Newton thought it did, Einstein said the idea that matter reaches out into space and pulls things toward it was rediculous, and part of his theory of relativity explains gravity as the distortion or curvature of space around massive objects which change their path by bending space, like a Bowling ball on a matress bending the matress towards the bowling ball.
mass varies directly with gravitational force. Gravitational force is just another way of saying weight, which is represented by the equation, F=W=mg ; where F is force of gravity, W is weight, m is mass, and g is acceleration due to earths gravity (roughly 9.8 m/s2)
At a very deep level this is one of the great mysteries that science is presently grappling with. Is there a Higgs Boson or not? The simple answer is that mass attracts mass. Newton wrote the force equation F = m*a Force equals mass times accelleration accelleration in your question is the gravitational acelleration, at the earths surface about 9.8 m/s2 A more complex answer is that mass deforms space-time and two masses deform space-time in such a way that they approach each other.
The Sun's unique conditions cause it to exert many strange forces. Due to the rotation and immense mass of the Sun, it has a large gravitational pull. Modern science tells us that the more mass an object has, the greater its gravitaional pull. The Sun accounts for almost all the mass in our Solar System, thus keeping the planets in orbit. In addition, the enormous spinning mass of the Sun, and the fiery plasma its made of, allows the Sun to exert a spinning, oddly shaped magnetic field.
It comes about because the Sun is far more massive than any of the planets.
Gravity works both ways, when the Sun pulls on the Earth there is an equal and opposite force on the Sun. But it's so massive it hardly moves at all.
All matter, including every star, planet, galaxy, or whatever, anywhere in the universe, exerts the same force of gravity, as described by Newton's Law of Universal Gravitation.
Moons revolve around planets, not the Sun. Planets revolve around the Sun.
Gravity is not picky. The sun's gravity holds everything in the solar system in place, by definition. That includes earth.
Yes, easily, because the Sun is much bigger than all the planets combined. The Sun could also swallow up all of the dwarf planets as well.
All planets orbit the Sun.
Because it is very massive and therefore its gravity is the strongest of all objects in the solar system, reaching right out to very far out dwarf planets like Eris and Sedna.
Because it is very massive and therefore its gravity is the strongest of all objects in the solar system, reaching right out to very far out dwarf planets like Eris and Sedna.
Gravitation keeps the planets from being pulled into the Sun.
Because the planets are close enough to the sun to be affected by its gravitational field.
The Sun.
All matter, including every star, planet, galaxy, or whatever, anywhere in the universe, exerts the same force of gravity, as described by Newton's Law of Universal Gravitation.
Science observes and measures gravity, and forms theories about it, but it does not answer 'why'. Nobody knows why the force of gravity exists. That isn't a question for science, it's theology. But we know the Sun exerts a force on all the planets, and it's inverse-square, which means that the force is one quarter at twice the distance, so at Neptune it is still there but only 1/900 as strong as it is at the Earth.
Newton- he created the law of universal gravitation, which states that all objects in the universe have gravity.
The force of universal gravitation and momentum.
The elliptical orbit of planets is a result of the gravitation of the sun and the tangential velocity of the planet.
according to newton's law of gravitation every object in the nature attract other due to its gravitational pull so planets revolve around sun.
Elliptical orbits of the planets around the sun actually match what we observe. Newton's Theory of Universal Gravitation states that planets will move around the sun in elliptical orbits.