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| Boilerpipe Text | From Wikipedia, the free encyclopedia
Hydrostatic pressure
is the
static pressure
exerted at a point of interest by the
weight
of a
fluid
column above the point.
Due to the fundamental nature of fluids, a fluid cannot remain at rest under the presence of a
shear stress
. However, fluids can exert
pressure
normal
to any contacting surface. If a point in the fluid is thought of as an infinitesimally small cube, then it follows from the principles of equilibrium that the pressure on every side of this unit of fluid must be equal. If this were not the case, the fluid would move in the direction of the resulting force. Thus, the
pressure
on a fluid at rest is
isotropic
; i.e., it acts with equal magnitude in all directions. This characteristic allows fluids to transmit force through the length of pipes or tubes; i.e., a force applied to a fluid in a pipe is transmitted, via the fluid, to the other end of the pipe. This principle was first formulated, in a slightly extended form, by
Blaise Pascal
, and is now called
Pascal's law
.
[
citation needed
]
In a fluid at rest, all frictional and inertial stresses vanish and the state of stress of the system is called
hydrostatic
. When this condition of
V
= 0
is applied to the
Navier–Stokes equations
for viscous fluids or
Euler equations (fluid dynamics)
for ideal inviscid fluid, the gradient of pressure becomes a function of body forces only.
The Navier-Stokes momentum equations are:
Navier–Stokes momentum equation
(
convective form
)
By setting the
flow velocity
:
, they become simply:
or:
This is the general form of Stevin's law: the
pressure gradient
equals the
body force
force density
field.
Let us now consider two particular cases of this law. In case of a
conservative
body force with
scalar potential
:
:
the Stevin equation becomes:
That can be integrated to give:
So in this case the pressure difference is the opposite of the difference of the scalar potential associated to the body force.
In the other particular case of a body force of constant direction along z:
the generalised Stevin's law above becomes:
That can be integrated to give another (less-) generalised Stevin's law:
where:
Simplification for liquids
[
edit
]
For water and other liquids, this integral can be simplified significantly for many practical applications, based on the following two assumptions. Since many liquids can be considered
incompressible
, a reasonable good estimation can be made from assuming a constant density throughout the liquid. The same assumption cannot be made within a gaseous environment. Also, since the height
of the fluid column between
z
and
z
0
is often reasonably small compared to the radius of the Earth, one can neglect the variation of
g
. Under these circumstances, one can transport out of the integral the density and the gravity acceleration and the law is simplified into the formula
where
is the height
z
−
z
0
of the liquid column between the test volume and the zero reference point of the pressure. This formula is often called
Stevin's
law.
[
1
]
[
2
]
One could arrive to the above formula also by considering the first particular case of the equation for a conservative body force field: in fact the body force field of uniform intensity and direction:
is conservative, so one can write the body force density as:
Then the body force density has a simple
scalar potential
:
And the pressure difference follows another time the Stevin's law:
The reference point should lie at or below the surface of the liquid. Otherwise, one has to split the integral into two (or more) terms with the constant
ρ
liquid
and
ρ
(
z
′)
above
. For example, the
absolute pressure
compared to vacuum is
where
is the total height of the liquid column above the test area to the surface, and
p
0
is the
atmospheric pressure
, i.e., the pressure calculated from the remaining integral over the air column from the liquid surface to infinity. This can easily be visualized using a
pressure prism
.
Hydrostatic pressure has been used in the preservation of foods in a process called
pascalization
.
[
3
]
In medicine, hydrostatic pressure in
blood vessels
is the pressure of the blood against the wall. It is the opposing force to
oncotic pressure
. In capillaries, hydrostatic pressure (also known as capillary blood pressure) is higher than the opposing “colloid
osmotic pressure
” in blood—a “constant” pressure primarily produced by circulating albumin—at the arteriolar end of the capillary. This pressure forces plasma and nutrients out of the capillaries and into surrounding tissues. Fluid and the cellular wastes in the tissues enter the capillaries at the venule end, where the hydrostatic pressure is less than the osmotic pressure in the vessel.
[
4
]
Atmospheric pressure
[
edit
]
Statistical mechanics
shows that, for a pure
ideal gas
of constant temperature
T
in the earth gravitational field, its pressure,
p
will vary with height,
h
, as
where
g
is the
acceleration due to gravity
T
is the
absolute temperature
k
is
Boltzmann constant
M
is the
molecular mass
of the gas
p
is the pressure
h
is the height
This is known as the
barometric formula
, and may be derived from assuming the pressure is
hydrostatic
.
If there are multiple types of molecules in the gas, the
partial pressure
of each type will be given by this equation. Under most conditions, the distribution of each species of gas is independent of the other species.
Any body of arbitrary shape which is immersed, partly or fully, in a fluid will experience the action of a net force in the opposite direction of the local pressure gradient. If this pressure gradient arises from gravity, the net force is in the vertical direction opposite that of the gravitational force. This vertical force is termed buoyancy or buoyant force and is equal in magnitude, but opposite in direction, to the weight of the displaced fluid. Mathematically,
where
ρ
is the density of the fluid,
g
is the acceleration due to gravity, and
V
is the volume of fluid directly above the curved surface.
[
5
]
In the case of a
ship
, for instance, its weight is balanced by pressure forces from the surrounding water, allowing it to float. If more cargo is loaded onto the ship, it would sink more into the water – displacing more water and thus receive a higher buoyant force to balance the increased weight.
