Playground

Interactive Maxwell-Boltzmann speed distribution curve: adjust temperature and molecular mass to see the distribution reshape with marked most-probable, average, and RMS speeds.

Variables

SymbolNameSIDimensionRange
vvMolecular speed
Speed of an individual gas molecule
m/sL·T⁻¹0 – 2000
mmMolecular mass
Mass of a single gas molecule
kgM1e-27 – 1e-24
TTTemperature
Absolute temperature of the gas
KΘ50 – 5000
kBk_BBoltzmann constant
Relates average kinetic energy of particles to temperature
J/KM·L²·T⁻²·Θ⁻¹1.380649e-23 – 1.380649e-23

Deep dive

Derivation
Maxwell derived the speed distribution by assuming: (1) velocity components v_x, v_y, v_z are independent, (2) the distribution is isotropic, (3) the distribution depends only on speed |v|. These constraints uniquely determine a Gaussian for each component: f(v_i) ∝ exp(−mv_i²/2k_BT). Converting to spherical coordinates in velocity space introduces the 4πv² factor (density of states), giving f(v) = 4πn(m/2πk_BT)^(3/2) v² exp(−mv²/2k_BT). Key speeds: v_mp = √(2k_BT/m), ⟨v⟩ = √(8k_BT/πm), v_rms = √(3k_BT/m).
Experimental verification
Stern's molecular beam experiment (1920) and Zartman-Ko experiment (1930) directly measured molecular speed distributions by spinning slotted drums. Modern laser spectroscopy and time-of-flight mass spectrometry confirm the distribution to high precision.
Common misconceptions
  • The most probable speed, mean speed, and RMS speed are three different values — v_mp < ⟨v⟩ < v_rms
  • The distribution is not symmetric — it has a long tail toward high speeds (right-skewed) because the v² factor grows faster than the exponential decays at moderate v
  • This distribution applies only to classical ideal gases — quantum gases (fermions and bosons) follow Fermi-Dirac or Bose-Einstein distributions respectively
Real-world applications
  • Escape velocity of atmospheric gases — explains why Earth retains N₂ but loses H₂ and He
  • Reaction rate theory (Arrhenius equation) — only molecules in the high-speed tail have enough energy to react
  • Semiconductor physics — electron energy distributions in non-degenerate semiconductors
  • Gas effusion rates through small orifices (Graham's law)

Worked examples

Most probable speed of N₂ at 300 K

Given:
m:
4.65e-26
T:
300
k_B:
1.380649e-23
Find: v_mp
Solution

v_mp = √(2k_BT/m) = √(2 × 1.380649×10⁻²³ × 300 / 4.65×10⁻²⁶) = 422 m/s

RMS speed of He at 300 K

Given:
m:
6.646e-27
T:
300
k_B:
1.380649e-23
Find: v_rms
Solution

v_rms = √(3k_BT/m) = √(3 × 1.380649×10⁻²³ × 300 / 6.646×10⁻²⁷) = 1367 m/s

Scenarios

What if…
  • scenario:
    What if you double the temperature?
    answer:
    The most probable speed increases by √2 ≈ 1.41× (since v_mp ∝ √T). The distribution broadens and shifts right, with more molecules in the high-speed tail. At 600 K, N₂ molecules would have v_mp ≈ 597 m/s.
  • scenario:
    What if you compare H₂ and Xe at the same temperature?
    answer:
    H₂ (m = 3.35×10⁻²⁷ kg) moves ~8× faster than Xe (m = 2.18×10⁻²⁵ kg) because v_mp ∝ 1/√m. This is why hydrogen escapes Earth's atmosphere but xenon does not — the tail of H₂'s distribution exceeds escape velocity (11.2 km/s).
  • scenario:
    What if temperature approaches absolute zero?
    answer:
    The distribution collapses to a spike near v = 0. All molecules would be nearly stationary. In reality, quantum effects take over before T = 0 — Bose-Einstein condensation occurs for bosonic atoms, and the classical Maxwell-Boltzmann picture fails.
Limiting cases
  • condition:
    T → 0
    result:
    Distribution collapses to delta at v = 0
    explanation:
    At absolute zero all molecules would be stationary (quantum effects intervene before this).
  • condition:
    T → ∞
    result:
    Distribution flattens and shifts to high v
    explanation:
    Higher temperature spreads the distribution and increases the most probable speed.
  • condition:
    m → 0 (light particles)
    result:
    Peak shifts to very high speeds
    explanation:
    Lighter molecules (H₂, He) move much faster than heavy ones (Xe) at the same temperature.

Context

James Clerk Maxwell · 1860

Maxwell derived this distribution at age 29, founding statistical mechanics. Boltzmann later generalized it to all energy forms, creating the Boltzmann distribution.

Hook

In a room full of air, are all molecules moving at the same speed?

Find the most probable speed of nitrogen molecules (m = 4.65×10⁻²⁶ kg) at 300 K using k_B = 1.380649×10⁻²³ J/K.

Dimensions: [f(v)] = [n](([m]/[k_B][T])^(3/2))[v²]exp(−[mv²/2k_BT]) → m⁻³·(kg/(J/K·K))^(3/2)·(m/s)² = m⁻³·(s/m)³·(m²/s²) = m⁻³·s/m = s/m⁴ → probability density per unit speed per unit volume ✓
Validity: Valid for classical ideal gases in thermal equilibrium. Breaks down for quantum gases (Bose-Einstein or Fermi-Dirac statistics required at very low T or high density), relativistic speeds, and strongly interacting systems.

Related formulas