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All lessons Thermodynamics25 min

The Ideal Gas Law

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01
Hook
02
Explore
03
Formalize
04
Practice
05
Challenge
Interactive simulation
01

Hook

A bicycle tyre is inflated to the correct pressure on a cold winter morning (5°C). That afternoon, parked in the sun, the tyre gets hot — and blows out. Nothing leaked. You didn't pump more air in. The amount of gas is identical. So why did higher temperature destroy a perfectly good tyre? And if you measured the tyre pressure before and after heating, could you have predicted the blowout?

02

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Spoilers

The Ideal Gas Law — summary and key formula

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The question

A bicycle tyre is inflated to the correct pressure on a cold winter morning (5°C). That afternoon, parked in the sun, the tyre gets hot — and blows out. Nothing leaked. You didn't pump more air in. The amount of gas is identical. So why did higher temperature destroy a perfectly good tyre? And if you measured the tyre pressure before and after heating, could you have predicted the blowout?

A gas isn't like a solid or liquid — it responds dramatically to temperature. Heat the same gas in a fixed container and its pressure climbs relentlessly. The molecules move faster, hit the walls harder and more often, and the walls eventually can't hold. The ideal gas law ties together pressure, volume, temperature, and amount of gas in one equation — and gives you the power to predict exactly when a tyre, a pressure vessel, or an autoclave will fail.

The key idea

Three special cases of the ideal gas law hide inside it: Boyle's Law (fix T: if you halve the volume, pressure doubles — PV = constant), Charles's Law (fix P: volume is proportional to Kelvin temperature — V/T = constant), and Gay-Lussac's Law (fix V: pressure is proportional to Kelvin temperature — P/T = constant). The full law PV = nRT unifies all three. n is the amount of gas in moles, R = 8.314 J/(mol·K) is the universal gas constant — the same for every gas.

The ideal gas law works because it models a gas as point particles in constant random motion that only interact during elastic collisions. This is a simplification — real gases deviate at very high pressures or very low temperatures — but it is astonishingly accurate for most everyday conditions. Key insight: temperature must always be in Kelvin. Using Celsius would give wrong ratios, since 0°C is not 'zero energy' — absolute zero (0 K) is.

The formula

PV=nRTPV = nRTPV=nRT
  • ·P = pressure (Pa)
  • ·V = volume (m³)
  • ·n = amount of substance (mol)
  • ·R = 8.314 J/(mol·K)
  • ·T = temperature in Kelvin