
Sir Isaac Newton, born in 1642 or 1643, was an influential mathematician, physicist, and philosopher. He developed his three laws of motion in 1666, at the age of 23, and presented them in his seminal work Philosophiæ Naturalis Principia Mathematica in 1687. Newton's first law of motion, also known as the law of inertia, states that an object at rest will remain at rest, and an object in motion will continue moving at a constant speed in a straight line unless acted upon by an external force. This law was influenced by the work of predecessors like Galileo, who recognized the tendency of objects to resist changes in their state of motion. Newton's laws of motion have been fundamental in the development of classical mechanics and have been widely applied and verified over the past 300 years.
| Characteristics | Values |
|---|---|
| Date of discovery | 1666 |
| Age at discovery | 23 years old |
| Publication of laws | 1687 |
| Publication title | "Philosophiæ Naturalis Principia Mathematica" |
| Other names | "Mathematical Principles of Natural Philosophy", "Principia Mathematica" |
| Basis of laws | Math, physics, optics, astronomy, previous scientists' theories |
| Number of laws | 3 |
| First law | "A body at rest will remain at rest, and a body in motion will remain in motion unless it is acted upon by an external force." |
| Second law | "The force acting on an object is equal to the mass of that object times its acceleration." |
| Third law | "For every action, there is an equal and opposite reaction." |
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What You'll Learn
- Newton's first law is sometimes referred to as the Law of Inertia
- Newton's laws form the basis of the first branch of physics, known as classical mechanics
- Newton's laws are often stated in terms of point or particle masses
- Newton's laws of motion were influenced by the work of Galileo Galilei and René Descartes
- Newton's laws of motion relate an object’s motion to the forces acting on it

Newton's first law is sometimes referred to as the Law of Inertia
Sir Isaac Newton, born in 1643, was one of the most influential scientists of all time. He developed his theories of gravitation in 1666 when he was just 23 years old. Newton's first law of motion, often referred to as the Law of Inertia, states that an object at rest will remain at rest, and an object in motion will continue moving with a constant speed and in a straight line unless it is acted upon by an external force. This means that an object will not change its velocity unless a force acts upon it, and if all external forces cancel each other out, there is no net force acting on the object.
The concept of inertia was first formulated by Galileo Galilei for horizontal motion on Earth. Galileo concluded that the "natural" behaviour of a moving body was to keep moving until something else interfered with it. However, he thought that a body moving a long distance inertially would follow the curve of the Earth. This idea was later corrected by Isaac Beeckman, Descartes, and Pierre Gassendi, who recognised that inertial motion should be in a straight line. Newton built upon these ideas and formulated his three laws of motion, which were first stated in his "Philosophiæ Naturalis Principia Mathematica" (Mathematical Principles of Natural Philosophy) in 1687.
Newton's laws refer to the motion of objects in an inertial reference frame, where an object remains at rest or moves with a constant velocity unless acted upon by an external force. By developing these laws, Newton simplified objects by reducing them to mathematical points without considering factors such as friction, air resistance, or material properties. Instead, he focused on outcomes that could be illustrated wholly with reference to mass, length, and time.
Newton's laws of motion form the basis of classical mechanics, the study of the motion of massive objects, and are widely used even today. They have important applications in various scientific fields, including astronomy, chemistry, geology, and engineering.
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Newton's laws form the basis of the first branch of physics, known as classical mechanics
Newton's three laws of motion, first stated in 1687, form the basis of classical mechanics, the first branch of physics. Classical mechanics is the study of the motion of massive objects and is the foundation for other branches of physics. It also has important applications in astronomy, chemistry, geology, and engineering. Newton's laws refer to the motion of objects in an inertial reference frame, which can be described as a system in which an object remains at rest or moves with constant linear motion unless acted upon by an external force.
Newton's first law of motion, also known as the law of inertia, states that an object at rest will remain at rest, and an object in motion will continue moving with the same speed and in a straight line unless acted upon by an external force. This law was first formulated by Galileo Galilei for horizontal motion on Earth and was later generalized by René Descartes and others.
Newton's second law of motion defines force as equal to the change in momentum (mass times velocity) per change in time. It also states that the net force on a body is equal to the body's acceleration multiplied by its mass.
Newton's third law of motion, the law of action and reaction, states that for every action (force) in nature, there is an equal and opposite reaction. For example, when an object is pushed in one direction, there is always an equal resistance from the opposite direction.
Newton's laws of motion were developed by expanding upon the ideas of previous scientists like Galileo, Aristotle, and Descartes. Newton combined knowledge of celestial motions with the study of events on Earth, showing that one theory of mechanics could encompass both. His work revolutionized science and provided a foundation for classical mechanics, which has been further developed and extended by later scientists.
