One Gas, a Hundred Billion Different Speeds

The previous section handed us a single number and called it the speed of a nitrogen molecule at 300 K: vrms=517v_{rms} = 517 m/s. Now let us admit what that number was hiding.

No molecule is obliged to move at 517 m/s. In any real sample, at this instant, some molecules are crawling along at 40 m/s and some are tearing about at 1500 m/s, and a collision a nanosecond from now will change both. A molecule's speed is not a property it has; it is something that happens to it, over and over, two billion times a second.

So what survives? Not any individual speed — but the proportions. At a fixed temperature, the fraction of molecules moving between, say, 400 m/s and 500 m/s is a rock-steady number, even though the particular molecules occupying that band are swapped out constantly. Individual speeds churn; the distribution of speeds does not budge.

Key Point: A gas in equilibrium has a fixed distribution of molecular speeds, even though no individual molecule keeps its speed for more than a nanosecond. Every collision that removes a molecule from one speed range puts another one into it. This steady spread is what we are about to describe, and it is what vrmsv_{rms} was a single crude summary of.

James Clerk Maxwell worked out the shape of that spread in 1859, and Ludwig Boltzmann later derived it from more general principles — which is why it is called the Maxwell-Boltzmann distribution of molecular speeds.

A note on where this sits. The speed distribution and the formulas for the average and most probable speeds sit outside the body text of the rationalised syllabus, but Boards, JEE and NEET ask for the shape of the curve, the ordering of the three speeds and their ratio every single year — so they are developed here in full.

What the curve actually plots

Write F(v)F(v) for the speed distribution function. It is defined so that

F(v)dv=the fraction of molecules with speeds between v and v+dvF(v)\,dv = \text{the fraction of molecules with speeds between } v \text{ and } v + dv

Two consequences follow immediately, and everything else in this section is built on them.

Key Point — how to read a distribution curve:

  • The area under the whole curve is 1, because every molecule has some speed: 0F(v)dv=1\int_0^{\infty} F(v)\,dv = 1
  • The area between two speeds is the fraction of molecules in that range: fraction with v1<v<v2=v1v2F(v)dv\text{fraction with } v_1 < v < v_2 = \int_{v_1}^{v_2} F(v)\,dv

It is the area that carries the meaning, not the height. The height F(v)F(v) on its own is a fraction per unit speed range — you cannot read a number of molecules off it without choosing a width.

[JEE Tip] This is the single most common misreading in the whole topic. "What fraction of molecules move at exactly 500 m/s?" has the answer zero — a single speed is a line of zero width, and a line encloses no area. Every meaningful question about the distribution is a question about a range.

The shape, and why it has that shape

Maxwell speed curve from v-squared factor times exponential, with shaded fraction bands

Written out, the distribution is

F(v)=4π(m2πkBT)3/2v2emv2/2kBTF(v) = 4\pi \left(\frac{m}{2\pi k_B T}\right)^{3/2} v^2 e^{-mv^2/2k_BT}

You are not asked to reproduce that. You are asked to know its shape, and the shape is decided by a tug of war between the only two parts that depend on vv:

1. The v2v^2 factor pushes the curve up. Velocity is a three-dimensional vector, and there are far more ways to have a large speed than a small one — think of all the directions a fast molecule could be pointing. The number of available velocity states grows as v2v^2, which is why the curve climbs at first.

2. The exponential emv2/2kBTe^{-mv^2/2k_BT} pulls it down. Going fast costs kinetic energy, and at temperature TT the supply of energy is limited. This Boltzmann factor makes high speeds exponentially unlikely.

Multiply the two and you get the lopsided hump in the figure:

  • It starts at zero. At v=0v = 0 the v2v^2 factor is zero, so F(0)=0F(0) = 0. No molecules are at rest. A molecule with exactly zero speed would have to have all three velocity components exactly zero at once, and there is precisely one way to do that against infinitely many ways to be moving.
  • It rises to a single peak. The peak is where the two factors balance, and the speed at which it sits gets a name in a moment.
  • It falls away with a long tail, and it is NOT symmetric. Past the peak the exponential wins and the curve drops — but it never reaches zero. There is always some fraction of molecules at any speed you care to name, however large. The curve is squashed against the wall at v=0v = 0 on the left and free to run on forever to the right, so it cannot possibly be a symmetric bell.

[Board Important] "The Maxwell distribution is a symmetric bell curve about vrmsv_{rms}" is false, and it is offered as a distractor constantly. It is asymmetric, it starts at the origin, and its peak is at neither the mean nor the rms speed.

Reading a real number off it

Panel (b) of the figure is nitrogen at 300 K, cut into three bands. Those percentages are not decorations — each is the area of its band, and they were obtained by integrating F(v)F(v):

Speed range for nitrogen at 300 K Fraction of molecules
slower than 400 m/s 38.4%
between 400 and 800 m/s 55.0%
faster than 800 m/s 6.6%
all speeds 100%

Notice the arithmetic: 38.4+55.0+6.6=10038.4 + 55.0 + 6.6 = 100, exactly, because the three bands between them cover every possible speed. Any question that gives you two of these and asks for the third is asking you to subtract from 100%.

How the Curve Moves

The curve is not one fixed shape. It has exactly two knobs: the temperature and the molar mass. Learn what each does and you can answer most graph questions on this topic without calculating anything.

Knob 1: raise the temperature

Nitrogen speed curves at three temperatures, equal areas, peak lowers and shifts right

Heat the gas up and three things happen together:

  1. The peak moves to the right. Molecules get faster, so the commonest speed rises — and it rises as T\sqrt{T}, like every other speed in this chapter.
  2. The peak gets lower.
  3. The curve gets broader — the speeds spread out over a wider range.

Points 2 and 3 are not independent, and this is the part worth understanding rather than memorising.

Key Point — why heating LOWERS the peak: The area under the curve must stay equal to 1, because heating a sealed gas does not create or destroy a single molecule. If the curve spreads sideways, it must sag downwards to keep the same area. The curve flattens and shifts right; it does not simply slide right.

That constraint is exactly why the figure's three curves, at 300 K, 600 K and 1200 K, all enclose the same area even though they look so different. The peak height falls as 1T\frac{1}{\sqrt{T}} while the width grows as T\sqrt{T}, and the product — the area — never changes.

