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Bernoulli's Equation

Bernoulli's equation says that in a steady, incompressible, frictionless flow, the sum of pressure, kinetic energy per unit volume, and potential energy per unit volume stays constant along a streamline. In everyday terms: where a fluid speeds up, its pressure drops. For example, air moving over the curved top of an aeroplane wing speeds up, lowering the pressure above the wing and helping to create lift. It is a cornerstone of fluid dynamics and is used in carburettors, Venturi meters, and aerodynamics.

Chemical Process Design Fluid Mechanics
VORZEP · FLUID MECHANICS & ENERGY TOOLS

Bernoulli's Equation Calculator

Solve the classic streamline energy balance P + ½ρv² + ρgh = C for any of its three unknowns — static pressure, flow velocity, or elevation — with step-by-step math, a live pipe schematic, and companion head and energy metrics.

P + ½ · ρ · v² + ρ · g · h = C · static + dynamic + hydrostatic = total
Solve for
Static Pressure (P) The thermodynamic pressure of the fluid at the point of interest — the pressure a gauge or static port would read. Absolute sea-level air is 101,325 Pa; gauge pressures may be negative. In a moving stream this is the pressure perpendicular to the flow, not the stagnation pressure.
Pa
Static pressure must be a finite number.
Flow Velocity (v) The speed of the fluid along the streamline at the point of interest. Typical: 0.5–3 m/s in building pipework, 5–15 m/s in ducts, 20–60 m/s in wind, and 200–300 m/s at an aircraft wing. Above roughly 100 m/s in air (M ≈ 0.3) the incompressible Bernoulli form starts to lose accuracy.
m/s
Velocity must be zero or greater.
Elevation (h) Height of the point above an arbitrary but fixed datum. Only differences in h matter, so the datum can be chosen wherever convenient. Negative values mean the point lies below the datum. For air at sea level, 10 m of elevation is only ~120 Pa; for water it is ~98,000 Pa — which is why elevation dominates in hydraulics and barely matters in low-speed gas flows.
m
Elevation must be a finite number.
kg/m³
Density must be greater than zero.
Pa
Total pressure constant must be a finite number.
STATIC PRESSURE (P)
101,325.0 Pa
101.33 kPa · 1.013 bar · 14.70 psi
FAST FLOW — HIGH-SPEED DUCT / STORM
P = C − ½ρv² − ρgh
Step-by-step solution
Static pressure vs. velocity
Current ρ ρ × 0.8 ρ × 1.2
Static pressure vs. elevation
Current v v × 0.6 v × 1.5
Sensitivity (+1% input)
Companion head & energy metrics
Energy balance along a streamline — live schematic
Static pressure P Dynamic pressure ½ρv² Hydrostatic pressure ρgh
What Bernoulli's equation really measures
Pstatic pressure
+
½ρv²dynamic pressure
+
ρghhydrostatic pressure
=
Ctotal pressure

It is an energy budget, not a force balance

Each term in Bernoulli's equation has units of pressure (Pa = J/m³), so the equation is really a statement of energy conservation per unit volume. Static pressure is flow work, ½ρv² is kinetic energy density, and ρgh is gravitational potential energy density. Along a streamline in steady, incompressible, inviscid flow their sum is constant — energy can move between the three buckets but the total cannot change.

Faster flow means lower static pressure

If elevation is constant, C = P + ½ρv², so any increase in velocity must be paid for by a drop in static pressure. This is the Venturi effect and the reason a carburettor, a spray gun, and an airliner's wing all work. Doubling velocity quadruples the dynamic pressure term, so the static pressure penalty grows fast — at 100 m/s in sea-level air the dynamic pressure is already 6,125 Pa, about 6% of atmospheric pressure.