[
citation needed
]
Discovery of the principle of buoyancy is attributed to
Archimedes
.
Hydrostatic force on submerged surfaces
[
edit
]
The horizontal and vertical components of the hydrostatic force acting on a submerged surface are given by the following formula:
[
5
]
where
p
c
is the pressure at the centroid of the vertical projection of the submerged surface
A
is the area of the same vertical projection of the surface
ρ
is the density of the fluid
g
is the acceleration due to gravity
V
is the volume of fluid directly above the curved surface
Hydrostatics
Vertical pressure variation
^
Bettini, Alessandro (2016).
A Course in Classical Physics 2—Fluids and Thermodynamics
. Springer. p. 8.
ISBN
978-3-319-30685-8
.
^
Mauri, Roberto (8 April 2015).
Transport Phenomena in Multiphase Flow
. Springer. p. 24.
ISBN
978-3-319-15792-4
. Retrieved
3 February
2017
.
^
Brown, Amy Christian (2007).
Understanding Food: Principles and Preparation
(3 ed.). Cengage Learning. p. 546.
ISBN
978-0-495-10745-3
.
^
This article incorporates
text
available under the
CC BY 4.0
license.
Betts, J Gordon; Desaix, Peter; Johnson, Eddie; Johnson, Jody E; Korol, Oksana; Kruse, Dean; Poe, Brandon; Wise, James; Womble, Mark D; Young, Kelly A (September 16, 2023).
Anatomy & Physiology
. Houston: OpenStax CNX. 26.1 Body fluids and fluid compartments.
ISBN
978-1-947172-04-3
.
^
a
b
Fox, Robert; McDonald, Alan; Pritchard, Philip (2012).
Fluid Mechanics
(8 ed.).
John Wiley & Sons
. pp.
76–
83.
ISBN
978-1-118-02641-0
. |
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## Contents
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- [1 Background](https://en.wikipedia.org/wiki/Hydrostatic_pressure#Background)
- [2 Formulation](https://en.wikipedia.org/wiki/Hydrostatic_pressure#Formulation)
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- [3 Applications](https://en.wikipedia.org/wiki/Hydrostatic_pressure#Applications)
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- [3\.1 Medicine](https://en.wikipedia.org/wiki/Hydrostatic_pressure#Medicine)
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- [5 See also](https://en.wikipedia.org/wiki/Hydrostatic_pressure#See_also)
- [6 References](https://en.wikipedia.org/wiki/Hydrostatic_pressure#References)
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# Hydrostatic pressure
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From Wikipedia, the free encyclopedia
Physical quantity
**Hydrostatic pressure** is the [static pressure](https://en.wikipedia.org/wiki/Static_pressure "Static pressure") exerted at a point of interest by the [weight](https://en.wikipedia.org/wiki/Weight "Weight") of a [fluid](https://en.wikipedia.org/wiki/Fluid "Fluid") column above the point.
## Background
\[[edit](https://en.wikipedia.org/w/index.php?title=Hydrostatic_pressure&action=edit§ion=1 "Edit section: Background")\]
Due to the fundamental nature of fluids, a fluid cannot remain at rest under the presence of a [shear stress](https://en.wikipedia.org/wiki/Shear_stress "Shear stress"). However, fluids can exert [pressure](https://en.wikipedia.org/wiki/Pressure "Pressure") [normal](https://en.wikipedia.org/wiki/Surface_normal "Surface normal") to any contacting surface. If a point in the fluid is thought of as an infinitesimally small cube, then it follows from the principles of equilibrium that the pressure on every side of this unit of fluid must be equal. If this were not the case, the fluid would move in the direction of the resulting force. Thus, the [pressure](https://en.wikipedia.org/wiki/Fluid_pressure "Fluid pressure") on a fluid at rest is [isotropic](https://en.wikipedia.org/wiki/Isotropic "Isotropic"); i.e., it acts with equal magnitude in all directions. This characteristic allows fluids to transmit force through the length of pipes or tubes; i.e., a force applied to a fluid in a pipe is transmitted, via the fluid, to the other end of the pipe. This principle was first formulated, in a slightly extended form, by [Blaise Pascal](https://en.wikipedia.org/wiki/Blaise_Pascal "Blaise Pascal"), and is now called [Pascal's law](https://en.wikipedia.org/wiki/Pascal%27s_law "Pascal's law").\[*[citation needed](https://en.wikipedia.org/wiki/Wikipedia:Citation_needed "Wikipedia:Citation needed")*\]
## Formulation
\[[edit](https://en.wikipedia.org/w/index.php?title=Hydrostatic_pressure&action=edit§ion=2 "Edit section: Formulation")\]
In a fluid at rest, all frictional and inertial stresses vanish and the state of stress of the system is called *hydrostatic*. When this condition of *V* = 0 is applied to the [Navier–Stokes equations](https://en.wikipedia.org/wiki/Navier%E2%80%93Stokes_equations "Navier–Stokes equations") for viscous fluids or [Euler equations (fluid dynamics)](https://en.wikipedia.org/wiki/Euler_equations_\(fluid_dynamics\) "Euler equations (fluid dynamics)") for ideal inviscid fluid, the gradient of pressure becomes a function of body forces only. The Navier-Stokes momentum equations are:
**Navier–Stokes momentum equation** (*convective form*)
ρ
D
u
D
t
\=
−
∇
\[
p
−
ζ
(
∇
⋅
u
)
\]
\+
∇
⋅
{
μ
\[
∇
u
\+
(
∇
u
)
T
−
2
3
(
∇
⋅
u
)
I
\]
}
\+
ρ
g
.
{\\displaystyle \\rho {\\frac {\\mathrm {D} \\mathbf {u} }{\\mathrm {D} t}}=-\\nabla \[p-\\zeta (\\nabla \\cdot \\mathbf {u} )\]+\\nabla \\cdot \\left\\{\\mu \\left\[\\nabla \\mathbf {u} +(\\nabla \\mathbf {u} )^{\\mathrm {T} }-{\\tfrac {2}{3}}(\\nabla \\cdot \\mathbf {u} )\\mathbf {I} \\right\]\\right\\}+\\rho \\mathbf {g} .}
![{\\displaystyle \\rho {\\frac {\\mathrm {D} \\mathbf {u} }{\\mathrm {D} t}}=-\\nabla \[p-\\zeta (\\nabla \\cdot \\mathbf {u} )\]+\\nabla \\cdot \\left\\{\\mu \\left\[\\nabla \\mathbf {u} +(\\nabla \\mathbf {u} )^{\\mathrm {T} }-{\\tfrac {2}{3}}(\\nabla \\cdot \\mathbf {u} )\\mathbf {I} \\right\]\\right\\}+\\rho \\mathbf {g} .}](https://wikimedia.org/api/rest_v1/media/math/render/svg/6fd98d1bcacc93a84fa4fc981a05a200e680be04)
By setting the [flow velocity](https://en.wikipedia.org/wiki/Flow_velocity "Flow velocity") :u \= 0 {\\displaystyle \\mathbf {u} =\\mathbf {0} } , they become simply:
0
\=
−
∇
p
\+
ρ
g
{\\displaystyle \\mathbf {0} =-\\nabla p+\\rho \\mathbf {g} }