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Newton's laws are often stated in terms of point or particle masses
The story of an apple falling on Sir Isaac Newton's head is a famous legend, but there is no evidence to support it. Documents indicate that he saw an apple fall, which may have given him the idea of figuring out gravity. Newton's laws of motion were developed after many years of studying math, physics, optics, and astronomy.
Newton's first law of motion states that an object at rest remains at rest, and an object in motion remains in motion at a constant speed and in a straight line unless acted on by an unbalanced force. This is often referred to as the \"law of inertia." Newton's second law defines a force to be equal to the change in momentum (mass times velocity) per change in time. The third law states that for every action (force) in nature, there is an equal and opposite reaction.
Newton's laws of motion are often stated in terms of point or particle masses, meaning bodies with negligible volume. This is a reasonable approximation for real bodies when the motion of internal parts can be neglected, and when the separation between bodies is much larger than their size. This simplification allowed Newton to ignore factors such as friction, air resistance, temperature, and material properties, focusing solely on outcomes related to mass, length, and time.
Newton's laws of motion form the basis of classical mechanics, a branch of physics that studies the motion of massive objects. Classical mechanics also has applications in other areas of science, including astronomy, chemistry, geology, and engineering. Newton's work built upon the ideas of previous scientists like Galileo, Aristotle, and Descartes, and his laws were first presented in his seminal work \"Principia Mathematica Philosophiae Naturalis\" in 1687.
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Newton's laws of motion were influenced by the work of Galileo Galilei and René Descartes
The three laws of motion were first stated by Isaac Newton in his Philosophiæ Naturalis Principia Mathematica, originally published in 1687. Newton's laws refer to the motion of objects in an inertial reference frame. Newton's work expanded on the ideas of previous scientists like Galileo Galilei and René Descartes, turning theories into practice.
Galileo Galilei, a contemporary of Newton's, was one of the most influential scientists of his time. He is credited with formulating the law of inertia, which states that a body at rest will remain at rest, and a body in motion will continue moving at a steady speed in a straight line unless acted upon by an external force. This was a fundamental assumption of classical mechanics and a key influence on Newton's work. Galileo's experiments with balls rolling down inclined planes helped him deduce this principle. He also recognized that the Earth's gravity affects vertical but not horizontal motion, and his work on projectiles influenced Newton's second law.
René Descartes introduced the concept of inertia in his "laws of nature" in "The World" (written 1629-1633 but not published until 1664). Descartes' first law of nature states that a body, when left to itself, continues in the same state, and his second law states that a body, when left to itself, moves in a straight line. These laws influenced Newton, but he ultimately rejected Descartes' aetherial explanations of force.
Newton's laws of motion were influenced by the work of Galileo and Descartes, but he also built upon the ideas of other scientists such as Aristotle, Johannes Kepler, Nicolaus Copernicus, and Christiaan Huygens. Newton's unique approach to natural philosophy involved beginning with a mathematical construct and building on it, comparing it to the real world to show that his system accurately accounted for it.
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Newton's laws of motion relate an object’s motion to the forces acting on it
Newton's laws of motion explain the relationship between a physical object and the forces acting upon it. Newton's three laws of motion were first stated in his Philosophiæ Naturalis Principia Mathematica, originally published in 1687. However, he developed the theories of gravitation in 1666 when he was just 23 years old.
The first law of motion, often referred to as the ""law of inertia", states that an object at rest will remain at rest, and an object in motion will continue moving at a constant speed and in a straight line unless it is acted upon by an external force. In other words, an object will not change its motion unless a force acts on it.
The second law of motion defines force as equal to change in momentum (mass times velocity) per change in time. Therefore, the force on an object is equal to its mass times its acceleration. Objects will move faster and farther when pushed harder, and heavier objects require more force to move the same distance as lighter objects.
The third law of motion states that for every action (force) in nature, there is an equal and opposite reaction. If object A exerts a force on object B, object B will exert an equal and opposite force on object A. In other words, forces are the result of interactions.
Newton's laws of motion are important because they are the foundation of classical mechanics, which is one of the main branches of physics. Classical mechanics also has important applications in other areas of science, including astronomy, chemistry, geology, and engineering.
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Frequently asked questions
An object at rest remains at rest, and an object in motion remains in motion at a constant speed and in a straight line unless acted on by an unbalanced force. This is often referred to as the "law of inertia".
Newton studied natural philosophy at Trinity College, Cambridge, and later became a professor at Cambridge. He developed the theories of gravitation in 1666 when he was 23 years old. In 1687, he published his "Philosophiæ Naturalis Principia Mathematica" (Mathematical Principles of Natural Philosophy), which became the foundation of classical mechanics.
The first law of motion states that every object will remain at rest or in uniform motion in a straight line unless compelled to change by the action of an external force. This tendency to resist changes in the state of motion is called inertia.











































