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| Meta Title | Hydrostatics | Fluid Pressure, Buoyancy & Equilibrium | Britannica |
| Meta Description | Hydrostatics, Branch of physics that deals with the characteristics of fluids at rest, particularly with the pressure in a fluid or exerted by a fluid (gas or liquid) on an immersed body. In applications, the principles of hydrostatics are used for problems relating to pressure in deep water |
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| Boilerpipe Text | Top Questions
What is fluid mechanics?
What is a fluid in science?
What are some important properties of fluids?
How is pressure created and measured in fluids?
What is buoyancy, and how does it affect objects in water?
How is fluid mechanics used in real-life situations like airplanes and weather?
fluid mechanics
,
science
concerned with the
response of fluids
to forces exerted upon them. It is a branch of classical
physics
with applications of great importance in hydraulic and
aeronautical engineering
,
chemical engineering
,
meteorology
, and zoology.
The most familiar fluid is of course
water
, and an encyclopaedia of the 19th century probably would have dealt with the subject under the separate headings of
hydrostatics
, the science of water at rest, and hydrodynamics, the science of water in
motion
.
Archimedes
founded hydrostatics in about 250
bc
when, according to
legend
, he leapt out of his bath and ran naked through the streets of Syracuse crying āEureka!ā; it has undergone rather little development since. The foundations of hydrodynamics, on the other hand, were not laid until the 18th century when mathematicians such as
Leonhard Euler
and
Daniel Bernoulli
began to explore the consequences, for a virtually continuous medium like water, of the
dynamic
principles that Newton had enunciated for systems composed of discrete particles. Their work was continued in the 19th century by several mathematicians and physicists of the first rank, notably G.G. Stokes and William Thomson. By the end of the century explanations had been found for a host of intriguing phenomena having to do with the flow of water through tubes and orifices, the waves that ships moving through water leave behind them, raindrops on windowpanes, and the like. There was still no proper understanding, however, of problems as fundamental as that of water flowing past a fixed obstacle and exerting a
drag force
upon it; the theory of potential flow, which worked so well in other
contexts
, yielded results that at relatively high flow rates were grossly at variance with experiment. This problem was not properly understood until 1904, when the German physicist
Ludwig Prandtl
introduced the concept of the
boundary layer
(see below
Hydrodynamics: Boundary layers and separation
). Prandtlās career continued into the period in which the first manned aircraft were developed. Since that time, the flow of
air
has been of as much interest to physicists and engineers as the flow of water, and hydrodynamics has, as a consequence, become fluid
dynamics
. The term fluid mechanics, as used here, embraces both fluid
dynamics
and the subject still generally referred to as hydrostatics.
One other representative of the 20th century who deserves mention here besides Prandtl is
Geoffrey Taylor
of England. Taylor remained a classical physicist while most of his contemporaries were turning their attention to the problems of atomic structure and
quantum mechanics
, and he made several unexpected and important discoveries in the
field
of fluid mechanics. The richness of fluid mechanics is due in large part to a term in the basic equation of the motion of fluids which is nonlinearā
i.e.,
one that involves the fluid
velocity
twice over. It is characteristic of systems described by nonlinear equations that under certain conditions they become unstable and begin behaving in ways that seem at first sight to be totally chaotic. In the case of fluids, chaotic behaviour is very common and is called turbulence. Mathematicians have now begun to recognize patterns in
chaos
that can be analyzed fruitfully, and this development suggests that fluid mechanics will remain a field of active research well into the 21st century. (For a discussion of the concept of
chaos
, see
physical science, principles of
.)
Fluid mechanics is a subject with almost endless ramifications, and the account that follows is necessarily incomplete. Some knowledge of the basic properties of fluids will be needed; a survey of the most relevant properties is given in the next section. For further details, see
thermodynamics
and
liquid
.
Basic properties of
fluids
Fluids are not strictly continuous media in the way that all the successors of Euler and Bernoulli have assumed, for they are composed of discrete molecules. The molecules, however, are so small and, except in gases at very low pressures, the number of molecules per millilitre is so enormous that they need not be viewed as individual
entities
. There are a few liquids, known as liquid crystals, in which the molecules are packed together in such a way as to make the properties of the medium locally anisotropic, but the vast majority of fluids (including air and water) are
isotropic
. In fluid mechanics, the state of an isotropic fluid may be completely described by defining its mean mass per unit volume, or
density
(Ļ), its
temperature
(
T
), and its velocity (
v
) at every point in space, and just what the connection is between these macroscopic properties and the positions and velocities of individual molecules is of no direct relevance.
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A word perhaps is needed about the difference between
gases
and
liquids
, though the difference is easier to perceive than to describe. In gases the molecules are sufficiently far apart to move almost independently of one another, and gases tend to expand to fill any volume available to them. In liquids the molecules are more or less in contact, and the short-range attractive forces between them make them cohere; the molecules are moving too fast to settle down into the ordered
arrays
that are characteristic of solids, but not so fast that they can fly apart. Thus, samples of liquid can exist as drops or as jets with free surfaces, or they can sit in beakers constrained only by gravity, in a way that samples of
gas
cannot. Such samples may evaporate in time, as molecules one by one pick up enough speed to escape across the free surface and are not replaced. The lifetime of liquid drops and jets, however, is normally long enough for evaporation to be ignored.
