A principle stating that a particular measurable property of an isolated system remains constant.A conservation law is a rule of nature stating that a particular measurable property of an isolated system remains constant as the system evolves over time. These properties — such as energy, momentum, electric charge, or angular momentum — are not created or destroyed, only transferred or transformed from one form to another. Conservation laws are among the most fundamental tools in physics, providing deep constraints on what processes are possible, regardless of the intricate details of the interactions involved.
The modern concept was crystallized in the 17th–19th centuries with Descartes' momentum, Leibniz's vis viva (early kinetic energy), and Lavoisier's mass conservation. The rigorous link to symmetry was established by Emmy Noether in 1918.
Conservation laws arise from symmetries of nature, a connection formalized by Emmy Noether's theorem (1918). For example, the conservation of energy follows from the fact that the laws of physics do not change over time; conservation of momentum follows from their invariance under spatial translations; conservation of angular momentum from rotational symmetry. In practice, these laws act as 'rules of the game' — when analyzing a system, physicists can use them to predict outcomes without solving every microscopic equation. For instance, in a collision, the total momentum before and after must match, which immediately constrains the possible final velocities.
Conservation laws underpin everything from orbital mechanics (spacecraft trajectories) to particle physics (predicting decay products) and engineering (designing efficient engines).
The conservation of electric charge is so precise that experiments have set a lower limit on the proton's lifetime at over 10^34 years — vastly longer than the age of the universe.
