Rocket equation
Δv = u · ln(m₀ / m_f) — the velocity a rocket gains by expelling propellant, derived from momentum conservation.
Definition
The rocket equation, usually called the Tsiolkovsky equation, relates the velocity change Δv a rocket can produce to its exhaust velocity u and the ratio of its initial to final mass. Because the mass ratio enters logarithmically, every increment of additional Δv costs exponentially more propellant — a relation that dominates the economics and engineering of spaceflight.
For chemical rockets, exhaust velocities are limited by the energy density of the propellant to around 4.5 km/s. Reaching low Earth orbit requires roughly 9.4 km/s of Δv, which forces a mass ratio near 8: eight kilograms of propellant per kilogram of everything else. This is why launch vehicles are mostly fuel tanks, why multi-stage rockets exist, and why electric propulsion (with u ≈ 30 km/s) is so attractive for deep-space missions despite its low thrust.
History
Derived by Konstantin Tsiolkovsky in 1903 in his paper "The Exploration of Cosmic Space by Means of Reaction Devices." Independently rederived by Robert Esnault-Pelterie (1913) and Robert Goddard (1919).