
A natural satellite is an astronomical body that orbits a planet, such as the Moon orbiting Earth.Natural satellites are celestial bodies in orbit around planets. Their orbits are shaped by the planet's gravitational pull and centrifugal force of inertia. Moons can have different origins: captured asteroids, formed together with the planet, or ejected from a giant impact (like Earth's Moon).
The first observations of planetary satellites were made by Galileo Galilei in 1610, when he discovered the four largest moons of Jupiter: Io, Europa, Ganymede, and Callisto. Around the same time, Johannes Kepler formulated laws describing the motion of planets and their satellites. Modern research includes the search for exomoons around distant stars and the study of subsurface oceans on Europa and Enceladus through missions like Europa Clipper.
A satellite is held in orbit by the planet's gravitational pull according to Newton's law of universal gravitation. The centrifugal force of inertia balances the attraction, creating an elliptical orbit according to Kepler's laws. Tidal forces, caused by the gravity gradient, slow rotation, leading to tidal locking (one side always faces the planet). The same mechanism causes tidal heating of the interior, fueling activity on Io and Enceladus.
Satellites stabilize the planet's axial tilt, influencing climate, and serve as bases for future interplanetary missions.
Some moons, such as Titan at Saturn, have a dense atmosphere and lakes of methane — the only bodies in the Solar System besides Earth with liquid basins on the surface.










