How to Use This Problem Bank

Ten sections of theory, and now the part that actually earns marks. What follows is 48 worked problems covering the whole chapter, from single-substitution drills up to the multi-step questions that decide ranks. They are arranged easy first, hard last, in eight parts that follow the order the chapter was taught in.

Work them with a pen. Cover the solution, try it, then compare — and read the check at the end of each one, because the check is where the marks usually leak away.

Six formula boxes: counting, one state, two states, speeds, energy, collisions

Notation for This Chapter

Key Point — THIS CHAPTER'S NOTATION:

  • nn is the NUMBER DENSITY, molecules per cubic metre, n=NVn = \frac{N}{V}.
  • μ\mu is the number of MOLES. The previous chapter used nn for moles; here it is the reverse, and so is every kinetic-theory formula and every exam paper.
  • NN is the number of molecules, NAN_A the Avogadro number, and μ=NNA=MM0\mu = \frac{N}{N_A} = \frac{M}{M_0}.
  • M0M_0 is the molar mass in kg/mol; MM is the total mass of the sample; m=M0NAm = \frac{M_0}{N_A} is the mass of one molecule.
  • EE is translational kinetic energy only. UU is the full internal energy. They coincide only for a monatomic gas.
  • CpC_p and CvC_v are molar specific heats in J/(mol K); lowercase cpc_p, cvc_v are per kilogram.

So every formula carried over from thermodynamics gets rewritten here: PV=μRTPV = \mu RT, not nRTnRT; ΔQ=μCvΔT\Delta Q = \mu C_v \Delta T, not nCvΔTnC_v\Delta T. Get used to it now — it is the convention you will meet in the question paper.

The four questions to ask before you write anything

  1. Is the temperature in kelvin? Every ratio T2T1\frac{T_2}{T_1}, every speed formula, every gas-law step needs absolute temperature. Only a bare difference ΔT\Delta T is the same number in Celsius and in kelvin. This is the single commonest wrong answer in the chapter.
  2. Is the molar mass in kilograms per mole? Oxygen is 0.0320.032, not 3232. Getting this wrong makes a speed come out 1000=31.6\sqrt{1000} = 31.6 times too small, and the answer still looks like a number, which is why it slips through.
  3. Which of the three speeds does the question want? Energy wants vrmsv_{rms}; a collision count wants vˉ\bar{v}; the peak of the distribution is vmpv_{mp}. Name it out loud before you substitute.
  4. Is the amount of gas fixed? If it is, P1V1T1=P2V2T2\frac{P_1V_1}{T_1} = \frac{P_2V_2}{T_2} does the whole job. If gas leaks in or out, μ\mu changes and you must go through PV=μRTPV = \mu RT twice, once at each state.

Key Point — every formula this section uses, in one place: μ=MM0=NNA,m=M0NA,n=NV\mu = \frac{M}{M_0} = \frac{N}{N_A}, \qquad m = \frac{M_0}{N_A}, \qquad n = \frac{N}{V} PV=μRT,PV=NkBT,P=nkBT,P=ρRTM0PV = \mu RT, \qquad PV = Nk_BT, \qquad P = nk_BT, \qquad P = \frac{\rho R T}{M_0} P1V1T1=P2V2T2,Ptotal=P1+P2+P3+\frac{P_1V_1}{T_1} = \frac{P_2V_2}{T_2}, \qquad P_{\text{total}} = P_1 + P_2 + P_3 + \dots P=13nmv2=13ρv2,PV=23E,E=32NkBTP = \frac{1}{3}nm\overline{v^2} = \frac{1}{3}\rho\,\overline{v^2}, \qquad PV = \frac{2}{3}E, \qquad E = \frac{3}{2}Nk_BT 12mv2=32kBT,vrms=3RTM0=3kBTm\frac{1}{2}m\overline{v^2} = \frac{3}{2}k_BT, \qquad v_{rms} = \sqrt{\frac{3RT}{M_0}} = \sqrt{\frac{3k_BT}{m}} vˉ=8RTπM0,vmp=2RTM0,vmp:vˉ:vrms=2:8π:3\bar{v} = \sqrt{\frac{8RT}{\pi M_0}}, \qquad v_{mp} = \sqrt{\frac{2RT}{M_0}}, \qquad v_{mp} : \bar{v} : v_{rms} = \sqrt{2} : \sqrt{\frac{8}{\pi}} : \sqrt{3} U=f2μRT,Cv=f2R,Cp=Cv+R,γ=1+2fU = \frac{f}{2}\mu RT, \qquad C_v = \frac{f}{2}R, \qquad C_p = C_v + R, \qquad \gamma = 1 + \frac{2}{f} l=12nπd2=kBT2πd2P,fcoll=vˉl,τ=1fcolll = \frac{1}{\sqrt{2}\,n\pi d^2} = \frac{k_BT}{\sqrt{2}\,\pi d^2 P}, \qquad f_{\text{coll}} = \frac{\bar{v}}{l}, \qquad \tau = \frac{1}{f_{\text{coll}}} r1r2=M0,2M0,1(equal P and T)\frac{r_1}{r_2} = \sqrt{\frac{M_{0,2}}{M_{0,1}}} \quad \text{(equal } P \text{ and } T\text{)}

The Maxwell distribution, the formulas for vˉ\bar{v} and vmpv_{mp}, Graham's law and the pressure law all sit outside the rationalised syllabus body text, yet a large fraction of the problems below cannot be done without them, and Boards, JEE and NEET ask about them every year. They are used freely here.

The constants used throughout

Every solution also restates the constants it uses inside itself, so you never have to scroll back.

Quantity Value used
Boltzmann constant kBk_B 1.38×10231.38 \times 10^{-23} J/K
Gas constant RR 8.314 J/(mol K)
Avogadro number NAN_A 6.022×10236.022 \times 10^{23} per mol
1 atmosphere 1.013×1051.013 \times 10^{5} Pa
Absolute zero offset 0°C =273.15= 273.15 K
Molar volume at STP 22.4 litres
gg 9.8 m/s2^2
Density of water 1000 kg/m3^3
CvC_v monatomic / rigid diatomic / rigid non-linear polyatomic 12.47 / 20.79 / 24.94 J/(mol K)
γ\gamma for the same three 53\frac{5}{3} / 75\frac{7}{5} / 43\frac{4}{3}

[Board Important] Every solution below writes the formula on its own line before any number goes into it, converts the molar mass on a line of its own, and names which speed it is using. Do all three in the exam. A correct formula with an arithmetic slip still earns most of the marks; a gram-per-mole inside a square root loses them all.

Solved Examples

Part 1: Molecules, Sizes and Counting

Six warm-ups. No gas laws yet — just Avogadro's number used carefully, and the two length scales that make a gas a gas.

Example 1: From grams to molecules, and back

A sealed flask holds 5.6 g of nitrogen gas (M0=28M_0 = 28 g/mol). Find (a) the number of moles, (b) the number of molecules, (c) the number of nitrogen atoms, and (d) the mass of a single molecule.

Solution:

Constants: NA=6.022×1023N_A = 6.022 \times 10^{23} per mole.

  1. Convert the molar mass first, as a habit, even where the answer does not need it: M0=28 g/mol=0.028 kg/molM_0 = 28 \ \text{g/mol} = 0.028 \ \text{kg/mol}

  2. (a) Moles. μ=MM0\mu = \frac{M}{M_0}, with both masses in the same unit: μ=5.628=0.20 mol\mu = \frac{5.6}{28} = 0.20 \ \text{mol}

  3. (b) Molecules. N=μNA=0.20×6.022×1023=1.20×1023N = \mu N_A = 0.20 \times 6.022 \times 10^{23} = 1.20 \times 10^{23}

  4. (c) Atoms. Nitrogen gas is N2N_2two atoms per molecule: atoms=2N=2.41×1023\text{atoms} = 2N = 2.41 \times 10^{23}

  5. (d) Mass of one molecule. m=M0NA=0.0286.022×1023=4.65×1026 kgm = \frac{M_0}{N_A} = \frac{0.028}{6.022 \times 10^{23}} = 4.65 \times 10^{-26} \ \text{kg} Check: N×m=1.204×1023×4.65×1026=5.6×103N \times m = 1.204 \times 10^{23} \times 4.65 \times 10^{-26} = 5.6 \times 10^{-3} kg, which is the 5.6 g we started from.

Final Answer: 0.200.20 mol; 1.20×10231.20 \times 10^{23} molecules; 2.41×10232.41 \times 10^{23} atoms; 4.65×10264.65 \times 10^{-26} kg per molecule.

Takeaway: Molecules and atoms are not the same count. Any diatomic gas doubles the atom count, and questions that ask for "the number of atoms in 5.6 g of nitrogen" are testing exactly that.

Example 2: Sizing a single atom from a bucket of liquid

Liquid argon has a density of about 1400 kg/m3^3 and a molar mass of 39.9 g/mol. Estimate the diameter of one argon atom, assuming the atoms in the liquid are packed so as to fill the space.

Solution:

Constants: NA=6.022×1023N_A = 6.022 \times 10^{23} per mole.

  1. Volume of one mole of the liquid. Convert the molar mass: M0=39.9 g/mol=0.0399 kg/molM_0 = 39.9 \ \text{g/mol} = 0.0399 \ \text{kg/mol} Vmole=M0ρ=0.03991400=2.85×105 m3V_{\text{mole}} = \frac{M_0}{\rho} = \frac{0.0399}{1400} = 2.85 \times 10^{-5} \ \text{m}^3

  2. Volume per atom. Vatom=VmoleNA=2.85×1056.022×1023=4.73×1029 m3V_{\text{atom}} = \frac{V_{\text{mole}}}{N_A} = \frac{2.85 \times 10^{-5}}{6.022 \times 10^{23}} = 4.73 \times 10^{-29} \ \text{m}^3

  3. Turn a volume into a diameter. Model the atom as a sphere of diameter dd, so Vatom=π6d3V_{\text{atom}} = \frac{\pi}{6}d^3: d=(6Vatomπ)1/3=(6×4.73×10293.1416)1/3=(9.04×1029)1/3d = \left(\frac{6 V_{\text{atom}}}{\pi}\right)^{1/3} = \left(\frac{6 \times 4.73 \times 10^{-29}}{3.1416}\right)^{1/3} = \left(9.04 \times 10^{-29}\right)^{1/3} d=4.49×1010 m=4.5 A˚d = 4.49 \times 10^{-10} \ \text{m} = 4.5 \ \text{Å}

  4. Sanity check. Atoms come out a few angstroms across whatever substance you start from. A liquid is close-packed rather than perfectly space-filling, so this slightly overestimates dd — an estimate, not a measurement.

Final Answer: d4.5×1010d \approx 4.5 \times 10^{-10} m, about 4.5 Å.

Takeaway: A density plus a molar mass gives you the size of an atom. The whole trick is Vatom=M0ρNAV_{\text{atom}} = \frac{M_0}{\rho N_A}, and then a cube root. It works for any liquid or solid.

Example 3: How far apart are the molecules of a gas?

Nitrogen gas is held at 1 atm and 27°C. Find its number density, the volume available to each molecule, and the average spacing between neighbouring molecules. Compare that spacing with a molecular diameter of 3.7 Å.

Solution:

Constants: kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K; 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. Kelvin first. T=27+273.15=300.15 K300 KT = 27 + 273.15 = 300.15 \ \text{K} \approx 300 \ \text{K}

  2. Number density from P=nkBTP = nk_BT. Here nn is molecules per cubic metre, not moles: n=PkBT=1.013×1051.38×1023×300=2.45×1025 per m3n = \frac{P}{k_BT} = \frac{1.013 \times 10^{5}}{1.38 \times 10^{-23} \times 300} = 2.45 \times 10^{25} \ \text{per m}^3

  3. Volume per molecule is just the reciprocal: V1=1n=12.45×1025=4.09×1026 m3V_1 = \frac{1}{n} = \frac{1}{2.45 \times 10^{25}} = 4.09 \times 10^{-26} \ \text{m}^3

  4. Spacing. Give each molecule a little cube of side rˉ\bar{r}: rˉ=V11/3=(4.09×1026)1/3=3.44×109 m=34.4 A˚\bar{r} = V_1^{1/3} = (4.09 \times 10^{-26})^{1/3} = 3.44 \times 10^{-9} \ \text{m} = 34.4 \ \text{Å}

  5. Compare with the molecule itself. rˉd=34.43.7=9.3\frac{\bar{r}}{d} = \frac{34.4}{3.7} = 9.3

Final Answer: n=2.45×1025n = 2.45 \times 10^{25} per m3^3; 4.09×10264.09 \times 10^{-26} m3^3 each; spacing 34.434.4 Å, about 9 molecular diameters.

Takeaway: In a gas at ordinary pressure the molecules sit roughly ten diameters apart. That single number is why the ideal gas model works: for most of its life a molecule is nowhere near another one, so the intermolecular forces have nothing to act on.

Example 4: What fraction of a compressed gas is actually molecule?

Nitrogen is compressed to 5 atm at 300 K. Taking the molecular diameter as 3.7 Å, find the fraction of the container's volume that the molecules themselves occupy.

Solution:

Constants: kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K; 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. Number density at 5 atm. n=PkBT=5×1.013×1051.38×1023×300=1.22×1026 per m3n = \frac{P}{k_BT} = \frac{5 \times 1.013 \times 10^{5}}{1.38 \times 10^{-23} \times 300} = 1.22 \times 10^{26} \ \text{per m}^3

  2. Volume of one molecule, treated as a sphere of diameter d=3.7×1010d = 3.7 \times 10^{-10} m: vmol=π6d3=3.14166(3.7×1010)3=2.65×1029 m3v_{\text{mol}} = \frac{\pi}{6}d^3 = \frac{3.1416}{6}\left(3.7 \times 10^{-10}\right)^3 = 2.65 \times 10^{-29} \ \text{m}^3

  3. Fraction. Molecular volume per cubic metre of gas, divided by that cubic metre: fraction=nvmol=1.22×1026×2.65×1029=3.24×103\text{fraction} = n\,v_{\text{mol}} = 1.22 \times 10^{26} \times 2.65 \times 10^{-29} = 3.24 \times 10^{-3} =0.32%= 0.32\%

  4. What it means. Even at five atmospheres, 99.7% of the vessel is empty space. But notice the fraction is proportional to PP at fixed TT — squeeze the same gas to 100 atm and it rises to about 6.5%, and at that point the finite size of the molecules is no longer negligible and the gas stops being ideal.

Final Answer: about 3.2×1033.2 \times 10^{-3}, i.e. 0.32% of the volume.

Takeaway: The "molecules are point-like" assumption is a statement about pressure, not about molecules. It holds because nvmol1n v_{\text{mol}} \ll 1, and that fails the moment you compress hard enough.

Example 5: The molecules in one breath

A quiet breath draws in about 500 cm3^3 of air at 1 atm and body temperature, 37°C. Find the number of moles, the number of molecules, and the mass of that air. Take the mean molar mass of air to be 28.9 g/mol.