or:
∇
p
\=
ρ
g
{\\displaystyle \\nabla p=\\rho \\mathbf {g} }

This is the general form of Stevin's law: the [pressure gradient](https://en.wikipedia.org/wiki/Pressure_gradient "Pressure gradient") equals the [body force](https://en.wikipedia.org/wiki/Body_force "Body force") [force density](https://en.wikipedia.org/wiki/Force_density "Force density") field.
Let us now consider two particular cases of this law. In case of a [conservative](https://en.wikipedia.org/wiki/Conservative_force "Conservative force") body force with [scalar potential](https://en.wikipedia.org/wiki/Scalar_potential "Scalar potential") :ϕ {\\displaystyle \\phi } :
ρ
g
\=
−
∇
ϕ
{\\displaystyle \\rho \\mathbf {g} =-\\nabla \\phi }

the Stevin equation becomes:
∇
p
\=
−
∇
ϕ
{\\displaystyle \\nabla p=-\\nabla \\phi }

That can be integrated to give:
Δ
p
\=
−
Δ
ϕ
{\\displaystyle \\Delta p=-\\Delta \\phi }

So in this case the pressure difference is the opposite of the difference of the scalar potential associated to the body force. In the other particular case of a body force of constant direction along z:
g
\=
−
g
(
x
,
y
,
z
)
k
^
{\\displaystyle \\mathbf {g} =-g(x,y,z){\\hat {k}}}

the generalised Stevin's law above becomes:
∂
p
∂
z
\=
−
ρ
(
x
,
y
,
z
)
g
(
x
,
y
,
z
)
{\\displaystyle {\\frac {\\partial p}{\\partial z}}=-\\rho (x,y,z)g(x,y,z)}

That can be integrated to give another (less-) generalised Stevin's law:
p
(
x
,
y
,
z
)
−
p
0
(
x
,
y
)
\=
−
∫
0
z
ρ
(
x
,
y
,
z
′
)
g
(
x
,
y
,
z
′
)
d
z
′
{\\displaystyle p(x,y,z)-p\_{0}(x,y)=-\\int \_{0}^{z}\\rho (x,y,z')g(x,y,z')dz'}

where:
- p
{\\displaystyle p}

is the hydrostatic pressure (Pa),
- ρ
{\\displaystyle \\rho }

is the fluid [density](https://en.wikipedia.org/wiki/Density "Density") (kg/m3),
- g
{\\displaystyle g}

is [gravitational](https://en.wikipedia.org/wiki/Gravity "Gravity") acceleration (m/s2),
- z
{\\displaystyle z}

is the height (parallel to the direction of gravity) of the test area (m),
- 0
{\\displaystyle 0}

is the height of the [zero reference point of the pressure](https://en.wikipedia.org/wiki/Pressure_measurement#Absolute,_gauge_and_differential_pressures_%E2%80%94_zero_reference "Pressure measurement") (m)
- p
0
{\\displaystyle p\_{0}}

