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Laws of Motion
Quick Motion Lessonshttp://www.physics247.com/motionquicklessons/index.shtmlNewton's laws of motionFrom 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)
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
This is expressed by the equation:
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
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.
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