There are two sorts of
stress
that may exist in any solid or fluid medium, and the difference between them may be illustrated by reference to a brick held between two hands. If the holder moves his hands toward each other, he exerts
pressure
on the brick; if he moves one hand toward his body and the other away from it, then he exerts what is called a
shear stress
. A solid substance such as a brick can withstand stresses of both types, but fluids, by definition, yield to shear stresses no matter how small these stresses may be. They do so at a rate determined by the fluidās
viscosity
. This property, about which more will be said later, is a measure of the
friction
that arises when
adjacent
layers of
fluid
slip over one another. It follows that the shear stresses are everywhere zero in a fluid at rest and in
equilibrium
, and from this it follows that the pressure (that is,
force
per unit area) acting perpendicular to all planes in the fluid is the same irrespective of their orientation (
Pascalās law
). For an isotropic fluid in equilibrium there is only one value of the local pressure (
p
) consistent with the stated values for Ļ and
T
. These three quantities are linked together by what is called the
equation of state
for the fluid.
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For gases at low pressures the equation of state is simple and well known. It is
where
R
is the
universal gas constant
(8.3 joules per degree Celsius per mole) and
M
is the
molar mass
, or an average molar mass if the gas is a mixture; for air, the
appropriate
average is about 29 Ć 10
ā3
kilogram per mole. For other fluids knowledge of the equation of state is often incomplete. Except under very extreme conditions, however, all one needs to know is how the density
changes
when the pressure is changed by a small amount, and this is described by the
compressibility
of the
fluidāeither the
isothermal compressibility, β
T
, or the
adiabatic compressibility, β
S
, according to circumstance. When an element of fluid is compressed, the work done on it tends to heat it up. If the heat has time to drain away to the surroundings and the temperature of the fluid remains essentially unchanged throughout, then β
T
is the relevant quantity. If virtually none of the heat escapes, as is more commonly the case in flow problems because the
thermal conductivity
of most fluids is poor, then the flow is said to be
adiabatic, and β
S
is needed instead. (The
S
refers to
entropy
, which remains constant in an
adiabatic process
provided that it takes place slowly enough to be treated as āreversibleā in the thermodynamic sense.) For gases that obey equation (
118
), it is evident that
p
and Ļ are proportional to one another in an isothermal process, and
In reversible adiabatic processes for such gases, however, the temperature rises on compression at a rate such that
and
where γ is about 1.4 for air and takes similar values for other common gases. For liquids the ratio between the isothermal and adiabatic compressibilities is much closer to
unity
. For liquids, however, both compressibilities are normally much less than
p
ā1
, and the simplifying assumption that they are zero is often justified.
The factor γ is not only the ratio between two compressibilities; it is also the ratio between two principal
specific heats
. The molar specific heat is the amount of heat required to raise the temperature of one mole through one degree. This is greater if the substance is allowed to expand as it is heated, and therefore to do work, than if its volume is fixed. The principal molar specific heats,
C
P
and
C
V
, refer to heating at constant pressure and constant volume, respectively, and
For air,
C
P
is about 3.5
R
.
Solids can be stretched without breaking, and liquids, though not gases, can withstand stretching, too. Thus, if the pressure is steadily reduced in a
specimen
of very pure water, bubbles will ultimately appear, but they may not do so until the pressure is negative and well below -10
7
newton per square metre; this is 100 times greater in magnitude than the (positive) pressure exerted by the Earthās
atmosphere
. Water owes its high ideal strength to the fact that rupture involves breaking links of attraction between molecules on either side of the plane on which rupture occurs; work must be done to break these links. However, its strength is drastically reduced by anything that provides a nucleus at which the process known as
cavitation
(formation of vapour- or gas-filled cavities) can begin, and a liquid containing suspended dust particles or
dissolved
gases is liable to cavitate quite easily.
Work also must be done if a free liquid drop of spherical shape is to be drawn out into a long thin cylinder or deformed in any other way that increases its surface area. Here again work is needed to break intermolecular links. The surface of a liquid behaves, in fact, as if it were an elastic membrane under tension, except that the tension exerted by an elastic membrane increases when the membrane is stretched in a way that the tension exerted by a liquid surface does not.
Surface tension
is what causes liquids to rise up capillary tubes, what supports hanging liquid drops, what limits the formation of ripples on the surface of liquids, and so on. |
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**hydrostatics**, Branch of [physics](https://www.britannica.com/science/physics-science) that deals with the [characteristics](https://www.britannica.com/dictionary/characteristics) of [fluids](https://www.britannica.com/science/fluid-physics) at rest, particularly with the [pressure](https://www.britannica.com/science/pressure) in a [fluid](https://www.britannica.com/science/fluid-physics) or exerted by a fluid (gas or liquid) on an immersed body. In applications, the principles of hydrostatics are used for problems relating to pressure in deep water (pressure increases with depth) and high in the [atmosphere](https://www.britannica.com/science/atmosphere) (pressure lessens with altitude).