[JEE Tip] A graph question showing two Maxwell curves at different temperatures where the hotter one is both taller and wider is showing you an impossible gas. Check the areas first; it is often the whole question.

What flattening does to the tail

Look at panel (b) of that figure, because it holds the most useful fact in the section.

Nitrogen at Fraction of molecules faster than 1000 m/s
300 K 1.06%
600 K 13.20%
1200 K 42.24%

Doubling the temperature from 300 K to 600 K raises vrmsv_{rms} by only 2=1.41\sqrt{2} = 1.41, a modest 41%. But it multiplies the number of molecules beyond 1000 m/s by 12.5. The tail responds far more violently than the average does, and that single sentence is the explanation of evaporation, of atmospheric escape and of chemical reaction rates, which close this section.

Knob 2: change the gas

Speed distributions of helium, nitrogen and carbon dioxide at equal area and temperature

Now hold the temperature fixed and swap in a heavier gas. Everything runs backwards:

Key Point — heavier gas at the same temperature: The curve sharpens and shifts left. A heavier molecule is slower (all speeds go as 1M0\frac{1}{\sqrt{M_0}}), so the peak moves left; and since the area is still 1, a narrower curve must be a taller one. Light gas: broad, low, far to the right. Heavy gas: narrow, tall, hugging the left.

The figure shows helium (M0=0.004M_0 = 0.004 kg/mol), nitrogen (0.0280.028) and carbon dioxide (0.0440.044) all at 300 K. Helium's curve sprawls out past 2500 m/s; carbon dioxide's is a sharp spike near 340 m/s. Same temperature, same average kinetic energy per molecule, wildly different speeds — exactly what the previous section promised.

The two knobs on one line

every characteristic speed    TM0\text{every characteristic speed} \; \propto \; \sqrt{\frac{T}{M_0}}

  • Raise TT four times and every speed doubles, and the curve flattens and stretches right.
  • Use a gas four times heavier and every speed halves, and the curve sharpens and squeezes left.
  • Raise TT four times AND use a gas four times heavier and the curve is identical to what you started with. Only the ratio TM0\frac{T}{M_0} matters.

[NEET Important] That last line is a favourite. Oxygen at 1200 K has exactly the same speed distribution as helium at 150 K, because 12000.032=1500.004\frac{1200}{0.032} = \frac{150}{0.004}. Check the ratio before you compute anything.

The Three Characteristic Speeds

A whole curve is awkward to carry around, so we summarise it with numbers. The trouble is that a lopsided curve has no single obvious centre — and three perfectly reasonable definitions give three different answers.

Most probable, mean and rms speeds marked on one curve with fixed ratios

1. The most probable speed, vmpv_{mp}

The speed at the peak of the curve — the single commonest speed in the gas, the one more molecules have than any other. Find it by setting dFdv=0\frac{dF}{dv} = 0, and it comes out at

vmp=2kBTm=2RTM0v_{mp} = \sqrt{\frac{2k_BT}{m}} = \sqrt{\frac{2RT}{M_0}}

2. The average (mean) speed, vˉ\bar{v}

Add up every molecule's speed and divide by the number of molecules. As an integral over the distribution, vˉ=0vF(v)dv\bar{v} = \int_0^{\infty} v \, F(v)\, dv, and the answer is

vˉ=8kBTπm=8RTπM0\bar{v} = \sqrt{\frac{8k_BT}{\pi m}} = \sqrt{\frac{8RT}{\pi M_0}}

That stray π\pi in the denominator is the giveaway that you are looking at the mean speed and not something else. It is the only one of the three with a π\pi in it.

3. The root mean square speed, vrmsv_{rms}

Already derived in the previous section from 12mv2=32kBT\frac{1}{2}m\overline{v^2} = \frac{3}{2}k_BT, and repeated here only so the family is together:

vrms=v2=3kBTm=3RTM0v_{rms} = \sqrt{\overline{v^2}} = \sqrt{\frac{3k_BT}{m}} = \sqrt{\frac{3RT}{M_0}}

The ordering and the ratio — memorise this line

Strip out the common RTM0\sqrt{\frac{RT}{M_0}} and all that is left is the numerical coefficient: 2\sqrt{2}, 8/π\sqrt{8/\pi}, 3\sqrt{3}. Since 2<8π=2.546<32 < \frac{8}{\pi} = 2.546 < 3, the order can never change.

Key Point — the three speeds, in order, always: vmp<vˉ<vrmsv_{mp} < \bar{v} < v_{rms} vmp:vˉ:vrms  =  2:8π:3  =  1:1.128:1.225v_{mp} : \bar{v} : v_{rms} \;=\; \sqrt{2} : \sqrt{\frac{8}{\pi}} : \sqrt{3} \;=\; 1 : 1.128 : 1.225 This ratio is a pure number. It does not depend on the gas, on the temperature, on the pressure or on anything else. Know one of the three speeds and you know the other two by multiplication.

Two more forms of the same fact, both worth having ready:

vrmsvˉ=3π8=1.0854andvˉvrms=0.9213\frac{v_{rms}}{\bar{v}} = \sqrt{\frac{3\pi}{8}} = 1.0854 \qquad\text{and}\qquad \frac{\bar{v}}{v_{rms}} = 0.9213

So vˉ\bar{v} and vrmsv_{rms} differ by only about 8.5% — close enough that swapping them is easy, and far enough apart that a marker will notice.

[NEET Important] The mnemonic that survives exam pressure: "most probable is the smallest, rms is the biggest, mean is in the middle", and 1:1.128:1.2251 : 1.128 : 1.225. If you can only hold one number, hold 1.2251.225 — that is 3/2\sqrt{3/2}, the jump from vmpv_{mp} straight to vrmsv_{rms}.

The numbers, at 300 K

Note that every row is in the ratio 1:1.128:1.2251 : 1.128 : 1.225 — read down any column and you see the 1M0\frac{1}{\sqrt{M_0}} law; read across any row and you see the fixed ratio.

Gas M0M_0 (kg/mol) vmpv_{mp} (m/s) vˉ\bar{v} (m/s) vrmsv_{rms} (m/s)
Hydrogen, H2_2 0.002 1579 1782 1934
Helium, He 0.004 1117 1260 1368
Nitrogen, N2_2 0.028 422 476 517
Oxygen, O2_2 0.032 395 445 484
Carbon dioxide, CO2_2 0.044 337 380 412

And for air at STP — 273 K, with an average molar mass of 0.0290.029 kg/mol — the three come out as vmp=396v_{mp} = 396 m/s, vˉ=447\bar{v} = 447 m/s and vrms=485v_{rms} = 485 m/s. Keep those three straight: the mean-free-path section uses 447 m/s, and 485 m/s is the rms value for the same air. They are not interchangeable.

