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Friction

Friction resists motion and converts mechanical energy into heat.

Friction

Friction is the force that opposes the relative motion of solid surfaces, fluid layers, or material elements when they slide or grind against one another. Its consequences can be dramatic: rubbing pieces of wood together to start a fire is one example, and wear from friction can degrade performance or damage components. Worldwide, frictional energy losses are estimated to account for roughly 20% of total energy expenditure.

The retarding force in friction arises from many contributors, including the deformation of surface asperities, the generation of electrical charges, and changes in local material structure. When two bodies in contact move relative to each other, mechanical energy is transformed into heat, the free energy of structural changes, and other forms of dissipation. The total energy dissipated per unit distance moved equals the retarding frictional force (F = E/d). Because the interactions are so complex, calculating friction from first principles is difficult, so empirical methods are often used for analysis and theory development.

Several types of friction exist. Dry friction opposes the lateral motion of two solid surfaces in contact; it is subdivided into static friction (between non-moving surfaces) and kinetic friction (between moving surfaces). Except at the atomic or molecular scale, dry friction generally comes from the interaction of surface features called asperities. Fluid friction occurs between layers of a viscous fluid moving relative to each other. Lubricated friction is a case of fluid friction where a lubricant separates two solid surfaces. Skin friction is a component of drag that resists the motion of a fluid across a body’s surface. Internal friction resists motion between the elements of a solid material as it deforms.

The study of friction, called tribology, has a history spanning more than 2,000 years. Ancient authors such as Aristotle, Vitruvius, and Pliny the Elder explored its causes and mitigation, and Themistius noted in 350 A.D. that it is easier to keep a moving body in motion than to start one at rest. Leonardo da Vinci discovered the classic laws of sliding friction in 1493, but his notebooks remained unpublished. Guillaume Amontons rediscovered these laws in 1699, formulating them as Amonton’s three laws of dry friction, and explained friction in terms of surface irregularities and the force needed to lift the weight pressing surfaces together. Bernard Forest de Bélidor and Leonhard Euler later elaborated this view, with Euler deriving the angle of repose and distinguishing static from kinetic friction in 1750. John Theophilus Desaguliers first recognized the role of adhesion in 1734, proposing that microscopic forces cause surfaces to stick and that friction is the force needed to tear them apart. Charles-Augustin de Coulomb investigated four main factors in 1785: the nature of materials and their coatings, surface area, normal pressure, and the time surfaces remained in contact; he also considered sliding velocity, temperature, and humidity. Johann Andreas von Segner had already distinguished static from dynamic friction in 1758. Pieter van Musschenbroek explained the effect of time of repose in 1762 by noting that fibers in surfaces mesh together over time, increasing friction. John Leslie criticized the views of Amontons and Coulomb, arguing that if friction came from weight being drawn up asperities, it should be balanced by descending the opposite slope; he also doubted adhesion’s role, which he thought should equally accelerate and retard motion. Instead, Leslie saw friction as a time-dependent process of flattening and pressing down asperities, creating new obstacles.

During the development of the law of conservation of energy and the first law of thermodynamics, friction was recognized as converting mechanical work into heat. Benjamin Thompson reported on cannon boring experiments in 1798. Arthur Jules Morin developed the concept of sliding versus rolling friction in 1833. Julius Robert Mayer frictionally heated paper pulp and measured the temperature rise in 1842, and James Prescott Joule published “The Mechanical Equivalent of Heat” in 1845, specifying the amount of work needed to produce a unit of heat from friction. Osborne Reynolds derived the equation of viscous flow in 1866, completing the classic empirical model of static, kinetic, and fluid friction.

field
Physics, Engineering
known_for
Force resisting relative motion; types include dry, fluid, lubricated, skin, and internal friction
energy_impact
Frictional energy losses account for about 20% of total world energy expenditure
study_name
Tribology

Lore & Background

Friction is the force that opposes the relative motion of solid surfaces, fluid layers, or material elements sliding or grinding against each other. Its appearance is not a single physical form but rather a phenomenon observed in countless interactions, from the slow slide of a blue plate down a slope compared to a green one due to differing friction, to the heat generated by rubbing wood to start a fire. The range of friction is universal, affecting all scales of matter in contact, from simulated blocks with fractal rough surfaces exhibiting static interactions to the internal resistance within a solid material undergoing deformation. Its habitat is wherever surfaces or fluid layers meet and move relative to one another, including dry solid surfaces, viscous fluid layers, lubricated interfaces, and the skin of a body moving through a fluid. Defining characteristics include its role as a retarding force that converts mechanical energy into heat, structural changes, and other dissipative forms; the total dissipated energy per unit distance is the frictional force. Friction is not a single process but arises from many contributors, such as the deformation of surface asperities, the generation of electric charges, and changes in local structure. The complexity of these interactions makes first-principles calculation difficult, leading to reliance on empirical methods. Frictional energy losses account for roughly 20% of the world’s total energy expenditure, and the study of friction, known as tribology, has a history spanning over 2,000 years.