Solution:

Constants: R=8.314R = 8.314 J/(mol K); kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K; NA=6.022×1023N_A = 6.022 \times 10^{23} per mole; 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. Everything into SI. T=37+273.15=310.15 K,V=500 cm3=5.00×104 m3T = 37 + 273.15 = 310.15 \ \text{K}, \qquad V = 500 \ \text{cm}^3 = 5.00 \times 10^{-4} \ \text{m}^3

  2. Moles, from PV=μRTPV = \mu RT: μ=PVRT=1.013×105×5.00×1048.314×310.15=50.652578.6=1.96×102 mol\mu = \frac{PV}{RT} = \frac{1.013 \times 10^{5} \times 5.00 \times 10^{-4}}{8.314 \times 310.15} = \frac{50.65}{2578.6} = 1.96 \times 10^{-2} \ \text{mol}

  3. Molecules. N=μNA=1.964×102×6.022×1023=1.18×1022N = \mu N_A = 1.964 \times 10^{-2} \times 6.022 \times 10^{23} = 1.18 \times 10^{22}

  4. Cross-check by the other road, using P=nkBTP = nk_BT: n=PkBT=1.013×1051.38×1023×310.15=2.37×1025 per m3n = \frac{P}{k_BT} = \frac{1.013 \times 10^{5}}{1.38 \times 10^{-23} \times 310.15} = 2.37 \times 10^{25} \ \text{per m}^3 N=nV=2.37×1025×5.00×104=1.18×1022N = nV = 2.37 \times 10^{25} \times 5.00 \times 10^{-4} = 1.18 \times 10^{22} \quad \checkmark

  5. Mass. M=μM0=1.964×102×28.9=0.568 gM = \mu M_0 = 1.964 \times 10^{-2} \times 28.9 = 0.568 \ \text{g}

Final Answer: 0.01960.0196 mol, 1.18×10221.18 \times 10^{22} molecules, mass about 0.570.57 g.

Takeaway: PV=μRTPV = \mu RT and P=nkBTP = nk_BT are the same equation divided by NAN_A. Solving a counting problem both ways costs thirty seconds and catches a stray factor of 6×10236 \times 10^{23} instantly.

Example 6: A drop of water, counted three ways

A drop of water has a mass of 1.8 g. Find the number of water molecules in it, the total number of atoms, and the average spacing between neighbouring molecules. Molar mass of water is 18 g/mol and its density is 1000 kg/m3^3.

Solution:

Constants: NA=6.022×1023N_A = 6.022 \times 10^{23} per mole.

  1. Moles and molecules. μ=1.818=0.10 mol,N=0.10×6.022×1023=6.02×1022\mu = \frac{1.8}{18} = 0.10 \ \text{mol}, \qquad N = 0.10 \times 6.022 \times 10^{23} = 6.02 \times 10^{22}

  2. Atoms. Each H2OH_2O carries 3 nuclei: atoms=3N=1.81×1023\text{atoms} = 3N = 1.81 \times 10^{23}

  3. Volume of the drop. V=Mρ=1.8×1031000=1.8×106 m3V = \frac{M}{\rho} = \frac{1.8 \times 10^{-3}}{1000} = 1.8 \times 10^{-6} \ \text{m}^3

  4. Volume per molecule, then spacing. V1=VN=1.8×1066.022×1022=2.99×1029 m3V_1 = \frac{V}{N} = \frac{1.8 \times 10^{-6}}{6.022 \times 10^{22}} = 2.99 \times 10^{-29} \ \text{m}^3 rˉ=V11/3=3.10×1010 m=3.1 A˚\bar{r} = V_1^{1/3} = 3.10 \times 10^{-10} \ \text{m} = 3.1 \ \text{Å}

  5. Compare with Example 3. In the gas the spacing was 34.4 Å; in the liquid it is 3.1 Å — about 11 times smaller, so about 113130011^3 \approx 1300 times denser. That is the whole difference between a liquid and a gas in one number.

Final Answer: 6.02×10226.02 \times 10^{22} molecules, 1.81×10231.81 \times 10^{23} atoms, spacing 3.1\approx 3.1 Å.

Takeaway: In a liquid the spacing is essentially the molecular size; in a gas it is ten times larger. Every difference between the two phases — compressibility, fixed volume, intermolecular forces mattering — follows from that one factor of ten.

Part 2: The Ideal Gas Equation in All Four Forms

Six problems on the one equation that appears in four disguises. Pick the form whose symbols match the data you were handed, and check with a second form whenever you can.

Key Point: The four forms are PV=μRTPV = \mu RT (moles), PV=NkBTPV = Nk_BT (molecules), P=nkBTP = nk_BT (number density) and P=ρRTM0P = \frac{\rho R T}{M_0} (density). They are one equation. R=kBNAR = k_B N_A and M0=mNAM_0 = m N_A are the only bridges you need.

Example 7: One gas sample, all four forms

A rigid 2.0-litre vessel holds 8.0 g of oxygen (M0=32M_0 = 32 g/mol) at 300 K. Find its pressure four separate times, once from each form of the ideal gas equation.

Solution:

Constants: R=8.314R = 8.314 J/(mol K); kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K; NA=6.022×1023N_A = 6.022 \times 10^{23} per mole.

  1. The data in SI. V=2.0 L=2.0×103 m3,M=8.0 g=8.0×103 kgV = 2.0 \ \text{L} = 2.0 \times 10^{-3} \ \text{m}^3, \qquad M = 8.0 \ \text{g} = 8.0 \times 10^{-3} \ \text{kg} M0=32 g/mol=0.032 kg/molM_0 = 32 \ \text{g/mol} = 0.032 \ \text{kg/mol}

  2. Form 1 — moles. μ=MM0=8.032=0.25 mol\mu = \frac{M}{M_0} = \frac{8.0}{32} = 0.25 \ \text{mol} P=μRTV=0.25×8.314×3002.0×103=3.12×105 PaP = \frac{\mu RT}{V} = \frac{0.25 \times 8.314 \times 300}{2.0 \times 10^{-3}} = 3.12 \times 10^{5} \ \text{Pa}

  3. Form 2 — molecules. N=μNA=0.25×6.022×1023=1.51×1023N = \mu N_A = 0.25 \times 6.022 \times 10^{23} = 1.51 \times 10^{23} P=NkBTV=1.51×1023×1.38×1023×3002.0×103=3.12×105 PaP = \frac{Nk_BT}{V} = \frac{1.51 \times 10^{23} \times 1.38 \times 10^{-23} \times 300}{2.0 \times 10^{-3}} = 3.12 \times 10^{5} \ \text{Pa}

  4. Form 3 — number density. n=NV=1.5055×10232.0×103=7.53×1025 per m3n = \frac{N}{V} = \frac{1.5055 \times 10^{23}}{2.0 \times 10^{-3}} = 7.53 \times 10^{25} \ \text{per m}^3 P=nkBT=7.53×1025×1.38×1023×300=3.12×105 PaP = nk_BT = 7.53 \times 10^{25} \times 1.38 \times 10^{-23} \times 300 = 3.12 \times 10^{5} \ \text{Pa}

  5. Form 4 — density. ρ=MV=8.0×1032.0×103=4.0 kg/m3\rho = \frac{M}{V} = \frac{8.0 \times 10^{-3}}{2.0 \times 10^{-3}} = 4.0 \ \text{kg/m}^3 P=ρRTM0=4.0×8.314×3000.032=3.12×105 PaP = \frac{\rho R T}{M_0} = \frac{4.0 \times 8.314 \times 300}{0.032} = 3.12 \times 10^{5} \ \text{Pa}

Final Answer: P=3.12×105P = 3.12 \times 10^{5} Pa 3.08\approx 3.08 atm, by all four routes.

Takeaway: Choose the form whose symbols the question already gives you. Given a mass, use μ\mu or ρ\rho; given a count, use NN or nn. Converting the data to fit a memorised form is where the time and the marks go.

Example 8: Molar volume, at 27°C and at 0°C

Find the volume occupied by one mole of an ideal gas at 1 atm and 27°C. Then show that the same calculation at 0°C gives the familiar 22.4 litres.

Solution:

Constants: R=8.314R = 8.314 J/(mol K); 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. At 27°C. Kelvin first: T=27+273.15=300.15 KT = 27 + 273.15 = 300.15 \ \text{K} V=μRTP=1×8.314×300.151.013×105=2.463×102 m3=24.63 LV = \frac{\mu RT}{P} = \frac{1 \times 8.314 \times 300.15}{1.013 \times 10^{5}} = 2.463 \times 10^{-2} \ \text{m}^3 = 24.63 \ \text{L}

  2. At 0°C, which is T=273.15T = 273.15 K: V=1×8.314×273.151.013×105=2.242×102 m3=22.42 LV = \frac{1 \times 8.314 \times 273.15}{1.013 \times 10^{5}} = 2.242 \times 10^{-2} \ \text{m}^3 = 22.42 \ \text{L}

  3. Why the number is famous. Nothing in that line refers to which gas it is. One mole of helium, of oxygen and of carbon dioxide all occupy 22.4 L at 0°C and 1 atm — which is Avogadro's hypothesis, arriving as a consequence rather than an assumption.

  4. The ratio check. The two volumes should be in the ratio of the absolute temperatures: 24.6322.42=1.0986,300.15273.15=1.0988\frac{24.63}{22.42} = 1.0986, \qquad \frac{300.15}{273.15} = 1.0988 \quad \checkmark

Final Answer: 24.6324.63 L at 27°C; 22.4222.42 L at 0°C.

Takeaway: 22.4 litres is not a property of a gas — it is a property of a temperature and a pressure. Quoting it at room temperature is a standard slip; at 27°C the molar volume is nearly 25 litres.

Example 9: What does the air in a classroom weigh?

A classroom measures 8.0 m by 6.0 m by 3.5 m. The air in it is at 1 atm and 300 K, and its mean molar mass is 28.9 g/mol. Find the density of the air, the mass of air in the room, and the number of moles.

Solution:

Constants: R=8.314R = 8.314 J/(mol K); 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. Volume. V=8.0×6.0×3.5=168 m3V = 8.0 \times 6.0 \times 3.5 = 168 \ \text{m}^3

  2. Density, from the density form. Convert the molar mass first: M0=28.9 g/mol=0.0289 kg/molM_0 = 28.9 \ \text{g/mol} = 0.0289 \ \text{kg/mol} ρ=PM0RT=1.013×105×0.02898.314×300=2927.62494.2=1.17 kg/m3\rho = \frac{P M_0}{RT} = \frac{1.013 \times 10^{5} \times 0.0289}{8.314 \times 300} = \frac{2927.6}{2494.2} = 1.17 \ \text{kg/m}^3

  3. Mass. M=ρV=1.174×168=197 kgM = \rho V = 1.174 \times 168 = 197 \ \text{kg}

  4. Cross-check through moles. μ=PVRT=1.013×105×1688.314×300=6823 mol\mu = \frac{PV}{RT} = \frac{1.013 \times 10^{5} \times 168}{8.314 \times 300} = 6823 \ \text{mol} M=μM0=6823×0.0289=197 kgM = \mu M_0 = 6823 \times 0.0289 = 197 \ \text{kg} \quad \checkmark

Final Answer: ρ=1.17\rho = 1.17 kg/m3^3; about 197 kg of air; 6823 moles.

Takeaway: Air is not weightless — a small classroom holds about two hundred kilograms of it. You do not feel it because it pushes up on you as hard as it pushes down.

Example 10: Compressed and heated at the same time

A fixed mass of gas is at 2.0×1052.0 \times 10^{5} Pa in a volume of 3.0 litres at 300 K. It is compressed to 1.2 litres and simultaneously heated to 400 K. Find the new pressure.

Solution:

  1. Is the amount of gas fixed? Yes — nothing leaks. So μ\mu cancels and the combined form applies: P1V1T1=P2V2T2\frac{P_1V_1}{T_1} = \frac{P_2V_2}{T_2}

  2. Both temperatures are already absolute (300 K, 400 K), so no conversion is needed. Volumes may stay in litres because they appear as a ratio.

  3. Rearrange, then substitute. P2=P1×V1V2×T2T1=2.0×105×3.01.2×400300P_2 = P_1 \times \frac{V_1}{V_2} \times \frac{T_2}{T_1} = 2.0 \times 10^{5} \times \frac{3.0}{1.2} \times \frac{400}{300} P2=2.0×105×2.5×1.333=6.67×105 PaP_2 = 2.0 \times 10^{5} \times 2.5 \times 1.333 = 6.67 \times 10^{5} \ \text{Pa}

  4. Sense check. Squeezing raises the pressure, heating raises it further, so the answer must exceed 2.0×1052.0 \times 10^{5} Pa — and it does, by a factor of 103\frac{10}{3}.

Final Answer: P2=6.67×105P_2 = 6.67 \times 10^{5} Pa.

Takeaway: Write the ratio form, not PV=μRTPV = \mu RT, whenever the amount of gas is unchanged. Units that appear on both sides cancel, so litres and atmospheres are perfectly safe there — but kelvin is not optional.

Example 11: A gauge that does not read what you think

A nitrogen cylinder of volume 15 litres has a pressure gauge reading 12 atm at 300 K. Find the number of moles and the mass of nitrogen inside. Molar mass of nitrogen is 28 g/mol.

Solution:

Constants: R=8.314R = 8.314 J/(mol K); 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. The trap, dealt with first. A pressure gauge reads the excess over atmospheric. The gas equation wants the absolute pressure: P=Pgauge+Patm=12+1=13 atm=13×1.013×105=1.317×106 PaP = P_{\text{gauge}} + P_{\text{atm}} = 12 + 1 = 13 \ \text{atm} = 13 \times 1.013 \times 10^{5} = 1.317 \times 10^{6} \ \text{Pa}

  2. Volume in SI. V=15 L=1.5×102 m3V = 15 \ \text{L} = 1.5 \times 10^{-2} \ \text{m}^3

  3. Moles. μ=PVRT=1.317×106×1.5×1028.314×300=197532494.2=7.92 mol\mu = \frac{PV}{RT} = \frac{1.317 \times 10^{6} \times 1.5 \times 10^{-2}}{8.314 \times 300} = \frac{19753}{2494.2} = 7.92 \ \text{mol}

  4. Mass. M=μM0=7.92×28=222 gM = \mu M_0 = 7.92 \times 28 = 222 \ \text{g}

  5. What the trap costs. Using the gauge reading of 12 atm instead would give μ=7.31\mu = 7.31 mol and 205205 g — an error of nearly 8%, and it grows as the cylinder empties.

Final Answer: 7.927.92 mol, about 222 g of nitrogen.

Takeaway: Gauge pressure plus one atmosphere equals absolute pressure. Any problem that says "gauge" is testing that line and nothing else. Bubbles, tyres and cylinders are the usual settings.

Example 12: Pumping a room down to two per cent

A sealed room of volume 60 m3^3 contains air at 1 atm and 300 K. A pump reduces the pressure to 2% of atmospheric at the same temperature. How many molecules were removed, and what mass of air is that? Take the mean molar mass of air as 28.9 g/mol.

Solution:

Constants: R=8.314R = 8.314 J/(mol K); kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K; NA=6.022×1023N_A = 6.022 \times 10^{23} per mole.

  1. Moles at the start. μ1=P1VRT=1.013×105×608.314×300=6.078×1062494.2=2437 mol\mu_1 = \frac{P_1V}{RT} = \frac{1.013 \times 10^{5} \times 60}{8.314 \times 300} = \frac{6.078 \times 10^{6}}{2494.2} = 2437 \ \text{mol}

  2. Moles at the end. Same VV, same TT, so μP\mu \propto P: μ2=0.02×2437=48.7 mol\mu_2 = 0.02 \times 2437 = 48.7 \ \text{mol}

  3. Removed. Δμ=243748.7=2388 mol\Delta\mu = 2437 - 48.7 = 2388 \ \text{mol} ΔN=Δμ×NA=2388×6.022×1023=1.44×1027 molecules\Delta N = \Delta\mu \times N_A = 2388 \times 6.022 \times 10^{23} = 1.44 \times 10^{27} \ \text{molecules}

  4. Mass removed. ΔM=Δμ×M0=2388×0.0289=69.0 kg\Delta M = \Delta\mu \times M_0 = 2388 \times 0.0289 = 69.0 \ \text{kg}

  5. Cross-check the count directly. At the start, n1=P1kBT=1.013×1051.38×1023×300=2.45×1025 per m3n_1 = \frac{P_1}{k_BT} = \frac{1.013 \times 10^{5}}{1.38 \times 10^{-23} \times 300} = 2.45 \times 10^{25} \ \text{per m}^3 N1=n1V=1.47×1027,0.98N1=1.44×1027N_1 = n_1 V = 1.47 \times 10^{27}, \qquad 0.98 N_1 = 1.44 \times 10^{27} \quad \checkmark

Final Answer: about 1.44×10271.44 \times 10^{27} molecules, a mass of about 69 kg.

