Part of JTHERM-02 — Kinetic Theory of Gases

Molecular Speeds

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Three characteristic speeds describe molecular motion, each derived from the Maxwell-Boltzmann distribution:

RMS speed: vrms=v2=3kBT/m=3RT/Mv_{\text{rms}} = \sqrt{\overline{v^2}} = \sqrt{3k_BT/m} = \sqrt{3RT/M}. Appears in pressure and energy calculations. Always the largest of the three.

Average speed: vavg=8kBT/(πm)=8RT/(πM)v_{\text{avg}} = \sqrt{8k_BT/(\pi m)} = \sqrt{8RT/(\pi M)}. Used in mean free path and collision rate calculations.

Most probable speed: vmp=2kBT/m=2RT/Mv_{\text{mp}} = \sqrt{2k_BT/m} = \sqrt{2RT/M}. The peak of the Maxwell distribution curve. Always the smallest.

The universal ratio is vmp:vavg:vrms=1:1.128:1.224=2:8/π:3v_{\text{mp}} : v_{\text{avg}} : v_{\text{rms}} = 1 : 1.128 : 1.224 = \sqrt{2} : \sqrt{8/\pi} : \sqrt{3}. All three scale as T\sqrt{T} and 1/M1/\sqrt{M}: lighter and hotter gases have faster molecules.

Key applications: the speed of sound vs=γRT/Mv_s = \sqrt{\gamma RT/M} relates to vrmsv_{\text{rms}} by vs=vrmsγ/3v_s = v_{\text{rms}}\sqrt{\gamma/3}. The escape velocity comparison determines which gases an atmosphere retains — if vrms>vescape/6v_{\text{rms}} > v_{\text{escape}}/6, the gas gradually escapes (explaining why Earth retains N2_2 and O2_2 but not H2_2 or He).

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