RMS speed of molecules
Open a bottle of perfume in a still room and the smell reaches the far corner in minutes, not instantly and not in hours. That delay is a clue: gas molecules are not crawling, they are flying at speeds close to a rifle bullet's, but in every random direction at once, colliding billions of times a second and zig-zagging their way across the room. No two molecules share exactly the same speed at any instant, so "the speed of a gas molecule" only makes sense as a statistical average over the whole swarm. The root-mean-square (rms) speed, , is the specific average kinetic theory hands us — not the plain mean, but the square root of the mean of the squared speeds. It falls straight out of the kinetic-theory pressure formula you have already derived, ties pressure and temperature together at the molecular level, and explains everyday facts from why helium balloons deflate faster than air-filled ones to why Earth kept its atmosphere while the Moon did not.
The root-mean-square speed of gas molecules, , grows with the square root of absolute temperature, shrinks with the square root of molar mass, and — at fixed temperature — does not depend on pressure at all.
The core idea
Kinetic theory begins with the pressure a swarm of molecules exerts on a container wall, derived from Newton's laws applied to elastic collisions:
where: is the gas pressure, is the gas density, and is the mean of the squared molecular speeds (averaged over every molecule in the sample). Taking the square root of defines the root-mean-square speed,
Two sub-points worth separating out before the main derivation:
- rms is not the plain average. Squaring every speed before averaging gives extra statistical weight to the fastest molecules, so always comes out a little larger than the simple arithmetic-mean speed of the same sample. The ISC syllabus works only with ; you are not asked to compute or compare the mean or most-probable speed.
- Two equivalent working formulas exist. is the direct kinetic-theory result; combining it with the ideal gas law gives the far more usable , worked out below.
The figure compares for four common gases at the same room temperature, making the dependence visible at a glance: hydrogen's molar mass is sixteen times smaller than oxygen's, so its rms speed is times larger, exactly the pattern the bars show. Notice, too, that all four bars sit in the hundreds-to-thousands-of-metres-per-second range — comparable to rifle-bullet speeds — even though the gas as a whole (say, the air in a room) is not visibly rushing anywhere, because the molecules' motion is random in direction and constantly interrupted by collisions, not a steady drift.
Effect of temperature and pressure. , so rms speed rises with absolute temperature — faster molecules carry more kinetic energy, matching the kinetic interpretation of temperature. At constant temperature, is independent of pressure: compressing a gas raises in exact step with , so is unchanged. And , which is why hydrogen and helium move far faster than oxygen or carbon dioxide at the same temperature, and why Earth retains its heavier atmospheric gases while light hydrogen slowly escapes over geological time.
The goal of this derivation is to turn the kinetic-theory pressure relation , which involves the hard-to-measure quantities density and mean-square speed, into the standard working formula , which uses only the temperature and molar mass every textbook and exam question actually supplies.
Step 1. Start from the definition of rms speed applied to the kinetic-theory pressure result. Since and , rearranging for and substituting gives .
Step 2. Bring in the ideal gas equation for moles of gas occupying volume at temperature : , so .
Step 3. Express the density in terms of the same moles. The total mass of gas is , where is the molar mass, so .
Step 4. Substitute both expressions into . The volume and mole number appear in both numerator and denominator and cancel completely:
where: is the universal gas constant, is the absolute temperature in kelvin, and is the molar mass in kg/mol (SI units throughout — using grams instead of kilograms is the single commonest error here).
Step 5. Read off the result. depends only on temperature and molar mass, with pressure and density having dropped out entirely — confirming algebraically what was stated qualitatively above, that rms speed at fixed is independent of pressure. The cancellation of and in Step 4 is the real engine of the whole derivation: it is precisely what lets a formula built from bulk, container-dependent quantities like pressure and density collapse into one that depends only on the intrinsic properties of the gas — its temperature and the identity (molar mass) of its molecules.
Worked example
Find the rms speed of oxygen molecules () at .
Step 1. Write the formula: .
Step 2. Substitute values:
Step 3. Evaluate: . Oxygen molecules at room temperature move at roughly 480 m/s on average — faster than the speed of sound in air, even though sound itself travels a little slower because it propagates via collisions between molecules, not via any single molecule's flight path. The mismatch is a useful sanity check to remember: a sound wave is a coordinated disturbance passed molecule to molecule, so it necessarily travels slower than the individual molecules' own random thermal speed.
Competitive stretch
Hydrogen gas at (that is, ) has rms speed . At what temperature does its rms speed double?
Step 1. Since is unchanged, , so .
Step 2. Setting gives , so () — quadrupling the absolute temperature, not doubling it, because of the square-root dependence.
Cross-check. Compute both rms speeds directly with instead of relying on the ratio: at , ; at , , which is indeed double . This confirms the proportionality shortcut without needing to trust it blindly — a useful habit whenever a problem gives you a ratio rather than asking for an absolute number.
Common traps
- Assuming rms speed doubles when temperature in degrees Celsius doubles — the relation only holds with in kelvin, never Celsius, since only absolute temperature has physical meaning as a measure of average molecular kinetic energy.
- Believing that compressing a gas at constant temperature speeds its molecules up — it does not, since rises in step with , leaving unchanged; only heating the gas, not squeezing it, raises molecular speed.
- Confusing rms speed with average speed or most-probable speed — these are three genuinely different statistical averages of the same underlying speed distribution; the ISC syllabus needs only , so resist the temptation to memorise formulas for the other two.
- Using molar mass in grams instead of kilograms in — since is already in SI units, must be in kg/mol, or the computed speed comes out too large by a factor of about 31.6 (the square root of 1000).
Ask the tutor: want to walk through why pressure alone can't change rms speed, or practice comparing rms speeds across different gases at the same temperature?
Why is rms speed used instead of just averaging all the molecular speeds directly?
Because kinetic theory naturally produces the mean of the squared speeds, not the mean speed itself — it comes straight out of the pressure derivation, which involves momentum and hence velocity squared, so squaring is built into the physics before any averaging happens. Squaring first also weights fast molecules more heavily than slow ones, so is always a little larger than the plain arithmetic-mean speed of the same sample of molecules. For ISC purposes you only need to work with ; the average and most-probable speeds belong to the fuller Maxwell-Boltzmann distribution treatment, which lies outside this syllabus and is not examined here.
Does raising the pressure of a gas at constant temperature make its molecules move faster?
No, and this trips up many students. From , raising pressure at fixed temperature — say, by compressing the gas into a smaller volume — increases the density by exactly the same factor as , since squeezing the same mass of gas into less space raises both together. The ratio , and hence , therefore stays unchanged. Only a change in absolute temperature, or switching to a gas of different molar mass, actually alters the rms speed of the molecules.
Why do light gases like hydrogen and helium escape Earth's atmosphere while oxygen and nitrogen stay?
Because , lighter molecules move faster at the same temperature — hydrogen at 300 K moves roughly four times faster than oxygen, as the bar chart above shows. Hydrogen and helium reach speeds high enough that a meaningful fraction of them exceed Earth's escape velocity (about 11.2 km/s) over long timescales and gradually leak into space, while the much slower, heavier oxygen and nitrogen molecules stay gravitationally bound to the planet. This is a direct, qualitative consequence of the dependence in , without needing any escape-velocity calculation for the ISC syllabus.