This article was most recently revised and updated by [Robert Curley](https://www.britannica.com/editor/Robert-Curley/6737).
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[AI-generated answers](https://www.britannica.com/about-britannica-ai) from Britannica articles. AI makes mistakes, so verify using Britannica articles.
[fluid mechanics](https://www.britannica.com/science/fluid-mechanics)
- [Introduction](https://www.britannica.com/science/fluid-mechanics)
- [Basic properties of fluids](https://www.britannica.com/science/fluid-mechanics#ref77478)
- [Hydrostatics](https://www.britannica.com/science/fluid-mechanics/Hydrostatics)
- [Differential manometers](https://www.britannica.com/science/fluid-mechanics/Hydrostatics#ref77480)
- [Archimedesā principle](https://www.britannica.com/science/fluid-mechanics/Hydrostatics#ref77481)
- [Surface tension of liquids](https://www.britannica.com/science/fluid-mechanics/Hydrostatics#ref77482)
- [Hydrodynamics](https://www.britannica.com/science/fluid-mechanics/Hydrodynamics)
- [Bernoulliās law](https://www.britannica.com/science/fluid-mechanics/Hydrodynamics#ref77484)
- [Waves on shallow water](https://www.britannica.com/science/fluid-mechanics/Waves-on-shallow-water)
- [Compressible flow in gases](https://www.britannica.com/science/fluid-mechanics/Waves-on-shallow-water#ref77486)
- [Viscosity](https://www.britannica.com/science/fluid-mechanics/Viscosity)
- [Stresses in laminar motion](https://www.britannica.com/science/fluid-mechanics/Viscosity#ref77488)
- [Bulk viscosity](https://www.britannica.com/science/fluid-mechanics/Viscosity#ref77489)
- [Measurement of shear viscosity](https://www.britannica.com/science/fluid-mechanics/Viscosity#ref77490)
- [Navier-stokes equation](https://www.britannica.com/science/fluid-mechanics/Navier-stokes-equation)
- [Potential flow](https://www.britannica.com/science/fluid-mechanics/Navier-stokes-equation#ref77492)
- [Potential flow with circulation: vortex lines](https://www.britannica.com/science/fluid-mechanics/Navier-stokes-equation#ref77493)
- [Waves on deep water](https://www.britannica.com/science/fluid-mechanics/Waves-on-deep-water)
- [Boundary layers and separation](https://www.britannica.com/science/fluid-mechanics/Waves-on-deep-water#ref77495)
- [Drag](https://www.britannica.com/science/fluid-mechanics/Drag)
- [Lift](https://www.britannica.com/science/fluid-mechanics/Drag#ref77497)
- [Turbulence](https://www.britannica.com/science/fluid-mechanics/Turbulence)
- [Convection](https://www.britannica.com/science/fluid-mechanics/Turbulence#ref77499)
[References & Edit History](https://www.britannica.com/science/fluid-mechanics/additional-info) [Related Topics](https://www.britannica.com/facts/fluid-mechanics)
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# fluid mechanics
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Written by
[Thomas E. Faber Lecturer in Physics, University of Cambridge, 1959ā93; Fellow of Corpus Christi College, Cambridge. Author of *Fluid Dynamics for Physicists* and others.](https://www.britannica.com/contributor/Thomas-E-Faber/3527)
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- What is fluid mechanics?
- What is a fluid in science?
- What are some important properties of fluids?
- How is pressure created and measured in fluids?
- What is buoyancy, and how does it affect objects in water?
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**fluid mechanics**, [science](https://www.britannica.com/science/science) concerned with the [response of fluids](https://www.britannica.com/science/fluid-flow) to forces exerted upon them. It is a branch of classical [physics](https://www.britannica.com/science/physics-science) with applications of great importance in hydraulic and [aeronautical engineering](https://www.britannica.com/technology/aerospace-engineering), [chemical engineering](https://www.britannica.com/technology/chemical-engineering), [meteorology](https://www.britannica.com/science/meteorology), and zoology.