is the hydrostatic pressure field (Pa) along x and y at the zero reference point
### Simplification for liquids
\[[edit](https://en.wikipedia.org/w/index.php?title=Hydrostatic_pressure&action=edit§ion=3 "Edit section: Simplification for liquids")\]
For water and other liquids, this integral can be simplified significantly for many practical applications, based on the following two assumptions. Since many liquids can be considered [incompressible](https://en.wikipedia.org/wiki/Incompressible_flow "Incompressible flow"), a reasonable good estimation can be made from assuming a constant density throughout the liquid. The same assumption cannot be made within a gaseous environment. Also, since the height Δ z {\\displaystyle \\Delta z}  of the fluid column between z and *z*0 is often reasonably small compared to the radius of the Earth, one can neglect the variation of [g](https://en.wikipedia.org/wiki/Gravity "Gravity"). Under these circumstances, one can transport out of the integral the density and the gravity acceleration and the law is simplified into the formula
Δ
p
(
z
)
\=
ρ
g
Δ
z
,
{\\displaystyle \\Delta p(z)=\\rho g\\Delta z,}

where Δ z {\\displaystyle \\Delta z}  is the height *z* − *z*0 of the liquid column between the test volume and the zero reference point of the pressure. This formula is often called [Stevin's](https://en.wikipedia.org/wiki/Simon_Stevin "Simon Stevin") law.[\[1\]](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_note-1)[\[2\]](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_note-2) One could arrive to the above formula also by considering the first particular case of the equation for a conservative body force field: in fact the body force field of uniform intensity and direction:
ρ
g
(
x
,
y
,
z
)
\=
−
ρ
g
k
^
{\\displaystyle \\rho \\mathbf {g} (x,y,z)=-\\rho g{\\hat {k}}}

is conservative, so one can write the body force density as:
ρ
g
\=
∇
(
−
ρ
g
z
)
{\\displaystyle \\rho \\mathbf {g} =\\nabla (-\\rho gz)}

Then the body force density has a simple [scalar potential](https://en.wikipedia.org/wiki/Scalar_potential "Scalar potential"):
ϕ
(
z
)
\=
−
ρ
g
z
{\\displaystyle \\phi (z)=-\\rho gz}

And the pressure difference follows another time the Stevin's law:
Δ
p
\=
−
Δ
ϕ
\=
ρ
g
Δ
z
{\\displaystyle \\Delta p=-\\Delta \\phi =\\rho g\\Delta z}

The reference point should lie at or below the surface of the liquid. Otherwise, one has to split the integral into two (or more) terms with the constant *ρ*liquid and *ρ*(*z*′)above. For example, the [absolute pressure](https://en.wikipedia.org/wiki/Pressure_measurement#Absolute,_gauge_and_differential_pressures_-_zero_reference "Pressure measurement") compared to vacuum is
p
\=
ρ
g
Δ
z
\+
p
0
,
{\\displaystyle p=\\rho g\\Delta z+p\_{\\mathrm {0} },}

where Δ z {\\displaystyle \\Delta z}  is the total height of the liquid column above the test area to the surface, and *p*0 is the [atmospheric pressure](https://en.wikipedia.org/wiki/Atmospheric_pressure "Atmospheric pressure"), i.e., the pressure calculated from the remaining integral over the air column from the liquid surface to infinity. This can easily be visualized using a [pressure prism](https://en.wikipedia.org/wiki/Pressure_prism "Pressure prism").
## Applications
\[[edit](https://en.wikipedia.org/w/index.php?title=Hydrostatic_pressure&action=edit§ion=4 "Edit section: Applications")\]
Hydrostatic pressure has been used in the preservation of foods in a process called [pascalization](https://en.wikipedia.org/wiki/Pascalization "Pascalization").[\[3\]](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_note-3)
### Medicine
\[[edit](https://en.wikipedia.org/w/index.php?title=Hydrostatic_pressure&action=edit§ion=5 "Edit section: Medicine")\]
In medicine, hydrostatic pressure in [blood vessels](https://en.wikipedia.org/wiki/Blood_vessel "Blood vessel") is the pressure of the blood against the wall. It is the opposing force to [oncotic pressure](https://en.wikipedia.org/wiki/Oncotic_pressure "Oncotic pressure"). In capillaries, hydrostatic pressure (also known as capillary blood pressure) is higher than the opposing “colloid [osmotic pressure](https://en.wikipedia.org/wiki/Osmotic_pressure "Osmotic pressure")” in blood—a “constant” pressure primarily produced by circulating albumin—at the arteriolar end of the capillary. This pressure forces plasma and nutrients out of the capillaries and into surrounding tissues. Fluid and the cellular wastes in the tissues enter the capillaries at the venule end, where the hydrostatic pressure is less than the osmotic pressure in the vessel.[\[4\]](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_note-Openstax_Anatomy_&_Physiology_attribution-4)
### Atmospheric pressure
\[[edit](https://en.wikipedia.org/w/index.php?title=Hydrostatic_pressure&action=edit§ion=6 "Edit section: Atmospheric pressure")\]
[Statistical mechanics](https://en.wikipedia.org/wiki/Statistical_mechanics "Statistical mechanics") shows that, for a pure [ideal gas](https://en.wikipedia.org/wiki/Ideal_gas "Ideal gas") of constant temperature *T* in the earth gravitational field, its pressure, *p* will vary with height, *h*, as
p
(
h
)
\=
p
(
0
)
e
−
M
g
h
k
T
{\\displaystyle p(h)=p(0)e^{-{\\frac {Mgh}{kT}}}}

