Understanding the Bernoulli Equation
The Bernoulli equation is a statement of energy conservation for a fluid moving along a streamline. For steady, incompressible, frictionless (inviscid) flow, the sum of three pressure terms — static, dynamic, and hydrostatic — stays constant from one point to another, even as the fluid speeds up, slows down, or changes elevation. It explains why fluid pressure drops where it speeds up through a constriction, why an airfoil generates lift, and how a Venturi meter or Pitot tube can measure flow rate from a pressure reading.
The formula
For two points, 1 and 2, along the same streamline:
P₁ + ½ρv₁² + ρgh₁ = P₂ + ½ρv₂² + ρgh₂
- P is the static (absolute) pressure at the point, in pascals.
- ρ (rho) is the fluid density, in kg/m³ — about 1000 for water and 1.2 for air at sea level.
- v is the flow velocity at the point, in m/s. The term ½ρv² is the dynamic pressure.
- g is standard gravity, 9.80665 m/s², and h is elevation, in meters. The term ρgh is the hydrostatic pressure.
How this calculator works
Enter the fluid density and the known pressure, velocity, and elevation at Point 1, plus the velocity and elevation at Point 2. The calculator rearranges the equation above to solve for the unknown pressure at Point 2:
P₂ = P₁ + ½ρ(v₁² − v₂²) + ρg(h₁ − h₂)
It also reports the dynamic pressure change (the effect of the velocity difference alone), the hydrostatic pressure change (the effect of the elevation difference alone), and the Bernoulli constant — the total pressure at Point 1, which should equal the total pressure at Point 2 as a built-in check that energy is conserved between the two points.
Assumptions and limits
This form of the equation assumes steady flow (conditions don't change with time), an incompressible fluid (constant density — a good approximation for liquids and for gases well below the speed of sound), no viscous friction losses along the path, and no pump or turbine adding or removing energy between the two points. Real pipe flow includes friction, which the Darcy-Weisbach or Hazen-Williams equations account for separately as head loss.