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Mechanical Properties of Fluids Formula Sheet

Fluids and properties of matter formulasClass 11AP Physics 2Updated 1 Nov 2026

P=P0+ρghP = P_0 + \rho g h
where
  • P absolute pressure at depth h Pa
  • P₀ pressure at the free surface (often atmospheric) Pa
  • ρ density of the fluid kg/m³
  • g acceleration due to gravity m/s²
  • h depth below the surface m

This mechanical properties of fluids formula sheet gathers every result you need for fluids at rest, fluids in motion, liquid surfaces and the elastic behaviour of solids, starting from the pressure at depth, P=P0+ρghP = P_0 + \rho g h. It follows the order of the Class 11 chapters on mechanical properties of fluids and of solids, and it also covers the fluids unit of AP Physics 2.

It is a study summary, not an official exam sheet. Boards and exam bodies set and supply their own formula lists where they allow one. Use the tables below to revise, and follow the links to the full pages for symbols, derivations and worked problems.

Mechanical properties of fluids formula sheet: P = P₀ + ρgh

Quick facts

  • Hydrostatics

    P=P0+ρghP = P_0 + \rho g h
  • Buoyancy

    Fb=ρfVgF_b = \rho_f V g
  • Continuity

    A1v1=A2v2A_1 v_1 = A_2 v_2
  • Bernoulli

    P+12ρv2+ρgh=constantP + \frac{1}{2}\rho v^2 + \rho g h = \text{constant}
  • Viscosity

    F=ηAdvdxF = \eta A \frac{dv}{dx}
  • Surface tension

    T=FLT = \frac{F}{L}
  • Elasticity

    modulus=stressstrain\text{modulus} = \frac{\text{stress}}{\text{strain}}

How the mechanical properties of fluids formula sheet fits together

Think of the chapter as four connected blocks.

  1. Matter in bulk. Everything starts with density, mass per volume. Its cousins are relative density (compared with water), bulk density and tapped density (for powders and soils) and linear density (mass per metre of a string).
  2. Fluids at rest. Density times g times depth gives pressure. The pressure difference between the top and bottom of an object gives the buoyant force.
  3. Fluids in motion. Mass conservation gives the continuity equation, energy conservation gives Bernoulli's principle, and internal friction gives viscosity. Viscosity in turn sets the terminal velocity of falling spheres and the critical velocity where flow turns turbulent.
  4. Surfaces and solids. A liquid surface has surface tension and stores surface energy. A solid under load has stress and strain, and dividing one by the other gives a modulus of elasticity.

Notice how often one formula feeds the next. If you know where each one comes from, you rarely need to memorise more than a handful.

Density, pressure and buoyancy formulas

Fluids at rest
QuantityFormulaSI unitFull page
Densityρ=mV\rho = \frac{m}{V}kg/m³Density
Relative densityρρwater\frac{\rho}{\rho_{water}}noneRelative density
Bulk densitymdryVtotal\frac{m_{dry}}{V_{total}}kg/m³Bulk density
Linear densityμ=mL\mu = \frac{m}{L}kg/mLinear density
PressureP=FAP = \frac{F}{A}PaPressure
Pressure at depthP=P0+ρghP = P_0 + \rho g hPaPressure
Pascal's law (hydraulic lift)F1A1=F2A2\frac{F_1}{A_1} = \frac{F_2}{A_2}NPressure
Upthrust (buoyancy)Fb=ρfVgF_b = \rho_f V gNBuoyant force

Pressure at a given depth does not depend on the shape of the container, and the buoyant force does not depend on what the object is made of. Both facts catch students out more than the formulas themselves.

Fluid flow and viscosity formulas

Fluids in motion
QuantityFormulaSI unitFull page
Equation of continuityAvAv is the same at every sectionm³/sflow rate Q = Av
Bernoulli's principleP+12ρv2+ρgh=constP + \frac{1}{2}\rho v^2 + \rho g h = \text{const}Paenergy per volume
Speed of efflux (Torricelli's law)v=2ghv = \sqrt{2 g h}m/shole at depth h
Newton's law of viscosityF=ηAdvdxF = \eta A \frac{dv}{dx}NViscosity
Viscosity coefficientη=FA (dv/dx)\eta = \frac{F}{A\,(dv/dx)}Pa sCoefficient of viscosity
Velocity gradientΔvΔx\frac{\Delta v}{\Delta x}s⁻¹Velocity gradient
Stokes' lawF=6πηrvF = 6\pi\eta r vNViscous force
Terminal velocityvt=2r2(ρ−σ)g9ηv_t = \frac{2r^2(\rho - \sigma)g}{9\eta}m/sTerminal velocity
Reynolds numberRe=ρvDηR_e = \frac{\rho v D}{\eta}noneCritical velocity

For boats on moving water, the river's own speed is found with the speed of stream formula, a relative motion result that often turns up beside this chapter.

