USAPhO Guide

USAPhO/Thermodynamics

Kinetic Theory of Gases

Deriving pressure from molecules hitting a wall, and what temperature really measures.

Frequent on exams40 min read32 problems

In the previous lesson you tracked heat and work going in and out of a gas without ever asking what the gas was made of. A cylinder of air was a black box with a pressure, a volume and a temperature painted on the side. The first law told you how those three bookkeeping numbers had to balance, and that was enough to solve a great many problems.

Now open the box. Inside are something like 102510^{25} molecules per cubic metre, each one flying in a straight line until it hits something, each one obeying nothing more exotic than F=maF = ma and conservation of momentum. Nothing in there knows what "pressure" or "temperature" means. So where do those quantities come from? If you can answer that (if you can get from bouncing billiard balls to PV=NkBTPV = Nk_BT using only mechanics you already have) then temperature stops being a reading on a thermometer and becomes something you can picture.

Pressure is a rain of impacts

Hold your palm out. Air pushes on it with about 10510^5 newtons per square metre, roughly the weight of a small car spread over the palm, and you feel nothing because the same push acts on the other side. That push is not a fluid leaning on you. It is roughly 102710^{27} separate collisions per second, each one far too small and far too brief to notice individually. Averaged over any time you can perceive, the hail of impacts is perfectly steady, and you call the average force per unit area pressure.

The word average is doing the real work there. Individual molecules arrive at all speeds and all angles. What you want is the mean rate at which they deliver momentum to a wall, and momentum delivery per unit time is force: that is Newton's second law written as F=Δp/ΔtF = \Delta p / \Delta t, and it is the single tool this whole derivation runs on.

Figure 1. A box of gas. Drag the temperature up and watch the molecules speed up; drag the molar mass up and watch them slow down at the same temperature. The readout gives the rms speed, and molecules currently touching the right wall are highlighted.

Counting the hits

Take a cube of side LL, volume V=L3V = L^3, holding NN identical molecules each of mass mm. Pick the wall on the right, the one perpendicular to the xx axis, with area A=L2A = L^2. Assume the molecules bounce elastically off the walls and, for now, that they do not hit each other. (They do, constantly, but a collision between two molecules just swaps their momenta around inside the gas and does not change the total delivered to the wall.)

Follow one molecule with velocity components vxv_x, vyv_y, vzv_z. When it strikes the right wall it reverses vxv_x and leaves vyv_y and vzv_z alone. Its momentum in the xx direction goes from +mvx+mv_x to −mvx-mv_x, a change of −2mvx-2mv_x. By Newton's third law the wall receives +2mvx+2mv_x.

∣Δpwall∣=2mvx|\Delta p_{\text{wall}}| = 2mv_x

How often does that happen? After bouncing off the right wall the molecule crosses to the left wall and comes back, a round trip of distance 2L2L at constant xx speed vxv_x. So the time between successive hits on the right wall is Δt=2L/vx\Delta t = 2L / v_x, and the average force this one molecule exerts is

F1=2mvx2L/vx=mvx2LF_1 = \frac{2mv_x}{2L/v_x} = \frac{mv_x^2}{L}
Figure 2. One elastic bounce. The velocity component along the wall normal flips sign, so the momentum handed to the wall is twice the incoming amount. The dashed slab is the region a molecule must already be inside if it is to reach the wall in a short time.

Add up all NN molecules. They have different vxv_x, so what appears is the sum of vx2v_x^2 over the whole gas, which is NN times the average value vx2‾\overline{v_x^2}:

F=Nmvx2‾LF = \frac{Nm\overline{v_x^2}}{L}

Now use symmetry. There is no reason a gas in a box should prefer one direction, so vx2‾=vy2‾=vz2‾\overline{v_x^2} = \overline{v_y^2} = \overline{v_z^2}. Since the speed satisfies v2=vx2+vy2+vz2v^2 = v_x^2 + v_y^2 + v_z^2, averaging gives v2‾=3vx2‾\overline{v^2} = 3\overline{v_x^2}, so vx2‾=13v2‾\overline{v_x^2} = \tfrac13 \overline{v^2}. Divide the force by the area A=L2A = L^2 and note L2⋅L=VL^2 \cdot L = V:

P=FA=Nmv2‾3L3=13NmVv2‾P = \frac{F}{A} = \frac{Nm\overline{v^2}}{3L^3} = \frac{1}{3}\frac{Nm}{V}\overline{v^2}

The combination Nm/VNm/V is just the mass density ρ\rho. So

P=13ρv2‾P = \tfrac13 \rho \overline{v^2}

That is a real result and it is worth pausing on. Pressure rises if you pack in more mass per unit volume, and rises with the square of the molecular speed: one factor because each impact is harder, one because impacts come more often.

