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  2. Newton's laws of motion - Wikipedia

    en.wikipedia.org/wiki/Newton's_laws_of_motion

    Newton's third law must be modified in special relativity. The third law refers to the forces between two bodies at the same moment in time, and a key feature of special relativity is that simultaneity is relative. Events that happen at the same time relative to one observer can happen at different times relative to another.

  3. Reaction (physics) - Wikipedia

    en.wikipedia.org/wiki/Reaction_(physics)

    One problem frequently observed by physics educators is that students tend to apply Newton's third law to pairs of 'equal and opposite' forces acting on the same object. [5] [6] [7] This is incorrect; the third law refers to forces on two different objects. In contrast, a book lying on a table is subject to a downward gravitational force ...

  4. Fictitious force - Wikipedia

    en.wikipedia.org/wiki/Fictitious_force

    (A d'Alembert force is not to be confused with a contact force arising from the physical interaction between two objects, which is the subject of Newton's third law – 'action is reaction'. [ 13 ] [ 14 ] In terms of the example of the passenger vehicle above, a contact force emerges when the body of the passenger touches the backrest of the ...

  5. Force - Wikipedia

    en.wikipedia.org/wiki/Force

    Newton's Third Law is a result of applying symmetry to situations where forces can be attributed to the presence of different objects. The third law means that all forces are interactions between different bodies. [18] [19] and thus that there is no such thing as a unidirectional force or a force that acts on only one body.

  6. Centrifugal force - Wikipedia

    en.wikipedia.org/wiki/Centrifugal_force

    These fictitious forces are necessary for the formulation of correct equations of motion in a rotating reference frame [15] [16] and allow Newton's laws to be used in their normal form in such a frame (with one exception: the fictitious forces do not obey Newton's third law: they have no equal and opposite counterparts). [15]

  7. Classical mechanics - Wikipedia

    en.wikipedia.org/wiki/Classical_mechanics

    So long as the force acting on a particle is known, Newton's second law is sufficient to describe the motion of a particle. Once independent relations for each force acting on a particle are available, they can be substituted into Newton's second law to obtain an ordinary differential equation, which is called the equation of motion.

  8. Motion - Wikipedia

    en.wikipedia.org/wiki/Motion

    Classical mechanics is fundamentally based on Newton's laws of motion. These laws describe the relationship between the forces acting on a body and the motion of that body. They were first compiled by Sir Isaac Newton in his work Philosophiæ Naturalis Principia Mathematica, which was first published on July 5, 1687. Newton's three laws are:

  9. Newton's law of universal gravitation - Wikipedia

    en.wikipedia.org/wiki/Newton's_law_of_universal...

    Newton's law of gravitation resembles Coulomb's law of electrical forces, which is used to calculate the magnitude of the electrical force arising between two charged bodies. Both are inverse-square laws , where force is inversely proportional to the square of the distance between the bodies.

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