4.1 Fluid Statics, Manometry, Hydrostatic Force & Buoyancy

Key Takeaways

  • Hydrostatic pressure increases linearly with depth in an incompressible fluid according to $P = P_0 + \rho g h$, acting perpendicular to any submerged boundary.
  • Differential manometers utilize static fluid columns to measure pressure differences between two points using the hydrostatic principle $\sum \gamma_i h_i$.
  • The resultant hydrostatic force on a plane submerged surface is $F_R = \gamma h_c A$, acting at the center of pressure $y_{cp} = y_c + I_{\bar{x}} / (y_c A)$, which always lies below the centroid.
  • Curved surface hydrostatic forces are evaluated by separating horizontal components ($F_H = \gamma h_c A_{proj}$) and vertical components equal to the weight of the fluid column above ($F_V = \gamma V_{vol}$).
  • Floating body stability depends on metacentric height $GM = MB - GB = I_{waterline} / V_{submerged} - GB$, where $GM > 0$ ensures a positive restoring moment against tipping.
Last updated: July 2026

4.1 Fluid Statics, Manometry, Hydrostatic Force & Buoyancy

Fluid statics is the branch of fluid mechanics that analyzes fluids at rest. In static fluids, no relative motion exists between adjacent fluid layers, meaning shear stresses are strictly zero ($ \tau = 0$). Consequently, all forces exerted by static fluids on submerged surfaces act normal (perpendicular) to the boundary surface. Mastery of fluid statics, hydrostatic pressure distributions, manometry, and floating stability is vital for mechanical engineers designing hydraulic structures, pressure vessels, storage tanks, and naval vessels.


1. Fundamental Fluid Properties

To analyze fluid behavior under static and dynamic conditions, key physical properties must be defined:

  • Density ($ \rho$): Mass per unit volume, measured in $\text{kg/m}^3$ (SI) or $\text{slugs/ft}^3$ (English). For pure water at standard condition ($4^\circ\text{C}$), $\rho_w = 1000\text{ kg/m}^3 = 1.94\text{ slugs/ft}^3$.
  • Specific Weight ($ \gamma$): Weight per unit volume, defined as $\gamma = \rho g$. For water at $4^\circ\text{C}$, $\gamma_w = 9810\text{ N/m}^3 = 9.81\text{ kN/m}^3 = 62.4\text{ lbf/ft}^3$.
  • Specific Gravity ($SG$): Dimensionless ratio of fluid density to standard reference fluid density (water for liquids, air for gases): SG=ρρwater=γγwaterSG = \frac{\rho}{\rho_{water}} = \frac{\gamma}{\gamma_{water}}
  • Dynamic Viscosity ($ \mu$): Measure of fluid resistance to shear deformation, expressed in $\text{Pa}\cdot\text{s}$ ($ \text{N}\cdot\text{s/m}^2$) or $\text{lbf}\cdot\text{s/ft}^2$.
  • Kinematic Viscosity ($ \nu$): Ratio of dynamic viscosity to density: ν=μρ[m2/s or ft2/s]\nu = \frac{\mu}{\rho} \quad [\text{m}^2/\text{s} \text{ or } \text{ft}^2/\text{s}]
  • Bulk Modulus of Elasticity ($K$): Measure of fluid compressibility, defined as the pressure increase required to produce a unit relative volume decrease: K=VdPdV=ρdPdρK = -V \frac{dP}{dV} = \rho \frac{dP}{d\rho}
  • Surface Tension ($ \sigma$): Tensile force per unit length acting at liquid-gas or liquid-liquid interfaces due to molecular cohesion ($ \text{N/m}$). Capillary rise or depression in a tube of diameter $d$ is given by: h=4σcosθγdh = \frac{4 \sigma \cos \theta}{\gamma d}
Fluid PropertyWater ($20^\circ\text{C}$)Mercury ($20^\circ\text{C}$)SAE 30 Oil ($20^\circ\text{C}$)Air ($20^\circ\text{C}$, 1 atm)
**Density ($
\rho$) [$\text{kg/m}^3$]**$998$$13,550$$891$$1.204$
**Specific Weight ($
\gamma$) [$\text{kN/m}^3$]**$9.79$$133.0$$8.74$$0.0118$
Specific Gravity ($SG$)$1.00$$13.56$$0.89$$0.0012$
**Dynamic Viscosity ($
\mu$) [$\text{Pa}\cdot\text{s}$]**$1.002 \times 10^{-3}$$1.56 \times 10^{-3}$$0.29$$1.82 \times 10^{-5}$
Bulk Modulus ($K$) [$\text{GPa}$]$2.19$$28.5$$1.50$$0.000142$

2. Pascal's Law & Hydrostatic Pressure Distribution

Pascal's Law states that pressure applied to a confined static fluid is transmitted undiminished in all directions throughout the fluid and acts with equal force on equal areas.

