quantity

velocity

Rate of change of position of a fluid element, measured along or transverse to flow.
43 related articles · 6 formulas

Description

Velocity in fluid dynamics is the rate of change of position of a fluid element, measured along or transverse to the flow direction. It is a fundamental field variable that describes how fluid particles move through space and time. Understanding velocity is crucial for analyzing fluid behavior, from laminar flows in porous media to turbulent eddies in oceans and atmospheres.

History

The concept of velocity in fluids was formalized by Leonhard Euler in the 18th century, who introduced the idea of a velocity field. Later, Claude-Louis Navier and George Gabriel Stokes developed the equations that bear their names, providing a mathematical framework for velocity in viscous flows.

How it works

Velocity is a vector quantity, meaning it has both magnitude and direction. In fluid dynamics, it is often described by a velocity field, which assigns a velocity vector to every point in the fluid. This field is governed by equations like the Navier-Stokes equations, which relate velocity to pressure, density, and external forces. Measurements of velocity can be made using techniques like particle image velocimetry or Doppler anemometry.

In practice

Velocity measurements are used in weather forecasting to track wind patterns, in oceanography to monitor currents, and in engineering to design pipelines and aircraft.

Fun fact

In turbulent flows, velocity fluctuates chaotically, and even the most powerful supercomputers cannot fully simulate the smallest eddies.

Concept graph →

Formulas

$$v = H d$$
Recessional velocity of galaxies is proportional to their distance.
What is in the formula
vvariableRecessional velocity of a galaxy — velocity metre per second
HvariableHubble parameter (time-dependent) — hubble parameter per second
dvariableProper distance to the galaxy — distance metre
$$\Delta z = \frac{v}{c}$$
Relates redshift to line-of-sight velocity.
What is in the formula
Δzvariableredshift change — redshift
vvariableline-of-sight velocity — velocity metre per second
cvariablespeed of light — speed of light metre per second
$$v^2 = \frac{G M}{r}$$
Orbital speed squared equals gravitational constant times mass over radius.
What is in the formula
vvariableorbital speed — velocity metre per second
Mvariablecentral mass — mass kilogram
rvariableorbital radius — radius metre
GconstantUniversal constant of gravitation, determining the strength of gravitational force. — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared
$$1+z = rac{1}{ rac{ ext{v}}{c} ext{cos} heta ext{ sign} ext{ adjusted}}$$
Redshift due to relative motion between observer and source.
What is in the formula
zvariableredshift parameter — redshift
vvariablerelative velocity between source and observer — velocity metre per second
θvariableangle between velocity vector and line of sight — angle radian
cconstantspeed of light in vacuum — speed of light = 299792458 metre per second
cosoperatortrigonometric cosine function — cosine
$$F = \frac{2 A s}{c} \cdot \frac{1 - v/c}{1 + v/c}$$
Force on a moving solar sail due to reflected light.
What is in the formula
FvariableForce on the sail — force newton
AvariableArea of the sail — area square metre
svariablePoynting flux (power per unit area) of incident light — irradiance watt per square metre
vvariableSpeed of the sail relative to the light source — velocity metre per second
cconstantUniversal constant, speed of light in vacuum — speed of light = 299792458 metre per second
\cdotoperatorProduct of quantities — multiplication
\frac{1 - v/c}{1 + voperatorRatio of reflected to incident photon energy and rate — doppler factor squared
$$\frac{\nu_{\text{out}}}{\nu_{\text{in}}} = \frac{1 - v/c}{1 + v/c}$$
Frequency shift for light reflected from a moving mirror.
What is in the formula
\nu_{\text{out}}variableObserved frequency of reflected light — frequency hertz
\nu_{\text{in}}variableFrequency of incident light in the source frame — frequency hertz
vvariableSpeed of the mirror relative to the source — velocity metre per second
cconstantUniversal constant, speed of light in vacuum — speed of light = 299792458 metre per second
\frac{1 - v/c}{1 + voperatorRatio of observed to emitted frequency for a receding source — doppler factor

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