where
- g is the [acceleration due to gravity](https://en.wikipedia.org/wiki/Standard_gravity "Standard gravity")
- T is the [absolute temperature](https://en.wikipedia.org/wiki/Absolute_temperature "Absolute temperature")
- k is [Boltzmann constant](https://en.wikipedia.org/wiki/Boltzmann_constant "Boltzmann constant")
- M is the [molecular mass](https://en.wikipedia.org/wiki/Molecular_mass "Molecular mass") of the gas
- p is the pressure
- h is the height
This is known as the [barometric formula](https://en.wikipedia.org/wiki/Barometric_formula "Barometric formula"), and may be derived from assuming the pressure is [hydrostatic]().
If there are multiple types of molecules in the gas, the [partial pressure](https://en.wikipedia.org/wiki/Partial_pressure "Partial pressure") of each type will be given by this equation. Under most conditions, the distribution of each species of gas is independent of the other species.
## Buoyancy
\[[edit](https://en.wikipedia.org/w/index.php?title=Hydrostatic_pressure&action=edit§ion=7 "Edit section: Buoyancy")\]
Main article: [Buoyancy](https://en.wikipedia.org/wiki/Buoyancy "Buoyancy")
Any body of arbitrary shape which is immersed, partly or fully, in a fluid will experience the action of a net force in the opposite direction of the local pressure gradient. If this pressure gradient arises from gravity, the net force is in the vertical direction opposite that of the gravitational force. This vertical force is termed buoyancy or buoyant force and is equal in magnitude, but opposite in direction, to the weight of the displaced fluid. Mathematically,
F
\=
ρ
g
V
{\\displaystyle F=\\rho gV}

where ρ is the density of the fluid, g is the acceleration due to gravity, and V is the volume of fluid directly above the curved surface.[\[5\]](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_note-F-M-5) In the case of a [ship](https://en.wikipedia.org/wiki/Ship "Ship"), for instance, its weight is balanced by pressure forces from the surrounding water, allowing it to float. If more cargo is loaded onto the ship, it would sink more into the water – displacing more water and thus receive a higher buoyant force to balance the increased weight.\[*[citation needed](https://en.wikipedia.org/wiki/Wikipedia:Citation_needed "Wikipedia:Citation needed")*\]
Discovery of the principle of buoyancy is attributed to [Archimedes](https://en.wikipedia.org/wiki/Archimedes "Archimedes").
### Hydrostatic force on submerged surfaces
\[[edit](https://en.wikipedia.org/w/index.php?title=Hydrostatic_pressure&action=edit§ion=8 "Edit section: Hydrostatic force on submerged surfaces")\]
The horizontal and vertical components of the hydrostatic force acting on a submerged surface are given by the following formula:[\[5\]](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_note-F-M-5)
F
h
\=
p
c
A
F
v
\=
ρ
g
V
{\\displaystyle {\\begin{aligned}F\_{\\mathrm {h} }&=p\_{\\mathrm {c} }A\\\\F\_{\\mathrm {v} }&=\\rho gV\\end{aligned}}}

where
- *p*c is the pressure at the centroid of the vertical projection of the submerged surface
- A is the area of the same vertical projection of the surface
- ρ is the density of the fluid
- g is the acceleration due to gravity
- V is the volume of fluid directly above the curved surface
## See also
\[[edit](https://en.wikipedia.org/w/index.php?title=Hydrostatic_pressure&action=edit§ion=9 "Edit section: See also")\]
- [Hydrostatics](https://en.wikipedia.org/wiki/Hydrostatics "Hydrostatics")
- [Vertical pressure variation](https://en.wikipedia.org/wiki/Vertical_pressure_variation "Vertical pressure variation")
## References
\[[edit](https://en.wikipedia.org/w/index.php?title=Hydrostatic_pressure&action=edit§ion=10 "Edit section: References")\]
1. **[^](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_ref-1)**
Bettini, Alessandro (2016). *A Course in Classical Physics 2—Fluids and Thermodynamics*. Springer. p. 8. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)")
[978-3-319-30685-8](https://en.wikipedia.org/wiki/Special:BookSources/978-3-319-30685-8 "Special:BookSources/978-3-319-30685-8")
.
2. **[^](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_ref-2)**
Mauri, Roberto (8 April 2015). [*Transport Phenomena in Multiphase Flow*](https://books.google.com/books?id=S3L0BwAAQBAJ&pg=PA24). Springer. p. 24. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)")
[978-3-319-15792-4](https://en.wikipedia.org/wiki/Special:BookSources/978-3-319-15792-4 "Special:BookSources/978-3-319-15792-4")
. Retrieved 3 February 2017.
3. **[^](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_ref-3)**
Brown, Amy Christian (2007). [*Understanding Food: Principles and Preparation*](https://books.google.com/books?id=edPzm5KSMmYC) (3 ed.). Cengage Learning. p. 546. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)")
[978-0-495-10745-3](https://en.wikipedia.org/wiki/Special:BookSources/978-0-495-10745-3 "Special:BookSources/978-0-495-10745-3")
.
4. **[^](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_ref-Openstax_Anatomy_&_Physiology_attribution_4-0)**
*[](https://creativecommons.org/licenses/by/4.0/ "creativecommons:by/4.0/") This article incorporates [text](https://openstax.org/books/anatomy-and-physiology/pages/26-1-body-fluids-and-fluid-compartments) available under the [CC BY 4.0](https://creativecommons.org/licenses/by/4.0/ "creativecommons:by/4.0/") license.*
Betts, J Gordon; Desaix, Peter; Johnson, Eddie; Johnson, Jody E; Korol, Oksana; Kruse, Dean; Poe, Brandon; Wise, James; Womble, Mark D; Young, Kelly A (September 16, 2023). *Anatomy & Physiology*. Houston: OpenStax CNX. 26.1 Body fluids and fluid compartments. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)")
[978-1-947172-04-3](https://en.wikipedia.org/wiki/Special:BookSources/978-1-947172-04-3 "Special:BookSources/978-1-947172-04-3")
.
5. ^ [***a***](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_ref-F-M_5-0) [***b***](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_ref-F-M_5-1)
Fox, Robert; McDonald, Alan; Pritchard, Philip (2012). *Fluid Mechanics* (8 ed.). [John Wiley & Sons](https://en.wikipedia.org/wiki/John_Wiley_%26_Sons "John Wiley & Sons"). pp. 76–83\. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)")
[978-1-118-02641-0](https://en.wikipedia.org/wiki/Special:BookSources/978-1-118-02641-0 "Special:BookSources/978-1-118-02641-0")
.