Elevation matters enormously in liquids, barely in gases

The hydrostatic term ρgh scales with density. Ten metres of elevation costs 98,000 Pa in water — nearly a full atmosphere — but only 120 Pa in air. That is why hydraulic engineers think in metres of head and aerodynamicists ignore elevation altogether. In gas flows at low Mach number, the ρgh term is usually dropped, giving the familiar P + ½ρv² = constant.

It fails where friction and turbulence live

Bernoulli's equation holds strictly only for steady, incompressible, inviscid flow along a streamline. Real flows have viscosity, so mechanical energy is converted to heat and total pressure falls in the direction of flow. Pumps add energy and turbines remove it. The extended form P₁ + ½ρv₁² + ρgh₁ + w_pump = P₂ + ½ρv₂² + ρgh₂ + losses is what engineers actually use for pipe networks.

How to Use This Calculator

Bernoulli's equation links three quantities at a point on a streamline: static pressure P, velocity v, and elevation h — tied together by the constant total pressure C and the fluid density ρ.

1. Choose what to solve for

Pick P, v, or h from the toggle. The calculator rearranges P + ½ρv² + ρgh = C automatically for whichever variable you choose.

2. Set the fluid density

Use the density presets — helium, air at two densities, fresh water, seawater, mercury — or type your own value. Density scales the dynamic and hydrostatic terms directly.

3. Supply the total pressure constant C

C is the conserved total pressure. If you know the conditions at a reference station, compute C there (P + ½ρv² + ρgh) and enter it here. The "Demo" preset reproduces the default air case.

4. Read the result and verdict

The result card shows the solved value in SI plus the equivalent in kPa, bar and psi (for pressure) or km/h, knots and ft/s (for velocity). A colour-coded verdict classifies the flow speed.

5. Check the pressure budget and schematic

The pressure-budget bars show how much of the total pressure is static, dynamic and hydrostatic. The schematic shows the pipe, the flow arrows, the pressure arrows, and the elevation above datum.

6. Switch to Advanced for depth

Advanced mode adds a P-vs-h chart, a +1% sensitivity check on every input, and companion metrics including velocity head, pressure head, total head, stagnation pressure and Mach number.

What This Tool Offers

Built around the classic streamline energy balance P + ½ρv² + ρgh = C, the fundamental link between pressure, speed, and height in a moving fluid.

Three-way solving

Solve for static pressure, flow velocity, or elevation. The calculator rearranges Bernoulli's equation for whichever variable you choose.

Live streamline schematic

A datum-referenced pipe diagram with flow arrows scaled to velocity, pressure arrows scaled to static pressure, and a dimension line scaled to elevation.

Pressure budget bars

See at a glance how the total pressure splits between static, dynamic and hydrostatic contributions — and how that split changes as you drag the sliders.

Flow-regime verdict

Each result is classified from fluid at rest through creeping, slow, moderate, fast, and high-speed flow, with a note when compressibility starts to matter.

Multi-unit hints

Each field shows the value converted to related units — kPa, bar and psi for pressure; km/h, knots and ft/s for velocity; feet for elevation.

Reference tables

A pressure unit converter, a dynamic-pressure lookup grid across five densities, typical Bernoulli values by situation, and a full variable reference table.

Reference Tables & Conversions

A pressure unit converter, a dynamic-pressure lookup grid, typical values by situation, and the full variable list.

Pressure unit converter

Pa
kPa
bar
psi
atm
m H₂O
= 101,325 Pa = 101.325 kPa = 1.01325 bar = 14.6959 psi = 1 atm

Dynamic Pressure ½ρv² Lookup

Dynamic pressure in pascals for a range of velocities and fluid densities. Computed from q = ½ρv².

Velocity (m/s)Helium 0.166Air 1.000Air 1.225Water 998Seawater 1025

Typical Bernoulli Values by Situation

Representative values for the three terms and the resulting total pressure constant. g = 9.80665 m/s².

