phenomenon

gravitational interaction

The mutual attraction between celestial bodies that influences their motion and orbits.
9 related articles

Description

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.

History

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.

How it works

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.

In practice

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.

Fun fact

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.

Related articles · 9

Quantum Physics2026-08-082 minarXiv:2608.08128express
Thermal gravitons steer the force of gravity
Drop a pebble into a pond, and ripples spread across the water. In much the same way, any body, even the tiniest, perturbs the gravitational field around it. In empty, cold space, these perturbations, like ripples on a calm surface, make two nearby objects always repel each other.
General Relativity2026-07-232 minarXiv:2607.21066express
Gravitational Waves at the Horizon: Silence Instead of an Explosion
An eardrum at the very edge of a waterfall. Sound behaves strangely here: echoes don't multiply: they fade. That's exactly what gravitational waves look like at the horizon of a black hole — the boundary beyond which even light disappears.
HEP Theory2026-06-181 minarXiv:2606.20334express
Vacuum’s Memory: How Information Survives in a Black Hole
The black hole paradox has haunted physicists for decades. If a hole evaporates, where does its contents go? Discoveries by Stephen Hawking and Jacob Bekenstein showed that saving the laws of nature requires an unconventional move. Imagine the universe as a woven blanket of invisible threads.
Quantum Physics2026-05-251 minarXiv:2605.26240express
Gravity creates a quantum dance of two mirrors
Two tiny mirrors in a vacuum are like figure skaters in a pairs routine. Their oscillations are synchronized by an invisible gravitational thread. When cooled to millionths of a degree above zero, this thread turns them into a single quantum link — the motion of one instantly echoes in the other.
High Energy2026-05-222 minarXiv:2605.24281express
Twin Black Holes: Why Light Ones Are Lazy and Heavy Ones Are Tops
Two figure skaters glide on the ice. One is light and cautious, barely rotating. The other is massive and fast, spinning with all its might, and in different directions at that. That's roughly the picture painted by gravitational waves from black hole mergers.
Statistical Mech2026-05-021 minarXiv:2605.01421express
Repulsion That Pretends to Be Attraction
A handful of rice thrown into a glass of water scatters — the grains spread apart. Now imagine each grain propels itself forward with stubborn persistence and bounces off softly upon collision. Such particles are called active: they spend their own energy to move, like bacteria or microscopic robots.
Galaxies2026-04-021 minarXiv:2604.01643express
How to Get By Without Dark Matter?
Stars on the outskirts of galaxies rotate unexpectedly fast. According to Newton, the farther from the center, the slower the motion should be, like in a round dance, where the outer dancers move more slowly. But in reality, stellar outskirts race along almost as fast as the core, resembling a giant carousel: on it, the outer horses fly faster so as not to fall behind the inner ones.
Quantum Physics2026-02-222 minarXiv:2602.19306express
Gravitational Entanglement: A Quantum Dance That Ignores Mass
Picture heavy balls resting on a stretchy trampoline: each one sinks into the fabric, and their dents overlap, causing the balls to roll toward each other. This analogy helps explain how gravity — the curvature of spacetime — links massive particles. But what if you bring gravity and quantum mechanics together?
Mesoscale2026-01-251 minarXiv:2601.17727express
Magnetic Vortices Attract and Repel in Waves
Two tiny magnetic vortices, called skyrmions, drift across a thin film. As they approach each other, the force between them isn't a simple attraction or repulsion, but an alternation of the two, as if two floats on water were converging and diverging, obeying an invisible wave.