Where each one sits on the curve

The three speeds cut the distribution into pieces whose sizes are, remarkably, the same for every gas at every temperature — because the whole curve just stretches, and the three markers stretch with it.

Region Fraction of molecules
slower than vmpv_{mp} 42.8%
between vmpv_{mp} and vˉ\bar{v} 10.5%
between vˉ\bar{v} and vrmsv_{rms} 7.5%
faster than vrmsv_{rms} 39.2%

[JEE Tip] Read the first and last rows again. Fewer than half the molecules are slower than the most probable speed, and nearly 40% are faster than the rms speed. That is what asymmetry does: the long tail on the right drags both vˉ\bar{v} and vrmsv_{rms} up above the peak, so neither of them is a "halfway" speed. The median speed is not any of the three.

Which Speed Does Which Job

Three speeds, three jobs. Pick the wrong one and your answer is wrong by a fixed, embarrassing, easily-spotted percentage.

Key Point — the assignment, and it is not negotiable:

  • vrmsv_{rms} for anything built on v2v^2 — kinetic energy 12mv2\frac{1}{2}m\overline{v^2}, the pressure P=13nmv2P = \frac{1}{3}nm\overline{v^2}, the temperature relation 12mv2=32kBT\frac{1}{2}m\overline{v^2} = \frac{3}{2}k_BT. Energy is quadratic in speed, so the mean of the squares is what the physics actually contains.
  • vˉ\bar{v} for anything that counts distance travelled — the mean free path, the collision frequency fcoll=vˉlf_{\text{coll}} = \frac{\bar{v}}{l}, the collision time τ=lvˉ\tau = \frac{l}{\bar{v}}, effusion and diffusion rates. These count how far a molecule gets per second, and that is an ordinary average of speed.
  • vmpv_{mp} when the question is about the peak — the commonest speed, the position of the maximum, or scaling a curve.

What goes wrong when you swap them

Because the ratio is fixed, so is the error. These three numbers are worth knowing, because recognising one of them in a wrong answer tells you instantly what happened.

  • Using vˉ\bar{v} where vrmsv_{rms} belongs, in an energy formula. You compute 12m(vˉ)2\frac{1}{2}m(\bar{v})^2 instead of 12mv2\frac{1}{2}m\overline{v^2}, and since (vˉ)2=83πv2=0.849v2(\bar{v})^2 = \frac{8}{3\pi}\overline{v^2} = 0.849\,\overline{v^2}, your energy comes out 15.1% too low. Every time.
  • Using vrmsv_{rms} where vˉ\bar{v} belongs, in a collision count. The collision frequency comes out 1.08541.0854 times too big — 8.5% too high.
  • Quoting vmpv_{mp} where vrmsv_{rms} was wanted. That is a factor of 3/2=1.225\sqrt{3/2} = 1.225, so the answer is 18.4% too low.

[JEE Tip] If a numerical answer is out by roughly 8.5%, 15% or 18%, and everything else looks right, you have used the wrong molecular speed. Check that before you check your arithmetic.

The heart of it: v2\overline{v^2} is not (vˉ)2(\bar{v})^2

Everything above rests on one piece of mathematics that has nothing to do with gases, and it is worth doing with numbers you can count on your fingers.

Take two molecules, one at 300 m/s and one at 500 m/s.

Route A — average first, then square. vˉ=300+5002=400 m/s(vˉ)2=160000 m2/s2\bar{v} = \frac{300 + 500}{2} = 400 \text{ m/s} \quad\Longrightarrow\quad (\bar{v})^2 = 160000 \text{ m}^2\text{/s}^2

Route B — square first, then average. v2=3002+50022=90000+2500002=170000 m2/s2\overline{v^2} = \frac{300^2 + 500^2}{2} = \frac{90000 + 250000}{2} = 170000 \text{ m}^2\text{/s}^2 vrms=170000=412.3 m/sv_{rms} = \sqrt{170000} = 412.3 \text{ m/s}

170000160000170000 \neq 160000, and 412.3400412.3 \neq 400. Squaring and averaging do not commute.

Try it with five molecules at 200, 400, 600, 800 and 1000 m/s and the gap widens:

vˉ=200+400+600+800+10005=600 m/s,(vˉ)2=360000\bar{v} = \frac{200+400+600+800+1000}{5} = 600 \text{ m/s}, \qquad (\bar{v})^2 = 360000 v2=40000+160000+360000+640000+10000005=440000,vrms=663.3 m/s\overline{v^2} = \frac{40000+160000+360000+640000+1000000}{5} = 440000, \qquad v_{rms} = 663.3 \text{ m/s}

Key Point: v2(vˉ)2\overline{v^2} \geq (\bar{v})^2 always, with equality only if every molecule has exactly the same speed. The difference v2(vˉ)2\overline{v^2} - (\bar{v})^2 is the spread of the speeds, and it is never negative. That is why vrmsvˉv_{rms} \geq \bar{v}, always — the ordering of the three speeds is a mathematical fact about spread, not a special property of gases.

Squaring punishes the fast molecules more than it rewards the slow ones: doubling a speed quadruples its square. So the fast tail pulls v2\overline{v^2} up harder than it pulls vˉ\bar{v} up, and vrmsv_{rms} ends up on top.

For the Maxwell distribution in particular, the gap is fixed:

v2(vˉ)2=3π8=1.178\frac{\overline{v^2}}{(\bar{v})^2} = \frac{3\pi}{8} = 1.178

Take the square root of 1.1781.178 and you get 1.08541.0854 — the same vrmsvˉ\frac{v_{rms}}{\bar{v}} from the previous block, arriving by a different road.

[Board Important] A two-mark question that reads "show with an example that the mean square speed is not the square of the mean speed" wants exactly the two-molecule calculation above. Write both routes out, get 170000170000 against 160000160000, and say the difference is the spread. Full marks.

The Tail That Runs the World

The average speed of a gas explains very little. The tail — the small fraction of molecules moving far faster than average — explains a surprising amount, and it does so because it is so exquisitely sensitive to temperature.

