The "figure" is the gravitational constant.
The force of gravity is the same everywhere in the universe. What do you mean exactly? You can calculate the force of gravity between any two objects with the following formular Mass times (multiplied by) Mass divided by distance squared.
It will be larger between the large objects. This force is equal to the universal gravitational constant times the two masses of the objects, all divided by the square of the distance apart the objects are.
The gravity never goes to exactly zero. Off in the most distant galaxy we can see, the gravitational force of the Moon (or the Earth, or for that matter you) is not zero. It's immeasurably small, but it's not zero. However, there is a point directly between the Earth and the Moon where the gravity of the two exactly balance each other. At less than this distance from the Moon, the net force is towards the Moon; at more than this distance, the net force is towards the Earth. It is located where the mass of the Earth divided by the distance to Earth squared is equal to the mass of the Moon divided by the distance to the Moon squared. The exact distance of this point from the center of the Moon varies since the distance between the Earth and the Moon is not constant, but it's roughly 10% of the center-to-center distance between the Earth and the Moon.
Nothing happens to gravity. It always works according to the same exact formula,regardless of how far apart or close together the objects are.According to that formula, we can see that when the objects are closer together,the gravitational force between them becomes greater.
Orbital motion in general depends on the mass of the two objects interacting, and the distance between them. Mathematically, the force of gravitational attraction between two masses is proportional to the product of the two masses, divided by the square of the distance between them, times the gravitational constant (G = 6.67428 x10-11 (m/kg)2): F = G (m1m2/r2) "Force equals gravitational constant times the quantity of mass 1 times mass 2 divided by radius squared". The speed of a planet moving in its orbit is basically a case of circular motion. Planetary orbits are not perfectly circular, but if they were, uniform circular motion and its speed is described mathematically: V = r (Δθ/Δt) or V = rω Where V is velocity (speed and direction), r is radius (in meters), θ (Greek theta) is the angle swept by the arc, and t is time (in seconds). For the second formula, ω (Greek omega) is angular rate of rotation. Δ (Greek delta) basically means "change". So you can read the first formula as "velocity equals radius times the quantity of change in angle divided by change in time". In actual astronomy, since the orbits are not perfect circles, the math is somewhat more complicated. But this is the essence.
The gravitational force between two 1 kg bodies that are 1 meter apart is approximately 6.67 x 10^-11 Newtons, which is the universal gravitational constant multiplied by the product of the masses divided by the square of the distance between them.
Time = (distance) divided by (speed) Distance = (speed) multiplied by (time) Speed = (distance) divided by (time)
Doubling the distance between two objects decreases the gravitational force between them by a factor of four. This is because gravitational force decreases with the square of the distance according to the inverse square law.
The gravitational and electric fields share similarities in that they are vector fields and both transmit forces between objects, Gravitational force is equal to the product of two MASSES divided by the distance between them squared. Electric force is equal to the product of two CHARGES divided by the distance between them squared.
Speed / (Divided by) Distance X (multiplied by) Time
Gravitational Energy is E = -GmM/r where G is gravitational Constant, m and M are two masses and r is the distance separating the masses. The description is embedded in the mathematical relationship; the product of two masses divided by the distance r between them scaled by the gravitational constant G.
The force of gravity is the same everywhere in the universe. What do you mean exactly? You can calculate the force of gravity between any two objects with the following formular Mass times (multiplied by) Mass divided by distance squared.
Yes it's the law of gravity which describes the interaction between the planet and the Sun. The force is calculated from the masses of the Sun and the planet multiplied together and divided by the square of the distance, then multiplied by the universal gravitational constant. The force is proportional to the inverse-square of the distance (doubling the distance makes the force one quarter as strong), and Isaac Newton showed that a force obeying that law gives orbits that conform to Kepler's laws of planetary motion which was previously deduced from observations.
It will be larger between the large objects. This force is equal to the universal gravitational constant times the two masses of the objects, all divided by the square of the distance apart the objects are.
If the gravitational force decreases according to the square of the distance, then if the distance is doubled the force becomes one forth of what it was. So if you doubled the the distance between the two objects then they would have a gravitational force of 125 Newtons. That happens because 2 squared is 4 and 500 divided by 4 is 125.
The gravitational attraction between two objects depends on both their masses and the distance between them. It is proportional to the product of the masses of the two objects divided by the distance between them (mass1 x mass2)/ distance between.
The equation for the force between two objects is given by Newton's law of universal gravitation: F = G * (m1 * m2) / r^2, where F is the force, G is the gravitational constant, m1 and m2 are the masses of the objects, and r is the distance between the centers of the objects.