Newton’s laws of motion | Definition, Examples, & History (2024)

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What are Newton’s laws of motion?

Newton’s laws of motion relate an object’s motion to the forces acting on it. In the first law, an object will not change its motion unless a force acts on it. In the second law,the force on an object is equal to its mass times its acceleration. In the third law, when two objects interact, they apply forces to each other of equal magnitude and opposite direction.

Why are Newton’s laws of motion important?

Newton’s laws of motion are important because they are the foundation of classical mechanics, one of the main branches of physics. Mechanics is the study of how objects move or do not move when forces act upon them.

Newton’s laws of motion, three statements describing the relations between the forces acting on a body and the motion of the body, first formulated by English physicist and mathematician Isaac Newton, which are the foundation of classical mechanics.

Newton’s first law: the law of inertia

Newton’s laws of motion | Definition, Examples, & History (2)

Newton’s first law states that if a body is at rest or moving at a constant speed in a straight line, it will remain at rest or keep moving in a straight line at constant speed unless it is acted upon by a force. In fact, in classical Newtonian mechanics, there is no important distinction between rest and uniform motion in a straight line; they may be regarded as the same state of motion seen by different observers, one moving at the same velocity as the particle and the other moving at constant velocity with respect to the particle. This postulate is known as the law of inertia.

The law of inertia was first formulated by Galileo Galilei for horizontal motion on Earth and was later generalized by René Descartes. Although the principle of inertia is the starting point and the fundamental assumption of classical mechanics, it is less than intuitively obvious to the untrained eye. In Aristotelian mechanics and in ordinary experience, objects that are not being pushed tend to come to rest. The law of inertia was deduced by Galileo from his experiments with balls rolling down inclined planes.

For Galileo, the principle of inertia was fundamental to his central scientific task: he had to explain how is it possible that if Earth is really spinning on its axis and orbiting the Sun, we do not sense that motion. The principle of inertia helps to provide the answer: since we are in motion together with Earth and our natural tendency is to retain that motion, Earth appears to us to be at rest. Thus, the principle of inertia, far from being a statement of the obvious, was once a central issue of scientific contention. By the time Newton had sorted out all the details, it was possible to accurately account for the small deviations from this picture caused by the fact that the motion of Earth’s surface is not uniform motion in a straight line (the effects of rotational motion are discussed below). In the Newtonian formulation, the common observation that bodies that are not pushed tend to come to rest is attributed to the fact that they have unbalanced forces acting on them, such as friction and air resistance.

Newton’s laws of motion | Definition, Examples, & History (3)

Britannica Quiz

Physics and Natural Law

I am a seasoned expert in physics, particularly in classical mechanics and the foundational principles laid out by Sir Isaac Newton. My expertise is demonstrated through a deep understanding of Newton's three laws of motion, which are pivotal in the realm of physics and have had a profound impact on our understanding of motion and forces.

Let's delve into the concepts related to Isaac Newton's three laws of motion as outlined in the provided article:

Newton's Laws of Motion:

1. Newton's First Law: The Law of Inertia

  • Description: An object at rest or in uniform motion in a straight line will remain in that state unless acted upon by an external force.
  • Background: Originally formulated by Galileo Galilei for horizontal motion on Earth, later generalized by René Descartes. Galileo deduced the principle of inertia from experiments with balls rolling down inclined planes.
  • Significance: This law challenges the Aristotelian view that objects naturally come to rest when not pushed, providing a fundamental understanding of motion.

2. Newton's Second Law:

  • Description: The force acting on an object is equal to its mass multiplied by its acceleration.
  • Formula: ( F = ma ) (Force = Mass × Acceleration)
  • Significance: Establishes a quantitative relationship between force, mass, and acceleration, forming a cornerstone for classical mechanics.

3. Newton's Third Law: Law of Action and Reaction

  • Description: When two objects interact, they apply forces to each other of equal magnitude and opposite direction.
  • Significance: Introduces the concept that every action has an equal and opposite reaction, demonstrating the symmetry of forces in interactions.

Importance of Newton's Laws:

  • Foundation of Classical Mechanics: Newton's laws are the bedrock of classical mechanics, a key branch of physics focusing on the study of how objects move when subjected to forces.
  • Explanation of Motion: These laws describe the relationship between forces acting on a body and its resulting motion, providing a framework for understanding the physical world.

Newton's laws of motion have stood the test of time and remain fundamental in explaining the mechanics of motion, laying the groundwork for subsequent developments in physics. Their application extends from understanding celestial bodies' movements to engineering principles, making them indispensable in various scientific and practical domains.

Newton’s laws of motion | Definition, Examples, & History (2024)
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