Here is how thin the tail is, for any gas at any temperature, measured in multiples of the most probable speed:

Molecules faster than Fraction
vmpv_{mp} 57.2%
2vmp2\,v_{mp} 4.6%
3vmp3\,v_{mp} 4.4×1044.4 \times 10^{-4}, about 1 in 2300
4vmp4\,v_{mp} 5.2×1075.2 \times 10^{-7}, about 1 in 2 million
5vmp5\,v_{mp} 8.1×10118.1 \times 10^{-11}, about 1 in 12 billion

The fall is savage — but it never reaches zero, and warming the gas slides the whole curve right underneath these fixed thresholds, which is where the drama comes from.

1. Evaporation, and why it cools

A puddle of water at 30°C is nowhere near its boiling point, yet it dries up. Why?

Because the molecules in it also have a distribution of speeds, and only the ones at the very top of the tail have enough kinetic energy to break free of the attractions holding the liquid together. Those escape. The ones left behind are, by construction, the slower ones — so the average kinetic energy of the remaining liquid drops, and the liquid gets colder. That is why sweat cools you, why a wet earthen pot keeps water cool, and why blowing across hot tea works: you sweep away the escaped fast molecules before they can come back, so the escaping continues.

Warm the puddle and the tail beyond the escape threshold swells enormously — which is why evaporation speeds up so sharply with temperature, long before boiling.

2. Why Earth has no hydrogen but plenty of nitrogen

To leave Earth for good, a molecule high in the atmosphere needs the escape speed, about 11.211.2 km/s. Up in the exosphere the temperature is around 1000 K. Compare two gases there:

Gas at 1000 K vmpv_{mp} escape speed in units of vmpv_{mp} Fraction fast enough to escape
Hydrogen, H2_2 2883 m/s 3.9 about 1.3×1061.3 \times 10^{-6}
Helium, He 2039 m/s 5.5 about 5×10135 \times 10^{-13}
Nitrogen, N2_2 771 m/s 14.5 about 109110^{-91}

For hydrogen, roughly one molecule in a million is fast enough at any moment — and over billions of years, with collisions constantly refilling the tail, that is more than enough to strip the planet bare. For nitrogen the fraction is 109110^{-91}, which over the age of the universe is indistinguishable from never. Earth kept its nitrogen and oxygen and lost its hydrogen and helium, and the entire explanation is where those numbers sit in the tail.

[NEET Important] The Moon has no atmosphere for the same reason with the numbers pushed further: its escape speed is only about 2.42.4 km/s, so even nitrogen and oxygen sit near enough to the top of the tail to have leaked away. Jupiter, cold and massive, kept even its hydrogen.

3. Why reaction rates climb so steeply with temperature

A chemical reaction usually needs the colliding molecules to arrive with more than some minimum energy — the activation energy. Only tail molecules qualify.

Take an activation energy of 50 kJ/mol, which is unremarkable, and nitrogen-sized molecules. The threshold speed works out at about 1890 m/s, and integrating the distribution above it gives:

  • at 300 K: a fraction 1.02×1081.02 \times 10^{-8}
  • at 310 K: a fraction 1.93×1081.93 \times 10^{-8}

A rise of just 10 kelvin — about 3% in absolute temperature — nearly doubles the number of molecules that can react. Meanwhile vrmsv_{rms} went up by a feeble 1.65%. That is the origin of the chemist's rule of thumb that reaction rates roughly double for every ten-degree rise, and it is a statement about the tail, not about the average.

Key Point: Averages change slowly with temperature, as T\sqrt{T}. Tails change exponentially. Whenever a physical process has a threshold — escape from a liquid, escape from a planet, getting over an activation barrier — the rate is governed by the tail, and it will be far more temperature-sensitive than any average suggests.

The trap list for this section

  • Never mix up the three speeds. vmp<vˉ<vrmsv_{mp} < \bar{v} < v_{rms}, in the ratio 1:1.128:1.2251 : 1.128 : 1.225, always.
  • vrmsv_{rms} for energy and pressure, vˉ\bar{v} for mean free path and collision rate. Swapping costs 15.1% or 8.5% respectively.
  • v2(vˉ)2\overline{v^2} \neq (\bar{v})^2. Square first, then average — the other order is a different (and smaller) number.
  • The curve is asymmetric and starts at the origin. Not a symmetric bell, and not centred on vrmsv_{rms}.
  • Area, not height. A fraction of molecules is always an area between two speeds; the fraction at exactly one speed is zero.
  • Equal areas. Curves at two temperatures, or for two gases, must enclose the same area. Hotter means flatter and wider; heavier means taller and narrower.
  • M0M_0 in kg/mol, TT in kelvin. Every one of the three formulas carries the same molar-mass hazard: oxygen is 0.0320.032, never 32.
  • Only TM0\frac{T}{M_0} matters for the shape. Two gases with the same TM0\frac{T}{M_0} have identical distributions.

Solved Examples

Constants used throughout: kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K; R=8.314R = 8.314 J/(mol K); NA=6.022×1023N_A = 6.022 \times 10^{23} per mole; 0°C=273.150°C = 273.15 K.

Example 1: All three speeds for oxygen

Find vmpv_{mp}, vˉ\bar{v} and vrmsv_{rms} for oxygen at 27°C. Molar mass of oxygen is 32 g/mol. Verify that your three answers are in the standard ratio.

Solution:

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

  2. Molar mass to kilograms per mole, on its own line, always. M0=32 g/mol=0.032 kg/molM_0 = 32 \text{ g/mol} = 0.032 \text{ kg/mol}

  3. The common core. All three formulas share RTM0\frac{RT}{M_0}, so compute it once: RTM0=8.314×3000.032=77950 m2/s2\frac{RT}{M_0} = \frac{8.314 \times 300}{0.032} = 77950 \text{ m}^2\text{/s}^2

  4. Now just attach the three coefficients. vmp=2×77950=155900=395 m/sv_{mp} = \sqrt{2 \times 77950} = \sqrt{155900} = 395 \text{ m/s} vˉ=8π×77950=198500=445 m/s\bar{v} = \sqrt{\frac{8}{\pi} \times 77950} = \sqrt{198500} = 445 \text{ m/s} vrms=3×77950=233850=484 m/sv_{rms} = \sqrt{3 \times 77950} = \sqrt{233850} = 484 \text{ m/s}

  5. Check the ordering and the ratio. 395<445<484395 < 445 < 484 \quad\checkmark 445395=1.1271.128,484395=1.225\frac{445}{395} = 1.127 \approx 1.128, \qquad \frac{484}{395} = 1.225 \quad\checkmark

Final Answer: vmp=395v_{mp} = 395 m/s, vˉ=445\bar{v} = 445 m/s, vrms=484v_{rms} = 484 m/s.

