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Newtonian Physics

Newtonian physics, often referred to as classical mechanics, is the foundation of the physical sciences laid down by Sir Isaac Newton in the late 17th century. This branch of physics describes the motion of bodies under the influence of forces, focusing on the concepts of mass, momentum, force, and energy within the framework of three-dimensional Euclidean space.

Historical Context

The development of Newtonian physics began with Newton's publication of "Philosophiæ Naturalis Principia Mathematica" (Mathematical Principles of Natural Philosophy) in 1687. This work introduced Newton's three laws of motion and the law of universal gravitation, which together form the core of Newtonian mechanics:

Key Concepts

Motion and Forces

Newtonian mechanics deals with the motion of objects due to forces. Here are some key ideas:

Newton's Influence on Physics

Newton's work not only revolutionized the understanding of motion but also set the stage for many subsequent scientific discoveries. His mathematical approach to physics, combining algebra and calculus, provided a toolset for scientists to analyze complex physical phenomena. Newton's laws held up well until the advent of Einstein's theory of relativity and quantum mechanics in the 20th century, which provided explanations for phenomena outside the scope of Newtonian mechanics.

Limitations

While Newtonian physics is exceptionally accurate for macroscopic objects moving at speeds much less than the speed of light, it fails in:

Sources

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See Also

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