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ideal gas lawequation

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In 1834, Émile Clapeyron combined the experimental laws of Boyle, Charles, and Gay-Lussac into the single equation pV = nRT. This elegant formula describes the equilibrium state of an ideal gas — a model where molecules are considered point-like and non-interacting. It works as a 'switch' between the volume, pressure, and temperature of a gas, allowing prediction of the behavior of real gases under ordinary conditions.

How it works

A balloon slightly expands in the sun — a demonstration of the law. In engines, a piston moves under the pressure of hot gases. Meteorologists calculate the expansion of air when heated. Breathing: the lungs change volume, and air enters due to the pressure difference.

💡 If you leave a ball in the sun, it inflates itself — not magic, but the temperature increase raises the pressure with almost constant volume.
pV = nRT
p — gas pressure (Pa), V — volume (m³), n — amount of substance (mol), R — universal gas constant (R ≈ 8.314 J/(mol·K)), T — absolute temperature (K)
U = \frac{3}{2} nRT
U — internal energy (J), n — amount of substance (mol), R — universal gas constant (R ≈ 8.314 J/(mol·K)), T — absolute temperature (K)
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Related concepts
exoplanet atmosphereinternal energyinterstellar mediumplasmatemperature
Related laws
first law of thermodynamicsBoltzmann distribution

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