Takeaway: Compute RTM0\frac{RT}{M_0} once and reuse it three times. The three speeds differ only by the coefficient under the root — 22, 8π\frac{8}{\pi}, 33 — so doing the shared arithmetic once saves two-thirds of the work and removes two chances to slip.

Example 2: One speed given, the other two wanted

The rms speed of nitrogen at a certain temperature is 517 m/s. Without finding the temperature, find the average and most probable speeds.

Solution:

  1. Use the ratio, not the formulas. Since vmp:vˉ:vrms=1:1.128:1.225v_{mp} : \bar{v} : v_{rms} = 1 : 1.128 : 1.225 at every temperature, the temperature is not needed and is not asked for.

  2. Most probable speed. Divide by 1.2251.225: vmp=vrms1.225=5171.225=422 m/sv_{mp} = \frac{v_{rms}}{1.225} = \frac{517}{1.225} = 422 \text{ m/s}

  3. Average speed. Either multiply vmpv_{mp} by 1.1281.128, or divide vrmsv_{rms} by 1.08541.0854: vˉ=422×1.128=476 m/sorvˉ=5171.0854=476 m/s\bar{v} = 422 \times 1.128 = 476 \text{ m/s} \qquad\text{or}\qquad \bar{v} = \frac{517}{1.0854} = 476 \text{ m/s} The two routes agree, which is the check.

  4. Sanity. 422<476<517422 < 476 < 517, in the right order and all in the few-hundred-metres-per-second band where molecular speeds live.

Final Answer: vˉ=476\bar{v} = 476 m/s and vmp=422v_{mp} = 422 m/s.

Takeaway: When a question gives you one of the three speeds and asks for another, the temperature and molar mass are decoration. The ratio 1:1.128:1.2251 : 1.128 : 1.225 does the whole job in one multiplication.

Example 3: Identifying a gas from its peak

The speed distribution of a certain gas at 300 K peaks at 500 m/s. Identify the gas, and find its average and rms speeds.

Solution:

  1. The peak is vmpv_{mp}, by definition. So vmp=2RTM0=500 m/sv_{mp} = \sqrt{\frac{2RT}{M_0}} = 500 \text{ m/s}

  2. Square and rearrange for the molar mass. M0=2RTvmp2=2×8.314×3005002=4988250000=0.01995 kg/molM_0 = \frac{2RT}{v_{mp}^2} = \frac{2 \times 8.314 \times 300}{500^2} = \frac{4988}{250000} = 0.01995 \text{ kg/mol}

  3. Convert to the units a periodic table uses. M0=0.01995 kg/mol=19.95 g/mol20 g/molM_0 = 0.01995 \text{ kg/mol} = 19.95 \text{ g/mol} \approx 20 \text{ g/mol} That is neon. (The unit assertion holds: 0.01995<10.01995 < 1, so the molar mass really is in kg/mol.)

  4. The other two speeds, straight from the ratio. vˉ=1.128×500=564 m/s,vrms=1.225×500=612 m/s\bar{v} = 1.128 \times 500 = 564 \text{ m/s}, \qquad v_{rms} = 1.225 \times 500 = 612 \text{ m/s}

Final Answer: The gas is neon, M020M_0 \approx 20 g/mol; vˉ=564\bar{v} = 564 m/s and vrms=612v_{rms} = 612 m/s.

Takeaway: A peak on a speed-distribution graph is vmpv_{mp}, so it is a direct measurement of TM0\frac{T}{M_0}. Reading the peak position off an experimental curve is a genuine way to weigh a molecule — and note that the answer came out in kg/mol and had to be multiplied by 1000 to be recognisable.

Example 4: Mean square is not the square of the mean

Five molecules have speeds 200, 400, 600, 800 and 1000 m/s. Find (a) the average speed, (b) the mean square speed, (c) the rms speed, and (d) show that v2(vˉ)2\overline{v^2} \neq (\bar{v})^2. Compare the ratio vrmsvˉ\frac{v_{rms}}{\bar{v}} with the value 1.08541.0854 that a full Maxwell distribution would give.

Solution:

  1. (a) Average speed — add and divide: vˉ=200+400+600+800+10005=30005=600 m/s\bar{v} = \frac{200 + 400 + 600 + 800 + 1000}{5} = \frac{3000}{5} = 600 \text{ m/s}

  2. (b) Mean square speed — square each, then average: v2=2002+4002+6002+8002+100025=40000+160000+360000+640000+10000005\overline{v^2} = \frac{200^2 + 400^2 + 600^2 + 800^2 + 1000^2}{5} = \frac{40000 + 160000 + 360000 + 640000 + 1000000}{5} v2=22000005=440000 m2/s2\overline{v^2} = \frac{2200000}{5} = 440000 \text{ m}^2\text{/s}^2

  3. (c) Rms speed: vrms=440000=663.3 m/sv_{rms} = \sqrt{440000} = 663.3 \text{ m/s}

  4. (d) The comparison. (vˉ)2=6002=360000butv2=440000(\bar{v})^2 = 600^2 = 360000 \qquad\text{but}\qquad \overline{v^2} = 440000 They differ by 8000080000, and the mean square is the larger one — as it must be, because that difference is the spread of the speeds and a spread cannot be negative.

  5. The ratio. vrmsvˉ=663.3600=1.106\frac{v_{rms}}{\bar{v}} = \frac{663.3}{600} = 1.106 A real Maxwell distribution gives 1.08541.0854. Ours is a little higher because five evenly spaced speeds are a wider, flatter spread than the real curve, which bunches most molecules near the peak.

Final Answer: (a) 600 m/s; (b) 4.4×1054.4 \times 10^{5} m2^2/s2^2; (c) 663.3 m/s; (d) 440000360000440000 \neq 360000, and vrmsvˉ=1.106\frac{v_{rms}}{\bar{v}} = 1.106 against 1.0854 for a true Maxwell gas.