Surface tension and elasticity formulas

Liquid surfaces
QuantityFormulaSI unitFull page
Surface tensionT=FLT = \frac{F}{L}N/mSurface tension
Surface energyW=T ΔAW = T\,\Delta AJSurface energy
Excess pressure, drop2Tr\frac{2T}{r}PaSurface tension
Excess pressure, soap bubble4Tr\frac{4T}{r}PaSurface tension
Capillary riseh=2Tcos⁡θrρgh = \frac{2T\cos\theta}{r\rho g}mSurface tension
Elastic solids
QuantityFormulaSI unitFull page
Stressσ=FA\sigma = \frac{F}{A}PaStress
StrainΔLL\frac{\Delta L}{L}noneStrain
Modulus of elasticitystressstrain\frac{\text{stress}}{\text{strain}}PaModulus of elasticity
Young's modulusY=FLA ΔLY = \frac{FL}{A\,\Delta L}PaYoung's modulus
Bulk modulusK=−ΔPΔV/VK = -\frac{\Delta P}{\Delta V/V}PaBulk modulus
Modulus of rigidityG=F/AθG = \frac{F/A}{\theta}PaModulus of rigidity

All three moduli, stress and pressure share the dimensions [M¹ L⁻¹ T⁻²]. Step by step working sits on the pages for the dimensions of stress and the dimensions of surface tension.

Worked example: a pipe that narrows

Example: continuity and Bernoulli together

Water flows through a horizontal pipe whose cross section shrinks from 4.0 cm² to 1.0 cm². In the wide part the speed is 2.0 m/s. Find the speed in the narrow part and the pressure difference between the two parts.

Continuity: v2=A1v1A2=4.0×2.01.0=8.0 m/sv_2 = \frac{A_1 v_1}{A_2} = \frac{4.0 \times 2.0}{1.0} = 8.0\ \text{m/s}. The area ratio is the same in cm² or m², so no conversion is needed here.

Bernoulli with equal heights: P1−P2=12ρ(v22−v12)=12(1000)(64−4.0)=3.0×104 PaP_1 - P_2 = \frac{1}{2}\rho (v_2^2 - v_1^2) = \frac{1}{2}(1000)(64 - 4.0) = 3.0\times10^4\ \text{Pa}

The pressure is 30 kPa lower in the narrow section, where the water moves faster.

Example: water from a tank

A tank is filled with water to 5.0 m above a small hole near its base. How fast does the water leave the hole?

v=2gh=2×9.8×5.0=98=9.9 m/sv = \sqrt{2 g h} = \sqrt{2 \times 9.8 \times 5.0} = \sqrt{98} = 9.9\ \text{m/s}

This is the speed a stone would reach falling freely through 5.0 m.

Study tips and exam traps

  • Gauge or absolute. ρgh is gauge pressure. Add P₀ only when the question asks for total pressure.
  • Fluid density in buoyancy. The upthrust uses the density of the liquid, not the object.
  • Radius, not diameter. Stokes' law, terminal velocity and capillary rise all take the radius.
  • Two surfaces. Soap films and bubbles double the surface terms: F = 2TL, excess pressure 4T/r.
  • Viscosity in poise. Convert to Pa s by dividing by 10.
  • Mass is not force. Stress and pressure need a weight in newtons, m × g.
  • Unit squares and cubes. a square centimetre is 10⁻⁴ m², a litre is 10⁻³ m³ and a cubic centimetre 10⁻⁶ m³.
  • Sign of ΔV. In the bulk modulus formula ΔV is negative under compression; the minus sign keeps K positive.

A good revision routine is to cover the formula column of each table and write the formulas from memory, then check the units column without looking. If a unit will not come out right, the formula is wrong.

Frequently asked questions

What formulas are in the mechanical properties of fluids chapter?

The core set is P = P₀ + ρgh, Pascal's law, the buoyant force ρVg, the continuity equation, Bernoulli's principle, Torricelli's law, Newton's law of viscosity, Stokes' law, terminal velocity, Reynolds number and the surface tension results.

Can I take this page into an exam as my formula sheet?

Not for an exam hall. What you see here is a revision summary written for study. Each exam body decides whether to supply a list and what goes on it, so check yours and learn the rest by heart.

What is the most important formula for fluids at rest?

Pressure at depth, P = P₀ + ρgh. It explains hydraulic machines, dams, diving and, through the pressure difference on an object, the buoyant force.

Which formulas from mechanical properties of solids should I learn with fluids?

Stress = F/A, strain = ΔL/L, and the three moduli (Young's, bulk and rigidity). Bulk modulus also applies to liquids and gases.

Why do so many quantities here have the unit pascal?

Pressure, stress and all elastic moduli are force per unit area, or that divided by a dimensionless strain, so each has dimensions [M¹ L⁻¹ T⁻²] and the unit Pa.

Every formula in this section 21