Reader's Guide

Friction is a fundamental force with profound implications for energy use and mechanical design. Frictional energy losses account for about 20% of the total energy expenditure of the world, highlighting its economic and environmental significance. Key empirical laws—Amontons' first law (friction proportional to load), second law (friction independent of apparent contact area), and Coulomb's law (kinetic friction independent of sliding velocity)—remain foundational in engineering. The complexity of friction, involving asperity deformation, charge generation, and structural changes, makes first-principles calculation difficult, so empirical methods are often used. Understanding friction is critical for reducing wear, improving efficiency, and designing reliable mechanical systems.

Did You Know?

A Discipline Spans Three Scales of Reality

Frictional contact mechanics is not confined to a single level of observation; it operates across a remarkable range of physical scales. At the macroscopic level, the discipline asks how entire bodies move when they touch—why a rubber ball bounces the way it does on a hard floor, for instance, with the total force against indentation and lateral displacement serving as the key quantities. Stepping down to the intermediate scale, the focus shifts to the local stresses, strains, and deformations within and around the contact zone. This is where engineers analyze tire-pavement interaction, railway wheel-rail contact, and roller bearing performance, and where they probe surface wear and damage. At the smallest end, micro- and nano-scale contact mechanics feeds into tribology—unraveling the very origin of friction—and into the design of precision instruments such as atomic force microscopes and micro-electromechanical systems. The field's core literature places the intermediate scale at its center, seeking basic insight into stresses and deformations near the contact patch while deliberately setting aside the detailed molecular mechanisms that generate those stresses.

A Lineage of Thinkers Across Four Centuries

The intellectual architecture of frictional contact mechanics was built by a long succession of scientists, engineers, and mathematicians. Leonardo da Vinci, Guillaume Amontons, John Theophilus Desaguliers, Leonhard Euler, and Charles-Augustin de Coulomb laid early groundwork in understanding friction itself. Nikolai Pavlovich Petrov, Osborne Reynolds, and Richard Stribeck later extended that foundation with lubrication theories. On the deformation side, Robert Hooke and Joseph Louis Lagrange worked in the seventeenth and eighteenth centuries, while d'Alembert and Timoshenko followed in the nineteenth and twentieth. Heinrich Hertz's classical contribution to contact mechanics stands out as a landmark, and the fundamental solutions by Boussinesq and Cerruti remain primary tools for linearly elastic frictional contact problems. The first true frictional contact solutions came from F.W. For sliding, C.

The Stick-Slip Puzzle at the Heart of the Problem

At the center of every frictional contact analysis lies a deceptively simple observation: the stresses on each body's surface are not uniform. Because stress varies from point to point across the contact, so too do strain, deformation, and the motion of individual material particles. In some regions of the contact patch, particles of the two opposing bodies adhere and move together; in other regions, they slide past one another. This local relative sliding is termed micro-slip, and the partition of the contact area into stick (adhesion) zones and slip zones has direct, observable consequences—most notably in fretting wear, where material loss occurs only in those regions where both stress and local relative displacement coexist, meaning power is actually dissipated. Complicating matters further, the size, shape, and internal division of the contact patch into adhesion and slip areas are generally unknown before the analysis is performed. The geometry of the contact itself, and how it splits into sticking and sliding sub-regions, must be discovered as part of the solution rather than assumed as a given input.

From Elegant Theory to the Demands of Computation

The mathematical treatment of frictional contact problems has evolved from closed-form analytical solutions to sophisticated numerical and semi-analytical methods. In the 1950s, growing interest in railway wheel rolling contact prompted Kenneth L. Johnson to present an approximate approach for three-dimensional frictional problems with Hertzian geometry, revealing that spin creepage—symmetric about the contact patch center—produces a net lateral force in rolling conditions due to fore-aft differences in traction distribution. In the 1970s, variational approaches rooted in Duvaut and Lion's existence and uniqueness theories matured into finite element methods for general material models and geometries, with contributions from Laursen and Wriggers, while half-space-based methods like Kalker's CONTACT model addressed smooth-edged contact for linearly elastic materials. Because well-founded variational methods demand large computation times, a parallel family of approximate rolling-contact theories emerged, including Kalker's FASTSIM, the Shen-Hedrick-Elkins formula, and Polach's approach.

Frequently Asked Questions

Who is Friction?

Friction is the fundamental force in classical mechanics that opposes the relative sliding, grinding, or shearing of solid surfaces, fluid layers, and material elements pressed against one another. It appears in several forms, including dry, fluid, lubricated, skin, and internal friction.

What are Friction's powers/role?

Friction's core role is to resist relative motion between contacting bodies and convert ordered mechanical energy into thermal heat. Its dramatic consequences range from igniting fire through rubbed wood to consuming roughly 20% of the world's total energy expenditure.

How does Friction's story end?

Because friction is a persistent physical phenomenon rather than a plot arc, its 'ending' is the irreversible dissipation of usable mechanical energy into disordered heat. No engineered system can escape this, meaning friction always extracts a portion of energy from any moving assembly.

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