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Why does energy never simply disappear? Why is momentum always conserved? Why does a spinning planet keep spinning unless something acts on it?
For centuries, these seemed like separate rules of nature. Then, in 1918, the mathematician Emmy Noether revealed that they all shared the same origin.
Her insight was astonishingly elegant. Whenever the laws of physics remain unchanged under a continuous symmetry, a conservation law follows.
> Time symmetry gives rise to the conservation of energy.
> Spatial symmetry gives rise to the conservation of momentum.
> Rotational symmetry gives rise to the conservation of angular momentum.
Suddenly, conservation laws were no longer isolated facts. They became consequences of a hidden mathematical order woven into the fabric of the universe.

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