Takeaway: At constant volume and temperature, μ\mu, NN, nn and ρ\rho are all proportional to PP. Once you see that, "reduce the pressure to 2%" means "remove 98% of everything" without any further arithmetic.

Part 3: Leaks, Bubbles, Mixtures and Partial Pressures

Seven problems where either the amount of gas changes or there is more than one gas in the box. Both cases break the habit of reaching straight for P1V1T1=P2V2T2\frac{P_1V_1}{T_1} = \frac{P_2V_2}{T_2}.

A bubble rising through a lake and a gas cylinder before and after withdrawal

Example 13: The oxygen cylinder after a day's use

An oxygen cylinder of volume 40 litres has an initial gauge pressure of 20 atm at 27°C. After some oxygen is used, the gauge pressure has fallen to 14 atm and the temperature to 12°C. Estimate the mass of oxygen taken out. Molar mass of oxygen is 32 g/mol.

Solution:

Constants: R=8.314R = 8.314 J/(mol K); 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. Why the combined gas law is useless here. Gas has left the cylinder, so μ\mu is not the same at the two states. We must apply PV=μRTPV = \mu RT separately at each state and subtract.

  2. State 1, in absolute units. P1=(20+1) atm=21×1.013×105=2.127×106 PaP_1 = (20 + 1) \ \text{atm} = 21 \times 1.013 \times 10^{5} = 2.127 \times 10^{6} \ \text{Pa} T1=27+273.15=300.15 K,V=40 L=4.0×102 m3T_1 = 27 + 273.15 = 300.15 \ \text{K}, \qquad V = 40 \ \text{L} = 4.0 \times 10^{-2} \ \text{m}^3 μ1=P1VRT1=2.127×106×4.0×1028.314×300.15=850922495.4=34.10 mol\mu_1 = \frac{P_1V}{RT_1} = \frac{2.127 \times 10^{6} \times 4.0 \times 10^{-2}}{8.314 \times 300.15} = \frac{85092}{2495.4} = 34.10 \ \text{mol}

  3. State 2. P2=(14+1)×1.013×105=1.520×106 Pa,T2=12+273.15=285.15 KP_2 = (14 + 1) \times 1.013 \times 10^{5} = 1.520 \times 10^{6} \ \text{Pa}, \qquad T_2 = 12 + 273.15 = 285.15 \ \text{K} μ2=1.520×106×4.0×1028.314×285.15=607802370.6=25.64 mol\mu_2 = \frac{1.520 \times 10^{6} \times 4.0 \times 10^{-2}}{8.314 \times 285.15} = \frac{60780}{2370.6} = 25.64 \ \text{mol}

  4. Convert both to mass. With M0=32M_0 = 32 g/mol: M1=34.10×32=1091 g,M2=25.64×32=820 gM_1 = 34.10 \times 32 = 1091 \ \text{g}, \qquad M_2 = 25.64 \times 32 = 820 \ \text{g}

  5. Subtract. ΔM=1091820=271 g\Delta M = 1091 - 820 = 271 \ \text{g}

Final Answer: about 271271 g of oxygen was withdrawn.

Takeaway: A leak makes μ\mu a variable. The tell is a question that asks for a mass or a number rather than a pressure — you cannot get either out of a ratio equation in which μ\mu has already cancelled.

Example 14: The bubble that rises 25 metres

An air bubble of volume 2.0 cm3^3 forms at the bottom of a lake 25 m deep, where the water is at 15°C. It rises to the surface, where the temperature is 30°C. Find its volume there. Take the density of water as 1000 kg/m3^3, g=9.8g = 9.8 m/s2^2 and atmospheric pressure as 1.013×1051.013 \times 10^{5} Pa.

Solution:

  1. The pressure at the bottom is atmospheric plus the water column above: P1=Patm+ρgh=1.013×105+1000×9.8×25P_1 = P_{\text{atm}} + \rho g h = 1.013 \times 10^{5} + 1000 \times 9.8 \times 25 P1=1.013×105+2.45×105=3.463×105 Pa (=3.42 atm)P_1 = 1.013 \times 10^{5} + 2.45 \times 10^{5} = 3.463 \times 10^{5} \ \text{Pa} \ (= 3.42 \ \text{atm})

  2. The pressure at the surface is just atmospheric: P2=1.013×105 PaP_2 = 1.013 \times 10^{5} \ \text{Pa}

  3. Kelvin, both ends. T1=15+273.15=288.15 K,T2=30+273.15=303.15 KT_1 = 15 + 273.15 = 288.15 \ \text{K}, \qquad T_2 = 30 + 273.15 = 303.15 \ \text{K}

  4. The air inside the bubble is a fixed amount, so the combined form is the right tool: V2=V1×P1P2×T2T1=2.0×3.463×1051.013×105×303.15288.15V_2 = V_1 \times \frac{P_1}{P_2} \times \frac{T_2}{T_1} = 2.0 \times \frac{3.463 \times 10^{5}}{1.013 \times 10^{5}} \times \frac{303.15}{288.15} V2=2.0×3.419×1.052=7.19 cm3V_2 = 2.0 \times 3.419 \times 1.052 = 7.19 \ \text{cm}^3

  5. Which factor did the work? The pressure ratio contributed ×3.42\times 3.42 and the temperature ratio only ×1.05\times 1.05. The bubble grows because it is escaping the water, not because it is warming.

Final Answer: the bubble grows to about 7.27.2 cm3^3, roughly 3.63.6 times its original size.

Takeaway: A rising bubble is a pressure problem with a small temperature correction. Every 10.3 m of water adds one atmosphere, so a bubble doubles in volume in the first ten metres and grows more slowly after that.

Example 15: Helium and oxygen sharing one flask

A 5.0-litre flask at 300 K contains 4.0 g of helium (M0=4M_0 = 4 g/mol) and 16 g of oxygen (M0=32M_0 = 32 g/mol). Find the partial pressure of each gas, the total pressure, and the mole fraction of helium.

Solution:

Constants: R=8.314R = 8.314 J/(mol K); 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. Moles of each. μHe=4.04=1.00 mol,μO2=1632=0.50 mol\mu_{He} = \frac{4.0}{4} = 1.00 \ \text{mol}, \qquad \mu_{O_2} = \frac{16}{32} = 0.50 \ \text{mol}

  2. Partial pressure is the pressure each gas would exert alone in the whole 5.0 L: PHe=μHeRTV=1.00×8.314×3005.0×103=4.99×105 PaP_{He} = \frac{\mu_{He} RT}{V} = \frac{1.00 \times 8.314 \times 300}{5.0 \times 10^{-3}} = 4.99 \times 10^{5} \ \text{Pa} PO2=0.50×8.314×3005.0×103=2.49×105 PaP_{O_2} = \frac{0.50 \times 8.314 \times 300}{5.0 \times 10^{-3}} = 2.49 \times 10^{5} \ \text{Pa}

  3. Dalton's law — just add them. Ptotal=4.99×105+2.49×105=7.48×105 Pa=7.39 atmP_{\text{total}} = 4.99 \times 10^{5} + 2.49 \times 10^{5} = 7.48 \times 10^{5} \ \text{Pa} = 7.39 \ \text{atm}

  4. Mole fraction of helium. xHe=μHeμHe+μO2=1.001.50=0.667x_{He} = \frac{\mu_{He}}{\mu_{He} + \mu_{O_2}} = \frac{1.00}{1.50} = 0.667 and indeed PHePtotal=4.997.48=0.667\frac{P_{He}}{P_{\text{total}}} = \frac{4.99}{7.48} = 0.667, which is the same number — partial pressures are in the ratio of the mole numbers.

  5. Note what is equal and what is not. Both gases are at 300 K, so their molecules have the same average translational kinetic energy; but helium's molecules are 8 times lighter, so they move 8=2.83\sqrt{8} = 2.83 times faster.

Final Answer: PHe=4.99×105P_{He} = 4.99 \times 10^{5} Pa, PO2=2.49×105P_{O_2} = 2.49 \times 10^{5} Pa, total 7.48×1057.48 \times 10^{5} Pa; xHe=23x_{He} = \frac{2}{3}.

Takeaway: Equal masses are not equal moles, and only moles decide pressure. Four grams of helium beats sixteen grams of oxygen two to one, because a helium atom is eight times lighter.

Example 16: Adding a second gas without letting the first out

A 10-litre vessel holds nitrogen at 2.0 atm and 300 K. Now 8.0 g of helium (M0=4M_0 = 4 g/mol) is pumped in, the temperature being held at 300 K throughout. Find the new total pressure.

Solution:

Constants: R=8.314R = 8.314 J/(mol K); 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. The nitrogen does not care. Its volume and temperature are unchanged and none of it left, so its partial pressure is still PN2=2.0 atm=2.026×105 PaP_{N_2} = 2.0 \ \text{atm} = 2.026 \times 10^{5} \ \text{Pa} (For interest, μN2=PVRT=2.026×105×1028.314×300=0.812\mu_{N_2} = \frac{PV}{RT} = \frac{2.026 \times 10^{5} \times 10^{-2}}{8.314 \times 300} = 0.812 mol.)

  2. The helium's partial pressure, computed as though it were alone in the 10 litres: μHe=8.04=2.00 mol\mu_{He} = \frac{8.0}{4} = 2.00 \ \text{mol} PHe=μHeRTV=2.00×8.314×3001.0×102=4.99×105 Pa=4.92 atmP_{He} = \frac{\mu_{He}RT}{V} = \frac{2.00 \times 8.314 \times 300}{1.0 \times 10^{-2}} = 4.99 \times 10^{5} \ \text{Pa} = 4.92 \ \text{atm}

  3. Add. Ptotal=2.0+4.92=6.92 atm=7.01×105 PaP_{\text{total}} = 2.0 + 4.92 = 6.92 \ \text{atm} = 7.01 \times 10^{5} \ \text{Pa}

  4. Check by total moles. μtotal=0.812+2.00=2.812 mol\mu_{\text{total}} = 0.812 + 2.00 = 2.812 \ \text{mol} P=2.812×8.314×3001.0×102=7.01×105 PaP = \frac{2.812 \times 8.314 \times 300}{1.0 \times 10^{-2}} = 7.01 \times 10^{5} \ \text{Pa} \quad \checkmark

Final Answer: Ptotal=7.01×105P_{\text{total}} = 7.01 \times 10^{5} Pa, about 6.9 atm.

Takeaway: Adding a non-reacting gas never changes the pressure of the gas already there. Each species behaves as if the others were absent, which is Dalton's law and, molecularly, a consequence of the molecules not interacting.

Example 17: Forty per cent leaks out while the tank warms up

A rigid tank contains gas at 4.0×1054.0 \times 10^{5} Pa and 300 K. A slow leak removes 40% of the molecules, and by the time it is noticed the temperature has risen to 350 K. Find the new pressure.

Solution:

  1. Which quantities changed? VV is fixed. NN fell to 0.600.60 of its value. TT rose from 300 K to 350 K. Both temperatures are already absolute.

  2. Use the form with NN in it, because NN is what changed: P=NkBTVP2P1=N2N1×T2T1P = \frac{Nk_BT}{V} \quad\Longrightarrow\quad \frac{P_2}{P_1} = \frac{N_2}{N_1}\times\frac{T_2}{T_1}

  3. Substitute. P2P1=0.60×350300=0.60×1.1667=0.70\frac{P_2}{P_1} = 0.60 \times \frac{350}{300} = 0.60 \times 1.1667 = 0.70 P2=0.70×4.0×105=2.80×105 PaP_2 = 0.70 \times 4.0 \times 10^{5} = 2.80 \times 10^{5} \ \text{Pa}

  4. Reading the answer. The leak alone would have taken the pressure to 2.40×1052.40 \times 10^{5} Pa; the warming pushed it back up to 2.80×1052.80 \times 10^{5} Pa. A leak can be masked by a temperature rise, which is exactly why gas cylinders are checked at a stated temperature.

Final Answer: P2=2.80×105P_2 = 2.80 \times 10^{5} Pa.

Takeaway: When the amount of gas changes, put NN (or μ\mu) into the ratio explicitly: P2P1=N2N1V1V2T2T1\frac{P_2}{P_1} = \frac{N_2}{N_1}\cdot\frac{V_1}{V_2}\cdot\frac{T_2}{T_1}. Dropping the first factor is the standard error.

Example 18: Taking the water vapour out of moist air

A closed vessel at 40°C holds moist air at a total pressure of 1.0 atm. At that temperature the partial pressure of the water vapour is 7.4 kPa. Find the partial pressure of the dry air, and the fraction of the molecules in the vessel that are water molecules.

Solution:

Constants: 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. Dalton's law, rearranged. The total is the sum of the parts: Pdry=PtotalPwater=1.013×1057.4×103=9.39×104 PaP_{\text{dry}} = P_{\text{total}} - P_{\text{water}} = 1.013 \times 10^{5} - 7.4 \times 10^{3} = 9.39 \times 10^{4} \ \text{Pa}

  2. Fraction of molecules. At a common VV and TT, PNP \propto N, so the mole fraction and the pressure fraction are the same number: xwater=PwaterPtotal=7.4×1031.013×105=0.0731=7.3%x_{\text{water}} = \frac{P_{\text{water}}}{P_{\text{total}}} = \frac{7.4 \times 10^{3}}{1.013 \times 10^{5}} = 0.0731 = 7.3\%

  3. What this does not depend on. Nothing here needed the molar mass of water or of air. Partial pressures count molecules, not mass — the 7.3% is a fraction by number, and because water (18 g/mol) is lighter than air (28.9 g/mol) the fraction by mass is smaller, about 4.6%.

Final Answer: dry air 9.39×1049.39 \times 10^{4} Pa; water vapour is about 7.3% of the molecules.

Takeaway: A partial-pressure fraction is a fraction by number of molecules. Convert it to a mass fraction only by bringing in the molar masses; the two are equal only if the gases happen to have the same M0M_0.

Example 19: Three gases, one flask, one mean molar mass

A 20-litre vessel at 400 K holds 2.0 g of hydrogen, 28 g of nitrogen and 44 g of carbon dioxide. Find the total pressure, the mean molar mass of the mixture, and check the answer through the density form of the gas equation. Molar masses: H2H_2 2, N2N_2 28, CO2CO_2 44 g/mol.

Solution:

Constants: R=8.314R = 8.314 J/(mol K); 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. Moles of each — each comes out to a whole number here. μH2=2.02=1,μN2=2828=1,μCO2=4444=1\mu_{H_2} = \frac{2.0}{2} = 1, \qquad \mu_{N_2} = \frac{28}{28} = 1, \qquad \mu_{CO_2} = \frac{44}{44} = 1 μtotal=3.0 mol\mu_{\text{total}} = 3.0 \ \text{mol}

  2. Total pressure. P=μtotalRTV=3.0×8.314×4002.0×102=4.99×105 Pa=4.92 atmP = \frac{\mu_{\text{total}}RT}{V} = \frac{3.0 \times 8.314 \times 400}{2.0 \times 10^{-2}} = 4.99 \times 10^{5} \ \text{Pa} = 4.92 \ \text{atm} Each gas contributes exactly one third of this, 1.66×1051.66 \times 10^{5} Pa, because each supplies one third of the moles.

