See the below image for the Newtons law of gravitation with formula diagram. Science Concepts: • Newton’s Law of Gravita- tion states that two objects with masses m 1 and m 2 , with a distance r between their cen- ters, attract each other with a force F given by: F = Gm 1 m 2 /r 2 where G is the Universal Grav- itational Constant (equal to: 6.672 x 10 -11 Nm 2 /kg 2
Gravitational Force Formula According to Newton’s law of gravitation, the Gravitational force between two objects is directly proportional to the product of their masses. i.e. (Hz)→F ∝ M1M2 …(1) It is also inversely proportional to the square of the distance between the centre of the mass.
2 F= where F is the force of gravity, M is the mass of one object, m is the mass of a second object, r is the distance between them, and G=6.672 x 10 -11 Nm 2 /kg 2 is a constant called Newton’s Universal Gravitational Constant.
See the below image for the Newtons third law diagram. Newton’s third law. The third law states that all forces between two objects exist in equal magnitude and opposite direction: if one object A exerts a force FA on a second object B, then B simultaneously exerts a force FB on A, and the two forces are equal in magnitude and opposite in direction: FA = − FB.
Newton’s Third Law. The size of the forces on the first object equals the size of the force on the second object. The direction of the force on the first object is opposite to the direction of the force on the second object. Forces always come in pairs – equal and opposite action-reaction force pairs.
Newton’s laws of motion are three laws of classical mechanics that describe the relationship between the motion of an object and the forces acting on it. These laws can be paraphrased as follows: Law 1. A body continues in its state of rest, or in uniform motion in a straight line, unless acted upon by a force.
See the below image for the Newtons first law diagram. According to Newton’s first law of motion, a body continues to be in a state of rest or in a state of uniform motion along a straight line, unless an external force is applied on the body to change the state.” First law of motion defines inertia.
Newton’s laws first appeared in his masterpiece, Philosophiae Naturalis Principia Mathematica (1687), commonly known as the Principia. In 1543 Nicolaus Copernicus suggested that the Sun, rather than Earth, might be at the centre of the universe.
Newton’s second law is a quantitative description of the changes that a force can produce on the motion of a body. It states that the time rate of change of the momentum of a body is equal in both magnitude and direction to the force imposed on it.