The most familiar fluid is of course [water](https://www.britannica.com/science/water), and an encyclopaedia of the 19th century probably would have dealt with the subject under the separate headings of [hydrostatics](https://www.britannica.com/science/hydrostatics), the science of water at rest, and hydrodynamics, the science of water in [motion](https://www.britannica.com/science/motion-mechanics). [Archimedes](https://www.britannica.com/biography/Archimedes) founded hydrostatics in about 250 bc when, according to [legend](https://www.merriam-webster.com/dictionary/legend), he leapt out of his bath and ran naked through the streets of Syracuse crying āEureka!ā; it has undergone rather little development since. The foundations of hydrodynamics, on the other hand, were not laid until the 18th century when mathematicians such as [Leonhard Euler](https://www.britannica.com/biography/Leonhard-Euler) and [Daniel Bernoulli](https://www.britannica.com/biography/Daniel-Bernoulli) began to explore the consequences, for a virtually continuous medium like water, of the [dynamic](https://www.merriam-webster.com/dictionary/dynamic) principles that Newton had enunciated for systems composed of discrete particles. Their work was continued in the 19th century by several mathematicians and physicists of the first rank, notably G.G. Stokes and William Thomson. By the end of the century explanations had been found for a host of intriguing phenomena having to do with the flow of water through tubes and orifices, the waves that ships moving through water leave behind them, raindrops on windowpanes, and the like. There was still no proper understanding, however, of problems as fundamental as that of water flowing past a fixed obstacle and exerting a [drag force](https://www.britannica.com/science/drag) upon it; the theory of potential flow, which worked so well in other [contexts](https://www.merriam-webster.com/dictionary/contexts), yielded results that at relatively high flow rates were grossly at variance with experiment. This problem was not properly understood until 1904, when the German physicist [Ludwig Prandtl](https://www.britannica.com/biography/Ludwig-Prandtl) introduced the concept of the [boundary layer](https://www.britannica.com/science/boundary-layer) (see below [Hydrodynamics: Boundary layers and separation](https://www.britannica.com/science/fluid-mechanics/Waves-on-deep-water#ref77495)). Prandtlās career continued into the period in which the first manned aircraft were developed. Since that time, the flow of [air](https://www.britannica.com/science/aerodynamics) has been of as much interest to physicists and engineers as the flow of water, and hydrodynamics has, as a consequence, become fluid [dynamics](https://www.britannica.com/science/dynamics-physics). The term fluid mechanics, as used here, embraces both fluid [dynamics](https://www.merriam-webster.com/dictionary/dynamics) and the subject still generally referred to as hydrostatics.
One other representative of the 20th century who deserves mention here besides Prandtl is [Geoffrey Taylor](https://www.britannica.com/biography/Geoffrey-Ingram-Taylor) of England. Taylor remained a classical physicist while most of his contemporaries were turning their attention to the problems of atomic structure and [quantum mechanics](https://www.britannica.com/science/quantum-mechanics-physics), and he made several unexpected and important discoveries in the [field](https://www.britannica.com/science/field-physics) of fluid mechanics. The richness of fluid mechanics is due in large part to a term in the basic equation of the motion of fluids which is nonlinearā*i.e.,* one that involves the fluid [velocity](https://www.britannica.com/science/velocity) twice over. It is characteristic of systems described by nonlinear equations that under certain conditions they become unstable and begin behaving in ways that seem at first sight to be totally chaotic. In the case of fluids, chaotic behaviour is very common and is called turbulence. Mathematicians have now begun to recognize patterns in [chaos](https://www.britannica.com/science/chaos-theory) that can be analyzed fruitfully, and this development suggests that fluid mechanics will remain a field of active research well into the 21st century. (For a discussion of the concept of [chaos](https://www.merriam-webster.com/dictionary/chaos), see [physical science, principles of](https://www.britannica.com/science/principles-of-physical-science).)
Fluid mechanics is a subject with almost endless ramifications, and the account that follows is necessarily incomplete. Some knowledge of the basic properties of fluids will be needed; a survey of the most relevant properties is given in the next section. For further details, see [thermodynamics](https://www.britannica.com/science/thermodynamics) and [liquid](https://www.britannica.com/science/liquid-state-of-matter).
## Basic properties of [fluids](https://www.britannica.com/science/fluid-physics)
Fluids are not strictly continuous media in the way that all the successors of Euler and Bernoulli have assumed, for they are composed of discrete molecules. The molecules, however, are so small and, except in gases at very low pressures, the number of molecules per millilitre is so enormous that they need not be viewed as individual [entities](https://www.britannica.com/dictionary/entities). There are a few liquids, known as liquid crystals, in which the molecules are packed together in such a way as to make the properties of the medium locally anisotropic, but the vast majority of fluids (including air and water) are [isotropic](https://www.britannica.com/science/isotropy). In fluid mechanics, the state of an isotropic fluid may be completely described by defining its mean mass per unit volume, or [density](https://www.britannica.com/science/density) (Ļ), its [temperature](https://www.britannica.com/science/temperature) (*T*), and its velocity (*v*) at every point in space, and just what the connection is between these macroscopic properties and the positions and velocities of individual molecules is of no direct relevance.
[ Britannica Quiz All About Physics Quiz](https://www.britannica.com/quiz/all-about-physics-quiz)
A word perhaps is needed about the difference between [gases](https://www.britannica.com/science/gas-state-of-matter) and [liquids](https://www.britannica.com/science/liquid-state-of-matter), though the difference is easier to perceive than to describe. In gases the molecules are sufficiently far apart to move almost independently of one another, and gases tend to expand to fill any volume available to them. In liquids the molecules are more or less in contact, and the short-range attractive forces between them make them cohere; the molecules are moving too fast to settle down into the ordered [arrays](https://www.britannica.com/dictionary/arrays) that are characteristic of solids, but not so fast that they can fly apart. Thus, samples of liquid can exist as drops or as jets with free surfaces, or they can sit in beakers constrained only by gravity, in a way that samples of [gas](https://www.britannica.com/science/gas-state-of-matter) cannot. Such samples may evaporate in time, as molecules one by one pick up enough speed to escape across the free surface and are not replaced. The lifetime of liquid drops and jets, however, is normally long enough for evaporation to be ignored.