  3. Mean molar mass is total mass over total moles: M0,mean=2.0+28+443.0=743.0=24.7 g/mol=0.0247 kg/molM_{0,\text{mean}} = \frac{2.0 + 28 + 44}{3.0} = \frac{74}{3.0} = 24.7 \ \text{g/mol} = 0.0247 \ \text{kg/mol}

  4. Check through the density form. ρ=MV=74×1032.0×102=3.70 kg/m3\rho = \frac{M}{V} = \frac{74 \times 10^{-3}}{2.0 \times 10^{-2}} = 3.70 \ \text{kg/m}^3 P=ρRTM0,mean=3.70×8.314×4000.0247=4.99×105 PaP = \frac{\rho R T}{M_{0,\text{mean}}} = \frac{3.70 \times 8.314 \times 400}{0.0247} = 4.99 \times 10^{5} \ \text{Pa} \quad \checkmark

Final Answer: P=4.99×105P = 4.99 \times 10^{5} Pa; mean molar mass 24.724.7 g/mol.

Takeaway: A mixture obeys the gas equation with a mean molar mass defined as total mass divided by total moles, M0,mean=μiM0,iμiM_{0,\text{mean}} = \frac{\sum \mu_i M_{0,i}}{\sum \mu_i}. It is a mole-weighted average, not a plain one. Here the moles happened to be equal so the two coincide; take 4 g of hydrogen instead of 2 g and the mean drops to 1919 g/mol while the plain average of 22, 2828 and 4444 stays put.

Part 4: The Pressure Formula, Forwards and Backwards

Five problems on P=13nmv2=13ρv2P = \frac{1}{3}nm\overline{v^2} = \frac{1}{3}\rho\,\overline{v^2} — the one result that connects a mechanical push on a wall to the motion of individual molecules. Half the questions give you speeds and want a pressure; the other half do the reverse.

Key Point: P=13ρv2P = \frac{1}{3}\rho\,\overline{v^2} contains the mean of the squares v2\overline{v^2}, never the square of the mean. Rearranged, v2=vrms=3Pρ\sqrt{\overline{v^2}} = v_{rms} = \sqrt{\frac{3P}{\rho}} — which is why a pressure and a density alone are enough to get an rms speed, with no thermometer anywhere.

Example 20: Pressure from a density and a speed

Carbon dioxide has a density of 1.98 kg/m3^3 and its molecules have an rms speed of 393 m/s. Find the pressure of the gas.

Solution:

  1. The formula, in the form the data fits. We were handed a density, so use P=13ρv2P = \frac{1}{3}\rho\,\overline{v^2}

  2. Which speed is this? The formula wants the mean square speed, and vrmsv_{rms} is by definition its square root, so v2=vrms2\overline{v^2} = v_{rms}^2. Substituting vˉ\bar{v} or vmpv_{mp} here would be wrong. v2=(393)2=1.544×105 m2/s2\overline{v^2} = (393)^2 = 1.544 \times 10^{5} \ \text{m}^2/\text{s}^2

  3. Substitute. P=13×1.98×1.544×105=1.02×105 PaP = \frac{1}{3} \times 1.98 \times 1.544 \times 10^{5} = 1.02 \times 10^{5} \ \text{Pa}

  4. Sense check. That is 1.011.01 atm — and 1.98 kg/m3^3 is indeed close to the density of carbon dioxide at atmospheric pressure and room temperature, so the numbers hang together.

Final Answer: P1.02×105P \approx 1.02 \times 10^{5} Pa, essentially one atmosphere.

Takeaway: v2\overline{v^2} means vrms2v_{rms}^2. Any speed offered to this formula must be the rms one; if a problem gives you vˉ\bar{v} instead, convert first using vrms=3π8vˉ=1.085vˉv_{rms} = \sqrt{\frac{3\pi}{8}}\,\bar{v} = 1.085\,\bar{v}.

Example 21: Running the formula backwards to name the gas

A gas at 1.5×1051.5 \times 10^{5} Pa has a density of 2.4 kg/m3^3 and a temperature of 300 K. Find the rms speed of its molecules and identify the gas.

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. Which speed? The formula P=13ρv2P = \frac{1}{3}\rho\,\overline{v^2} contains the mean square speed, so rearranging it yields vrmsv_{rms} and nothing else. Speed straight from pressure and density — no temperature needed for this step: vrms=3Pρ=3×1.5×1052.4=1.875×105=433 m/sv_{rms} = \sqrt{\frac{3P}{\rho}} = \sqrt{\frac{3 \times 1.5 \times 10^{5}}{2.4}} = \sqrt{1.875 \times 10^{5}} = 433 \ \text{m/s}

  2. Now bring in the temperature to get the molar mass. Since vrms=3RTM0v_{rms} = \sqrt{\frac{3RT}{M_0}}, M0=3RTvrms2=3×8.314×3001.875×105=7482.61.875×105=0.0399 kg/molM_0 = \frac{3RT}{v_{rms}^2} = \frac{3 \times 8.314 \times 300}{1.875 \times 10^{5}} = \frac{7482.6}{1.875 \times 10^{5}} = 0.0399 \ \text{kg/mol}

  3. Convert back to the familiar unit. M0=0.0399 kg/mol=39.9 g/molM_0 = 0.0399 \ \text{kg/mol} = 39.9 \ \text{g/mol} That is argon.

  4. Round trip. Feeding M0=0.0399M_0 = 0.0399 kg/mol back in: vrms=3×8.314×3000.0399=433 m/sv_{rms} = \sqrt{\frac{3 \times 8.314 \times 300}{0.0399}} = 433 \ \text{m/s} \quad \checkmark

Final Answer: vrms=433v_{rms} = 433 m/s; the gas is argon, M0=39.9M_0 = 39.9 g/mol.

Takeaway: A molar mass in kg/mol comes out as a number like 0.0400.040, and a molar mass in g/mol as a number like 4040. If your rearranged formula produces 39.939.9 where kg/mol is expected, you have dropped a factor of 1000 somewhere.

Example 22: Which average does the pressure formula want?

Five molecules have speeds 300, 400, 500, 600 and 700 m/s. Find the mean speed, the mean square speed, the rms speed, and the square of the mean speed. Which of these belongs in P=13ρv2P = \frac{1}{3}\rho\,\overline{v^2}?

Solution:

  1. Mean speed — add and divide: vˉ=300+400+500+600+7005=25005=500 m/s\bar{v} = \frac{300 + 400 + 500 + 600 + 700}{5} = \frac{2500}{5} = 500 \ \text{m/s}

  2. Mean square speed — square first, then average: v2=3002+4002+5002+6002+70025=1,350,0005=2.70×105 m2/s2\overline{v^2} = \frac{300^2 + 400^2 + 500^2 + 600^2 + 700^2}{5} = \frac{1{,}350{,}000}{5} = 2.70 \times 10^{5} \ \text{m}^2/\text{s}^2

  3. Root mean square speed. vrms=2.70×105=519.6 m/sv_{rms} = \sqrt{2.70 \times 10^{5}} = 519.6 \ \text{m/s}

  4. Square of the mean, for contrast: (vˉ)2=5002=2.50×105 m2/s2(\bar{v})^2 = 500^2 = 2.50 \times 10^{5} \ \text{m}^2/\text{s}^2

  5. Compare. v2=2.70×105\overline{v^2} = 2.70 \times 10^5 but (vˉ)2=2.50×105(\bar{v})^2 = 2.50 \times 10^5 — using the square of the mean falls short of the true mean square by 2.702.502.70=7.4%\frac{2.70 - 2.50}{2.70} = 7.4\%, and vrmsv_{rms} exceeds vˉ\bar{v} by 3.9%. They are equal only if every molecule has the same speed; any spread at all makes vrms>vˉv_{rms} > \bar{v}.

  6. The answer to the question asked. The pressure formula and the energy formula both want v2\overline{v^2}, so PP here would use 2.70×1052.70 \times 10^{5} m2^2/s2^2.

Final Answer: vˉ=500\bar{v} = 500 m/s, v2=2.70×105\overline{v^2} = 2.70 \times 10^{5} m2^2/s2^2, vrms=519.6v_{rms} = 519.6 m/s, (vˉ)2=2.50×105(\bar{v})^2 = 2.50 \times 10^{5} m2^2/s2^2. Use v2\overline{v^2}.

Takeaway: v2(vˉ)2\overline{v^2} \neq (\bar{v})^2, always v2>(vˉ)2\overline{v^2} > (\bar{v})^2. Squaring rewards the fast molecules twice over. Using 12m(vˉ)2\frac{1}{2}m(\bar{v})^2 for the average kinetic energy underestimates it — here by 7.4%, and for a real Maxwellian gas by exactly 183π=15.1%1 - \frac{8}{3\pi} = 15.1\%. An underestimate is always measured against the true, larger value, so the denominator is v2\overline{v^2}, never (vˉ)2(\bar{v})^2.

Example 23: Squeezing the gas without warming it

Air at 1.0×1051.0 \times 10^{5} Pa has a density of 1.29 kg/m3^3. It is compressed isothermally to half its volume. Find the rms speed before and after, and the new pressure.

Solution:

  1. Before. vrms=3Pρ=3×1.0×1051.29=2.326×105=482 m/sv_{rms} = \sqrt{\frac{3P}{\rho}} = \sqrt{\frac{3 \times 1.0 \times 10^{5}}{1.29}} = \sqrt{2.326 \times 10^{5}} = 482 \ \text{m/s}

  2. What halving the volume does. The mass of gas is unchanged, so ρ2=2ρ1=2.58 kg/m3\rho_2 = 2\rho_1 = 2.58 \ \text{kg/m}^3 and at constant temperature Boyle's law gives P2=2P1=2.0×105P_2 = 2P_1 = 2.0 \times 10^{5} Pa.

  3. After. vrms=3×2.0×1052.58=2.326×105=482 m/sv_{rms} = \sqrt{\frac{3 \times 2.0 \times 10^{5}}{2.58}} = \sqrt{2.326 \times 10^{5}} = 482 \ \text{m/s} Identical, to every digit.

  4. Why it had to be. vrms=3RTM0v_{rms} = \sqrt{\frac{3RT}{M_0}} depends on temperature and molar mass and on nothing else. The compression was isothermal, so the speeds could not have changed. The pressure doubled purely because the molecules are hitting the walls twice as often, not because they are hitting harder.

Final Answer: vrms=482v_{rms} = 482 m/s both before and after; P2=2.0×105P_2 = 2.0 \times 10^{5} Pa.

Takeaway: Pressure has two ingredients — how hard each hit is, and how many hits per second. Isothermal compression changes only the second. A question that says "compressed isothermally" and then asks about molecular speed is asking you to answer "unchanged".

Example 24: The translational energy of the air in a room

A room of volume 60 m3^3 holds air at 1 atm and 300 K. Find the total translational kinetic energy of all the air molecules in it.

Solution:

Constants: R=8.314R = 8.314 J/(mol K); 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. The shortcut. Kinetic theory gives PV=23EPV = \frac{2}{3}E, where EE is the total translational kinetic energy. So E=32PVE = \frac{3}{2}PV

  2. Substitute — no temperature, no molar mass, no molecule count required. E=32×1.013×105×60=9.12×106 JE = \frac{3}{2} \times 1.013 \times 10^{5} \times 60 = 9.12 \times 10^{6} \ \text{J}

  3. Check by the long road. μ=PVRT=1.013×105×608.314×300=2437 mol\mu = \frac{PV}{RT} = \frac{1.013 \times 10^{5} \times 60}{8.314 \times 300} = 2437 \ \text{mol} E=32μRT=32×2437×8.314×300=9.12×106 JE = \frac{3}{2}\mu RT = \frac{3}{2} \times 2437 \times 8.314 \times 300 = 9.12 \times 10^{6} \ \text{J} \quad \checkmark

  4. Is it a big number? It is about the energy of a 1500 kg car travelling at 110 m/s. It is completely unavailable as useful work, because it is disordered — which is the entire subject of the previous chapter.

  5. A warning about EE and UU. Air is mostly diatomic, so its molecules also rotate. Its internal energy is U=52μRT=1.52×107U = \frac{5}{2}\mu RT = 1.52 \times 10^{7} J, larger than EE by a factor of 53\frac{5}{3}. The question asked for translational energy, so 9.12×1069.12 \times 10^{6} J is the answer.

Final Answer: E=9.12×106E = 9.12 \times 10^{6} J of translational kinetic energy.

Takeaway: E=32PVE = \frac{3}{2}PV needs only a pressure and a volume. But EE is translational only — for anything other than a monatomic gas, U>EU > E, and reading one symbol for the other is a favourite trap.

Part 5: Temperature, Molecular Energy and the rms Speed

Seven problems on the two results that make temperature mean something: 12mv2=32kBT\frac{1}{2}m\overline{v^2} = \frac{3}{2}k_BT per molecule, and vrms=3RTM0v_{rms} = \sqrt{\frac{3RT}{M_0}}. Every speed below shows the conversion of M0M_0 to kg/mol on a line of its own — that conversion is where this chapter's marks are won and lost.

Key Point: At a given temperature every gas has the same average translational kinetic energy per molecule, 32kBT\frac{3}{2}k_BT. It does not have the same speed: heavier molecules carry that energy more slowly, with vrms1M0v_{rms} \propto \frac{1}{\sqrt{M_0}}.

Example 25: A helium atom from a warm room to a stellar core

Estimate the average translational kinetic energy of a helium atom, and its rms speed, at (i) room temperature 27°C, (ii) 6000 K, the temperature of the Sun's visible surface, and (iii) 1.0×1071.0 \times 10^{7} K, a typical stellar core. Molar mass of helium is 4.0 g/mol.

Solution:

Constants: kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K; R=8.314R = 8.314 J/(mol K). 11 eV =1.6×1019= 1.6 \times 10^{-19} J.

  1. Convert the molar mass once, for all three parts: M0=4.0 g/mol=0.0040 kg/molM_0 = 4.0 \ \text{g/mol} = 0.0040 \ \text{kg/mol}

  2. Which speed? The question asks for a speed tied to an energy, so it is vrmsv_{rms} — the only one of the three that comes directly out of 12mv2=32kBT\frac{1}{2}m\overline{v^2} = \frac{3}{2}k_BT.

  3. (i) At T=27+273.15=300.15300T = 27 + 273.15 = 300.15 \approx 300 K. ε=32kBT=32(1.38×1023)(300)=6.21×1021 J=0.039 eV\overline{\varepsilon} = \frac{3}{2}k_BT = \frac{3}{2}(1.38 \times 10^{-23})(300) = 6.21 \times 10^{-21} \ \text{J} = 0.039 \ \text{eV} vrms=3RTM0=3×8.314×3000.0040=1.871×106=1.37×103 m/sv_{rms} = \sqrt{\frac{3RT}{M_0}} = \sqrt{\frac{3 \times 8.314 \times 300}{0.0040}} = \sqrt{1.871 \times 10^{6}} = 1.37 \times 10^{3} \ \text{m/s}

  4. (ii) At T=6000T = 6000 K — twenty times hotter, so the energy is twenty times larger and the speed 20=4.47\sqrt{20} = 4.47 times larger: ε=32(1.38×1023)(6000)=1.24×1019 J=0.78 eV\overline{\varepsilon} = \frac{3}{2}(1.38 \times 10^{-23})(6000) = 1.24 \times 10^{-19} \ \text{J} = 0.78 \ \text{eV} vrms=3×8.314×60000.0040=6.12×103 m/sv_{rms} = \sqrt{\frac{3 \times 8.314 \times 6000}{0.0040}} = 6.12 \times 10^{3} \ \text{m/s}

  5. (iii) At T=1.0×107T = 1.0 \times 10^{7} K. ε=32(1.38×1023)(1.0×107)=2.07×1016 J=1.29×103 eV\overline{\varepsilon} = \frac{3}{2}(1.38 \times 10^{-23})(1.0 \times 10^{7}) = 2.07 \times 10^{-16} \ \text{J} = 1.29 \times 10^{3} \ \text{eV} vrms=3×8.314×1.0×1070.0040=2.50×105 m/sv_{rms} = \sqrt{\frac{3 \times 8.314 \times 1.0 \times 10^{7}}{0.0040}} = 2.50 \times 10^{5} \ \text{m/s}

  6. What the last line means physically. About 1.3 keV per atom is comfortably more than the 24.6 eV needed to ionise helium — which is why a stellar core is a plasma of bare nuclei and free electrons, not a gas of atoms.

