The mutual attraction between celestial bodies that influences their motion and orbits.Gravitational interaction is the mutual attraction between any two objects with mass. It is the weakest of the four fundamental forces but acts over infinite range and is always attractive. This interaction governs the motion of planets around stars, stars within galaxies, and galaxies within clusters. It also shapes the large-scale structure of the universe, from the orbits of binary stars to the formation of black holes.
Isaac Newton formulated the law of universal gravitation in 1687. Albert Einstein's general relativity, published in 1915, provided a more accurate description that accounts for extreme conditions like black holes and gravitational waves.
According to general relativity, mass curves spacetime, and objects move along the straightest possible paths in this curved geometry. The more massive an object, the deeper the curvature it creates, and the stronger its gravitational pull on others. In the weak-field limit, this reduces to Newton's inverse-square law, where the force is proportional to the product of masses divided by the square of the distance between them.
Gravitational interactions are used to calculate satellite orbits, plan interplanetary missions using gravity assists, and detect exoplanets via the wobble they induce in their host stars.
Gravitational waves, ripples in spacetime caused by accelerating masses, were first directly detected in 2015 by LIGO, confirming a prediction Einstein made a century earlier.


