
The Navier-Stokes equations are partial differential equations that describe the motion of viscous fluid substances in various flow conditions.French engineer Claude-Louis Navier (1821) and British physicist George Stokes (1845) combined into a system equations expressing the conservation of mass and momentum in a viscous fluid. The momentum equation: ρ (∂v/∂t + v·∇v) = -∇p + μ ∇²v + f. The left side is mass times acceleration (including convective transport), the right side includes pressure forces, viscous friction, and external influences. The incompressibility condition ∇·v = 0 is added. Their genius was accounting for internal friction (the term with viscosity μ).
Claude-Louis Navier derived the equations in 1821, introducing a molecular hypothesis about forces between particles. In 1845, George Gabriel Stokes refined the derivation, abandoning molecular notions and formulating the commonly accepted form with a continuum approach. Later, Leonhard Euler derived equations for an ideal (inviscid) fluid, and Navier and Stokes added viscosity.
The equations are the foundation of hydro- and aerodynamics, meteorology, oceanography, astrophysics (accretion disks, interstellar medium). Depending on the Reynolds number, they describe laminar or turbulent flow. Numerical methods of computational fluid dynamics (CFD) allow modeling everything from blood flow to aircraft aerodynamics, but high turbulence requires supercomputers.
Weather forecasts, wing aerodynamics calculations, climate modeling, and ocean current simulations — all are built on these equations.
The Clay Mathematics Institute has announced a $1 million prize for proving that solutions to the equations always exist and do not 'blow up' (remain smooth) in the three-dimensional case — it is one of the Millennium Prize problems.
| y | variable | spatial coordinate perpendicular to flow — position metre |
| V | variable | fluid velocity in the flow direction — velocity metre per second |
| F | variable | body force per unit volume acting on the fluid — force density newton per cubic metre |
| ρ | variable | fluid mass density — mass density kilogram per cubic metre |
| η | constant | dynamic viscosity of the fluid — dynamic viscosity = material-dependent pascal second |
| d/dy | operator | derivative with respect to y — ordinary derivative |
| P | variable | Pressure — pressure pascal |
| r | variable | Radial coordinate — radius metre |
| m | variable | Enclosed mass — mass kilogram |
| ρ | variable | Mass density — mass density kilogram per metre cubed |
| G | constant | Universal gravitational constant — gravitational constant = 6.67430e-11 metre cubed per kilogram per second squared |
| c | constant | Speed of light in vacuum — speed of light = 299792458 metre per second |
| d/dr | operator | Derivative with respect to radial coordinate — derivative with respect to radius |
| P_r | variable | Radial pressure — pressure pascal |
| r | variable | Radial coordinate — radius metre |
| ε | variable | Energy density — energy density joule per cubic metre |
| m | variable | Mass enclosed within radius r — mass kilogram |
| P_t | variable | Tangential pressure — pressure pascal |
| G | constant | Fundamental constant governing gravitational strength — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared |
| c | constant | Universal speed limit for massless particles — speed of light = 299792458 metre per second |
| d/dr | operator | Differentiates a function with respect to r — ordinary derivative |
| P | variable | Pressure at radius r — pressure pascal |
| r | variable | Radial coordinate — radius metre |
| ε | variable | Energy density — energy density joule per cubic metre |
| m | variable | Mass enclosed within radius r — mass kilogram |
| d/dr | operator | Derivative with respect to radial coordinate — ordinary derivative |


















