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Laws of Motion

Home Albert Einstein Sir Issac Newton

Quick Motion Lessons

http://www.physics247.com/motionquicklessons/index.shtml 

Newton's laws of motion

From Wikipedia, the free encyclopedia.

The laws of motion (laws of inertia) are the three scientific laws which Isaac Newton described; regarding the motion of bodies. These laws are fundamental to classical mechanics.

Newton first defined these laws in Philosophiae Naturalis Principia Mathematica (1687) and, using his newly developed calculus, proved many results concerning "idealised" particles. In the third volume (of the text), he showed how, combined with his Law of Universal Gravitation, the laws of motion would explain Kepler's laws of planetary motion. Newton's laws were modified, in 1916, by Einstein's theory of relativity.

 

Newton's First Law (Law of Inertia)

bulletEvery object persists in its state of rest, or uniform motion (in a straight line); unless, it is compelled to change that state, by forces impressed on it.
bulletA body remains at rest, or moves in a straight line (at a constant velocity), unless acted upon by a net outside force.

This means that a stationary object will remain stationary, and a moving object will continue to move (forever and in the same manner), unless a force acts upon it. In everyday life, the force of friction usually acts upon moving objects. Newton's law indicates that some force (gravity) must be acting upon the planets, as they do not travel in a straight line.

Newton's Second Law

bulletThe time rate of change in momentum is proportional to the applied force and takes place in the direction of the force.
bulletThe acceleration of an object is proportional to the force acting upon it.

This is expressed by the equation:

bulletF = ma
bulletF = force
bulletm = mass
bulleta = acceleration.

This equation expresses that the more force an object receives, the greater its acceleration will be. The quantity m, or mass, in the above equation is the constant of proportionality, and is a characteristic of the object. This equation, therfore, indirectly defines the concept of mass.

Taken together with Newton's Third Law of Motion, it implies the Law of Conservation of Momentum.

 

Newton's Third Law

 

bulletWhenever one body exerts force upon a second body, the second body exerts an equal and opposite force upon the first body.
bulletFor every action, there is an equal and opposite reaction.
bulletForces always come in equal pairs.

If you strike an object with a force of 200 N, then the object also strikes you (with a force of 200 N). Not only does a bullet exert force upon a target; but, the target exerts equal force upon the bullet. Not only do planets accelerate toward stars; but, stars acclerate toward planets. The reaction force has the same line of action, and is of the same type and magnitude as the original force.

 

This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Foo".