Final Answer: 6.21×10216.21 \times 10^{-21} J and 1.371.37 km/s; 1.24×10191.24 \times 10^{-19} J and 6.126.12 km/s; 2.07×10162.07 \times 10^{-16} J and 2.50×1022.50 \times 10^{2} km/s.

Takeaway: Energy scales as TT; speed scales as T\sqrt{T}. Raising the temperature by a factor of 3.3×1043.3 \times 10^{4} raised the speed by only 3.3×104=183\sqrt{3.3 \times 10^{4}} = 183.

Example 26: Carbon dioxide, by both roads

Find the rms speed of carbon dioxide molecules at 300 K, once from the molar mass and once from the mass of a single molecule. Molar mass of CO2CO_2 is 44 g/mol.

Solution:

Constants: R=8.314R = 8.314 J/(mol K); kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K; NA=6.022×1023N_A = 6.022 \times 10^{23} per mole.

  1. Convert the molar mass — its own line, always: M0=44 g/mol=0.044 kg/molM_0 = 44 \ \text{g/mol} = 0.044 \ \text{kg/mol}

  2. Which speed? vrmsv_{rms}, because the question names it. (For reference at this temperature vˉ=380\bar{v} = 380 m/s and vmp=337v_{mp} = 337 m/s — all three differ, so naming one matters.)

  3. Route A — molar. vrms=3RTM0=3×8.314×3000.044=1.701×105=412 m/sv_{rms} = \sqrt{\frac{3RT}{M_0}} = \sqrt{\frac{3 \times 8.314 \times 300}{0.044}} = \sqrt{1.701 \times 10^{5}} = 412 \ \text{m/s}

  4. Route B — per molecule. First the mass of one CO2CO_2 molecule: m=M0NA=0.0446.022×1023=7.31×1026 kgm = \frac{M_0}{N_A} = \frac{0.044}{6.022 \times 10^{23}} = 7.31 \times 10^{-26} \ \text{kg} then vrms=3kBTm=3×1.38×1023×3007.31×1026=1.700×105=412 m/sv_{rms} = \sqrt{\frac{3k_BT}{m}} = \sqrt{\frac{3 \times 1.38 \times 10^{-23} \times 300}{7.31 \times 10^{-26}}} = \sqrt{1.700 \times 10^{5}} = 412 \ \text{m/s}

  5. They agree, as they must, since R=kBNAR = k_BN_A and M0=mNAM_0 = mN_A make the two expressions algebraically identical. Any disagreement bigger than rounding means a factor of NAN_A went astray.

Final Answer: vrms412v_{rms} \approx 412 m/s by both routes.

Takeaway: 3RTM0\sqrt{\frac{3RT}{M_0}} and 3kBTm\sqrt{\frac{3k_BT}{m}} are the same formula wearing different clothes. Use whichever matches the data; use both if you have thirty spare seconds.

Example 27: Warming argon until it matches helium

At what temperature will the rms speed of argon atoms equal the rms speed of helium atoms at 20-20°C? Atomic masses: argon 39.9 u, helium 4.0 u.

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. Kelvin, before anything else. THe=20+273.15=253.15 KT_{He} = -20 + 273.15 = 253.15 \ \text{K} A negative Celsius value entering a speed formula unconverted is the classic way to lose this question.

  2. Convert both molar masses: M0,He=4.0 g/mol=0.0040 kg/mol,M0,Ar=39.9 g/mol=0.0399 kg/molM_{0,He} = 4.0 \ \text{g/mol} = 0.0040 \ \text{kg/mol}, \qquad M_{0,Ar} = 39.9 \ \text{g/mol} = 0.0399 \ \text{kg/mol}

  3. Set the two rms speeds equal. We use vrmsv_{rms} because the question does; the ratio would be identical for vˉ\bar{v} or vmpv_{mp}, since all three carry the same T/M0\sqrt{T/M_0}: 3RTArM0,Ar=3RTHeM0,HeTArM0,Ar=THeM0,He\sqrt{\frac{3RT_{Ar}}{M_{0,Ar}}} = \sqrt{\frac{3RT_{He}}{M_{0,He}}} \quad\Longrightarrow\quad \frac{T_{Ar}}{M_{0,Ar}} = \frac{T_{He}}{M_{0,He}}

  4. Solve. TAr=THe×M0,ArM0,He=253.15×39.94.0=253.15×9.975=2525 KT_{Ar} = T_{He}\times\frac{M_{0,Ar}}{M_{0,He}} = 253.15 \times \frac{39.9}{4.0} = 253.15 \times 9.975 = 2525 \ \text{K} which is 2525273.15=22522525 - 273.15 = 2252°C.

  5. Check both speeds explicitly. vHe=3×8.314×253.150.0040=1256 m/s,vAr=3×8.314×25250.0399=1256 m/sv_{He} = \sqrt{\frac{3 \times 8.314 \times 253.15}{0.0040}} = 1256 \ \text{m/s}, \qquad v_{Ar} = \sqrt{\frac{3 \times 8.314 \times 2525}{0.0399}} = 1256 \ \text{m/s} \quad \checkmark

Final Answer: TAr2525T_{Ar} \approx 2525 K, about 2252°C.

Takeaway: Equal speeds means equal TM0\frac{T}{M_0}, not equal TT. The heavier gas always needs the hotter oven, by exactly the ratio of the molar masses.

Example 28: Three vessels of equal capacity

Three identical vessels at the same temperature and pressure contain neon (monatomic, 20.2 g/mol), chlorine (diatomic, 70.9 g/mol) and sulphur hexafluoride (polyatomic, 146 g/mol). (a) Do they contain equal numbers of molecules? (b) Is vrmsv_{rms} the same in the three? If not, where is it largest? Compute all three at 300 K.

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. (a) The count. From PV=NkBTPV = Nk_BT, with PP, VV and TT all equal, NN must be equal too. Yes — equal numbers of molecules, whatever the gas. That is Avogadro's hypothesis restated.

  2. (b) The speeds. vrms=3RTM0v_{rms} = \sqrt{\frac{3RT}{M_0}} contains M0M_0, so the speeds are not equal; the lightest gas is the fastest. Convert all three molar masses: M0,Ne=0.0202,M0,Cl2=0.0709,M0,SF6=0.146 kg/molM_{0,Ne} = 0.0202, \qquad M_{0,Cl_2} = 0.0709, \qquad M_{0,SF_6} = 0.146 \ \text{kg/mol}

  3. Compute, using vrmsv_{rms} because that is the speed the question names: vNe=3×8.314×3000.0202=609 m/sv_{Ne} = \sqrt{\frac{3 \times 8.314 \times 300}{0.0202}} = 609 \ \text{m/s} vCl2=3×8.314×3000.0709=325 m/sv_{Cl_2} = \sqrt{\frac{3 \times 8.314 \times 300}{0.0709}} = 325 \ \text{m/s} vSF6=3×8.314×3000.146=226 m/sv_{SF_6} = \sqrt{\frac{3 \times 8.314 \times 300}{0.146}} = 226 \ \text{m/s}

  4. Check the ratio. vNevSF6\frac{v_{Ne}}{v_{SF_6}} should be 14620.2=7.23=2.69\sqrt{\frac{146}{20.2}} = \sqrt{7.23} = 2.69, and 609226=2.69\frac{609}{226} = 2.69. \checkmark

  5. One thing that IS equal. All three are at 300 K, so the average translational kinetic energy per molecule is 32kBT=6.21×1021\frac{3}{2}k_BT = 6.21 \times 10^{-21} J in every vessel. Note that the internal energies differ, because neon has f=3f = 3 while the others have more.

Final Answer: (a) yes, equal numbers. (b) no — 609609, 325325 and 226226 m/s; neon is fastest.

Takeaway: Same PP, VV, TT means same NN and same energy per molecule, but never the same speed. Sort speeds by molar mass and you can answer this style of question without a calculator.

Example 29: Telling two isotopes of neon apart

Naturally occurring neon contains the isotopes of mass 20 u and 22 u. At the same temperature, by what percentage does the rms speed of the lighter isotope exceed that of the heavier? Compute both at 300 K.

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. Convert both molar masses: M0,20=20 g/mol=0.020 kg/mol,M0,22=22 g/mol=0.022 kg/molM_{0,20} = 20 \ \text{g/mol} = 0.020 \ \text{kg/mol}, \qquad M_{0,22} = 22 \ \text{g/mol} = 0.022 \ \text{kg/mol}

  2. The ratio. At a common TT, everything except M0M_0 cancels — and it cancels identically for vrmsv_{rms}, vˉ\bar{v} and vmpv_{mp}, so the answer does not depend on which of the three we choose. We use vrmsv_{rms}: v20v22=M0,22M0,20=2220=1.10=1.0488\frac{v_{20}}{v_{22}} = \sqrt{\frac{M_{0,22}}{M_{0,20}}} = \sqrt{\frac{22}{20}} = \sqrt{1.10} = 1.0488

  3. As a percentage. (1.04881)×100=4.9%(1.0488 - 1)\times 100 = 4.9\%

  4. The two speeds at 300 K, for scale. v20=3×8.314×3000.020=612 m/s,v22=3×8.314×3000.022=583 m/sv_{20} = \sqrt{\frac{3 \times 8.314 \times 300}{0.020}} = 612 \ \text{m/s}, \qquad v_{22} = \sqrt{\frac{3 \times 8.314 \times 300}{0.022}} = 583 \ \text{m/s}

  5. Why anyone cares. A 4.9% speed difference is enough to separate the isotopes by repeated diffusion — a slow process, since each pass enriches the mixture only slightly, but a workable one. It is how neon isotopes were first separated, and the same principle at a far worse mass ratio is used for uranium.

Final Answer: the lighter isotope is faster by about 4.9%; 612612 m/s against 583583 m/s at 300 K.

Takeaway: Isotope separation lives on v1M0v \propto \frac{1}{\sqrt{M_0}}. Because of the square root, a 10% mass difference buys only a 4.9% speed difference — which is exactly why the process needs so many stages.

Example 30: Faster than a bullet?

Find the rms speed of nitrogen molecules at 300 K (molar mass 28 g/mol), and compare it with a rifle bullet at 800 m/s. To what temperature would the nitrogen have to be raised for its molecules to have an rms speed of 800 m/s?

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. Convert the molar mass: M0=28 g/mol=0.028 kg/molM_0 = 28 \ \text{g/mol} = 0.028 \ \text{kg/mol}

  2. The speed now. We use vrmsv_{rms} because the comparison is with a definite kinetic energy: vrms=3RTM0=3×8.314×3000.028=2.672×105=517 m/sv_{rms} = \sqrt{\frac{3RT}{M_0}} = \sqrt{\frac{3 \times 8.314 \times 300}{0.028}} = \sqrt{2.672 \times 10^{5}} = 517 \ \text{m/s} So an ordinary nitrogen molecule in this room moves at about two thirds the speed of a rifle bullet.

  3. The temperature that would match the bullet. Rearranging, T=M0vrms23R=0.028×(800)23×8.314=1792024.94=718 KT = \frac{M_0 v_{rms}^2}{3R} = \frac{0.028 \times (800)^2}{3 \times 8.314} = \frac{17920}{24.94} = 718 \ \text{K} which is 718273.15=445718 - 273.15 = 445°C.

  4. Check with the scaling law. Tv2T \propto v^2, so T=300×(800517)2=300×2.395=718 KT = 300 \times \left(\frac{800}{517}\right)^2 = 300 \times 2.395 = 718 \ \text{K} \quad \checkmark

Final Answer: vrms=517v_{rms} = 517 m/s at 300 K; T=718T = 718 K (about 445°C) for 800 m/s.

Takeaway: Molecular speeds are comparable to the speed of sound and to bullets — a few hundred metres per second — which is not a coincidence: sound travels by molecular collisions, so it cannot outrun the molecules themselves.

Example 31: The same energy, very different speeds

A vessel holds a mixture of helium (4 g/mol) and oxygen (32 g/mol) at 300 K. Find the average translational kinetic energy of a molecule of each, and the rms speed of each. Which is larger, and by how much?

Solution:

Constants: kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K; R=8.314R = 8.314 J/(mol K).

  1. Energy first — and it is the same for both. ε=32kBT\overline{\varepsilon} = \frac{3}{2}k_BT contains no mass: ε=32(1.38×1023)(300)=6.21×1021 Jfor helium and for oxygen alike\overline{\varepsilon} = \frac{3}{2}(1.38 \times 10^{-23})(300) = 6.21 \times 10^{-21} \ \text{J} \quad \text{for helium and for oxygen alike}

  2. Convert both molar masses: M0,He=4 g/mol=0.004 kg/mol,M0,O2=32 g/mol=0.032 kg/molM_{0,He} = 4 \ \text{g/mol} = 0.004 \ \text{kg/mol}, \qquad M_{0,O_2} = 32 \ \text{g/mol} = 0.032 \ \text{kg/mol}

  3. Speeds — using vrmsv_{rms}, since it is the speed defined by that very energy: vHe=3×8.314×3000.004=1368 m/sv_{He} = \sqrt{\frac{3 \times 8.314 \times 300}{0.004}} = 1368 \ \text{m/s} vO2=3×8.314×3000.032=484 m/sv_{O_2} = \sqrt{\frac{3 \times 8.314 \times 300}{0.032}} = 484 \ \text{m/s}

  4. The ratio. vHevO2=0.0320.004=8=2.83\frac{v_{He}}{v_{O_2}} = \sqrt{\frac{0.032}{0.004}} = \sqrt{8} = 2.83

  5. Reconcile the two facts. Helium moves 2.83 times faster but is 8 times lighter, and 12mv2\frac{1}{2}mv^2 carries 8×(12.83)2=8×18=18 \times \left(\frac{1}{2.83}\right)^2 = 8 \times \frac{1}{8} = 1. The energies match exactly, as thermal equilibrium demands.

Final Answer: 6.21×10216.21 \times 10^{-21} J for both; vHe=1368v_{He} = 1368 m/s, vO2=484v_{O_2} = 484 m/s, a ratio of 2.832.83.

Takeaway: Thermal equilibrium equalises energies, not speeds. Whenever a question says "the same temperature", write 32kBT\frac{3}{2}k_BT down first — it is the quantity that is genuinely shared.

Part 6: The Three Speeds Compared

Four problems on vmpv_{mp}, vˉ\bar{v} and vrmsv_{rms} — which is which, how to convert between them, and why the ordering never changes.

Bar chart of the three molecular speeds for five gases at 300 K

Key Point: For any gas at any temperature, vmp=2RTM0<vˉ=8RTπM0<vrms=3RTM0v_{mp} = \sqrt{\frac{2RT}{M_0}} < \bar{v} = \sqrt{\frac{8RT}{\pi M_0}} < v_{rms} = \sqrt{\frac{3RT}{M_0}} in the fixed ratio 2:8π:3=1:1.128:1.225\sqrt{2} : \sqrt{\frac{8}{\pi}} : \sqrt{3} = 1 : 1.128 : 1.225. Only the overall scale moves with TT and M0M_0.

Example 32: All three speeds for hydrogen

Find vmpv_{mp}, vˉ\bar{v} and vrmsv_{rms} for hydrogen gas at 300 K, and verify that they stand in the standard ratio. Molar mass of hydrogen is 2.0 g/mol.