Takeaway: Square first, then average — never the other way round. The gap between v2\overline{v^2} and (vˉ)2(\bar{v})^2 is the spread of speeds, which is why vrmsv_{rms} always sits above vˉ\bar{v}, for any set of numbers whatsoever.

Example 5: Choosing the speed for a collision count

Air at STP has a mean free path of 2.1×1072.1 \times 10^{-7} m. Take the mean molar mass of air as 29 g/mol. Find the collision frequency of a molecule, using the correct speed — and then find what answer you would get with the wrong one, and by what percentage it is off.

Solution:

  1. Kelvin and kilograms first. T=273.15 K,M0=29 g/mol=0.029 kg/molT = 273.15 \text{ K}, \qquad M_0 = 29 \text{ g/mol} = 0.029 \text{ kg/mol}

  2. Which speed? Collision frequency counts how many collisions happen per second, which means how much distance is covered per second. Distance per second is an ordinary average of speed, so this wants vˉ\bar{v}. vˉ=8RTπM0=8×8.314×273.153.1416×0.029=199400=447 m/s\bar{v} = \sqrt{\frac{8RT}{\pi M_0}} = \sqrt{\frac{8 \times 8.314 \times 273.15}{3.1416 \times 0.029}} = \sqrt{199400} = 447 \text{ m/s}

  3. The collision frequency. fcoll=vˉl=4472.1×107=2.1×109 per secondf_{\text{coll}} = \frac{\bar{v}}{l} = \frac{447}{2.1 \times 10^{-7}} = 2.1 \times 10^{9} \text{ per second} and the collision time is τ=1fcoll=4.7×1010\tau = \frac{1}{f_{\text{coll}}} = 4.7 \times 10^{-10} s.

  4. Now the wrong road. With vrmsv_{rms} instead: vrms=3RTM0=3×8.314×273.150.029=485 m/sv_{rms} = \sqrt{\frac{3RT}{M_0}} = \sqrt{\frac{3 \times 8.314 \times 273.15}{0.029}} = 485 \text{ m/s} fcollwrong=4852.1×107=2.3×109 per secondf_{\text{coll}}^{\text{wrong}} = \frac{485}{2.1 \times 10^{-7}} = 2.3 \times 10^{9} \text{ per second}

  5. The size of the error. The ratio is exactly vrmsvˉ=1.0854\frac{v_{rms}}{\bar{v}} = 1.0854, so the wrong answer is 8.5% too high — every time, for every gas, at every temperature.

Final Answer: fcoll=2.1×109f_{\text{coll}} = 2.1 \times 10^{9} per second using vˉ=447\bar{v} = 447 m/s. Using vrms=485v_{rms} = 485 m/s instead gives 2.3×1092.3 \times 10^{9}, which is 8.5% too high.

Takeaway: The mean free path and the collision rate want vˉ\bar{v}; energy and pressure want vrmsv_{rms}. The 447 against 485 for air at STP is worth memorising as a pair — seeing 485 in a collision-rate answer is an instant diagnosis.

Example 6: Choosing the speed for an energy

For nitrogen at 300 K, find the average translational kinetic energy per molecule two ways: correctly, from 12mv2\frac{1}{2}m\overline{v^2}, and incorrectly, from 12m(vˉ)2\frac{1}{2}m(\bar{v})^2. Take M0=28M_0 = 28 g/mol. By what percentage does the wrong route fail?

Solution:

  1. Set up. M0=28M_0 = 28 g/mol =0.028= 0.028 kg/mol, and the mass of one molecule is 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}

  2. The two speeds at 300 K: vrms=3×8.314×3000.028=517 m/s,vˉ=8×8.314×3003.1416×0.028=476 m/sv_{rms} = \sqrt{\frac{3 \times 8.314 \times 300}{0.028}} = 517 \text{ m/s}, \qquad \bar{v} = \sqrt{\frac{8 \times 8.314 \times 300}{3.1416 \times 0.028}} = 476 \text{ m/s}

  3. Correct energy, using the mean square: ε=12mv2=12×4.65×1026×(517)2=6.21×1021 J\overline{\varepsilon} = \frac{1}{2} m \overline{v^2} = \frac{1}{2} \times 4.65 \times 10^{-26} \times (517)^2 = 6.21 \times 10^{-21} \text{ J} which is exactly 32kBT\frac{3}{2}k_BT at 300 K, as the previous section established.

  4. Wrong energy, using the square of the mean: 12m(vˉ)2=12×4.65×1026×(476)2=5.27×1021 J\frac{1}{2} m (\bar{v})^2 = \frac{1}{2} \times 4.65 \times 10^{-26} \times (476)^2 = 5.27 \times 10^{-21} \text{ J}

  5. The shortfall. The ratio of the two is (vˉ)2v2=8/π3=0.849\frac{(\bar{v})^2}{\overline{v^2}} = \frac{8/\pi}{3} = 0.849, so error=(10.849)×100=15.1% too low\text{error} = (1 - 0.849) \times 100 = 15.1\% \text{ too low}

Final Answer: Correct: 6.21×10216.21 \times 10^{-21} J. Using vˉ\bar{v}: 5.27×10215.27 \times 10^{-21} J, which is 15.1% too low.

Takeaway: Kinetic energy is quadratic in speed, so it needs the mean of the squares. A kinetic energy computed from the average speed is always short by 15.1% — a fixed penalty, because the ratio of the two speeds is fixed.

Example 7: Matching a mean speed to an rms speed

At what temperature will the average speed of oxygen molecules equal the rms speed of hydrogen molecules at 300 K? Molar masses: oxygen 32 g/mol, hydrogen 2 g/mol.

