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Newton's three physical laws of Motion.
Newton's Laws of Motion are three physical laws which provide relationships between the forces acting on a body and the motion of the body. Newton's Laws of Motion were first formulated by Sir Isaac Newton. Newton's Laws of Motion were first published in his work Philosophiae Naturalis Principia Mathematica (1687). Newton's Laws of Motion form the basis for classical mechanics. Newton used Laws of Motion to explain many results concerning the motion of physical objects. In the third volume of the text, he showed that the laws of motion, combined with his law of universal gravitation, explained Kepler's laws of planetary motion.
The three Laws of Motion.
Newton's Laws of Motion describe only the motion of a body as a whole and are valid only for motions relative to a reference frame. The following are brief modern formulations of Newton's three laws of motion:
It is important to note that these three laws together with his law of gravitation provide a satisfactory basis for the explanation of motion of everyday macroscopic objects under everyday conditions. However, when applied to extremely high speeds or extremely small objects, Newton's laws break down; this was remedied by Albert Einstein's Special theory of Relativity for high speeds and by quantum mechanics for small objects.
Newton's first law: law of inertia.
This law is also called the law of inertia or Galileo's principle.
The net force on an object is the vector sum of all the forces acting on the object. Newton's first law says that if this sum is zero, the state of motion of the object does not change. Essentially, it makes the following two points:
The first point seems relatively obvious to most people, but the second may take some thinking through, because we have no experience in every-day life of things that keep moving forever (except celestial bodies). If one slides a hockey puck along a table, it doesn't move forever, it slows and eventually comes to a stop. But according to Newton's laws, this is because a force is acting on the hockey puck and, sure enough, there is frictional force between the table and the puck, and that frictional force is in the direction opposite the movement. It is this force which causes the object to slow to a stop. In the absence of such a force, as approximated by an air hockey table or ice rink, the puck's motion would not slow.
Although the 'Law of Inertia' is commonly attributed to Galileo, Aristotle wrote the first known description of it:
However, a key difference between Galileo's idea from Aristotle's is that Galileo realized that force acting on a body determines acceleration, not velocity. This insight leads to Newton's First Law - no force means no acceleration, and hence the body will continue to maintain its velocity.
The Law of Inertia apparently occurred to many different natural philosophers independently. Inertia of motion was described in the third century BCE in the Mo Tzu, a collection of Chinese philosphical texts, and the 17th century philosopher René Descartes also formulated the law, although he did not perform any experiments to confirm it.
There are no perfect demonstrations of the law, as friction usually causes a force to act on a moving body, and even in Outer space gravitational forces act and cannot be shielded against, but the law serves to emphasize the elementary causes of changes in an object's state of motion: forces.
Newton's second law: historical development.
In an exact original 1792 translation (from Latin) Newton's Second Law of Motion reads:
Newton here is basically saying that the rate of change in the momentum of an object is directly proportional to the amount of force exerted upon the object. He also states that the change in direction of momentum is determined by the angle from which the force is applied.
However, it must be remembered that for Newton, mass was constant and independent of velocity. To take "motion" (motu) as meaning momentum gives a false impression of what Newton believed. Since he took mass as constant (part of the constant of proportionality) it can, in modern notation, be taken to the left of the derivative as mdv / dt. If m is dependent on velocity (or on time) as we would now hold, then m has to be included in the derivative, giving d(mv) / dt- or dp / dt.
Using momentum in the terminology (which would never have occurred to Newton) is a latter-day revision of the law to bring it into correspondence with special relativity.
Interestingly, Newton is restating in his further explanation another prior idea of Galileo, what we call today the Galilean transformation or the addition of velocities.
An interesting fact when studying Newton's Laws of Motion from the Principia is that Newton himself does not explicitly write formulae for his laws which was common in scientific writings of that time period. In fact, it is today commonly added when stating Newton's second law that Newton has said, "and inversely proportional to the mass of the object." This however is not found in Newton's second law as directly translated above. In fact, the idea of mass is not introduced until the third law.
In mathematical terms, the differential equation can be written as:
where F is force, m is mass, v is velocity, t is time and k is the constant of proportionality. The product of the mass and velocity is the momentum of the object.
If mass of an object in question is known to be constant and using the definition of acceleration, this differential equation can be rewritten as:
where a is the acceleration.
