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Law of atmospheres

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Density falls exponentially with height.

Key relationn = n₀e^{−mgh/kT}

In a uniform-temperature atmosphere density falls as n = n₀e^{−mgh/kT}, scale height kT/mg ≈ 8.5 km for air.

Worked example

At 8.5 km air density is about 37% of sea level.

Common mistake

Real atmosphere has temperature variation.

In more detail

The law of atmospheres describes how air pressure falls exponentially with altitude, P = P0 exp(−mgh/kT). Heavier gases fall off more quickly with height.

Real-world uses

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Frequently asked questions

Why does pressure fall exponentially?

Because the weight of each layer of air supports the layers above, and density depends on pressure.

Why is hydrogen rare in the atmosphere?

Light molecules escape to space because they are fast enough at high altitude.

Why does air thin out with height?

Gravity pulls the molecules downward, and the thermal motion spreads them out, so the density falls exponentially.

Related topics in Kinetic Theory & Statistical Physics

Maxwell–Boltzmann distribution · Most probable speed · Average, rms and most probable speeds · Diffusion · Fick's law · Graham's law of effusion

← All Kinetic Theory & Statistical Physics topics