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. Convert the molar mass: M0=2.0 g/mol=0.0020 kg/molM_0 = 2.0 \ \text{g/mol} = 0.0020 \ \text{kg/mol}

  2. Most probable speed — the peak of the distribution, the speed more molecules have than any other: vmp=2RTM0=2×8.314×3000.0020=2.494×106=1579 m/sv_{mp} = \sqrt{\frac{2RT}{M_0}} = \sqrt{\frac{2 \times 8.314 \times 300}{0.0020}} = \sqrt{2.494 \times 10^{6}} = 1579 \ \text{m/s}

  3. Average speed — the plain arithmetic mean, the one that belongs in a collision count: vˉ=8RTπM0=8×8.314×3003.1416×0.0020=3.176×106=1782 m/s\bar{v} = \sqrt{\frac{8RT}{\pi M_0}} = \sqrt{\frac{8 \times 8.314 \times 300}{3.1416 \times 0.0020}} = \sqrt{3.176 \times 10^{6}} = 1782 \ \text{m/s}

  4. Root mean square speed — the one tied to energy and to pressure: vrms=3RTM0=3×8.314×3000.0020=3.741×106=1934 m/sv_{rms} = \sqrt{\frac{3RT}{M_0}} = \sqrt{\frac{3 \times 8.314 \times 300}{0.0020}} = \sqrt{3.741 \times 10^{6}} = 1934 \ \text{m/s}

  5. The ratio. Divide through by the smallest: 1579:1782:1934  =  1:1.128:1.2251579 : 1782 : 1934 \;=\; 1 : 1.128 : 1.225 and 2:8π:3=1.414:1.596:1.732\sqrt{2} : \sqrt{\frac{8}{\pi}} : \sqrt{3} = 1.414 : 1.596 : 1.732, which after dividing by 1.4141.414 is 1:1.128:1.2251 : 1.128 : 1.225. \checkmark

Final Answer: vmp=1579v_{mp} = 1579 m/s, vˉ=1782\bar{v} = 1782 m/s, vrms=1934v_{rms} = 1934 m/s.

Takeaway: Memorise 1:1.128:1.2251 : 1.128 : 1.225. Then one speed gives you the other two in a single multiplication, with no square roots and no molar masses.

Example 33: Working back from an average speed

The average speed of the molecules of a certain gas at 400 K is 600 m/s. Find its most probable speed, its rms speed, and its molar mass.

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. Use the fixed ratio for the other two speeds. With vˉ\bar{v} known, vmpvˉ=28/π=1.4141.596=0.886vmp=0.886×600=532 m/s\frac{v_{mp}}{\bar{v}} = \frac{\sqrt{2}}{\sqrt{8/\pi}} = \frac{1.414}{1.596} = 0.886 \quad\Longrightarrow\quad v_{mp} = 0.886 \times 600 = 532 \ \text{m/s} vrmsvˉ=38/π=1.7321.596=1.085vrms=1.085×600=651 m/s\frac{v_{rms}}{\bar{v}} = \frac{\sqrt{3}}{\sqrt{8/\pi}} = \frac{1.732}{1.596} = 1.085 \quad\Longrightarrow\quad v_{rms} = 1.085 \times 600 = 651 \ \text{m/s}

  2. Check the ordering. 532<600<651532 < 600 < 651vmp<vˉ<vrmsv_{mp} < \bar{v} < v_{rms}, as it must be.

  3. The molar mass, from the formula that contains vˉ\bar{v} (not from vrmsv_{rms} — use the speed you were actually given): vˉ=8RTπM0M0=8RTπvˉ2\bar{v} = \sqrt{\frac{8RT}{\pi M_0}} \quad\Longrightarrow\quad M_0 = \frac{8RT}{\pi \bar{v}^2} M0=8×8.314×4003.1416×(600)2=266051.131×106=0.0235 kg/molM_0 = \frac{8 \times 8.314 \times 400}{3.1416 \times (600)^2} = \frac{26605}{1.131 \times 10^{6}} = 0.0235 \ \text{kg/mol}

  4. Back to the familiar unit. M0=0.0235 kg/mol=23.5 g/molM_0 = 0.0235 \ \text{kg/mol} = 23.5 \ \text{g/mol}

  5. Round trip. vˉ=8×8.314×400π×0.0235=600\bar{v} = \sqrt{\frac{8 \times 8.314 \times 400}{\pi \times 0.0235}} = 600 m/s. \checkmark

Final Answer: vmp=532v_{mp} = 532 m/s, vrms=651v_{rms} = 651 m/s, M023.5M_0 \approx 23.5 g/mol.

Takeaway: Put the speed you were given into the formula that contains that speed. Feeding a stated vˉ\bar{v} into 3RTM0\sqrt{\frac{3RT}{M_0}} gives a molar mass 17.8% too large, and nothing in the answer looks wrong.

Example 34: Matching oxygen's peak to hydrogen's average

At what temperature will the most probable speed of oxygen molecules equal the average speed of hydrogen molecules at 300 K? Molar masses: oxygen 32 g/mol, hydrogen 2.0 g/mol.

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. The target speed — hydrogen's average speed at 300 K. Convert first: M0,H2=2.0 g/mol=0.0020 kg/molM_{0,H_2} = 2.0 \ \text{g/mol} = 0.0020 \ \text{kg/mol} vˉH2=8RTπM0=8×8.314×3003.1416×0.0020=1782 m/s\bar{v}_{H_2} = \sqrt{\frac{8RT}{\pi M_0}} = \sqrt{\frac{8 \times 8.314 \times 300}{3.1416 \times 0.0020}} = 1782 \ \text{m/s}

  2. Now set oxygen's most probable speed equal to it. Note we must use vmpv_{mp} for oxygen and vˉ\bar{v} for hydrogen — different formulas, because the question named different speeds: M0,O2=32 g/mol=0.032 kg/molM_{0,O_2} = 32 \ \text{g/mol} = 0.032 \ \text{kg/mol} vmp=2RTO2M0,O2=1782 m/sv_{mp} = \sqrt{\frac{2RT_{O_2}}{M_{0,O_2}}} = 1782 \ \text{m/s}

  3. Solve for the temperature. TO2=M0,O2vmp22R=0.032×(1782)22×8.314=0.032×3.176×10616.63=6112 KT_{O_2} = \frac{M_{0,O_2}\,v_{mp}^2}{2R} = \frac{0.032 \times (1782)^2}{2 \times 8.314} = \frac{0.032 \times 3.176 \times 10^{6}}{16.63} = 6112 \ \text{K}

  4. Sanity check with a single ratio. Combining the two formulas, TO2TH2=82π×M0,O2M0,H2=4π×16=20.4TO2=20.4×300=6112 K\frac{T_{O_2}}{T_{H_2}} = \frac{8}{2\pi}\times\frac{M_{0,O_2}}{M_{0,H_2}} = \frac{4}{\pi}\times 16 = 20.4 \quad\Longrightarrow\quad T_{O_2} = 20.4 \times 300 = 6112 \ \text{K} \quad \checkmark

Final Answer: about 6.1×1036.1 \times 10^{3} K.

Takeaway: Read which speed is named on each side of the equality. Two different speeds means two different formulas, and the factor 4π=1.27\frac{4}{\pi} = 1.27 that separates them is precisely what the question is testing.

Example 35: Two gases with the same peak speed

At what temperature will helium have the same most probable speed as nitrogen at 300 K? Molar masses: helium 4.0 g/mol, nitrogen 28 g/mol. Compute the common speed.

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. Same speed, same formula on both sides, so the constants cancel and only TM0\frac{T}{M_0} survives: 2RTHeM0,He=2RTN2M0,N2THeM0,He=TN2M0,N2\sqrt{\frac{2RT_{He}}{M_{0,He}}} = \sqrt{\frac{2RT_{N_2}}{M_{0,N_2}}} \quad\Longrightarrow\quad \frac{T_{He}}{M_{0,He}} = \frac{T_{N_2}}{M_{0,N_2}}

  2. Solve. THe=TN2×M0,HeM0,N2=300×4.028=42.9 KT_{He} = T_{N_2}\times\frac{M_{0,He}}{M_{0,N_2}} = 300 \times \frac{4.0}{28} = 42.9 \ \text{K}

  3. The common speed. Convert and substitute, using vmpv_{mp} because that is the speed the question names: M0,N2=28 g/mol=0.028 kg/molM_{0,N_2} = 28 \ \text{g/mol} = 0.028 \ \text{kg/mol} vmp=2×8.314×3000.028=422 m/sv_{mp} = \sqrt{\frac{2 \times 8.314 \times 300}{0.028}} = 422 \ \text{m/s} and for helium, M0=0.0040M_0 = 0.0040 kg/mol: vmp=2×8.314×42.90.0040=422 m/sv_{mp} = \sqrt{\frac{2 \times 8.314 \times 42.9}{0.0040}} = 422 \ \text{m/s} \quad \checkmark

  4. A stronger statement than the question asked. Because all three speeds carry the same TM0\sqrt{\frac{T}{M_0}}, equal TM0\frac{T}{M_0} makes vmpv_{mp}, vˉ\bar{v} and vrmsv_{rms} match simultaneously — the two gases have identical speed distribution curves, not merely the same peak.

Final Answer: THe=42.9T_{He} = 42.9 K; the common most probable speed is 422422 m/s.

Takeaway: The whole Maxwell curve depends on TT and M0M_0 only through the combination M0T\frac{M_0}{T}. Match that one ratio and the two gases are statistically indistinguishable by speed.

Part 7: Degrees of Freedom, Internal Energy and Specific Heats

Seven problems that all start the same way: count ff first, then turn the handle. Nothing below can be done by remembering a specific heat; everything below falls out once the molecule has been drawn.

Key Point — the counting rules:

  • A molecule of NN atoms has 3N3N degrees of freedom in total: 3 translational, then 3 rotational (2 if the molecule is linear), and the rest vibrational.
  • Each translational or rotational degree of freedom contributes one quadratic term; each vibrational mode contributes two (kinetic plus potential).
  • ff is the count of quadratic terms, and then U=f2μRT,Cv=f2R,Cp=Cv+R,γ=1+2fU = \frac{f}{2}\mu RT, \qquad C_v = \frac{f}{2}R, \qquad C_p = C_v + R, \qquad \gamma = 1 + \frac{2}{f}
  • At ordinary temperatures vibration is frozen out, so treat molecules as rigid unless told otherwise.

Example 36: Counting ff for four real molecules

For krypton (Kr), hydrogen chloride (HCl), carbon disulphide (CS2CS_2, a linear triatomic) and ethane (C2H6C_2H_6, non-linear), find ff, CvC_v, CpC_p and γ\gamma, treating all of them as rigid.

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. Krypton. A noble gas — single atoms. N=1N = 1, so 3N=33N = 3, all translational; no orientation to specify, no bond to stretch. f=3,Cv=32R=12.47,Cp=52R=20.79 J/(mol K),γ=1+23=1.67f = 3, \qquad C_v = \tfrac{3}{2}R = 12.47, \qquad C_p = \tfrac{5}{2}R = 20.79 \ \text{J/(mol K)}, \qquad \gamma = 1 + \tfrac{2}{3} = 1.67

  2. Hydrogen chloride. Two atoms, 3N=63N = 6: 3 translational, 2 rotational (rotation about the bond axis does not count — the moment of inertia about that line is negligible), 1 vibrational, which is frozen out. f=3+2=5,Cv=52R=20.79,Cp=72R=29.10,γ=1.40f = 3 + 2 = 5, \qquad C_v = \tfrac{5}{2}R = 20.79, \qquad C_p = \tfrac{7}{2}R = 29.10, \qquad \gamma = 1.40

  3. Carbon disulphide. Three atoms, 3N=93N = 9 — but all three nuclei lie on one straight line, so the axis through them is dead and only 2 rotations count: f=3+2=5,Cv=20.79,Cp=29.10,γ=1.40f = 3 + 2 = 5, \qquad C_v = 20.79, \qquad C_p = 29.10, \qquad \gamma = 1.40 A three-atom molecule with a diatomic's specific heats.

  4. Ethane. Eight atoms, definitely not linear, so all 3 rotations are real: f=3+3=6,Cv=3R=24.94,Cp=4R=33.26,γ=1+26=1.33f = 3 + 3 = 6, \qquad C_v = 3R = 24.94, \qquad C_p = 4R = 33.26, \qquad \gamma = 1 + \tfrac{2}{6} = 1.33 Note that ff does not grow with the number of atoms once vibration is frozen out — ethane and ammonia and methane all give f=6f = 6.

  5. The summary table.

Molecule Shape ff CvC_v CpC_p γ\gamma
Kr single atom 3 12.47 20.79 1.67
HCl diatomic 5 20.79 29.10 1.40
CS2CS_2 linear triatomic 5 20.79 29.10 1.40
C2H6C_2H_6 non-linear 6 24.94 33.26 1.33

Final Answer: f=3,5,5,6f = 3, 5, 5, 6 respectively, with the specific heats and γ\gamma as tabulated.

Takeaway: "Triatomic" is not a value of ff; "linear or not" is. Carbon disulphide and carbon dioxide are both three-atom molecules that behave thermally like diatomics, and treating them as generic triatomics overstates CvC_v by 20%.

Example 37: The internal energy of a mixture

A vessel at 400 K contains 3.0 moles of argon, 2.0 moles of oxygen and 1.0 mole of methane. Treating all of them as rigid, find the total internal energy of the mixture, its effective molar CvC_v, and the extra energy needed to warm it by 50 K.

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. Count ff for each. Argon is monatomic, f=3f = 3. Oxygen is a rigid diatomic, f=5f = 5. Methane (CH4CH_4) is a five-atom, non-linear molecule, so f=3+3=6f = 3 + 3 = 6.

  2. Internal energy is additive — each gas stores its own share, and U=f2μRTU = \frac{f}{2}\mu RT: U=(32×3.0+52×2.0+62×1.0)RTU = \left(\frac{3}{2}\times 3.0 + \frac{5}{2}\times 2.0 + \frac{6}{2}\times 1.0\right) R T U=(4.5+5.0+3.0)×8.314×400=12.5×3325.6=4.16×104 JU = (4.5 + 5.0 + 3.0)\times 8.314 \times 400 = 12.5 \times 3325.6 = 4.16 \times 10^{4} \ \text{J}

  3. Effective CvC_v — total heat capacity divided by total moles: Cv,mix=3.0(12.47)+2.0(20.79)+1.0(24.94)3.0+2.0+1.0=37.41+41.57+24.946.0=103.926.0=17.32 J/(mol K)C_{v,\text{mix}} = \frac{3.0(12.47) + 2.0(20.79) + 1.0(24.94)}{3.0 + 2.0 + 1.0} = \frac{37.41 + 41.57 + 24.94}{6.0} = \frac{103.92}{6.0} = 17.32 \ \text{J/(mol K)}

  4. Heat to warm it by 50 K at constant volume. ΔU=(μiCv,i)ΔT=103.92×50=5.20×103 J\Delta U = \left(\sum \mu_i C_{v,i}\right)\Delta T = 103.92 \times 50 = 5.20 \times 10^{3} \ \text{J}

  5. Check against the other route. ΔU=6.0×17.32×50=5.20×103\Delta U = 6.0 \times 17.32 \times 50 = 5.20 \times 10^{3} J. \checkmark

Final Answer: U=4.16×104U = 4.16 \times 10^{4} J; Cv,mix=17.32C_{v,\text{mix}} = 17.32 J/(mol K); ΔU=5.20×103\Delta U = 5.20 \times 10^{3} J for a 50 K rise.