There are two sorts of [stress](https://www.britannica.com/science/stress-physics) that may exist in any solid or fluid medium, and the difference between them may be illustrated by reference to a brick held between two hands. If the holder moves his hands toward each other, he exerts [pressure](https://www.britannica.com/science/pressure) on the brick; if he moves one hand toward his body and the other away from it, then he exerts what is called a [shear stress](https://www.britannica.com/science/shear-stress). A solid substance such as a brick can withstand stresses of both types, but fluids, by definition, yield to shear stresses no matter how small these stresses may be. They do so at a rate determined by the fluidās [viscosity](https://www.britannica.com/science/viscosity). This property, about which more will be said later, is a measure of the [friction](https://www.britannica.com/science/friction) that arises when [adjacent](https://www.merriam-webster.com/dictionary/adjacent) layers of [fluid](https://www.britannica.com/science/fluid-pressure) slip over one another. It follows that the shear stresses are everywhere zero in a fluid at rest and in [equilibrium](https://www.merriam-webster.com/dictionary/equilibrium), and from this it follows that the pressure (that is, [force](https://www.britannica.com/science/force-physics) per unit area) acting perpendicular to all planes in the fluid is the same irrespective of their orientation ([Pascalās law](https://www.britannica.com/science/Pascals-principle)). For an isotropic fluid in equilibrium there is only one value of the local pressure (*p*) consistent with the stated values for Ļ and *T*. These three quantities are linked together by what is called the [equation of state](https://www.britannica.com/science/equation-of-state) for the fluid.
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For gases at low pressures the equation of state is simple and well known. It iswhere *R* is the [universal gas constant](https://www.britannica.com/science/universal-gas-constant) (8.3 joules per degree Celsius per mole) and *M* is the [molar mass](https://www.britannica.com/science/molar-mass), or an average molar mass if the gas is a mixture; for air, the [appropriate](https://www.britannica.com/dictionary/appropriate) average is about 29 Ć 10ā3 kilogram per mole. For other fluids knowledge of the equation of state is often incomplete. Except under very extreme conditions, however, all one needs to know is how the density [changes](https://www.britannica.com/science/isothermal-change) when the pressure is changed by a small amount, and this is described by the [compressibility](https://www.britannica.com/science/compressibility) of the fluidāeither the isothermal compressibility, β*T*, or the adiabatic compressibility, β*S*, according to circumstance. When an element of fluid is compressed, the work done on it tends to heat it up. If the heat has time to drain away to the surroundings and the temperature of the fluid remains essentially unchanged throughout, then β*T* is the relevant quantity. If virtually none of the heat escapes, as is more commonly the case in flow problems because the [thermal conductivity](https://www.britannica.com/science/thermal-conductivity) of most fluids is poor, then the flow is said to be adiabatic, and β*S* is needed instead. (The *S* refers to [entropy](https://www.merriam-webster.com/dictionary/entropy), which remains constant in an [adiabatic process](https://www.britannica.com/science/adiabatic-process) provided that it takes place slowly enough to be treated as āreversibleā in the thermodynamic sense.) For gases that obey equation ([118](https://www.britannica.com/science/hydrostatics#ref-15119)), it is evident that *p* and Ļ are proportional to one another in an isothermal process, and
In reversible adiabatic processes for such gases, however, the temperature rises on compression at a rate such thatandwhere γ is about 1.4 for air and takes similar values for other common gases. For liquids the ratio between the isothermal and adiabatic compressibilities is much closer to [unity](https://www.britannica.com/dictionary/unity). For liquids, however, both compressibilities are normally much less than *p*ā1, and the simplifying assumption that they are zero is often justified.
The factor γ is not only the ratio between two compressibilities; it is also the ratio between two principal [specific heats](https://www.britannica.com/science/specific-heat). The molar specific heat is the amount of heat required to raise the temperature of one mole through one degree. This is greater if the substance is allowed to expand as it is heated, and therefore to do work, than if its volume is fixed. The principal molar specific heats, *C**P* and *C**V*, refer to heating at constant pressure and constant volume, respectively, and
For air, *C**P* is about 3.5 *R*.
Solids can be stretched without breaking, and liquids, though not gases, can withstand stretching, too. Thus, if the pressure is steadily reduced in a [specimen](https://www.britannica.com/dictionary/specimen) of very pure water, bubbles will ultimately appear, but they may not do so until the pressure is negative and well below -107 newton per square metre; this is 100 times greater in magnitude than the (positive) pressure exerted by the Earthās [atmosphere](https://www.britannica.com/science/atmosphere). Water owes its high ideal strength to the fact that rupture involves breaking links of attraction between molecules on either side of the plane on which rupture occurs; work must be done to break these links. However, its strength is drastically reduced by anything that provides a nucleus at which the process known as [cavitation](https://www.britannica.com/science/cavitation) (formation of vapour- or gas-filled cavities) can begin, and a liquid containing suspended dust particles or [dissolved](https://www.britannica.com/dictionary/dissolved) gases is liable to cavitate quite easily.