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Hydrostatic pressure
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[Add topic](https://en.wikipedia.org/wiki/Hydrostatic_pressure) |
| Readable Markdown | From Wikipedia, the free encyclopedia
**Hydrostatic pressure** is the [static pressure](https://en.wikipedia.org/wiki/Static_pressure "Static pressure") exerted at a point of interest by the [weight](https://en.wikipedia.org/wiki/Weight "Weight") of a [fluid](https://en.wikipedia.org/wiki/Fluid "Fluid") column above the point.
Due to the fundamental nature of fluids, a fluid cannot remain at rest under the presence of a [shear stress](https://en.wikipedia.org/wiki/Shear_stress "Shear stress"). However, fluids can exert [pressure](https://en.wikipedia.org/wiki/Pressure "Pressure") [normal](https://en.wikipedia.org/wiki/Surface_normal "Surface normal") to any contacting surface. If a point in the fluid is thought of as an infinitesimally small cube, then it follows from the principles of equilibrium that the pressure on every side of this unit of fluid must be equal. If this were not the case, the fluid would move in the direction of the resulting force. Thus, the [pressure](https://en.wikipedia.org/wiki/Fluid_pressure "Fluid pressure") on a fluid at rest is [isotropic](https://en.wikipedia.org/wiki/Isotropic "Isotropic"); i.e., it acts with equal magnitude in all directions. This characteristic allows fluids to transmit force through the length of pipes or tubes; i.e., a force applied to a fluid in a pipe is transmitted, via the fluid, to the other end of the pipe. This principle was first formulated, in a slightly extended form, by [Blaise Pascal](https://en.wikipedia.org/wiki/Blaise_Pascal "Blaise Pascal"), and is now called [Pascal's law](https://en.wikipedia.org/wiki/Pascal%27s_law "Pascal's law").\[*[citation needed](https://en.wikipedia.org/wiki/Wikipedia:Citation_needed "Wikipedia:Citation needed")*\]
In a fluid at rest, all frictional and inertial stresses vanish and the state of stress of the system is called *hydrostatic*. When this condition of *V* = 0 is applied to the [Navier–Stokes equations](https://en.wikipedia.org/wiki/Navier%E2%80%93Stokes_equations "Navier–Stokes equations") for viscous fluids or [Euler equations (fluid dynamics)](https://en.wikipedia.org/wiki/Euler_equations_\(fluid_dynamics\) "Euler equations (fluid dynamics)") for ideal inviscid fluid, the gradient of pressure becomes a function of body forces only. The Navier-Stokes momentum equations are:
**Navier–Stokes momentum equation** (*convective form*)
![{\\displaystyle \\rho {\\frac {\\mathrm {D} \\mathbf {u} }{\\mathrm {D} t}}=-\\nabla \[p-\\zeta (\\nabla \\cdot \\mathbf {u} )\]+\\nabla \\cdot \\left\\{\\mu \\left\[\\nabla \\mathbf {u} +(\\nabla \\mathbf {u} )^{\\mathrm {T} }-{\\tfrac {2}{3}}(\\nabla \\cdot \\mathbf {u} )\\mathbf {I} \\right\]\\right\\}+\\rho \\mathbf {g} .}](https://wikimedia.org/api/rest_v1/media/math/render/svg/6fd98d1bcacc93a84fa4fc981a05a200e680be04)
By setting the [flow velocity](https://en.wikipedia.org/wiki/Flow_velocity "Flow velocity") :, they become simply:

or:

