object will accelerate by an amount proportional to the force and inversely proportional to its mass. This is more commonly expressed by the formula F=ma, where F is the force acting on the object, m is its masNewtonian mechanics, which includes Newton's three laws of motion as well as the law of gravity, is an amazingly precise theory of the dynamics of material bodies. Newtonian mechanics replaced Aristotilian natural philosophy shortly after it was proposed. As expressed in Newton's manuscript Philosophae Naturalis Principia Mathematica (Mathematical Principles of Natural Philosophy), published in 1687, Newtonian mechanics remained unchallenged for over 200 years.

The starting point of Newtonian mechanics is Newton's three laws of motion. The first law, known as the law of inertia, states that an object at rest will remain at rest and that an object in motion will remain in motion at constant velocity (speed and direction) unless acted upon by an outside force. The second law states that if an outside force acts upon an object, the object will accelerate by an amount proportional to the force and inversely proportional to its mass. This is more commonly expressed by the formula F=ma, where F is the force acting on the object, m is its mass

al philosophy shortly after it was proposed. As expressed in Newton's manuscript Philosophae Naturalis Principia Mathematica (Mathematical Principles of Natural Philosophy), published in 1687, Newtonian mechanics remained unchallenged for over 200 years.

The starting point of Newtonian mechanics is Newton's three laws of motion. The first law, known as the law of inertia, states that an object at rest will remain at rest and that an object in motion will remain in motion at constant velocity (speed and direction) unless acted upon by an outside force. The second law states that if an outside force acts upon an object, the object will accelerate by an amount proportional to the force and inversely proportional to its mass. This is more commonly expressed by the formula F=ma, where F is the force acting on the object, m is its mas

remained unchallenged for over 200 years.

The starting point of Newtonian mechanics is Newton's three laws of motion. The first law, known as the law of inertia, states that an object at rest will remain at rest and that an object in motion will remain in motion at constant velocity (speed and direction) unless acted upon by an outside force. The second law states that if an outside force acts upon an object, the object will accelerate by an amount proportional to the force and inversely proportional to its mass. This is more commonly expressed by the formula F=ma, where F is the force acting on the object, m is its mas

at rest and that an object in motion will remain in motion at constant velocity (speed and direction) unless acted upon by an outside force. The second law states that if an outside force acts upon an object, the object will accelerate by an amount proportional to the force and inversely proportional to its mass. This is more commonly expressed by the formula F=ma, where F is the force acting on the object, m is its mas object will accelerate by an amount proportional to the force and inversely proportional to its mass. This is more commonly expressed by the formula F=ma, where F is the force acting on the object, m is its mass, and a is its acceleration. The third law says that for every action there is an equal and opposite reaction. This law is equivalent to the conservation of momentum. It is the principle behind rocket engines.

The remaining piece is Newton's law of universal gravitation. This law states that two point masses experience an attractive gravitational force proportional to the product of their masses and inversely proportional to the square of the distance separating them. This is expressed mathematically by the formula F = GMm/r^2, where M is the mass of the first body, m is the mass of the second body, r is the distance separating the two bodies, and G is a constant known as the universal gravitational constant. This law explains how objects fall as well as how the orbital motions of the moon and planets.