AP® Physics 2: Algebra-Based review sheet from Aim for Five (aimforfive.com/physics-2/units/9/9-1)
Unit 9 · Topic 9.1
9.1 Kinetic Theory of Temperature and Pressure
Kinetic theory explains what a gas is doing at the atomic level. Pressure is the push of countless atoms bouncing off a surface, and temperature measures the average kinetic energy of those atoms. This topic links things you can measure with a gauge and a thermometer to the motion of particles you can't see.
Key terms
- pressure
- kinetic theory
- average kinetic energy
- Boltzmann constant
- root-mean-square speed
- Maxwell–Boltzmann distribution
What's changed recently
AP Physics 2 was revised for the 2024–25 school year. Its units are now numbered 9 to 15, picking up where AP Physics 1's Units 1–8 leave off, so thermodynamics is Unit 9 and this topic is 9.1. Older books and reviews number the course's units 1 to 7, with fluids as Unit 1 and thermodynamics as Unit 2.
Fluids (pressure in liquids, buoyancy and Bernoulli's equation) moved to AP Physics 1, so if an older Physics 2 review opens with fluids, you can skip that part. Going the other way, electric charge, simple circuits, and waves and sound left AP Physics 1, so this course now teaches them from the start (Units 10, 11 and 14).
The free-response questions changed in May 2025 to four set types: mathematical routines, translation between representations, experimental design and analysis, and qualitative/quantitative translation. Physics 2 free-response questions from 2024 and earlier are built differently.
Starting in May 2027, the multiple-choice section has 42 questions in 85 minutes (up from 40 in 80), and the four free-response questions take 95 minutes (down from 100). You can use a calculator and the equation sheet on both sections.
Where gas pressure comes from
A gas is a huge number of atoms flying around in random directions. When an atom hits a wall and bounces back, its momentum changes, so the wall must have pushed on it. By Newton's third law, the atom pushed back on the wall just as hard. One collision is a tiny tap, but trillions of them every second add up to a steady force.
Pressure is that force spread over an area: . Only the part of each push that is perpendicular to the surface counts. The unit is the pascal (1 Pa = 1 N/m²), and normal air pressure is about 1.0 × 10⁵ Pa, or 1 atmosphere.
Pressure isn't only at the walls. It exists everywhere inside the gas. If you placed a tiny surface anywhere in the middle of the container, atoms would hit both sides of it.
Collisions follow momentum rules
Atoms in an ideal gas collide elastically, with each other and with the walls. Momentum is conserved in atom–atom collisions, in one or two dimensions, just like the carts and pucks you studied in Physics 1.
For an atom of mass m that hits a wall head-on at speed v and bounces straight back, the change in momentum is 2mv (from +mv to −mv). A glancing hit changes only the perpendicular component of velocity, so it delivers less push.
Pressure goes up when collisions happen more often (more atoms, or a smaller container) or hit harder (faster atoms). Heating a gas does both at once.
Temperature is average kinetic energy
The temperature of a gas tells you the average translational kinetic energy of its atoms:
Here J/K is Boltzmann's constant and T must be in kelvins (K = °C + 273). Two big consequences follow. First, average kinetic energy is proportional to absolute temperature: double T in kelvins and you double . Second, it doesn't depend on which gas it is. Helium and argon at the same temperature have the same average kinetic energy per atom.
Setting gives the root-mean-square (rms) speed, . The rms speed is the square root of the average of the squared speeds. It's a typical speed, not the speed of every atom. Because m is in the denominator, lighter atoms move faster at the same temperature.
The Maxwell–Boltzmann distribution
Atoms in a gas don't all share one speed. Collisions constantly speed some up and slow others down. The Maxwell–Boltzmann distribution is a graph of how many atoms have each speed. It starts at zero (almost no atoms are nearly still), rises to a peak at the most probable speed, then falls off with a long tail toward high speeds. The curve is lopsided, with the tail stretching out to the right.
You need to know how its shape changes, not its formula.