Worth remembering

The factor of one third is not a fudge. It is the three dimensions: only the xx motion pushes on an xx-facing wall, and on average a molecule puts one third of its squared speed into each axis.

Quick check

A gas has density 1.25 kg per cubic metre and rms molecular speed 493 m/s. What is its pressure?

Pick one option first.

What temperature actually measures

Rewrite the pressure result by multiplying and dividing by 2:

PV=13Nmv2‾=23N(12mv2‾)=23NKˉPV = \tfrac13 Nm\overline{v^2} = \tfrac23 N\left(\tfrac12 m\overline{v^2}\right) = \tfrac23 N\bar K

where Kˉ=12mv2‾\bar K = \tfrac12 m \overline{v^2} is the average translational kinetic energy of one molecule. So PVPV is, up to a factor of 23\tfrac23, the total translational kinetic energy of the gas. Nothing experimental has entered yet; this is pure mechanics.

Now bring in the one measured fact: gases obey PV=NkBTPV = Nk_BT, with kB=1.38×10−23k_B = 1.38 \times 10^{-23} J/K. Set the two expressions for PVPV side by side and the NN cancels:

23Kˉ=kBT⟹Kˉ=12mv2‾=32kBT\tfrac23 \bar K = k_B T \qquad \Longrightarrow \qquad \bar K = \tfrac12 m\overline{v^2} = \tfrac32 k_B T

Temperature is average translational kinetic energy per molecule, in different units. That is the whole content of the word. A thermometer is an energy meter with an awkward scale.

Solve for the speed. The square root of v2‾\overline{v^2} is called the root-mean-square speed, written vrmsv_{\text{rms}}: square the speeds, take the mean, take the root, in that order:

vrms=3kBTm=3RTMv_{\text{rms}} = \sqrt{\frac{3k_BT}{m}} = \sqrt{\frac{3RT}{M}}

The second form uses per-mole quantities: MM is the molar mass in kg/mol and R=8.31R = 8.31 J/mol·K. Both forms give the same number, because R=NAkBR = N_A k_B and M=NAmM = N_A m. Use whichever matches the data you were given, and never mix them: putting a molar mass into the kBk_B formula is the most common way to be off by 102310^{23}.

Where this goes wrong

Equal temperature means equal average kinetic energy per molecule, not equal speed. In a helium–oxygen mixture at one temperature, every atom of helium and every molecule of oxygen has the same Kˉ\bar K, but helium is eight times lighter and so moves 8≈2.8\sqrt{8} \approx 2.8 times faster. If a problem asks you to compare kinetic energies of two gases at one temperature, the answer is 1 and you do not need any numbers.

Quick check

Argon atoms have rms speed 400 m/s at 290 K. What is their rms speed at 580 K?

Pick one option first.

Example 1: how fast is the air in this room

Nitrogen, M=0.0280M = 0.0280 kg/mol, at T=300T = 300 K.

vrms=3(8.31)(300)0.0280v_{\text{rms}} = \sqrt{\frac{3(8.31)(300)}{0.0280}}

The numerator is 3×8.31×300=74793 \times 8.31 \times 300 = 7479. Divide by 0.0280 to get 2.671×1052.671 \times 10^5. The square root is 517, so vrms=517v_{\text{rms}} = 517 m/s.

Carry that number. Air molecules move at roughly 500 m/s, a little faster than the 343 m/s speed of sound, which is exactly as it should be, since sound is carried by those molecules and cannot outrun them.

Example 2: a molecular beam that sticks

A beam of molecules, each of mass 3.00×10−263.00 \times 10^{-26} kg, hits a surface head-on at 600 m/s, at a rate of 5.00×10205.00 \times 10^{20} per second, spread over 2.00×10−42.00 \times 10^{-4} m². The molecules stick instead of bouncing. Find the pressure.