Key People:
[Sir James Lighthill](https://www.britannica.com/biography/James-Lighthill)
[Sir George Gabriel Stokes, 1st Baronet](https://www.britannica.com/biography/Sir-George-Gabriel-Stokes-1st-Baronet)
[Sir Horace Lamb](https://www.britannica.com/biography/Horace-Lamb)
[Henri-Ćmile Bazin](https://www.britannica.com/biography/Henri-Emile-Bazin)
[Henri Pitot](https://www.britannica.com/biography/Henri-Pitot)
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Related Topics:
[continuum mechanics](https://www.britannica.com/science/continuum-mechanics)
[aerostatics](https://www.britannica.com/science/aerostatics)
[dāAlembertās paradox](https://www.britannica.com/science/dAlemberts-paradox)
[hydrodynamics](https://www.britannica.com/science/hydrodynamics-physics)
[hydrokinetics](https://www.britannica.com/science/hydrokinetics)
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On the Web:
[Physics LibreTexts - Fluid Mechanics](https://phys.libretexts.org/Bookshelves/University_Physics/Book%3A_Introductory_Physics_-_Building_Models_to_Describe_Our_World_%28Martin_Neary_Rinaldo_and_Woodman%29/15%3A_Fluid_Mechanics) (Mar. 26, 2026)
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[See all related content](https://www.britannica.com/facts/fluid-mechanics)
Work also must be done if a free liquid drop of spherical shape is to be drawn out into a long thin cylinder or deformed in any other way that increases its surface area. Here again work is needed to break intermolecular links. The surface of a liquid behaves, in fact, as if it were an elastic membrane under tension, except that the tension exerted by an elastic membrane increases when the membrane is stretched in a way that the tension exerted by a liquid surface does not. [Surface tension](https://www.britannica.com/science/surface-tension) is what causes liquids to rise up capillary tubes, what supports hanging liquid drops, what limits the formation of ripples on the surface of liquids, and so on.
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- [University of Central Florida Pressbooks - University Physics Volume 1 - Fluid Dynamics](https://pressbooks.online.ucf.edu/osuniversityphysics/chapter/14-5-fluid-dynamics/)
- [MIT OpenCourseWare - Introduction to basic principles of fluid mechanics (PDF)](https://ocw.mit.edu/courses/2-016-hydrodynamics-13-012-fall-2005/b97992061b6ee90cd549e01a678b08e5_2005reading3.pdf)
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| Readable Markdown | Top Questions
- What is fluid mechanics?
- What is a fluid in science?
- What are some important properties of fluids?
- How is pressure created and measured in fluids?
- What is buoyancy, and how does it affect objects in water?
- How is fluid mechanics used in real-life situations like airplanes and weather?
**fluid mechanics**, [science](https://www.britannica.com/science/science) concerned with the [response of fluids](https://www.britannica.com/science/fluid-flow) to forces exerted upon them. It is a branch of classical [physics](https://www.britannica.com/science/physics-science) with applications of great importance in hydraulic and [aeronautical engineering](https://www.britannica.com/technology/aerospace-engineering), [chemical engineering](https://www.britannica.com/technology/chemical-engineering), [meteorology](https://www.britannica.com/science/meteorology), and zoology.
The most familiar fluid is of course [water](https://www.britannica.com/science/water), and an encyclopaedia of the 19th century probably would have dealt with the subject under the separate headings of [hydrostatics](https://www.britannica.com/science/hydrostatics), the science of water at rest, and hydrodynamics, the science of water in [motion](https://www.britannica.com/science/motion-mechanics). [Archimedes](https://www.britannica.com/biography/Archimedes) founded hydrostatics in about 250 bc when, according to [legend](https://www.merriam-webster.com/dictionary/legend), he leapt out of his bath and ran naked through the streets of Syracuse crying āEureka!ā; it has undergone rather little development since. The foundations of hydrodynamics, on the other hand, were not laid until the 18th century when mathematicians such as [Leonhard Euler](https://www.britannica.com/biography/Leonhard-Euler) and [Daniel Bernoulli](https://www.britannica.com/biography/Daniel-Bernoulli) began to explore the consequences, for a virtually continuous medium like water, of the [dynamic](https://www.merriam-webster.com/dictionary/dynamic) principles that Newton had enunciated for systems composed of discrete particles. Their work was continued in the 19th century by several mathematicians and physicists of the first rank, notably G.G. Stokes and William Thomson. By the end of the century explanations had been found for a host of intriguing phenomena having to do with the flow of water through tubes and orifices, the waves that ships moving through water leave behind them, raindrops on windowpanes, and the like. There was still no proper understanding, however, of problems as fundamental as that of water flowing past a fixed obstacle and exerting a [drag force](https://www.britannica.com/science/drag) upon it; the theory of potential flow, which worked so well in other [contexts](https://www.merriam-webster.com/dictionary/contexts), yielded results that at relatively high flow rates were grossly at variance with experiment. This problem was not properly understood until 1904, when the German physicist [Ludwig Prandtl](https://www.britannica.com/biography/Ludwig-Prandtl) introduced the concept of the [boundary layer](https://www.britannica.com/science/boundary-layer) (see below [Hydrodynamics: Boundary layers and separation](https://www.britannica.com/science/fluid-mechanics/Waves-on-deep-water#ref77495)). Prandtlās career continued into the period in which the first manned aircraft were developed. Since that time, the flow of [air](https://www.britannica.com/science/aerodynamics) has been of as much interest to physicists and engineers as the flow of water, and hydrodynamics has, as a consequence, become fluid [dynamics](https://www.britannica.com/science/dynamics-physics). The term fluid mechanics, as used here, embraces both fluid [dynamics](https://www.merriam-webster.com/dictionary/dynamics) and the subject still generally referred to as hydrostatics.
