Lagrange points are positions in space where the gravitational forces of two large celestial bodies (such as the Earth and the Sun) balance with the centripetal force felt by a smaller object, allowing the object to remain in a stable or semi-stable position relative to the larger bodies.
These points were first theorized by the French mathematician and physicist Joseph-Louis Lagrange in 1772 while studying the three-body problem. His work expanded upon earlier research by Leonhard Euler and led to the identification of five special points, now known as the Lagrange points (L1–L5).