This is the general form of Stevin's law: the [pressure gradient](https://en.wikipedia.org/wiki/Pressure_gradient "Pressure gradient") equals the [body force](https://en.wikipedia.org/wiki/Body_force "Body force") [force density](https://en.wikipedia.org/wiki/Force_density "Force density") field.
Let us now consider two particular cases of this law. In case of a [conservative](https://en.wikipedia.org/wiki/Conservative_force "Conservative force") body force with [scalar potential](https://en.wikipedia.org/wiki/Scalar_potential "Scalar potential") ::

the Stevin equation becomes:

That can be integrated to give:

So in this case the pressure difference is the opposite of the difference of the scalar potential associated to the body force. In the other particular case of a body force of constant direction along z:

the generalised Stevin's law above becomes:

That can be integrated to give another (less-) generalised Stevin's law:

where:
### Simplification for liquids
\[[edit](https://en.wikipedia.org/w/index.php?title=Hydrostatic_pressure&action=edit§ion=3 "Edit section: Simplification for liquids")\]
For water and other liquids, this integral can be simplified significantly for many practical applications, based on the following two assumptions. Since many liquids can be considered [incompressible](https://en.wikipedia.org/wiki/Incompressible_flow "Incompressible flow"), a reasonable good estimation can be made from assuming a constant density throughout the liquid. The same assumption cannot be made within a gaseous environment. Also, since the height  of the fluid column between z and *z*0 is often reasonably small compared to the radius of the Earth, one can neglect the variation of [g](https://en.wikipedia.org/wiki/Gravity "Gravity"). Under these circumstances, one can transport out of the integral the density and the gravity acceleration and the law is simplified into the formula

where  is the height *z* − *z*0 of the liquid column between the test volume and the zero reference point of the pressure. This formula is often called [Stevin's](https://en.wikipedia.org/wiki/Simon_Stevin "Simon Stevin") law.[\[1\]](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_note-1)[\[2\]](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_note-2) One could arrive to the above formula also by considering the first particular case of the equation for a conservative body force field: in fact the body force field of uniform intensity and direction:

is conservative, so one can write the body force density as:

Then the body force density has a simple [scalar potential](https://en.wikipedia.org/wiki/Scalar_potential "Scalar potential"):

And the pressure difference follows another time the Stevin's law:

The reference point should lie at or below the surface of the liquid. Otherwise, one has to split the integral into two (or more) terms with the constant *ρ*liquid and *ρ*(*z*′)above. For example, the [absolute pressure](https://en.wikipedia.org/wiki/Pressure_measurement#Absolute,_gauge_and_differential_pressures_-_zero_reference "Pressure measurement") compared to vacuum is

where  is the total height of the liquid column above the test area to the surface, and *p*0 is the [atmospheric pressure](https://en.wikipedia.org/wiki/Atmospheric_pressure "Atmospheric pressure"), i.e., the pressure calculated from the remaining integral over the air column from the liquid surface to infinity. This can easily be visualized using a [pressure prism](https://en.wikipedia.org/wiki/Pressure_prism "Pressure prism").
Hydrostatic pressure has been used in the preservation of foods in a process called [pascalization](https://en.wikipedia.org/wiki/Pascalization "Pascalization").[\[3\]](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_note-3)
In medicine, hydrostatic pressure in [blood vessels](https://en.wikipedia.org/wiki/Blood_vessel "Blood vessel") is the pressure of the blood against the wall. It is the opposing force to [oncotic pressure](https://en.wikipedia.org/wiki/Oncotic_pressure "Oncotic pressure"). In capillaries, hydrostatic pressure (also known as capillary blood pressure) is higher than the opposing “colloid [osmotic pressure](https://en.wikipedia.org/wiki/Osmotic_pressure "Osmotic pressure")” in blood—a “constant” pressure primarily produced by circulating albumin—at the arteriolar end of the capillary. This pressure forces plasma and nutrients out of the capillaries and into surrounding tissues. Fluid and the cellular wastes in the tissues enter the capillaries at the venule end, where the hydrostatic pressure is less than the osmotic pressure in the vessel.[\[4\]](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_note-Openstax_Anatomy_&_Physiology_attribution-4)
### Atmospheric pressure
\[[edit](https://en.wikipedia.org/w/index.php?title=Hydrostatic_pressure&action=edit§ion=6 "Edit section: Atmospheric pressure")\]
[Statistical mechanics](https://en.wikipedia.org/wiki/Statistical_mechanics "Statistical mechanics") shows that, for a pure [ideal gas](https://en.wikipedia.org/wiki/Ideal_gas "Ideal gas") of constant temperature *T* in the earth gravitational field, its pressure, *p* will vary with height, *h*, as

where
- g is the [acceleration due to gravity](https://en.wikipedia.org/wiki/Standard_gravity "Standard gravity")
- T is the [absolute temperature](https://en.wikipedia.org/wiki/Absolute_temperature "Absolute temperature")
- k is [Boltzmann constant](https://en.wikipedia.org/wiki/Boltzmann_constant "Boltzmann constant")
- M is the [molecular mass](https://en.wikipedia.org/wiki/Molecular_mass "Molecular mass") of the gas
- p is the pressure
- h is the height
This is known as the [barometric formula](https://en.wikipedia.org/wiki/Barometric_formula "Barometric formula"), and may be derived from assuming the pressure is [hydrostatic]().
If there are multiple types of molecules in the gas, the [partial pressure](https://en.wikipedia.org/wiki/Partial_pressure "Partial pressure") of each type will be given by this equation. Under most conditions, the distribution of each species of gas is independent of the other species.
Any body of arbitrary shape which is immersed, partly or fully, in a fluid will experience the action of a net force in the opposite direction of the local pressure gradient. If this pressure gradient arises from gravity, the net force is in the vertical direction opposite that of the gravitational force. This vertical force is termed buoyancy or buoyant force and is equal in magnitude, but opposite in direction, to the weight of the displaced fluid. Mathematically,