One other representative of the 20th century who deserves mention here besides Prandtl is [Geoffrey Taylor](https://www.britannica.com/biography/Geoffrey-Ingram-Taylor) of England. Taylor remained a classical physicist while most of his contemporaries were turning their attention to the problems of atomic structure and [quantum mechanics](https://www.britannica.com/science/quantum-mechanics-physics), and he made several unexpected and important discoveries in the [field](https://www.britannica.com/science/field-physics) of fluid mechanics. The richness of fluid mechanics is due in large part to a term in the basic equation of the motion of fluids which is nonlinearā*i.e.,* one that involves the fluid [velocity](https://www.britannica.com/science/velocity) twice over. It is characteristic of systems described by nonlinear equations that under certain conditions they become unstable and begin behaving in ways that seem at first sight to be totally chaotic. In the case of fluids, chaotic behaviour is very common and is called turbulence. Mathematicians have now begun to recognize patterns in [chaos](https://www.britannica.com/science/chaos-theory) that can be analyzed fruitfully, and this development suggests that fluid mechanics will remain a field of active research well into the 21st century. (For a discussion of the concept of [chaos](https://www.merriam-webster.com/dictionary/chaos), see [physical science, principles of](https://www.britannica.com/science/principles-of-physical-science).)
Fluid mechanics is a subject with almost endless ramifications, and the account that follows is necessarily incomplete. Some knowledge of the basic properties of fluids will be needed; a survey of the most relevant properties is given in the next section. For further details, see [thermodynamics](https://www.britannica.com/science/thermodynamics) and [liquid](https://www.britannica.com/science/liquid-state-of-matter).
## Basic properties of [fluids](https://www.britannica.com/science/fluid-physics)
Fluids are not strictly continuous media in the way that all the successors of Euler and Bernoulli have assumed, for they are composed of discrete molecules. The molecules, however, are so small and, except in gases at very low pressures, the number of molecules per millilitre is so enormous that they need not be viewed as individual [entities](https://www.britannica.com/dictionary/entities). There are a few liquids, known as liquid crystals, in which the molecules are packed together in such a way as to make the properties of the medium locally anisotropic, but the vast majority of fluids (including air and water) are [isotropic](https://www.britannica.com/science/isotropy). In fluid mechanics, the state of an isotropic fluid may be completely described by defining its mean mass per unit volume, or [density](https://www.britannica.com/science/density) (Ļ), its [temperature](https://www.britannica.com/science/temperature) (*T*), and its velocity (*v*) at every point in space, and just what the connection is between these macroscopic properties and the positions and velocities of individual molecules is of no direct relevance.
[ Britannica Quiz All About Physics Quiz](https://www.britannica.com/quiz/all-about-physics-quiz)
A word perhaps is needed about the difference between [gases](https://www.britannica.com/science/gas-state-of-matter) and [liquids](https://www.britannica.com/science/liquid-state-of-matter), though the difference is easier to perceive than to describe. In gases the molecules are sufficiently far apart to move almost independently of one another, and gases tend to expand to fill any volume available to them. In liquids the molecules are more or less in contact, and the short-range attractive forces between them make them cohere; the molecules are moving too fast to settle down into the ordered [arrays](https://www.britannica.com/dictionary/arrays) that are characteristic of solids, but not so fast that they can fly apart. Thus, samples of liquid can exist as drops or as jets with free surfaces, or they can sit in beakers constrained only by gravity, in a way that samples of [gas](https://www.britannica.com/science/gas-state-of-matter) cannot. Such samples may evaporate in time, as molecules one by one pick up enough speed to escape across the free surface and are not replaced. The lifetime of liquid drops and jets, however, is normally long enough for evaporation to be ignored.