Start where the derivation started: momentum per impact. A sticking molecule goes from mvmv to zero, so it delivers mvmv, not 2mv2mv.

Δp=(3.00×10−26)(600)=1.80×10−23 kg⋅m/s\Delta p = (3.00\times10^{-26})(600) = 1.80\times10^{-23}\ \text{kg·m/s}

Force is momentum per second, so multiply by the arrival rate:

F=(1.80×10−23)(5.00×1020)=9.00×10−3 NF = (1.80\times10^{-23})(5.00\times10^{20}) = 9.00\times10^{-3}\ \text{N}

Divide by the area:

P=9.00×10−32.00×10−4=45.0 PaP = \frac{9.00\times10^{-3}}{2.00\times10^{-4}} = 45.0\ \text{Pa}

Note what did not appear: no temperature, no kBk_B, no 13\tfrac13. The one third came from averaging over random directions, and a beam is not random: it all goes one way. When a problem gives you a rate of arrival, go back to F=Δp/ΔtF = \Delta p/\Delta t and build the answer from scratch.

Three different average speeds

Molecules do not all move at vrmsv_{\text{rms}}. Their speeds are spread out in the Maxwell distribution, and three different averages of that spread get used, all within a few percent of each other:

  • the most probable speed, 2RT/M\sqrt{2RT/M} (the peak of the curve,
  • the mean speed vˉ=8RT/(πM)\bar v = \sqrt{8RT/(\pi M)}) used for effusion and mean free path,
  • the rms speed 3RT/M\sqrt{3RT/M}: the one tied to energy, since energy needs v2‾\overline{v^2}.

They are in the ratio 2:8/π:3\sqrt{2} : \sqrt{8/\pi} : \sqrt{3}, that is 1.41:1.60:1.731.41 : 1.60 : 1.73. The rms speed is always the largest, because squaring weights the fast molecules more heavily before you average.

Figure 3. The spread of speeds. Raise the temperature and the whole curve shifts right and flattens; raise the molar mass and it squeezes left. Notice that the three marked speeds keep the same ratio no matter what you drag.

How far a molecule gets: mean free path

A nitrogen molecule at 500 m/s does not cross the room in a hundredth of a second. It crosses about 60 nanometres and hits something. Picture a molecule of diameter dd sweeping out a tube: it collides with any molecule whose centre lies within dd of its own centre line, so the tube has cross-section πd2\pi d^2. Travelling a length λ\lambda sweeps a volume πd2λ\pi d^2 \lambda, and that volume contains one other molecule when πd2λn=1\pi d^2 \lambda n = 1, where n=N/Vn = N/V is the number density. Because the targets are moving too, a careful treatment adds a factor of 2\sqrt{2}:

λ=12 πd2n\lambda = \frac{1}{\sqrt{2}\,\pi d^2 n}

Since P=nkBTP = nk_BT, you can swap nn for P/kBTP/k_BT and get λ=kBT/(2πd2P)\lambda = k_BT/(\sqrt{2}\pi d^2 P): the same statement, useful when a problem hands you a pressure instead of a density. The collision rate follows immediately: distance per second divided by distance per collision,

f=vˉλf = \frac{\bar v}{\lambda}
Figure 4. Mean free path lab. Shrink the molecules or thin the gas out and the path between collisions grows fast, because it goes as one over diameter squared. The readout gives both the path and the collisions per second.

Example 3: a molecular diameter from a measurement

A gas with n=2.70×1025n = 2.70 \times 10^{25} m⁻³ has a measured mean free path of 9.00×10−89.00 \times 10^{-8} m. What is the molecular diameter?

Rearrange for d2d^2 first, then take the root at the very end:

d2=12 πλnd^2 = \frac{1}{\sqrt{2}\,\pi \lambda n}

The denominator: 2 π=4.443\sqrt{2}\,\pi = 4.443; times 9.00×10−89.00 \times 10^{-8} gives 3.999×10−73.999 \times 10^{-7}; times 2.70×10252.70 \times 10^{25} gives 1.080×10191.080 \times 10^{19}. So d2=9.26×10−20d^2 = 9.26 \times 10^{-20} m², and

d=3.04×10−10 md = 3.04 \times 10^{-10}\ \text{m}

Three ångströms, which is the right size for a small molecule. Whenever you compute an atomic length, check it against that scale: if you get 10−510^{-5} m or 10−1510^{-15} m you have dropped a factor somewhere.

