Planets maintain their specific distances from the Sun due to the balance between gravitational forces and their orbital velocities. The Sun's gravity pulls planets inward, while the planets' momentum keeps them moving forward in their orbits. This delicate equilibrium results in stable orbits, as described by Kepler's laws of planetary motion. Additionally, the initial conditions of the solar system's formation influenced the distances and speeds of the planets.
The force of gravity between the planets and the sun keeps them in their respective orbits, maintaining their approximate distances from each other. This gravitational force acts as a centripetal force, balancing the planets' inertia and keeping them in stable orbits around the sun.
Planets orbit the Sun in elliptical paths, as described by Kepler's First Law of Planetary Motion. While these orbits are not perfect circles, they are generally close to circular for the major planets. The gravitational pull of the Sun keeps the planets in their orbits, and the specific shape and orientation of each orbit are determined by the planet's velocity and distance from the Sun.
Newton concluded that the force of gravity between the planets and the Sun keeps them in orbit. This force is proportional to the product of their masses and inversely proportional to the square of the distance between them, as described by his law of universal gravitation.
Gravitational force is what holds all the planets in their orbits around the sun. This force is determined by the mass of the objects and the distance between them. The gravitational pull of the sun keeps the planets in their respective orbits.
The gravitational force exerted by the Sun keeps all the planets in their orbits. This force balances the planets' tendency to move in a straight line and keeps them moving in elliptical orbits around the Sun.
The force of gravity between the planets and the sun keeps them in their respective orbits, maintaining their approximate distances from each other. This gravitational force acts as a centripetal force, balancing the planets' inertia and keeping them in stable orbits around the sun.
Gravity keeps the planets together
Planets orbit the Sun in elliptical paths, as described by Kepler's First Law of Planetary Motion. While these orbits are not perfect circles, they are generally close to circular for the major planets. The gravitational pull of the Sun keeps the planets in their orbits, and the specific shape and orientation of each orbit are determined by the planet's velocity and distance from the Sun.
The force that keeps all of our planets in rotation is gravity.
The gravity of there star keeps them on path and a planets moon is sun around by its planets gravitational force
The Sun has a powerful gravitational pull. This, combined with the velocities of the planets, keeps the planets in orbit.
The Sun's Gravitational pull keeps the planets orbiting it, not flying into deep space.
Gravity and motion. Gravity pulls the planets in and keeps them from flying away, while the velocity of the planets keeps them from being sucked in completely.
Actually, it's the gravity of the sun that keeps the planets in orbit around it. The force of gravity between the sun and the planets causes them to be pulled towards the sun, while their momentum keeps them moving in a circular or elliptical path.
Newton concluded that the force of gravity between the planets and the Sun keeps them in orbit. This force is proportional to the product of their masses and inversely proportional to the square of the distance between them, as described by his law of universal gravitation.
by the circulating belt it keeps the escalator rotating
Gravitational force is what holds all the planets in their orbits around the sun. This force is determined by the mass of the objects and the distance between them. The gravitational pull of the sun keeps the planets in their respective orbits.