Takeaway: Add the heat capacities μiCv,i\mu_i C_{v,i}, never the CvC_v values themselves. The effective CvC_v of a mixture is a mole-weighted average and lands between the smallest and largest of its parts.

Example 38: Predicted γ\gamma against measured γ\gamma

For helium, nitrogen, chlorine, carbon dioxide and ammonia, write down the γ\gamma that the rigid-molecule count predicts and compare it with the measured room-temperature values below. Where the two disagree, say why, and find the ff that the measurement actually implies for carbon dioxide, whose molar specific heat at constant volume measures 28.528.5 J/(mol K).

Gas Structure Measured γ\gamma
He single atom 1.67
N2N_2 diatomic 1.40
Cl2Cl_2 diatomic 1.32
CO2CO_2 linear triatomic 1.29
NH3NH_3 non-linear 1.31

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. Predict, from γ=1+2f\gamma = 1 + \frac{2}{f} with the rigid count.
Gas ff (rigid) Predicted γ\gamma Measured γ\gamma
He 3 1.67 1.67
N2N_2 5 1.40 1.40
Cl2Cl_2 5 1.40 1.32
CO2CO_2 5 1.40 1.29
NH3NH_3 6 1.33 1.31
  1. The two that agree exactly. Helium has nothing but translation, so there is nothing to go wrong. Nitrogen has a strong, stiff triple bond whose vibration needs a temperature of thousands of kelvin to wake up, so at 300 K it really is rigid.

  2. The three that fall short. Every measured value is below its prediction, and γ\gamma falls only when ff rises. So these molecules have more places to store energy than the rigid count allows: their vibrations are partly active at room temperature. Chlorine's bond is weak and floppy, carbon dioxide has four vibrational modes including a very soft bending one, and ammonia has six.

  3. What ff does the carbon dioxide measurement imply? Invert the formula: γ=1+2ff=2γ1=20.29=6.9\gamma = 1 + \frac{2}{f} \quad\Longrightarrow\quad f = \frac{2}{\gamma - 1} = \frac{2}{0.29} = 6.9 Now do it the sturdier way, straight from the measured Cv=28.5C_v = 28.5 J/(mol K): feff=2CvR=2×28.58.314=6.86f_{\text{eff}} = \frac{2C_v}{R} = \frac{2 \times 28.5}{8.314} = 6.86 The two routes tell the same story, and the small gap between 6.96.9 and 6.866.86 is pure rounding: γ1=0.29\gamma - 1 = 0.29 carries only two significant figures, so a shift of 0.0050.005 in γ\gamma moves ff by more than 0.10.1. When a calorimetric CvC_v is available, use it — near γ1.3\gamma \approx 1.3 the inversion of γ\gamma is a badly conditioned way to get ff. Take feff=6.86f_{\text{eff}} = 6.86 and Cv=28.5C_v = 28.5 J/(mol K), against 52R=20.79\frac{5}{2}R = 20.79 for the rigid prediction. The extra 28.520.79=7.728.5 - 20.79 = 7.7 J/(mol K) is 0.93R0.93\,R, a little under one whole vibrational mode's worth, which is what "partly active" looks like numerically.

  4. The direction of the error is the diagnostic. Measured γ\gamma below prediction means unfrozen vibration. Measured γ\gamma above prediction would mean a rotation is frozen out, which happens only at very low temperature.

Final Answer: predictions 1.671.67, 1.401.40, 1.401.40, 1.401.40, 1.331.33; the last three sit below because vibrational modes are partly active. For CO2CO_2 the measurement implies feff=6.86f_{\text{eff}} = 6.86 with Cv=28.5C_v = 28.5 J/(mol K).

Takeaway: A non-integer ff extracted from a measurement is not an error — it is a half-awake vibration. Classical equipartition can only give whole numbers; nature interpolates between them as the temperature rises.

Example 39: Eleven grams of carbon dioxide, warmed two ways

11 g of carbon dioxide (M0=44M_0 = 44 g/mol), treated as a rigid linear molecule, is warmed by 40 K. Find the heat needed (a) in a sealed rigid vessel and (b) at constant pressure, and the work the gas does in case (b).

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. Moles. μ=1144=0.25 mol\mu = \frac{11}{44} = 0.25 \ \text{mol}

  2. Count ff. CO2CO_2 is linear, so 3 translational + 2 rotational: f=5Cv=52R=20.79,Cp=72R=29.10 J/(mol K)f = 5 \quad\Longrightarrow\quad C_v = \tfrac{5}{2}R = 20.79, \qquad C_p = \tfrac{7}{2}R = 29.10 \ \text{J/(mol K)}

  3. (a) Constant volume. Note the μ\mu, not nn: ΔQV=μCvΔT=0.25×20.79×40=208 J\Delta Q_V = \mu\,C_v\,\Delta T = 0.25 \times 20.79 \times 40 = 208 \ \text{J}

  4. (b) Constant pressure. ΔQP=μCpΔT=0.25×29.10×40=291 J\Delta Q_P = \mu\,C_p\,\Delta T = 0.25 \times 29.10 \times 40 = 291 \ \text{J}

  5. The work done, which is the whole of the difference: ΔW=ΔQPΔQV=291208=83 J=μRΔT=0.25×8.314×40=83.1 J\Delta W = \Delta Q_P - \Delta Q_V = 291 - 208 = 83 \ \text{J} = \mu R\,\Delta T = 0.25 \times 8.314 \times 40 = 83.1 \ \text{J} \quad \checkmark

  6. What if you had treated CO2CO_2 as a generic triatomic with f=6f = 6? You would have got Cv=24.94C_v = 24.94 and ΔQV=249\Delta Q_V = 249 J — 20% too high. The word "linear" was the whole question.

Final Answer: 208208 J at constant volume, 291291 J at constant pressure, of which 8383 J became work.

Takeaway: ΔQPΔQV=μRΔT\Delta Q_P - \Delta Q_V = \mu R \Delta T for every ideal gas, with no ff in it. That extra heat is the work of pushing the atmosphere back, and it is the same for helium and for ammonia.

Example 40: Iodine at 1000 K, where the vibration is awake

Iodine vapour (I2I_2) at 1000 K is hot enough for its bond to vibrate freely. Find ff, CvC_v, CpC_p and γ\gamma, the internal energy of one mole, and how that energy is shared between translation, rotation and vibration.

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. Count, including the vibration. I2I_2 has N=2N = 2, so 3N=63N = 6 degrees of freedom: 3 translational, 2 rotational, 1 vibrational. The vibrational mode is worth two quadratic terms, because it stores kinetic and potential energy: f=3+2+2×1=7f = 3 + 2 + 2\times 1 = 7

  2. The specific heats. Cv=72R=29.10,Cp=92R=37.41 J/(mol K),γ=1+27=97=1.29C_v = \tfrac{7}{2}R = 29.10, \qquad C_p = \tfrac{9}{2}R = 37.41 \ \text{J/(mol K)}, \qquad \gamma = 1 + \tfrac{2}{7} = \tfrac{9}{7} = 1.29

  3. Internal energy of one mole at 1000 K. U=f2μRT=72×1×8.314×1000=2.91×104 JU = \frac{f}{2}\mu RT = \frac{7}{2}\times 1 \times 8.314 \times 1000 = 2.91 \times 10^{4} \ \text{J}

  4. The shares. Each quadratic term carries 12RT=4157\frac{1}{2}RT = 4157 J per mole: Utrans=3×4157=1.25×104 J(42.9%)U_{\text{trans}} = 3 \times 4157 = 1.25 \times 10^{4} \ \text{J} \quad (42.9\%) Urot=2×4157=8.31×103 J(28.6%)U_{\text{rot}} = 2 \times 4157 = 8.31 \times 10^{3} \ \text{J} \quad (28.6\%) Uvib=2×4157=8.31×103 J(28.6%)U_{\text{vib}} = 2 \times 4157 = 8.31 \times 10^{3} \ \text{J} \quad (28.6\%) and 12471+8314+8314=2909912471 + 8314 + 8314 = 29099 J. \checkmark

  5. Compare with the same gas cold. Rigid, at f=5f = 5, iodine would have Cv=20.79C_v = 20.79 and γ=1.40\gamma = 1.40. Switching on one vibration adds a full RR to CvC_v and drops γ\gamma by 0.110.11.

Final Answer: f=7f = 7, Cv=29.10C_v = 29.10, Cp=37.41C_p = 37.41 J/(mol K), γ=1.29\gamma = 1.29; U=2.91×104U = 2.91 \times 10^{4} J/mol, split 42.9%42.9\% / 28.6%28.6\% / 28.6%28.6\%.

Takeaway: One vibrational mode adds RR to CvC_v, never R2\frac{R}{2}. Iodine's bond is heavy and weak, so it wakes at a few hundred kelvin; nitrogen's needs several thousand. That is why "rigid" is a statement about temperature, not about the molecule alone.

Example 41: Silver, and how well the solid-state prediction does

Equipartition applied to a simple crystalline solid — each atom vibrating in three independent directions — predicts a molar heat capacity of 3R3R. Find the predicted molar and per-kilogram specific heats for silver (M0=108M_0 = 108 g/mol), and the heat needed to warm 500 g of silver by 50 K. The measured value is about 235 J/(kg K).

Solution:

Constants: R=8.314R = 8.314 J/(mol K).

  1. Where the 3R3R comes from. An atom in a solid does not translate freely; it oscillates about a lattice site in xx, yy and zz. Each direction is one vibrational mode, worth 2 quadratic terms, so f=6f = 6 and C=f2R=3R=3×8.314=24.94 J/(mol K)C = \frac{f}{2}R = 3R = 3 \times 8.314 = 24.94 \ \text{J/(mol K)}

  2. Per kilogram. Convert the molar mass on its own line: M0=108 g/mol=0.108 kg/molM_0 = 108 \ \text{g/mol} = 0.108 \ \text{kg/mol} c=CM0=24.940.108=231 J/(kg K)c = \frac{C}{M_0} = \frac{24.94}{0.108} = 231 \ \text{J/(kg K)}

  3. Against the measurement. 231231 predicted, 235235 measured — an agreement of better than 2%, from a model with no adjustable numbers in it at all.

  4. The heat needed. μ=500108=4.63 mol\mu = \frac{500}{108} = 4.63 \ \text{mol} ΔQ=μCΔT=4.63×24.94×50=5.77×103 J\Delta Q = \mu\,C\,\Delta T = 4.63 \times 24.94 \times 50 = 5.77 \times 10^{3} \ \text{J}

  5. Cross-check per kilogram. ΔQ=McΔT=0.500×230.9×50=5.77×103 J\Delta Q = M c\,\Delta T = 0.500 \times 230.9 \times 50 = 5.77 \times 10^{3} \ \text{J} \quad \checkmark

Final Answer: C=24.94C = 24.94 J/(mol K), c=231c = 231 J/(kg K); about 5.8×1035.8 \times 10^{3} J.

Takeaway: All ordinary solids have nearly the same MOLAR heat capacity, about 2525 J/(mol K) — so their per-kilogram values run inversely with molar mass. Light metals feel hard to heat; heavy metals feel easy.

Example 42: Beryllium, where the prediction fails

Beryllium has a molar mass of 9.01 g/mol and a measured specific heat capacity of about 1825 J/(kg K) at room temperature. Find its molar heat capacity and compare it with the 3R3R prediction. Explain the discrepancy.

Solution:

Constants: R=8.314R = 8.314 J/(mol K), so 3R=24.943R = 24.94 J/(mol K).

  1. Convert the molar mass: M0=9.01 g/mol=0.00901 kg/molM_0 = 9.01 \ \text{g/mol} = 0.00901 \ \text{kg/mol}

  2. Molar heat capacity from the per-kilogram value. C=cM0=1825×0.00901=16.4 J/(mol K)C = c\,M_0 = 1825 \times 0.00901 = 16.4 \ \text{J/(mol K)}

  3. Compare. C3R=16.424.94=0.66\frac{C}{3R} = \frac{16.4}{24.94} = 0.66 Only two thirds of the classical prediction — a serious failure, not a rounding error.

  4. Why. Beryllium atoms are very light and its lattice is unusually stiff, so its atoms vibrate at very high frequency. Classical equipartition assumes every mode can take up energy in arbitrarily small amounts; in reality a mode of frequency ν\nu needs a quantum hνh\nu, and when hνh\nu is comparable with kBTk_BT most of the modes cannot be excited at all. They are partly frozen out, so they store less than kBTk_BT each and CC falls below 3R3R.

  5. The pattern. The same argument explains why diamond — light carbon atoms, extremely stiff bonds — has a room-temperature molar heat capacity of only about 6 J/(mol K), a quarter of the prediction, while lead and silver sit right on it.

Final Answer: C=16.4C = 16.4 J/(mol K), about 66% of 3R3R; the shortfall is quantum freezing-out of high-frequency lattice vibrations.

Takeaway: Equipartition sets a ceiling, not a guarantee. A measured heat capacity is at or below the classical value; where it falls short, the missing modes are the stiffest and lightest ones, and heating the sample brings them back.

Part 8: Mean Free Path, Collisions and Diffusion

Six finishers. Every one of them needs the 2\sqrt{2}, and most of them need you to notice whether the number you were handed is a radius or a diameter.

Key Point: l=12nπd2=kBT2πd2P,fcoll=vˉl,τ=1fcoll=lvˉl = \frac{1}{\sqrt{2}\,n\pi d^2} = \frac{k_BT}{\sqrt{2}\,\pi d^2 P}, \qquad f_{\text{coll}} = \frac{\bar{v}}{l}, \qquad \tau = \frac{1}{f_{\text{coll}}} = \frac{l}{\bar{v}} The 2\sqrt{2} comes from the average relative speed of two moving molecules; leaving it out makes ll too large by 41%. And dd is the DIAMETER — a stated radius must be doubled before it is squared, or d2d^2 comes out four times too small. Collision frequency and collision time use the mean speed vˉ\bar{v}, never vrmsv_{rms}, because what matters is the average distance covered per second, not the average energy.

Example 43: Nitrogen under pressure — path, frequency and free time

Estimate the mean free path and the collision frequency of a nitrogen molecule in a cylinder holding nitrogen at 2.0 atm and 17°C. Take the radius of a nitrogen molecule as 1.0 Å and its molar mass as 28 g/mol. Compare the time a molecule spends flying freely with the time a single collision takes.

Solution:

Constants: kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K; R=8.314R = 8.314 J/(mol K); 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. The trap, dealt with first. The problem gives a radius. The formula wants a diameter: d=2r=2×1.0 A˚=2.0 A˚=2.0×1010 md = 2r = 2 \times 1.0 \ \text{Å} = 2.0 \ \text{Å} = 2.0 \times 10^{-10} \ \text{m}

  2. Kelvin, and the number density. T=17+273.15=290.15 K,P=2.0×1.013×105=2.026×105 PaT = 17 + 273.15 = 290.15 \ \text{K}, \qquad P = 2.0 \times 1.013 \times 10^{5} = 2.026 \times 10^{5} \ \text{Pa} n=PkBT=2.026×1051.38×1023×290.15=5.06×1025 per m3n = \frac{P}{k_BT} = \frac{2.026 \times 10^{5}}{1.38 \times 10^{-23} \times 290.15} = 5.06 \times 10^{25} \ \text{per m}^3

  3. Mean free path, with the 2\sqrt{2}: l=12nπd2=11.414×5.06×1025×3.1416×(2.0×1010)2l = \frac{1}{\sqrt{2}\,n\pi d^2} = \frac{1}{1.414 \times 5.06 \times 10^{25} \times 3.1416 \times (2.0 \times 10^{-10})^2} l=18.99×106=1.11×107 ml = \frac{1}{8.99 \times 10^{6}} = 1.11 \times 10^{-7} \ \text{m} (Dropping the 2\sqrt{2} would have given 1.57×1071.57 \times 10^{-7} m — 41% too large. Do not.)