Worth remembering

Mean free path depends on d2d^2, so a small error in diameter is a large error in λ\lambda. Conversely, extracting dd from a measured λ\lambda is forgiving, because the square root halves any error.

Effusion: leaking through a pinhole

Punch a hole so small that its width is much less than λ\lambda. Molecules do not flow through as a gust; they wander through one at a time, whenever a molecule happens to be heading that way. Counting how many cross a plane per unit area per unit time gives the effusion flux

Φ=14nvˉ\Phi = \tfrac14 n \bar v

The nvˉn\bar v is a rate per area from the same "how many are close enough and moving the right way" argument as before; the quarter comes from averaging over all the directions that count as towards the hole. Multiply by the hole area AA to get molecules per second: N˙=14nvˉA\dot N = \tfrac14 n\bar v A.

The consequence worth remembering is that vˉ∝1/M\bar v \propto 1/\sqrt{M}, so the lighter gas leaks faster:

rate1rate2=M2M1\frac{\text{rate}_1}{\text{rate}_2} = \sqrt{\frac{M_2}{M_1}}

and since a fixed amount of gas takes a time inversely proportional to the rate, t∝Mt \propto \sqrt{M}. That single square root is how uranium was enriched: 235^{235}UF₆ and 238^{238}UF₆ differ by less than one percent in mass, so one stage separates them by a factor of only 0.352/0.349=1.0043\sqrt{0.352/0.349} = 1.0043, and you must cascade hundreds of stages, each multiplying the enrichment.

Quick check

Oxygen (0.0320 kg/mol) takes 120 s to effuse through a pinhole. How long does the same amount of a gas with molar mass 0.0710 kg/mol take?

Pick one option first.

Recognising when this is the technique

Reach for kinetic theory when a problem mentions anything on the molecular scale: a molecule's mass, a number density in per cubic metre, a molecular diameter, a count of impacts per second, a hole gas leaks through. Thermodynamics alone can never produce those; only a molecular picture can.

Three more specific signals:

If the problem gives a temperature and asks for a speed (or the reverse), you want vrms=3RT/Mv_{\text{rms}} = \sqrt{3RT/M}. Check first whether you have molar mass with RR, or molecular mass with kBk_B.

If it gives a rate of molecules arriving and asks for force or pressure, do not use any formula from this lesson. Go back to F=Δp/ΔtF = \Delta p/\Delta t and decide whether each molecule delivers mvmv (sticks) or 2mv2mv (bounces).

If it compares two gases at the same temperature, the answer is almost always a square root of a mass ratio: for speeds, for effusion rates, for leak times. Equal kinetic energies, unequal speeds. And if it asks about kinetic energy rather than speed, the ratio is 1.

The one trap that catches good students is dimensional carelessness: MM in kg/mol, not g/mol, and TT in kelvin, always. Nitrogen is 0.0280 kg/mol, not 28.

You now have the microscopic machinery. Next you will see what happens when molecules can store energy in ways other than flying in a straight line (rotating, vibrating) and how the equipartition theorem turns that count of degrees of freedom into heat capacities you can measure. That is Ideal Gas Law and Equipartition.

Problems

Work these on paper, then check your answer here.

1.

Speed of a gas molecule

NormalWritten for this guidekinetic theory

What is the rms speed, in m/s, of a nitrogen molecule (28 g/mol) at 300 K? Use R=8.31R = 8.31 J/mol·K.

m/s
2.

Average translational KE at room temperature

EasyWritten for this guidekinetic energy

Use kB=1.38×10−23k_B = 1.38\times10^{-23} J/K. Find the average translational kinetic energy of a gas molecule at 300 K in J.

J
3.

RMS speed of nitrogen

EasyWritten for this guiderms speed

Nitrogen has molar mass 0.0280 kg/mol. Use R=8.31R = 8.31 J/mol·K. Find the rms speed of N₂ molecules at 300 K in m/s.

m/s
4.

RMS speed of helium

EasyWritten for this guiderms speed

Helium has molar mass 0.00400 kg/mol. Use R=8.31R = 8.31 J/mol·K. Find the rms speed of He atoms at 300 K in m/s.

m/s
5.