There are two sorts of [stress](https://www.britannica.com/science/stress-physics) that may exist in any solid or fluid medium, and the difference between them may be illustrated by reference to a brick held between two hands. If the holder moves his hands toward each other, he exerts [pressure](https://www.britannica.com/science/pressure) on the brick; if he moves one hand toward his body and the other away from it, then he exerts what is called a [shear stress](https://www.britannica.com/science/shear-stress). A solid substance such as a brick can withstand stresses of both types, but fluids, by definition, yield to shear stresses no matter how small these stresses may be. They do so at a rate determined by the fluidās [viscosity](https://www.britannica.com/science/viscosity). This property, about which more will be said later, is a measure of the [friction](https://www.britannica.com/science/friction) that arises when [adjacent](https://www.merriam-webster.com/dictionary/adjacent) layers of [fluid](https://www.britannica.com/science/fluid-pressure) slip over one another. It follows that the shear stresses are everywhere zero in a fluid at rest and in [equilibrium](https://www.merriam-webster.com/dictionary/equilibrium), and from this it follows that the pressure (that is, [force](https://www.britannica.com/science/force-physics) per unit area) acting perpendicular to all planes in the fluid is the same irrespective of their orientation ([Pascalās law](https://www.britannica.com/science/Pascals-principle)). For an isotropic fluid in equilibrium there is only one value of the local pressure (*p*) consistent with the stated values for Ļ and *T*. These three quantities are linked together by what is called the [equation of state](https://www.britannica.com/science/equation-of-state) for the fluid.
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For gases at low pressures the equation of state is simple and well known. It iswhere *R* is the [universal gas constant](https://www.britannica.com/science/universal-gas-constant) (8.3 joules per degree Celsius per mole) and *M* is the [molar mass](https://www.britannica.com/science/molar-mass), or an average molar mass if the gas is a mixture; for air, the [appropriate](https://www.britannica.com/dictionary/appropriate) average is about 29 Ć 10ā3 kilogram per mole. For other fluids knowledge of the equation of state is often incomplete. Except under very extreme conditions, however, all one needs to know is how the density [changes](https://www.britannica.com/science/isothermal-change) when the pressure is changed by a small amount, and this is described by the [compressibility](https://www.britannica.com/science/compressibility) of the fluidāeither the isothermal compressibility, β*T*, or the adiabatic compressibility, β*S*, according to circumstance. When an element of fluid is compressed, the work done on it tends to heat it up. If the heat has time to drain away to the surroundings and the temperature of the fluid remains essentially unchanged throughout, then β*T* is the relevant quantity. If virtually none of the heat escapes, as is more commonly the case in flow problems because the [thermal conductivity](https://www.britannica.com/science/thermal-conductivity) of most fluids is poor, then the flow is said to be adiabatic, and β*S* is needed instead. (The *S* refers to [entropy](https://www.merriam-webster.com/dictionary/entropy), which remains constant in an [adiabatic process](https://www.britannica.com/science/adiabatic-process) provided that it takes place slowly enough to be treated as āreversibleā in the thermodynamic sense.) For gases that obey equation ([118](https://www.britannica.com/science/hydrostatics#ref-15119)), it is evident that *p* and Ļ are proportional to one another in an isothermal process, and
In reversible adiabatic processes for such gases, however, the temperature rises on compression at a rate such thatandwhere γ is about 1.4 for air and takes similar values for other common gases. For liquids the ratio between the isothermal and adiabatic compressibilities is much closer to [unity](https://www.britannica.com/dictionary/unity). For liquids, however, both compressibilities are normally much less than *p*ā1, and the simplifying assumption that they are zero is often justified.
The factor γ is not only the ratio between two compressibilities; it is also the ratio between two principal [specific heats](https://www.britannica.com/science/specific-heat). The molar specific heat is the amount of heat required to raise the temperature of one mole through one degree. This is greater if the substance is allowed to expand as it is heated, and therefore to do work, than if its volume is fixed. The principal molar specific heats, *C**P* and *C**V*, refer to heating at constant pressure and constant volume, respectively, and
For air, *C**P* is about 3.5 *R*.
Solids can be stretched without breaking, and liquids, though not gases, can withstand stretching, too. Thus, if the pressure is steadily reduced in a [specimen](https://www.britannica.com/dictionary/specimen) of very pure water, bubbles will ultimately appear, but they may not do so until the pressure is negative and well below -107 newton per square metre; this is 100 times greater in magnitude than the (positive) pressure exerted by the Earthās [atmosphere](https://www.britannica.com/science/atmosphere). Water owes its high ideal strength to the fact that rupture involves breaking links of attraction between molecules on either side of the plane on which rupture occurs; work must be done to break these links. However, its strength is drastically reduced by anything that provides a nucleus at which the process known as [cavitation](https://www.britannica.com/science/cavitation) (formation of vapour- or gas-filled cavities) can begin, and a liquid containing suspended dust particles or [dissolved](https://www.britannica.com/dictionary/dissolved) gases is liable to cavitate quite easily.
Work also must be done if a free liquid drop of spherical shape is to be drawn out into a long thin cylinder or deformed in any other way that increases its surface area. Here again work is needed to break intermolecular links. The surface of a liquid behaves, in fact, as if it were an elastic membrane under tension, except that the tension exerted by an elastic membrane increases when the membrane is stretched in a way that the tension exerted by a liquid surface does not. [Surface tension](https://www.britannica.com/science/surface-tension) is what causes liquids to rise up capillary tubes, what supports hanging liquid drops, what limits the formation of ripples on the surface of liquids, and so on. |
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