Solution:

  1. Convert everything first. MO2=0.032 kg/mol,MH2=0.002 kg/mol,TH2=300 KM_{O_2} = 0.032 \text{ kg/mol}, \qquad M_{H_2} = 0.002 \text{ kg/mol}, \qquad T_{H_2} = 300 \text{ K}

  2. The target speed — hydrogen's rms speed at 300 K: vrms,H2=3×8.314×3000.002=3.741×106=1934 m/sv_{rms,H_2} = \sqrt{\frac{3 \times 8.314 \times 300}{0.002}} = \sqrt{3.741 \times 10^{6}} = 1934 \text{ m/s}

  3. Set oxygen's mean speed equal to it. Note the two different coefficients — this is exactly the trap the question is built around: 8RTO2πMO2=1934\sqrt{\frac{8 R T_{O_2}}{\pi M_{O_2}}} = 1934

  4. Square and solve. TO2=(1934)2×π×MO28R=3.741×106×3.1416×0.0328×8.314=37610066.51=5655 KT_{O_2} = \frac{(1934)^2 \times \pi \times M_{O_2}}{8R} = \frac{3.741 \times 10^{6} \times 3.1416 \times 0.032}{8 \times 8.314} = \frac{376100}{66.51} = 5655 \text{ K}

  5. Check by going forwards. At 5655 K, oxygen's mean speed is vˉ=8×8.314×56553.1416×0.032=1934 m/s\bar{v} = \sqrt{\frac{8 \times 8.314 \times 5655}{3.1416 \times 0.032}} = 1934 \text{ m/s} \quad\checkmark

Final Answer: 5655 K.

Takeaway: When the two speeds being matched are of different kinds, you cannot just cancel the coefficients. Had both been rms speeds, the answer would have been 300×16=4800300 \times 16 = 4800 K; the extra factor of 3π8=1.178\frac{3\pi}{8} = 1.178 that lifts it to 5655 K is precisely the vrmsv_{rms}-versus-vˉ\bar{v} difference.

Example 8: Reading fractions off a distribution

For nitrogen at 300 K (vmp=422v_{mp} = 422 m/s), 38.4% of molecules are slower than 400 m/s and 6.6% are faster than 800 m/s. Find (a) the fraction between 400 and 800 m/s, and (b) the fraction of molecules faster than the most probable speed. (c) A student says "the fraction of molecules moving at exactly 500 m/s is about 0.2%." What is wrong with that?

Solution:

  1. (a) The three bands cover every possible speed, so their areas must add to 1, that is to 100%: fraction between 400 and 800=10038.46.6=55.0%\text{fraction between 400 and 800} = 100 - 38.4 - 6.6 = 55.0\% No integration needed — just the fact that the total area is fixed.

  2. (b) Fraction faster than vmpv_{mp}. The fraction slower than vmpv_{mp} is 42.8% for any gas at any temperature, since the curve simply stretches and the marker stretches with it. So faster than vmp=10042.8=57.2%\text{faster than } v_{mp} = 100 - 42.8 = 57.2\% Note what this says: more than half the molecules are faster than the most probable speed. The curve's long right tail is why.

  3. (c) The student's error. "Exactly 500 m/s" is a single point on the speed axis, a range of zero width. The fraction of molecules in it is the area of a strip of zero width, which is zero. F(v)F(v) is a fraction per unit speed range, not a fraction; to get a number you must specify a band, such as "between 499 and 501 m/s".

Final Answer: (a) 55.0%; (b) 57.2%; (c) the fraction at exactly one speed is zero — a distribution gives fractions only over ranges.

Takeaway: Total area is 1, so complementary fractions are a subtraction, not an integral. And "what fraction has speed exactly vv" is always zero: read areas, never heights.

Example 9: What heating does to the whole curve

A sealed vessel of nitrogen is heated from 300 K to 1200 K. Describe what happens to (a) the most probable speed, (b) the height of the peak, (c) the area under the curve, and (d) the fraction of molecules faster than 1000 m/s, which is 1.06% at 300 K and 42.24% at 1200 K.

Solution:

  1. (a) The most probable speed. vmpTv_{mp} \propto \sqrt{T}, and the temperature has gone up four times, so vmp,2vmp,1=1200300=4=2\frac{v_{mp,2}}{v_{mp,1}} = \sqrt{\frac{1200}{300}} = \sqrt{4} = 2 vmp:422 m/s844 m/sv_{mp} : 422 \text{ m/s} \longrightarrow 844 \text{ m/s} The peak moves right, and it exactly doubles.

  2. (b) The height of the peak. The peak height goes as 1T\frac{1}{\sqrt{T}}, so it halves. In the figure earlier in this section it drops from about 1.97×1031.97 \times 10^{-3} to about 0.98×1030.98 \times 10^{-3} per (m/s).

  3. (c) The area. Unchanged, at exactly 1. The vessel is sealed, so not one molecule has been created or destroyed. This is the reason (a) and (b) had to move in opposite directions: the curve got twice as wide, so it had to get half as tall.

  4. (d) The tail. 42.241.06=39.8\frac{42.24}{1.06} = 39.8 Nearly forty times as many molecules are now above 1000 m/s. Compare that with the speeds themselves, which merely doubled.

  5. The moral. Multiplying TT by 4 doubles every characteristic speed but multiplies the population of a fixed high-speed band by about 40. Tails are exponential; averages are only square-root.

Final Answer: (a) doubles, 422 m/s to 844 m/s; (b) halves; (c) unchanged at 1; (d) grows by a factor of about 40.

Takeaway: Heating spreads molecules out; it does not make more of them. Right-and-down is the only way a normalised curve can move when it is heated, and any graph showing a hotter curve that is taller as well as wider is wrong.

Example 10: Why the atmosphere kept nitrogen and lost hydrogen

At an exospheric temperature of 1000 K, find the most probable speed of hydrogen (2 g/mol) and of nitrogen (28 g/mol), and compare each with Earth's escape speed of 11.211.2 km/s. Given that the fraction of molecules faster than the escape speed is about 1.3×1061.3 \times 10^{-6} for hydrogen and about 109110^{-91} for nitrogen, explain the composition of our atmosphere.

Solution:

  1. Convert, and check the kelvin. T=1000T = 1000 K is already absolute. MH2=0.002M_{H_2} = 0.002 kg/mol and MN2=0.028M_{N_2} = 0.028 kg/mol, both safely less than 1 as a molar mass in kg/mol must be.

  2. Most probable speeds. vmp,H2=2×8.314×10000.002=8.314×106=2883 m/sv_{mp,H_2} = \sqrt{\frac{2 \times 8.314 \times 1000}{0.002}} = \sqrt{8.314 \times 10^{6}} = 2883 \text{ m/s} vmp,N2=2×8.314×10000.028=5.939×105=771 m/sv_{mp,N_2} = \sqrt{\frac{2 \times 8.314 \times 1000}{0.028}} = \sqrt{5.939 \times 10^{5}} = 771 \text{ m/s}

  3. How far out on the tail is the escape speed? vescvmp,H2=112002883=3.9butvescvmp,N2=11200771=14.5\frac{v_{esc}}{v_{mp,H_2}} = \frac{11200}{2883} = 3.9 \qquad\text{but}\qquad \frac{v_{esc}}{v_{mp,N_2}} = \frac{11200}{771} = 14.5

  4. Read those against the tail table. At about 3.9 times the most probable speed, hydrogen still has roughly one molecule in a million above the line. At 14.5 times, nitrogen's fraction is around 109110^{-91} — a number so small that in the entire age of the Earth, with 104410^{44} molecules trying, not one would make it.