Using only SI Units for the definition of Newton, the constant of proportionality is unity (1). Hence:
However, it has been a common convention to describe Newton's second law in the mathematical formula F = ma where F is Force, a is acceleration and m is mass. This is actually a combination of laws two and three of Newton expressed in a very useful form. This formula in this form did not even begin to be used until the 18th century, after Newton's death, but it is implicit in his laws.
Newton's Third Law of Motion states:
The explanation of mass is expressed here for the first time in the words "reciprocally proportional to the bodies" which have now been traditionally added to Law 2 as "inversely proportional to the mass of the object." This is because Newton in his definition 1 had already stated that when he said "body" he meant "mass". Thus we arrive at F = ma. When the formula F = ma is taken into account, Law II can be also interpreted as a quantitative restatement of Law I, where mass also acts as a measurement of inertia.
Newton's third law: law of reciprocal actions.
Lex III: Actioni contrariam semper et æqualem esse reactionem: sive corporum duorum actiones in se mutuo semper esse æquales et in partes contrarias dirigi.
Newton's third law of motion follows mathematically from the law of conservation of momentum.
As shown in the diagram opposite, the skaters' forces on each other are equal in magnitude, and opposite in direction. Although the forces are equal, the accelerations are not: the less massive skater will have a greater acceleration due to Newton's second law.
If a basketball hits the ground, the basketball's force on the Earth is the same as Earth's force on the basketball. However, due to the ball's much smaller mass, Newton's second law predicts that its acceleration will be much greater than that of the Earth. Not only do Planets accelerate toward stars, but stars also accelerate toward planets.
The two forces in Newton's third law are of the same type, e.g., if the road exerts a forward frictional force on an accelerating car's tires, then it is also a frictional force that Newton's third law predicts for the tires pushing backward on the road.
Importance and range of validity of Newton's laws of motion.
Newton's laws were verified by experiment and observation for over 200 years, and they are excellent approximations at the scales and speeds of everyday life. Newton's laws of motion, together with his law of universal gravitation and the mathematical techniques of calculus, provided for the first time a unified quantitative explanation for a wide range of physical phenomena.
In quantum mechanics concepts such as force, momentum, and position are defined by linear operators that operate on the quantum state; at speeds that are much lower than the speed of light, Newton's laws are just as exact for these operators as they are for classical objects. At speeds comparable to the speed of light, the second law holds in the original form F = dp / dt, which says that the force is the derivative of the momentum of the object with respect to time, but some of the newer versions of the second law (such as the constant mass approximation above) do not hold at relativistic velocities.
Relationship to the conservation laws of motion.
The laws of conservation of momentum, energy, and angular momentum are of more general validity than Newton's laws, since they apply to both light and matter, and to both classical and non-classical physics.
Because force is the time derivative of momentum, the concept of force is redundant and subordinate to the conservation of momentum, and is not used in fundamental theories (e.g. quantum mechanics, quantum electrodynamics, general relativity, etc.). The standard model explains in detail how the three fundamental forces known as gauge forces originate out of exchange by virtual particles. Other forces such as gravity and fermionic degeneracy pressure arise from conditions in the equations of motion in the underlying theories.
Newton stated the third law within a world-view that assumed instantaneous action at a distance between material particles. However, he was prepared for philosophical criticism of this action at a distance, and it was in this context that he stated the famous phrase "I frame no hypotheses". In modern physics, action at a distance has been completely eliminated. For example, the electrons in the antenna of a radio transmitter do not necessarily act directly on the electrons in the receiver's antenna. According to an everyday timelike observer, momentum is handed off from the transmitter's electrons to the radio wave, and then to the receiver's electrons, and the whole process takes time. If the radio wave itself were to carry a stopwatch and a meterstick and find how long it takes for the momentum to be transferred and whether there is space between the two electrons, then from that perspective the transmitting electron acts directly and instantly on the receiving electron. Conservation of momentum is satisfied at all times and Newton's laws are applicable: for example, the second law does apply to the radio wave (see radiation pressure, radiation reaction force, etc.). Its applicability is guaranteed by accounting for radiowave momentum (see momentum of electromagnetic wave).
Conservation of energy was discovered nearly two centuries after Newton's lifetime, the long delay occurring because of the difficulty in understanding the role of microscopic and invisible forms of energy such as heat and infra-red light.
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