Pressure from gas density and rms speed

EasyWritten for this guidepressurekinetic theory

A gas has density 1.25 kg/m³ and its molecules have rms speed 493 m/s. Use P=13ρvˉ2P = \frac{1}{3}\rho \bar v^2. Find the pressure in Pa.

Pa
6.

Temperature doubling and rms speed

EasyWritten for this guiderms speed

Argon atoms have rms speed 400 m/s at 290 K. Find their rms speed at 580 K in m/s.

m/s
7.

Number density from pressure

EasyWritten for this guidenumber density

Use P=nkBTP = nk_BT with kB=1.38×10−23k_B = 1.38\times10^{-23} J/K. Find the number of molecules per cubic metre in a gas at 1.01×1051.01\times10^{5} Pa and 293 K.

m^-3
8.

Total translational KE of a mole

EasyWritten for this guidekinetic energy

Use R=8.31R = 8.31 J/mol·K. Find the total translational kinetic energy of 1.00 mol of ideal gas at 350 K in J.

J
9.

Temperature from a given rms speed

EasyWritten for this guiderms speed

Oxygen has molar mass 0.0320 kg/mol. Use R=8.31R = 8.31 J/mol·K. Find the temperature at which O₂ molecules have an rms speed of 600 m/s, in K.

K
10.

Mass of one molecule from rms speed

NormalWritten for this guidekinetic energy

A molecule of an unknown gas has rms speed 350 m/s at 273 K. Use kB=1.38×10−23k_B = 1.38\times10^{-23} J/K. Find the mass of one molecule in kg.

kg
11.

Comparing rms speeds of two gases

EasyWritten for this guiderms speedmolar mass

Hydrogen (0.00200 kg/mol) and oxygen (0.0320 kg/mol) are in the same container at the same temperature. Find the ratio vrms(H2)/vrms(O2)v_{rms}(\mathrm{H_2})/v_{rms}(\mathrm{O_2}) (dimensionless).

dimensionless
12.

Momentum transfer in one wall collision

NormalWritten for this guidemomentum transfer

A molecule of mass 5.00×10−265.00\times10^{-26} kg hits a wall head-on at 480 m/s and rebounds elastically at 480 m/s. Find the magnitude of the momentum delivered to the wall in kg·m/s.

kg·m/s
13.

Force from a stream of molecules

NormalWritten for this guidemomentum transferpressure

A wall is struck by 2.00×10222.00\times10^{22} molecules per second, each of mass 5.00×10−265.00\times10^{-26} kg, arriving head-on at 480 m/s and bouncing back elastically. Find the average force on the wall in N.

N
14.

Pressure from molecular bombardment

NormalWritten for this guidepressure

A wall of area 0.04000.0400 m2^2 feels an average force of 0.960 N from molecular impacts. Find the pressure in Pa.

Pa
15.

Pressure from number density and mean KE

NormalWritten for this guidepressurekinetic theory

Use P=23NVKˉP = \frac{2}{3}\frac{N}{V}\bar K. A gas has 3.00×10253.00\times10^{25} molecules per m³, each with average translational kinetic energy 6.21×10−216.21\times10^{-21} J. Find the pressure in Pa.

Pa
16.

Mean free path in air★

NormalWritten for this guidemean free path

Air molecules have effective diameter d=3.70×10−10d = 3.70\times10^{-10} m and number density 2.50×10252.50\times10^{25} m⁻³. Use λ=1/(2πd2n)\lambda = 1/(\sqrt{2}\pi d^2 n). Find the mean free path in m.

m
17.

Mean free path in a vacuum chamber

NormalWritten for this guidemean free path

A vacuum chamber at 300 K is pumped to 1.00×10−31.00\times10^{-3} Pa. The molecules have diameter 3.00×10−103.00\times10^{-10} m. Use kB=1.38×10−23k_B = 1.38\times10^{-23} J/K and λ=kBT/(2πd2P)\lambda = k_BT/(\sqrt{2}\pi d^2 P). Find the mean free path in m.

m
18.

Collision frequency

HardWritten for this guidemean free path

A molecule has mean free path 6.60×10−86.60\times10^{-8} m and mean speed 470 m/s. Find its collision rate in collisions per second.

s^-1
19.