where ρ is the density of the fluid, g is the acceleration due to gravity, and V is the volume of fluid directly above the curved surface.[\[5\]](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_note-F-M-5) In the case of a [ship](https://en.wikipedia.org/wiki/Ship "Ship"), for instance, its weight is balanced by pressure forces from the surrounding water, allowing it to float. If more cargo is loaded onto the ship, it would sink more into the water – displacing more water and thus receive a higher buoyant force to balance the increased weight.\[*[citation needed](https://en.wikipedia.org/wiki/Wikipedia:Citation_needed "Wikipedia:Citation needed")*\]
Discovery of the principle of buoyancy is attributed to [Archimedes](https://en.wikipedia.org/wiki/Archimedes "Archimedes").
### Hydrostatic force on submerged surfaces
\[[edit](https://en.wikipedia.org/w/index.php?title=Hydrostatic_pressure&action=edit§ion=8 "Edit section: Hydrostatic force on submerged surfaces")\]
The horizontal and vertical components of the hydrostatic force acting on a submerged surface are given by the following formula:[\[5\]](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_note-F-M-5)

where
- *p*c is the pressure at the centroid of the vertical projection of the submerged surface
- A is the area of the same vertical projection of the surface
- ρ is the density of the fluid
- g is the acceleration due to gravity
- V is the volume of fluid directly above the curved surface
- [Hydrostatics](https://en.wikipedia.org/wiki/Hydrostatics "Hydrostatics")
- [Vertical pressure variation](https://en.wikipedia.org/wiki/Vertical_pressure_variation "Vertical pressure variation")
1. **[^](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_ref-1)**
Bettini, Alessandro (2016). *A Course in Classical Physics 2—Fluids and Thermodynamics*. Springer. p. 8. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)")
[978-3-319-30685-8](https://en.wikipedia.org/wiki/Special:BookSources/978-3-319-30685-8 "Special:BookSources/978-3-319-30685-8")
.
2. **[^](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_ref-2)**
Mauri, Roberto (8 April 2015). [*Transport Phenomena in Multiphase Flow*](https://books.google.com/books?id=S3L0BwAAQBAJ&pg=PA24). Springer. p. 24. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)")
[978-3-319-15792-4](https://en.wikipedia.org/wiki/Special:BookSources/978-3-319-15792-4 "Special:BookSources/978-3-319-15792-4")
. Retrieved 3 February 2017.
3. **[^](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_ref-3)**
Brown, Amy Christian (2007). [*Understanding Food: Principles and Preparation*](https://books.google.com/books?id=edPzm5KSMmYC) (3 ed.). Cengage Learning. p. 546. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)")
[978-0-495-10745-3](https://en.wikipedia.org/wiki/Special:BookSources/978-0-495-10745-3 "Special:BookSources/978-0-495-10745-3")
.
4. **[^](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_ref-Openstax_Anatomy_&_Physiology_attribution_4-0)**
*[](https://creativecommons.org/licenses/by/4.0/ "creativecommons:by/4.0/") This article incorporates [text](https://openstax.org/books/anatomy-and-physiology/pages/26-1-body-fluids-and-fluid-compartments) available under the [CC BY 4.0](https://creativecommons.org/licenses/by/4.0/ "creativecommons:by/4.0/") license.*
Betts, J Gordon; Desaix, Peter; Johnson, Eddie; Johnson, Jody E; Korol, Oksana; Kruse, Dean; Poe, Brandon; Wise, James; Womble, Mark D; Young, Kelly A (September 16, 2023). *Anatomy & Physiology*. Houston: OpenStax CNX. 26.1 Body fluids and fluid compartments. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)")
[978-1-947172-04-3](https://en.wikipedia.org/wiki/Special:BookSources/978-1-947172-04-3 "Special:BookSources/978-1-947172-04-3")
.
5. ^ [***a***](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_ref-F-M_5-0) [***b***](https://en.wikipedia.org/wiki/Hydrostatic_pressure#cite_ref-F-M_5-1)
Fox, Robert; McDonald, Alan; Pritchard, Philip (2012). *Fluid Mechanics* (8 ed.). [John Wiley & Sons](https://en.wikipedia.org/wiki/John_Wiley_%26_Sons "John Wiley & Sons"). pp. 76–83\. [ISBN](https://en.wikipedia.org/wiki/ISBN_\(identifier\) "ISBN (identifier)")
[978-1-118-02641-0](https://en.wikipedia.org/wiki/Special:BookSources/978-1-118-02641-0 "Special:BookSources/978-1-118-02641-0")
. |
| Shard | 152 (laksa) |
| Root Hash | 17790707453426894952 |
| Unparsed URL | org,wikipedia!en,/wiki/Hydrostatic_pressure s443 |