- Hotter gas: the peak moves to a higher speed and gets lower, and the curve spreads out. More atoms are very fast.
- Same gas, same number of atoms: the area under the curve stays the same, because the area stands for the total number of atoms.
- Heavier atoms at the same temperature: the peak sits at a lower speed and the curve is taller and narrower.
Worked examples
Try each one yourself first, then open the solution.
- Example 1Calculator allowed
rms speed of helium
Helium atoms have a mass of 6.64 × 10⁻²⁷ kg. Find the average kinetic energy and the rms speed of the atoms in helium gas at 300 K.
Show the solutionHide the solution
- Step 1: Average kinetic energy: J.
- Step 2: Solve for the speed: .
- Step 3: That gives about 1370 m/s, roughly four times the speed of sound in air.
Answer: ≈ 6.2 × 10⁻²¹ J and ≈ 1.4 × 10³ m/s
- Example 2Calculator allowed
Doubling the temperature (classic trap)
A gas is heated from 20 °C to 40 °C. A student says the average kinetic energy of its atoms doubles. Is that right? To what Celsius temperature would you have to heat the gas to really double its average kinetic energy?
Show the solutionHide the solution
- Step 1: is proportional to absolute temperature, so convert to kelvins: 20 °C = 293 K and 40 °C = 313 K.
- Step 2: The ratio is 313/293 ≈ 1.07, so the average kinetic energy rises by only about 7%. The student is wrong.
- Step 3: To double , double the kelvin temperature: 2 × 293 K = 586 K, which is 586 − 273 = 313 °C.
- Step 4: Bonus: the rms speed goes as √T, so even at 586 K it rises only by a factor of √2 ≈ 1.41.
Answer: No; it rises about 7%. Doubling needs about 586 K, or 313 °C.
- Example 3Calculator allowed
Pressure from many collisions
In a simplified model, atoms of mass 6.6 × 10⁻²⁷ kg each hit a 0.010 m² wall head-on at 1200 m/s and bounce straight back. If 1.0 × 10²⁴ atoms hit the wall each second, what average pressure do they exert?
Show the solutionHide the solution
- Step 1: Momentum change of one atom: from +mv to −mv, so kg·m/s.
- Step 2: Average force = momentum delivered per second = (1.58 × 10⁻²³)(1.0 × 10²⁴) ≈ 15.8 N.
- Step 3: Pressure = F/A = 15.8 N / 0.010 m² ≈ 1.6 × 10³ Pa.
Answer: About 1.6 × 10³ Pa
Common mistakes
- Using Celsius in = or in any ratio. Always convert to kelvins first.
- Thinking heavier atoms have more kinetic energy at the same temperature. Same temperature means same average kinetic energy; heavier atoms just move slower.
- Treating as the speed of every atom. Atoms have a spread of speeds given by the Maxwell–Boltzmann distribution.
- Drawing a hotter Maxwell–Boltzmann curve taller. For the same number of atoms it gets lower and wider, keeping the same area.
On the exam
- Expect to sketch or compare Maxwell–Boltzmann curves for two temperatures, or for two gases at the same temperature, and justify the shapes.
- Factor-of-change questions are common: if T in kelvins goes up by 4, goes up by 4 and by 2.
- When explaining pressure, earn credit by naming the collisions, the momentum change at the wall, and the link between force and the rate of collisions.
Connected topics
Videos
Check yourself
4 questions on 9.1 Kinetic Theory of Temperature and Pressure. Pick an answer to see if you got it, and why.
A sample of helium gas is at 300 K. What is the average kinetic energy of a helium atom in the sample?
The absolute temperature of an ideal gas is doubled. By what factor does the root-mean-square speed of its atoms change?
A container holds a mixture of helium atoms (mass 4 u) and argon atoms (mass 40 u) in thermal equilibrium. Which statement correctly compares the two kinds of atoms?
What is the root-mean-square speed of helium atoms (mass kg each) in a gas at 300 K?
0 of 4 answered