  5. The consequence. Collisions constantly refill the tail, so hydrogen's one-in-a-million leaks away continuously and, over billions of years, completely. Nitrogen and oxygen never get a chance. Earth's atmosphere is 78% nitrogen and 21% oxygen with essentially no free hydrogen or helium, and the reason is the position of the escape speed on the Maxwell tail.

Final Answer: vmp=2883v_{mp} = 2883 m/s for hydrogen and 771 m/s for nitrogen; the escape speed is 3.9 times the first and 14.5 times the second, which is the difference between leaking away and staying forever.

Takeaway: Atmospheric escape is decided by where vescv_{esc} sits in units of vmpv_{mp}, not by whether the average molecule can escape. No average molecule ever escapes from anywhere; the tail does all the work.

Example 11: Two gases with the same distribution

(a) At 300 K, oxygen has some speed distribution. At what temperature would helium have exactly the same distribution curve? (b) Separately: for two gases A and B at the same temperature, vrmsv_{rms} of A equals vmpv_{mp} of B. Find MAMB\frac{M_A}{M_B}. Molar masses: oxygen 32 g/mol, helium 4 g/mol.

Solution:

  1. (a) What fixes the curve. Every speed in the distribution goes as TM0\sqrt{\frac{T}{M_0}}, and the curve's shape depends on nothing else. Two gases share a curve when they share TM0\frac{T}{M_0}: THeMHe=TO2MO2THe=300×0.0040.032=300×18=37.5 K\frac{T_{He}}{M_{He}} = \frac{T_{O_2}}{M_{O_2}} \quad\Longrightarrow\quad T_{He} = 300 \times \frac{0.004}{0.032} = 300 \times \frac{1}{8} = 37.5 \text{ K}

  2. Check it. vmpv_{mp} for helium at 37.5 K is 2×8.314×37.50.004=395\sqrt{\frac{2 \times 8.314 \times 37.5}{0.004}} = 395 m/s, which is exactly oxygen's vmpv_{mp} at 300 K. The curves are identical.

  3. (b) Setting an rms speed equal to a most probable speed. Same temperature, so TT cancels, but the coefficients do not: 3RTMA=2RTMB\sqrt{\frac{3RT}{M_A}} = \sqrt{\frac{2RT}{M_B}}

  4. Square both sides and cancel RTRT: 3MA=2MBMAMB=32=1.5\frac{3}{M_A} = \frac{2}{M_B} \quad\Longrightarrow\quad \frac{M_A}{M_B} = \frac{3}{2} = 1.5

  5. Does it make sense? vrmsv_{rms} has the bigger coefficient, so to bring it down to B's most probable speed, gas A must be the heavier one — and indeed MA>MBM_A > M_B.

Final Answer: (a) 37.537.5 K; (b) MAMB=32\frac{M_A}{M_B} = \frac{3}{2}.

Takeaway: Only the combination TM0\frac{T}{M_0} shapes the curve — so a light gas at low temperature can be an exact stand-in for a heavy gas at high temperature. And when you equate two different kinds of speed, carry the coefficients 22, 8π\frac{8}{\pi}, 33 through; they are the whole content of the question.

Example 12: The 10-degree rule for reaction rates

A reaction needs colliding molecules to arrive with a translational kinetic energy above 50 kJ/mol. For a gas of molar mass 28 g/mol, (a) find the threshold speed, and (b) given that the fraction of molecules above that speed is 1.02×1081.02 \times 10^{-8} at 300 K and 1.93×1081.93 \times 10^{-8} at 310 K, comment on how the reaction rate responds to a 10-degree rise, and contrast it with what happens to vrmsv_{rms}.

Solution:

  1. (a) Get the threshold energy per molecule. The 50 kJ/mol is per mole, so divide by NAN_A: E=500006.022×1023=8.30×1020 J per moleculeE = \frac{50000}{6.022 \times 10^{23}} = 8.30 \times 10^{-20} \text{ J per molecule}

  2. Mass of one molecule: m=0.0286.022×1023=4.65×1026 kgm = \frac{0.028}{6.022 \times 10^{23}} = 4.65 \times 10^{-26} \text{ kg}

  3. Set 12mv2=E\frac{1}{2}mv^2 = E and solve for the speed: vthr=2Em=2×8.30×10204.65×1026=3.57×106=1890 m/sv_{thr} = \sqrt{\frac{2E}{m}} = \sqrt{\frac{2 \times 8.30 \times 10^{-20}}{4.65 \times 10^{-26}}} = \sqrt{3.57 \times 10^{6}} = 1890 \text{ m/s} For reference, vrmsv_{rms} at 300 K is only 517 m/s, so the threshold sits at about 4.5vmp4.5\,v_{mp} — deep in the tail, which is why the fractions are around 10810^{-8}.

  4. (b) The effect of 10 kelvin. 1.93×1081.02×108=1.89\frac{1.93 \times 10^{-8}}{1.02 \times 10^{-8}} = 1.89 The number of molecules able to react nearly doubles.

  5. Now the contrast. Over the same 10 K, vrms(310)vrms(300)=310300=1.0165\frac{v_{rms}(310)}{v_{rms}(300)} = \sqrt{\frac{310}{300}} = 1.0165 a rise of just 1.65%.

  6. The point. A 1.65% change in the average produced an 89% change in the tail population. This is the origin of the familiar rule that reaction rates roughly double for every ten-degree rise in temperature, and it is a statement about the shape of the Maxwell tail, not about how fast the average molecule is going.

Final Answer: (a) vthr=1890v_{thr} = 1890 m/s; (b) the reactive fraction nearly doubles (factor 1.89) while vrmsv_{rms} rises by only 1.65%.

Takeaway: Any process with a threshold is governed by the tail, and tails are exponentially sensitive to temperature. Whenever a rate changes far faster with temperature than T\sqrt{T} would suggest, look for a threshold and a Maxwell tail behind it.