at their closest proximity,
locked in fixed crystalline position, incompressible, and, of course,
unable to flow. All materials become solid if one but reduces the
temperature sufficiently or increases the pressure upon them
sufficiently. Solid substances are mistakenly referred to as the
state in which molecules no longer move; actually they do oscillate
in place about their center point fixed by the intermolecular forces
holding the solid together.
At sufficiently high temperature (-259°C for H but
+3030°C for Os), that molecular vibration breaks free of its
fixed centers and the molecules, while still adjacent, may now flow
over one another in the liquid state. Liquids remain incompressible,
but the overcoming of the lock on position means that liquids are fluid,
filling their container to the level of their volume.
Both solids and liquids have interfaces (surfaces) which divide them
from their surroundings. Across that interface, at any temperature
above absolute zero, there is a finite vapor pressure of the substance.
That vapor only makes itself terribly obvious when the temperature rises
to the point that the vapor pressure competes with "atmospheric pressure,"
at which point, the liquid boils or the solid "sublimes." A common example
of a subliming solid is "dry ice," solid carbon dioxide, which skips its
liquid phase at ordinary pressures. The temperatures which liberate
elemental vapor at one atmospheric pressure can range from -269°C
for He to +5600°C for Rh.
Molecules don't change size when their condensed phases vaporize,
so their gases contain molecular mass of finite volume, but that
condensed volume is scattered at STP (Standard Temperature, 273°K,
and Pressure, 1 atm) over a vastly larger volume of the gas.
The increase will be in excess of 1,000 fold; so the normal assumption
(and one hallmark of an "ideal gas") is that the molecules may as well
be considered individually volumeless, point particles. In addition,
the force fields which held them together in their condensed phases are
still operational, but the forces fall effectively to nothing beyond a
few molecular diameters. The intermolecular spacing in the gas is so great
(over 50x solid spacing) that another assumption (and hallmark of an
"ideal gas") is that they no longer interact with one another.
Neither assumption is strictly true, yet the gas laws which result from
them give results which are about 99% accurate.
"Close enough for government work."
So if gas molecules don't see one another, it matters not to them even
what kind of molecules share the volume of the container with them;
that's Avogadro's Law. So an "ideal gas" can be of ANY substance.
In fact, the ONLY things which matter to an ideal gas are the
temperature (which influences their average flight speed) and the
walls of the vessel, against which they bash themselves with great
frequency and (another hidden ideal gas assumption) great elasticity.
That is, on every collision, gas molecules bounce back from the wall
undiminished in AVERAGE energy...so they keep it up forever.
Those bashing speeds vary with temperature and molecular weight,
but it is safe to say that gas molecules are running around at about the
speed of sound, 760 mph in air at STP. On these collisions, the forward
momentum of the molecules is reversed as they richochet. Changing momentum
means an equal-and-opposite (Newton's 2nd) force, obvious on the gas
molecule but operative on the wall as pressure! The force of the rebounds
per unit area of vessel surface is the very definition of pressure.
And from this definition, we can infer some ideal gas relations.
It is true that on each collision with the wall, the molecule can
exchange energy and either increase or decrease what it had,
but since the walls are all at the same temperature, the average energy
of colliding molecules continues to average to the same value.
In fact, if that collisional energy exchange DIDN'T take place,
you could never heat or cool gases by changing the temperature of
their vessel walls!
For example, doubling the volume alone will halve the gas density
(mass/unit volume) which halves the collisions per unit area which
halves the pressure! Simple. So pressure and volume are INVERSELY
related to one another: change either one by a factor F, say, and the
other will change by the factor 1/F. In other words, PV = constant;
that's Boyle's Law, and it holds as long as you don't mess around with
the temperature at the same time. That constancy of temperature ensures
constancy of molecular velocity.
But suppose you kept the volume fixed instead and chose to change the
temperature. Those molecular velocities change...but by how much?
Without proof, let us note that the kinetic energy (motion energy) of
molecules, ½ m v², is directly proportional to the absolute
temperature T measured in Kelvin. In other words, quadruple the T and
you double the molecular velocities. What effect does that have?
First, since the molecules are moving twice as fast, they hit the walls
twice as often; that alone would double the pressure.
But wait...there's more.
Second, molecules going twice as fast have twice as much momentum to
transmit on each collision; that too doubles the pressure.
So...quadrupling the temperature doubles the pressure TWICE;
a 4x T change has brought about a 4x P change. So pressure increases
DIRECTLY with temperature (in a fixed volume). Or P=(constant)*T.
Let's do another Gedanken experiment. (Einstein loved those.
Remember gedanken is German for thought.)
Suppose we double the temperature at fixed volume. The pressure doubles.
Then suppose we let the volume change to recover that original pressure
(while retaining the doubled temperature). Since that requires the
pressure to now decrease be the factor of 2, the volume must (by Boyle's
Law) increase by that same factor of 2! We've done one experiment in two
stages; what's wonderful about it is that the same result (doubled T,
doubled V, original P) would have been obtained if we did the experiment
all in one go simply by heating the gas to double its temperature while
keeping the pressure constant; e.g., the volume would change DIRECTLY
with temperature (at fixed pressure). That's Charles's Law: V=constant*T
(if P fixed).
So Boyle knows PV is fixed at fixed T. And Charles knows V/T is fixed at
fixed P. And Avogadro knows P/n is fixed at fixed V and T. n?
The number of moles of any ideal gas or mixture of such gases.
Remember that ideal gases act completely independently of one another;
so putting two different substances as ideal gases in a vessel means that
the total pressure is the sum of the independent substance pressures.
The relationship which brings all of these observations together,
codifies the behavior of all ideal gases, is
PV = nRT
where that new symbol R is a constant, specifically the Gas Constant,
which has the values
L atm J
R = 0.0821 ------- = 8.314 -------
mol K mol K
where the volume unit L = Liter = (dm)³ = 1000 cm³
and the energy unit J = Joule = km m²/ s² .
Note that if nRT are fixed, Boyle is happy.
Likewise if P and nR are fixed, Charles is happy.
Even Avogadro can buy into this if V and RT are fixed.
So PV = nRT is worth knowing.
Return to the CHM 1341 Lecture Notes or Go To Next or Previous Lectures.
Chris ParrUniversity of Texas at Dallas
Programs in Chemistry, Room BE3.506
P.O. Box 830688 M/S BE2.6 (for snailmail)
Richardson, TX 75083-0688
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Last modified 8 July 1997.