In 1644, the French philosopher René Descartes proposed that the total quantity of motion in the universe was conserved. He was wrong about the precise quantity (he conserved |mv|, ignoring direction), but the structural intuition — that something gets handed around between bodies during a collision and the total stays the same — was correct. Christiaan Huygens corrected Descartes in the 1650s by treating velocity as a vector, and Newton built the corrected version into the third law of his 1687 Principia. Conservation of momentum — that the total linear momentum of an isolated system never changes, no matter how its parts collide, explode, or interact — is one of the most empirically robust statements in physics, and it has survived every theoretical revolution since Newton.
Momentum is mass times velocity: 𝐩 = m·𝐯, a vector quantity. For a system of multiple bodies, the total momentum is the vector sum of individual momenta. Conservation of momentum: in the absence of external forces, the total momentum of a closed system is constant. The conservation follows directly from Newton's third law: if body A exerts force 𝐅 on body B, then B exerts −𝐅 on A; integrating over time, the impulses cancel and the total momentum is unchanged. Elastic collisions preserve both kinetic energy and momentum; inelastic collisions preserve only momentum (the lost energy goes to heat or deformation). Rocket propulsion (the rocket gains forward momentum exactly equal in magnitude to the rearward momentum of the exhaust), recoil from firing a bullet, the frictionless puck on an air table — all are immediate consequences. Generalizing: Noether's theorem (1918) shows that momentum conservation arises from the spatial-translation symmetry of the laws of physics — they don't change if you move your experiment to a different place. Special relativity modifies the formula: relativistic momentum is 𝐩 = γm𝐯, where γ = 1/√(1 − v²/c²); the conservation law is preserved, but the formula adjusts. Quantum mechanics makes momentum an operator whose eigenvalues are the possible measurement outcomes, with the de Broglie relation p = h/λ tying particle momentum to wavelength. The conservation survives intact: in every interaction at every scale ever measured, the total momentum balances. The principle is so reliable that missing momentum in a particle-physics experiment is one of the most powerful diagnostics for detecting otherwise-invisible particles — neutrinos were first inferred this way in beta decay (Pauli, 1930), and dark-matter searches at colliders look for the same signature today.
Spacecraft propulsion, automotive collision design, ballistics, recoilless rifles, turbine engineering, particle accelerators all use momentum conservation as a basic engineering primitive. Particle physics relies on it as a constraint when reconstructing collision events at the LHC: invisible particles reveal themselves as missing momentum in the detector. Atmospheric and oceanic dynamics (winds, currents, jet streams) are momentum-conservation problems at planetary scale. Newton's cradle, the executive desk-toy, is essentially a teaching apparatus for elastic collisions that has been rediscovered for two centuries because the principle never gets old.