Situationρ (kg/m³)v (m/s)h (m)P (Pa)½ρv² (Pa)ρgh (Pa)C (Pa)

Variable Reference

SymbolMeaningTypical rangeUnits
PStatic pressure0 – 10⁷Pa
vFlow velocity along the streamline0 – 300m/s
hElevation above datum−100 – 10 000m
ρFluid density0.09 (H₂) – 13 546 (Hg)kg/m³
gGravitational acceleration9.780 – 9.832m/s²
CTotal pressure constant (stagnation pressure when h is constant)depends on casePa
qDynamic pressure ½ρv²0 – 10⁶Pa
v²/2gVelocity head0 – 5000m
P/ρgPressure head0 – 1000m

What Does P + ½ρv² + ρgh = C Measure?

Bernoulli's equation is the statement of mechanical energy conservation for a fluid element moving along a streamline. It says that the sum of three energy densities — the static pressure P, the kinetic energy density ½ρv², and the gravitational potential energy density ρgh — stays constant as the element moves, provided the flow is steady, incompressible, and inviscid. It is one of the oldest results in fluid mechanics, published by Daniel Bernoulli in 1738, and it remains the single most useful shortcut in the subject.

Bernoulli's Equation Formula

The defining relationship between two points on the same streamline is:

P₁ + ½ρv₁² + ρgh₁ = P₂ + ½ρv₂² + ρgh₂ = C

For a single point, written with the constant on the right:

P + ½ρv² + ρgh = C

Rearranged to solve for each of the three unknowns:

P = C − ½ρv² − ρgh
v = √( 2 · (C − P − ρgh) / ρ )
h = (C − P − ½ρv²) / (ρg)

Dividing every term by ρg turns the equation into the head form used by hydraulic engineers:

P/(ρg) + v²/(2g) + h = H   (pressure head + velocity head + elevation head = total head)

Bernoulli Variables

SymbolMeaningNotes
PStatic pressurePressure perpendicular to the flow direction
½ρv²Dynamic pressureKinetic energy per unit volume; grows with v²
ρghHydrostatic pressureGravitational potential energy per unit volume
CTotal pressure constantConserved along a streamline in ideal flow
ρFluid densityAssumed constant (incompressible)
gGravitational acceleration9.80665 m/s² standard
hElevationMeasured from an arbitrary but fixed datum

How Each Variable Affects the Result

Because velocity enters the equation squared, it is by far the most powerful lever on static pressure. Doubling the flow speed quadruples the dynamic pressure term, so the static pressure must fall by four times as much. Density works the same way on both the dynamic and hydrostatic terms: switching from air to water multiplies both by roughly 800, which is why pressure changes in liquid systems are so much larger than in gas systems at the same speed.

Elevation is the slow, linear variable. In air the hydrostatic term is almost always negligible — climbing 100 m costs only about 1.2 kPa, roughly 1% of atmospheric pressure. In water the same 100 m costs about 980 kPa, ten atmospheres. That asymmetry is why the same equation serves both the aerodynamicist analysing a wing and the civil engineer designing a water tower.

The constant C is what makes the equation usable. If you can measure or compute the three terms at any single point on a streamline, you have C, and you can then find any one of the three terms at any other point on that same streamline. This is exactly how a Pitot-static tube works: it measures the stagnation pressure (where v = 0, so C = P + ρgh) and the static pressure at the same height, and their difference gives the dynamic pressure, and hence the airspeed.

Bernoulli Calculation Examples

Given: C = 102,976.38 Pa, ρ = 1.225 kg/m³, v = 50 m/s, h = 10 m — solve for P
P = C − ½ρv² − ρgh = 102,976.38 − 1,531.25 − 120.13 = 101,325.0 Pa
Given: C = 102,976.38 Pa, ρ = 1.225 kg/m³, P = 101,325 Pa, h = 10 m — solve for v
v = √( 2 · (102,976.38 − 101,325 − 120.13) / 1.225 ) = √(2 · 1,531.25 / 1.225) = 50.00 m/s
Given: C = 102,976.38 Pa, ρ = 1.225 kg/m³, P = 101,325 Pa, v = 50 m/s — solve for h
h = (102,976.38 − 101,325 − 1,531.25) / (1.225 × 9.80665) = 10.00 m
Given: air at 101,325 Pa moving at 80 m/s, level flight — solve for stagnation pressure
P₀ = P + ½ρv² = 101,325 + ½ × 1.225 × 80² = 101,325 + 3,920 = 105,245 Pa

