Mechanical Engineer's Handbook

Bernoulli’s Equation

When a fluid speeds up, its kinetic energy increases. That extra kinetic energy comes from work done by pressure differences and gravity. Bernoulli’s equation is the principle of conservation of energy applied to a moving, ideal fluid.

When fluid flows from a wider pipe into a narrower pipe, it speeds up to maintain a constant flow rate. To accelerate that fluid, a net force must push it forward, meaning the pressure behind the fluid in the wide section is higher than the pressure ahead of it in the narrow section. Higher speed corresponds to lower pressure. Additionally, pumping a fluid upward requires work against gravity, causing pressure to drop with increasing elevation.

Derivation of Bernoulli's Equation from Energy Conservation

Consider a small volume of fluid dVdV with mass dm=ρdVdm = \rho dV moving along a pipe from point 1 (height h1h_1, speed v1v_1, pressure p1p_1) to point 2 (height h2h_2, speed v2v_2, pressure p2p_2).

The net work done on this fluid element by surrounding pressure forces is:

dW=(p1p2)dVdW = (p_1 - p_2) dV

By the work-energy theorem, this work equals the change in kinetic energy plus the change in gravitational potential energy (dW=dK+dUdW = dK + dU):

(p1p2)dV=12(ρdV)(v22v12)+(ρdV)g(h2h1)(p_1 - p_2) dV = \frac{1}{2} (\rho dV) (v_2^2 - v_1^2) + (\rho dV) g (h_2 - h_1)

Dividing the entire equation by dVdV removes volume and yields energy per unit volume:

p1p2=12ρv2212ρv12+ρgh2ρgh1p_1 - p_2 = \frac{1}{2} \rho v_2^2 - \frac{1}{2} \rho v_1^2 + \rho g h_2 - \rho g h_1

Rearranging all point 1 terms to the left and point 2 terms to the right gives Bernoulli's equation:

p1+12ρv12+ρgh1=p2+12ρv22+ρgh2p_1 + \frac{1}{2} \rho v_1^2 + \rho g h_1 = p_2 + \frac{1}{2} \rho v_2^2 + \rho g h_2
(1)

Because points 1 and 2 are arbitrary choices along a path, this total sum remains constant along any streamline:

p+12ρv2+ρgh=constantp + \frac{1}{2} \rho v^2 + \rho g h = \text{constant}
(2)

Each term in Bernoulli's equation represents an energy density with units of Joules per cubic meter, which simplifies directly to Pascals (J/m3=N/m2=Pa\text{J/m}^3 = \text{N/m}^2 = \text{Pa}). The term pp is static pressure, 12ρv2\frac{1}{2} \rho v^2 is dynamic pressure (kinetic energy per unit volume), and ρgh\rho g h is hydrostatic pressure density (potential energy per unit volume).

Special Cases

If the fluid is static (v1=v2=0v_1 = v_2 = 0), the kinetic energy terms drop out, leaving p1+ρgh1=p2+ρgh2p_1 + \rho g h_1 = p_2 + \rho g h_2. Setting h1h2=hh_1 - h_2 = h reproduces the hydrostatic pressure formula p2=p1+ρghp_2 = p_1 + \rho g h.

If fluid flows horizontally without changing elevation (h1=h2h_1 = h_2), potential energy terms cancel, leaving Bernoulli's principle:

p1+12ρv12=p2+12ρv22p_1 + \frac{1}{2} \rho v_1^2 = p_2 + \frac{1}{2} \rho v_2^2
(3)

This equation shows that as fluid speed increases, static pressure decreases. If v2>v1v_2 > v_1, then p2p_2 must be less than p1p_1 for the sum to remain equal.

Applications

Entrainment occurs when a fluid moves rapidly through a narrow opening, dropping its pressure below atmospheric pressure and drawing surrounding fluid into the stream. Atomizers, carburetors, aspirators, and Bunsen burners rely on this effect.

Velocity measurement devices like Pitot-Prandtl tubes measure aircraft speed by bringing oncoming fluid to a complete stop at an opening (v1=0v_1 = 0). Comparing this stagnation pressure p1p_1 to static pressure p2p_2 from a side opening allows calculation of airspeed via vp1p2v \propto \sqrt{p_1 - p_2}.

Example 1

Water (ρ=1000 kg/m3\rho = 1000 \text{ kg/m}^3) flows horizontally through a pipe. At point 1, the water speed is 1.96 m/s1.96 \text{ m/s} and the absolute pressure is 4.24105 Pa4.24 \cdot 10^5 \text{ Pa}. The pipe then narrows, increasing the water speed at point 2 to 25.5 m/s25.5 \text{ m/s}. Find the absolute pressure at point 2.

Since the pipe is horizontal (h1=h2h_1 = h_2), use Bernoulli's principle (Equation 3) to solve for p2p_2.

Start with Bernoulli's principle for level flow (Equation 3):

p1+12ρv12=p2+12ρv22p_1 + \frac{1}{2} \rho v_1^2 = p_2 + \frac{1}{2} \rho v_2^2

Isolate p2p_2:

p2=p1+12ρ(v12v22)p_2 = p_1 + \frac{1}{2} \rho (v_1^2 - v_2^2)

Substitute the known values:

p2=4.24105 Pa+12(1000 kg/m3)[(1.96 m/s)2(25.5 m/s)2]p_2 = 4.24 \cdot 10^5 \text{ Pa} + \frac{1}{2} (1000 \text{ kg/m}^3) \left[ (1.96 \text{ m/s})^2 - (25.5 \text{ m/s})^2 \right]
p2=4.24105 Pa+500(3.84650.25) Pap_2 = 4.24 \cdot 10^5 \text{ Pa} + 500 \cdot (3.84 - 650.25) \text{ Pa}
p2=4.24105 Pa3.23105 Pa=1.01105 Pap_2 = 4.24 \cdot 10^5 \text{ Pa} - 3.23 \cdot 10^5 \text{ Pa} = 1.01 \cdot 10^5 \text{ Pa}

The pressure at the narrow section drops to atmospheric pressure (1.01105 Pa1.01 \cdot 10^5 \text{ Pa}) due to the sharp increase in speed.