Effusion rate ratio

NormalWritten for this guideeffusion

A container holds a mixture of helium (0.00400 kg/mol) and methane (0.0160 kg/mol) at one temperature. Gas leaks through a tiny hole. Find the ratio of the effusion rate of helium to that of methane (dimensionless).

dimensionless
20.

Effusion time comparison

HardWritten for this guideeffusion

It takes 120 s for a fixed amount of oxygen (0.0320 kg/mol) to effuse through a pinhole. Find the time for the same amount of an unknown gas of molar mass 0.0710 kg/mol under the same conditions, in s.

s
21.

Effusion flux through a hole★

Very HardWritten for this guideeffusionnumber density

Gas with number density 2.00×10252.00\times10^{25} m⁻³ and mean molecular speed 450 m/s escapes through a hole of area 1.00×10−81.00\times10^{-8} m². The effusion flux is 14nvˉ\frac{1}{4}n\bar v. Find the number of molecules leaving per second.

s^-1
22.

Kinetic energy of a whole tank of gas

NormalWritten for this guidekinetic energy

A 0.0500 m³ tank holds gas at 2.00×1052.00\times10^{5} Pa. Use Ktot=32PVK_{tot} = \frac{3}{2}PV. Find the total translational kinetic energy of the gas in J.

J
23.

RMS speed from pressure and density

NormalWritten for this guiderms speedpressure

Carbon dioxide at 1.01×1051.01\times10^{5} Pa has density 1.80 kg/m³. Use P=13ρvrms2P = \frac{1}{3}\rho v_{rms}^2. Find the rms speed in m/s.

m/s
24.

Molecules in a room

NormalWritten for this guidenumber density

A room measures 4.00×5.00×2.504.00 \times 5.00 \times 2.50 m and holds air at 1.01×1051.01\times10^{5} Pa and 293 K. Use kB=1.38×10−23k_B = 1.38\times10^{-23} J/K. Find the number of air molecules in the room.

molecules
25.

Escape speed and molecular speed★

HardWritten for this guiderms speed

The Moon's escape speed is 2380 m/s. Hydrogen has molar mass 0.00200 kg/mol; use R=8.31R = 8.31 J/mol·K. Find the temperature at which the rms speed of H₂ equals the Moon's escape speed, in K.

K
26.

Mean square speed from a small sample

HardWritten for this guiderms speed

Five molecules have speeds 300, 400, 500, 600 and 700 m/s. Find their rms speed in m/s.

m/s
27.

Kinetic energy ratio of two gases

EasyWritten for this guidekinetic energy

Neon and xenon are mixed in one container at 400 K. Find the ratio of the average translational kinetic energy of a neon atom to that of a xenon atom (dimensionless).

dimensionless
28.

Heating a sealed tank

NormalWritten for this guidepressurenumber density

A sealed rigid tank of gas is at 1.50×1051.50\times10^{5} Pa and 280 K. It is heated to 420 K. Find the new pressure in Pa.

Pa
29.

Molecular diameter from mean free path

HardWritten for this guidemean free path

A gas with number density 2.70×10252.70\times10^{25} m⁻³ has a measured mean free path of 9.00×10−89.00\times10^{-8} m. Use λ=1/(2πd2n)\lambda = 1/(\sqrt{2}\pi d^2 n). Find the molecular diameter in m.

m
30.

Isotope separation by effusion★

Very HardWritten for this guideeffusionmolar mass

Uranium hexafluoride made from 235^{235}U has molar mass 0.349 kg/mol; from 238^{238}U it is 0.352 kg/mol. A single effusion stage enriches the lighter species by the factor M238/M235\sqrt{M_{238}/M_{235}}. Find the overall enrichment factor after 20 identical stages (dimensionless).

dimensionless
31.

Pressure of a molecular beam that sticks

HardWritten for this guidemomentum transferpressure

A beam of molecules, each of mass 3.00×10−263.00\times10^{-26} kg, strikes a sticky surface head-on at 600 m/s at a rate of 5.00×10205.00\times10^{20} molecules per second over an area of 2.00×10−42.00\times10^{-4} m². The molecules stick rather than bounce. Find the pressure on the surface in Pa.

Pa

Also worth doing

Problems from past exams and textbooks, cited rather than reproduced.