Frequently Asked Questions

Four assumptions must hold for the simple form P + ½ρv² + ρgh = C to be valid: the flow must be steady (no change with time at a fixed point), incompressible (density constant), inviscid (no viscosity, hence no friction), and it must be applied along a single streamline (or in irrotational flow, where the constant is the same everywhere). Real flows violate at least the inviscid assumption, which is why the extended form with a loss term is used for pipe networks. For air below about Mach 0.3 the incompressible assumption is good to within 5%.

Because the total energy along the streamline is fixed. If the fluid speeds up, its kinetic energy density ½ρv² rises, and since the sum P + ½ρv² + ρgh must stay constant, the static pressure P must fall by exactly the same amount. Physically, the pressure gradient along the streamline is what accelerates the fluid in the first place — a favourable pressure gradient (pressure decreasing downstream) pushes the fluid forward and speeds it up. This is the principle behind the Venturi meter, the carburettor, the atomiser, and the generation of lift on an aircraft wing.

Whenever the hydrostatic pressure change is small compared with the dynamic and static terms you care about. For air at sea level, ρgh is only about 12 Pa per metre, so a 100 m elevation change contributes roughly 1.2 kPa — often negligible against atmospheric pressure of 101 kPa. For water, ρgh is about 9,800 Pa per metre, so even a 1 m change matters. The rule of thumb: compare ρgh with ½ρv². If ρgh is less than about 5% of the dynamic pressure, you can safely drop it and use P + ½ρv² = constant.

Static pressure P is the pressure the fluid exerts perpendicular to the flow — what a gauge flush with the pipe wall would read. Dynamic pressure q = ½ρv² is not a pressure you can measure directly; it is the kinetic energy per unit volume, expressed in pressure units. Stagnation pressure (also called total pressure) is what you measure at a point where the flow has been brought to rest isentropically, and it equals P + ½ρv² = P + q. A Pitot-static tube measures both static and stagnation pressure, and the difference between them is the dynamic pressure, which gives the airspeed. Note that in this calculator C is the total pressure including the elevation term, so C = P + q + ρgh.

Only partly, and the popular "equal transit time" story is wrong. Bernoulli's equation does correctly describe the pressure field around an aerofoil: where the air accelerates over the upper surface, the static pressure drops, and that lower pressure contributes to the lift. But the acceleration is caused by the aerofoil's shape and angle of attack deflecting the flow, and a complete lift explanation requires the circulation and the Kutta condition. The most robust statement is that lift is the reaction to the downward momentum imparted to the air, and the pressure distribution computed from Bernoulli (plus the viscous boundary condition) accounts for that reaction.

Head is energy per unit weight, expressed in metres. Dividing Bernoulli's equation through by ρg turns each term into a length: P/(ρg) is the pressure head (how high the pressure alone would push a column of the fluid), v²/(2g) is the velocity head, and h is the elevation head. Their sum is the total head H. Working in head is convenient because it is independent of the fluid — a pump rated at 30 m of head will lift water 30 m, or mercury 30 m, at the same volumetric flow rate. It also makes the energy bookkeeping visually intuitive: head is literally a height.