  4. Which speed for the collision count? The mean speed vˉ\bar{v}, because collisions are counted per metre travelled and vˉ\bar{v} is the average distance covered per second. Convert the molar mass: M0=28 g/mol=0.028 kg/molM_0 = 28 \ \text{g/mol} = 0.028 \ \text{kg/mol} vˉ=8RTπM0=8×8.314×290.153.1416×0.028=2.194×105=468 m/s\bar{v} = \sqrt{\frac{8RT}{\pi M_0}} = \sqrt{\frac{8 \times 8.314 \times 290.15}{3.1416 \times 0.028}} = \sqrt{2.194 \times 10^{5}} = 468 \ \text{m/s}

  5. Collision frequency and the free time between collisions. fcoll=vˉl=4681.11×107=4.21×109 per secondf_{\text{coll}} = \frac{\bar{v}}{l} = \frac{468}{1.11 \times 10^{-7}} = 4.21 \times 10^{9} \ \text{per second} τ=1fcoll=2.37×1010 s\tau = \frac{1}{f_{\text{coll}}} = 2.37 \times 10^{-10} \ \text{s}

  6. How long does one collision last? Roughly the time to cross one molecular diameter: tcolldvˉ=2.0×1010468=4.3×1013 st_{\text{coll}} \approx \frac{d}{\bar{v}} = \frac{2.0 \times 10^{-10}}{468} = 4.3 \times 10^{-13} \ \text{s} τtcoll=2.37×10104.3×10135.6×102\frac{\tau}{t_{\text{coll}}} = \frac{2.37 \times 10^{-10}}{4.3 \times 10^{-13}} \approx 5.6 \times 10^{2}

Final Answer: l=1.11×107l = 1.11 \times 10^{-7} m, fcoll=4.21×109f_{\text{coll}} = 4.21 \times 10^{9} s1^{-1}, τ=2.37×1010\tau = 2.37 \times 10^{-10} s; a molecule flies free for about 560 times as long as a collision lasts.

Takeaway: A gas molecule spends over 99.8% of its life flying in a straight line. That is the quantitative justification for the kinetic-theory assumption that collisions take negligible time — and the reason the ideal gas model survives four billion collisions a second.

Example 44: When pressure and temperature both change

A gas has a mean free path of 2.0×1072.0 \times 10^{-7} m at 1 atm and 300 K. Find its mean free path at 0.250.25 atm and 600 K, and say what happens to its collision frequency.

Solution:

  1. Read the scaling off the formula. From l=kBT2πd2Pl = \frac{k_BT}{\sqrt{2}\pi d^2 P}, with dd fixed, lTPl \propto \frac{T}{P}

  2. Apply both changes. l2l1=T2T1×P1P2=600300×10.25=2×4=8\frac{l_2}{l_1} = \frac{T_2}{T_1}\times\frac{P_1}{P_2} = \frac{600}{300}\times\frac{1}{0.25} = 2 \times 4 = 8 l2=8×2.0×107=1.6×106 ml_2 = 8 \times 2.0 \times 10^{-7} = 1.6 \times 10^{-6} \ \text{m}

  3. The collision frequency. fcoll=vˉlf_{\text{coll}} = \frac{\bar{v}}{l}, and vˉT\bar{v} \propto \sqrt{T}, so fcollTT/P=PTf_{\text{coll}} \propto \frac{\sqrt{T}}{T/P} = \frac{P}{\sqrt{T}} f2f1=P2P1×T1T2=0.25×12=0.177\frac{f_2}{f_1} = \frac{P_2}{P_1}\times\sqrt{\frac{T_1}{T_2}} = 0.25 \times \frac{1}{\sqrt{2}} = 0.177 so collisions become about 5.7 times rarer.

  4. A caution about the temperature alone. Heating a gas in a rigid sealed vessel does not change ll at all, because nn is fixed and l=12nπd2l = \frac{1}{\sqrt{2}n\pi d^2} has no TT in it. The TT in the kBT2πd2P\frac{k_BT}{\sqrt{2}\pi d^2 P} form is there only because PP was used in place of nn. Decide which is really held constant before you scale.

Final Answer: l2=1.6×106l_2 = 1.6 \times 10^{-6} m; the collision frequency falls to 0.1770.177 of its old value.

Takeaway: l1nl \propto \frac{1}{n} always; lTPl \propto \frac{T}{P} only when you are told the pressure. Confusing the two turns "heat a sealed cylinder" into a wrong answer every time.

Example 45: Extracting a molecular diameter from a measured path

The mean free path of a certain gas is measured as 7.0×1087.0 \times 10^{-8} m at 1 atm and 300 K. Estimate the diameter and the radius of its molecules.

Solution:

Constants: kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K; 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. Number density. n=PkBT=1.013×1051.38×1023×300=2.45×1025 per m3n = \frac{P}{k_BT} = \frac{1.013 \times 10^{5}}{1.38 \times 10^{-23} \times 300} = 2.45 \times 10^{25} \ \text{per m}^3

  2. Invert the mean free path formula, keeping the 2\sqrt{2}: l=12nπd2d2=12nπll = \frac{1}{\sqrt{2}\,n\pi d^2} \quad\Longrightarrow\quad d^2 = \frac{1}{\sqrt{2}\,n\pi l}

  3. Substitute. d2=11.414×2.45×1025×3.1416×7.0×108=17.61×1018=1.31×1019 m2d^2 = \frac{1}{1.414 \times 2.45 \times 10^{25} \times 3.1416 \times 7.0 \times 10^{-8}} = \frac{1}{7.61 \times 10^{18}} = 1.31 \times 10^{-19} \ \text{m}^2 d=3.63×1010 m=3.6 A˚d = 3.63 \times 10^{-10} \ \text{m} = 3.6 \ \text{Å}

  4. The radius, since half of all sources quote that instead: r=d2=1.8 A˚r = \frac{d}{2} = 1.8 \ \text{Å}

  5. Is it sensible? Molecular diameters run from about 2 Å (helium) to about 5 Å (large organics), so 3.6 Å is right in the ordinary range. Had we forgotten the 2\sqrt{2}, we would have got d=4.3d = 4.3 Å — a 19% overestimate, since dl1/2d \propto l^{-1/2} softens the error.

Final Answer: d3.6×1010d \approx 3.6 \times 10^{-10} m; radius about 1.8×10101.8 \times 10^{-10} m.

Takeaway: This inversion is how molecular sizes were first measured. Mean free paths come out of viscosity and diffusion experiments, and a cube-and-square-root later you have the size of something nobody can see.

Example 46: Helium against argon — two diameters and two masses

Helium (diameter 2.18 Å, 4.0 g/mol) and argon (diameter 3.64 Å, 39.9 g/mol) are each held at 1 atm and 300 K. Compare their mean free paths and their collision frequencies.

Solution:

Constants: kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K; R=8.314R = 8.314 J/(mol K); 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. Same PP and TT means the same number density for both: n=PkBT=1.013×1051.38×1023×300=2.45×1025 per m3n = \frac{P}{k_BT} = \frac{1.013 \times 10^{5}}{1.38 \times 10^{-23}\times 300} = 2.45 \times 10^{25} \ \text{per m}^3

  2. Mean free paths. lHe=12nπd2=11.414×2.45×1025×3.1416×(2.18×1010)2=1.94×107 ml_{He} = \frac{1}{\sqrt{2}\,n\pi d^2} = \frac{1}{1.414 \times 2.45 \times 10^{25}\times 3.1416 \times (2.18 \times 10^{-10})^2} = 1.94 \times 10^{-7} \ \text{m} lAr=11.414×2.45×1025×3.1416×(3.64×1010)2=6.94×108 ml_{Ar} = \frac{1}{1.414 \times 2.45 \times 10^{25}\times 3.1416 \times (3.64 \times 10^{-10})^2} = 6.94 \times 10^{-8} \ \text{m} lHelAr=(3.642.18)2=2.79\frac{l_{He}}{l_{Ar}} = \left(\frac{3.64}{2.18}\right)^2 = 2.79 Helium travels nearly three times further between collisions — because it is thinner, not because it is lighter. Mass does not appear in ll at all.

  3. Mean speeds — the speed a collision count wants. Convert both molar masses: M0,He=0.0040 kg/mol,M0,Ar=0.0399 kg/molM_{0,He} = 0.0040 \ \text{kg/mol}, \qquad M_{0,Ar} = 0.0399 \ \text{kg/mol} vˉHe=8×8.314×3003.1416×0.0040=1260 m/s,vˉAr=8×8.314×3003.1416×0.0399=399 m/s\bar{v}_{He} = \sqrt{\frac{8 \times 8.314 \times 300}{3.1416 \times 0.0040}} = 1260 \ \text{m/s}, \qquad \bar{v}_{Ar} = \sqrt{\frac{8 \times 8.314 \times 300}{3.1416 \times 0.0399}} = 399 \ \text{m/s}

  4. Collision frequencies. fcoll,He=12601.94×107=6.51×109 s1,fcoll,Ar=3996.94×108=5.75×109 s1f_{\text{coll},He} = \frac{1260}{1.94 \times 10^{-7}} = 6.51 \times 10^{9} \ \text{s}^{-1}, \qquad f_{\text{coll},Ar} = \frac{399}{6.94 \times 10^{-8}} = 5.75 \times 10^{9} \ \text{s}^{-1} fcoll,Hefcoll,Ar=1.13\frac{f_{\text{coll},He}}{f_{\text{coll},Ar}} = 1.13

  5. The point. The mean free paths differ by a factor of 2.8, but the collision frequencies differ by only 13%, because helium's greater speed almost exactly compensates its longer path. Two very different molecules, nearly the same number of collisions per second.

Final Answer: lHe=1.94×107l_{He} = 1.94 \times 10^{-7} m and lAr=6.94×108l_{Ar} = 6.94 \times 10^{-8} m (ratio 2.792.79); fHe=6.51×109f_{He} = 6.51 \times 10^{9} s1^{-1} and fAr=5.75×109f_{Ar} = 5.75 \times 10^{9} s1^{-1} (ratio 1.131.13).

Takeaway: ll depends on size only; fcollf_{\text{coll}} depends on size and mass. A question about path length never needs a molar mass; a question about frequency always does.

Example 47: Timing two gases through the same pinhole

Under identical conditions, a fixed volume of nitrogen (M0=28M_0 = 28 g/mol) takes 60 s to escape through a small hole, while the same volume of an unknown gas takes 22.4 s. Identify the unknown gas.

Solution:

  1. Graham's law. At equal pressure and temperature the rate of diffusion or effusion goes as r1M0rXrN2=M0,N2M0,Xr \propto \frac{1}{\sqrt{M_0}} \quad\Longrightarrow\quad \frac{r_X}{r_{N_2}} = \sqrt{\frac{M_{0,N_2}}{M_{0,X}}}

  2. Rate is inversely proportional to time for the same volume, so rXrN2=tN2tX=6022.4=2.68\frac{r_X}{r_{N_2}} = \frac{t_{N_2}}{t_X} = \frac{60}{22.4} = 2.68

  3. Square and rearrange. M0,N2M0,X=(2.68)2=7.18M0,X=287.18=3.9 g/mol\frac{M_{0,N_2}}{M_{0,X}} = (2.68)^2 = 7.18 \quad\Longrightarrow\quad M_{0,X} = \frac{28}{7.18} = 3.9 \ \text{g/mol}

  4. Identify. 3.93.9 g/mol is helium (4.0 g/mol) — nothing else is that light except hydrogen, which is 2.0.

  5. Why the square root. Graham's law is really the statement vˉ1M0\bar{v} \propto \frac{1}{\sqrt{M_0}} in disguise: a molecule escapes at a rate set by how fast it arrives at the hole, and that is its mean speed. Helium's mean speed at 300 K is 1260 m/s against nitrogen's 476 m/s, a ratio of 2.65 — matching the 2.68 above to within rounding.

Final Answer: M0,X3.9M_{0,X} \approx 3.9 g/mol; the gas is helium.

Takeaway: Longer time means slower rate means heavier gas. Invert the times before you square them; taking tXtN2\frac{t_X}{t_{N_2}} the wrong way up gives a molar mass of 200 g/mol and an answer that ought to look obviously wrong.

Example 48: Why the smell takes minutes to cross the room

Methane (M0=16M_0 = 16 g/mol) and sulphur dioxide (M0=64M_0 = 64 g/mol) are released under identical conditions. (a) Which diffuses faster, and by what factor? (b) If methane crosses a room in 25 s, how long does sulphur dioxide take? (c) Their molecules move at hundreds of metres per second — why does either take that long to cross a 5 m room? Take the molecular diameter as 4.0 Å, the pressure as 1 atm and the temperature as 300 K.

Solution:

Constants: kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K; R=8.314R = 8.314 J/(mol K); 1 atm =1.013×105= 1.013 \times 10^{5} Pa.

  1. (a) Graham's law. rCH4rSO2=M0,SO2M0,CH4=6416=4=2.0\frac{r_{CH_4}}{r_{SO_2}} = \sqrt{\frac{M_{0,SO_2}}{M_{0,CH_4}}} = \sqrt{\frac{64}{16}} = \sqrt{4} = 2.0 Methane diffuses exactly twice as fast.

  2. (b) Time is inversely proportional to rate. tSO2=2.0×25=50 st_{SO_2} = 2.0 \times 25 = 50 \ \text{s}

  3. Check through the mean speeds — the speed diffusion depends on. Convert both molar masses: M0,CH4=0.016 kg/mol,M0,SO2=0.064 kg/molM_{0,CH_4} = 0.016 \ \text{kg/mol}, \qquad M_{0,SO_2} = 0.064 \ \text{kg/mol} vˉCH4=8×8.314×3003.1416×0.016=630 m/s,vˉSO2=8×8.314×3003.1416×0.064=315 m/s\bar{v}_{CH_4} = \sqrt{\frac{8 \times 8.314 \times 300}{3.1416 \times 0.016}} = 630 \ \text{m/s}, \qquad \bar{v}_{SO_2} = \sqrt{\frac{8 \times 8.314 \times 300}{3.1416 \times 0.064}} = 315 \ \text{m/s} A ratio of exactly 2.0. \checkmark

  4. (c) The mean free path is why. n=PkBT=2.45×1025 per m3n = \frac{P}{k_BT} = 2.45 \times 10^{25} \ \text{per m}^3 l=12nπd2=11.414×2.45×1025×3.1416×(4.0×1010)2=5.7×108 ml = \frac{1}{\sqrt{2}\,n\pi d^2} = \frac{1}{1.414 \times 2.45 \times 10^{25}\times 3.1416 \times (4.0 \times 10^{-10})^2} = 5.7 \times 10^{-8} \ \text{m} A molecule travels 630 m/s but only about 57 nm in a straight line before it is knocked in a new direction. Its path is a random zig-zag, and for a random walk the net displacement after NN steps is only Nl\sqrt{N}\,l, not NlNl. To make net progress of 5 m, N=(55.7×108)28×1015 stepsN = \left(\frac{5}{5.7 \times 10^{-8}}\right)^2 \approx 8 \times 10^{15} \ \text{steps}

  5. Reading the answer. The molecule is fast; the route is hopeless. That is the entire explanation of why a gas leak is smelt across a kitchen in minutes rather than in the 8 ms a straight flight would take — and also why a draught, which moves the whole air bodily, delivers the smell far quicker than diffusion ever could.

Final Answer: (a) methane, by a factor of 2.0; (b) 50 s; (c) because the mean free path is only about 57 nm, so the molecule random-walks and needs some 101610^{16} steps to get 5 m.

Takeaway: Diffusion is slow because it is a random walk, not because molecules are slow. Net displacement grows as N\sqrt{N}, which is why doubling the distance costs four times the time.