Very accurate for streamline-aligned, low-viscosity, low-Mach flows away from walls, and progressively worse as you approach the four assumptions' limits. Viscous losses in a long pipe can consume most of the available pressure, and they grow with the square of velocity and with pipe length. Compressibility becomes significant above roughly Mach 0.3 in air, where the isentropic relations must be used instead. Rotational flow behind a bluff body invalidates the single-streamline constant. In practice, engineers use Bernoulli as the ideal baseline and add a discharge coefficient or a loss coefficient to account for reality — a Venturi meter, for instance, typically discharges at 95–98% of the Bernoulli-predicted value.

Calculating...

Variables

Symbol Quantity Unit
P Pressure Pa
ρ Density kg/m³
v Velocity m/s
g Gravitational acceleration m/s²
h Height m

What it means

Bernoulli’s equation is a statement of conservation of mechanical energy for a fluid flowing along a streamline, assuming steady, incompressible, and inviscid flow. It states that the sum of the pressure energy (P), kinetic energy per unit volume (½ρv²), and potential energy per unit volume (ρgh) is constant. This equation is widely used to analyse fluid flow in pipes, nozzles, venturis, and around airfoils. It explains phenomena such as the lift on an aeroplane wing and the operation of a carburettor. In engineering, it is used to calculate flow rates from pressure measurements (e.g., pitot tubes), to design piping systems, and to estimate pump head requirements. The equation is derived from Newton’s second law and is valid for frictionless flow. In practice, corrections for friction losses (via the Darcy‑Weisbach equation) and minor losses are added. Bernoulli’s equation is a cornerstone of fluid dynamics and is taught in all introductory fluid mechanics courses.

Worked example

Bernoulli's Equation – Two Examples

Real‑World
Scenario: At a pipe point, P = 101,325 Pa, v = 0 m/s, h = 0, ρ = 1.225 kg/m³. Find the Bernoulli constant.
ParameterValue
P101,325 Pa
ρ1.225 kg/m³
v0 m/s
g9.81 m/s²
h0 m
1Constant = P + ½ρv² + ρgh = 101,325 Pa
Result 101,325 Pa ✓ Atmospheric
Scenario: P = 100,000 Pa, v = 20 m/s, ρ = 1.225 kg/m³, h = 0. Determine the constant.
ParameterValue
P100,000 Pa
v20 m/s
ρ1.225 kg/m³
1½ρv² = 0.5×1.225×400 = 245 Pa
2Constant = 100000 + 245 = 100,245 Pa
Result 100,245 Pa ✓ Energy conserved
Key insight: The sum of pressure, kinetic, and potential energy is constant along a streamline.

Common mistakes

  • Assumptions: Bernoulli applies to steady, inviscid, incompressible flow along a streamline. Do not use it for compressible, unsteady, or viscous flows without correction.
  • Units: All terms must have the same units (pressure: Pa, velocity term: Pa, elevation term: Pa). Use consistent units.
  • Reference points: The equation is valid between two points on the same streamline; ensure both points are on the same streamline.
  • Friction losses: For real fluids, add a head loss term; Bernoulli alone is an idealisation.
  • Elevation term: Use the same datum for both points.

Applications

Bernoulli's equation, P + ½ρv² + ρgh = constant, expresses the conservation of mechanical energy along a streamline for steady, inviscid, incompressible flow. It relates pressure, velocity, and elevation, making it a fundamental tool in fluid mechanics. Engineers use it to design piping systems, to measure flow rates using venturi meters and pitot tubes, and to analyse the performance of pumps, turbines, and aircraft wings. In hydraulic engineering, it helps calculate water levels in reservoirs and flow through sluices. The equation also explains phenomena such as the lift on an airfoil (where higher velocity reduces pressure) and the entrainment of air in aspirators. By applying Bernoulli's principle, engineers can predict pressure drops, identify energy losses, and optimise system performance.

  • Design of flow measurement devices (venturi, orifice, pitot tube)
  • Analysis of pipe networks and hydraulic systems
  • Performance prediction of pumps and turbines
  • Aerodynamic design of aircraft wings and vehicle bodies
  • Sizing of nozzles, diffusers, and ejectors