In a static fluid column subjected to gravity, the hydrostatic pressure variation is derived from force equilibrium on an infinitesimal fluid element $dAz$: dPdz=γ=ρg\frac{dP}{dz} = -\gamma = -\rho g

Integrating for an incompressible fluid (constant density $\rho$) from the free surface where pressure is $P_0$ at height $z_0$ down to depth $h = z_0 - z$ yields the Fundamental Hydrostatic Equation: P=P0+ρgh=P0+γhP = P_0 + \rho g h = P_0 + \gamma h

Gage Pressure vs. Absolute Pressure

  • Absolute Pressure ($P_{abs}$): Measured relative to absolute vacuum ($0\text{ Pa abs}$).
  • Gage Pressure ($P_{gage}$): Measured relative to local atmospheric pressure ($P_{atm} = 101.325\text{ kPa} = 14.7\text{ psi}$). Pabs=Pgage+PatmP_{abs} = P_{gage} + P_{atm}

3. Manometry Principles

Manometers measure static fluid pressure differences using balanced columns of liquid with known specific weights.

Manometer Equation Rules:

  1. Start at a known point of pressure (e.g., pipe center $P_A$ or open atmosphere $P_{atm}$).
  2. Move along the fluid columns: add hydrostatic pressure increment $+\gamma h$ when moving vertically downward, and subtract $-\gamma h$ when moving vertically upward.
  3. Continuous fluid layers of identical density across a continuous horizontal plane have equal pressure.
  4. Equate the accumulated sum to the pressure at the destination point $P_B$.

For a U-tube differential manometer connected between pipe A and pipe B containing manometric fluid of specific weight $\gamma_m$: PA+γ1h1γmhmγ2h2=PB    PAPB=γ2h2+γmhmγ1h1P_A + \gamma_1 h_1 - \gamma_m h_m - \gamma_2 h_2 = P_B \implies P_A - P_B = \gamma_2 h_2 + \gamma_m h_m - \gamma_1 h_1


4. Hydrostatic Force on Submerged Surfaces

Plane Submerged Surfaces

For a flat surface of total area $A$ inclined at angle $\theta$ to the free surface:

  1. Resultant Force Magnitude ($F_R$): The total force equals the product of pressure at the centroid ($P_c$) and total surface area ($A$): FR=PcA=γhcA=γ(ycsinθ)AF_R = P_c A = \gamma h_c A = \gamma (y_c \sin \theta) A where $h_c$ is vertical depth to centroid, and $y_c$ is inclined distance from free surface along the plane.

  2. Center of Pressure ($y_{cp}$): The location where resultant force $F_R$ acts. Because hydrostatic pressure increases linearly with depth, the center of pressure always lies below the centroid ($y_{cp} > y_c$): ycp=yc+IxˉycAy_{cp} = y_c + \frac{I_{\bar{x}}}{y_c A} xcp=xc+IxˉyˉycAx_{cp} = x_c + \frac{I_{\bar{x}\bar{y}}}{y_c A} where $I_{\bar{x}}$ is area moment of inertia about the centroidal axis parallel to the free surface.

Common centroidal area moments of inertia:

  • Rectangle ($b \times h$): $A = bh$, $y_c = h/2$, $I_{\bar{x}} = \frac{b h^3}{12}$
  • Circle (diameter $d$): $A = \frac{\pi d^2}{4}$, $I_{\bar{x}} = \frac{\pi d^4}{64}$
  • Triangle (base $b$, height $h$): $A = \frac{bh}{2}$, $y_c = \frac{2h}{3}$ from apex, $I_{\bar{x}} = \frac{b h^3}{36}$

Curved Submerged Surfaces

Hydrostatic force on a curved surface is calculated by resolving into horizontal and vertical components:

  • Horizontal Component ($F_H$): Equal to the force on the projection of the curved surface onto a vertical plane: FH=γhc,projAprojF_H = \gamma h_{c,proj} A_{proj} acting through the center of pressure of the projected vertical area.

  • Vertical Component ($F_V$): Equal to the weight of the real or imaginary fluid column extending directly above the curved surface up to the free surface level: FV=γVvolumeF_V = \gamma V_{volume} acting vertically through the center of gravity of the fluid volume.

  • Resultant Hydrostatic Force ($F_R$): FR=FH2+FV2,θforce=arctan(FVFH)F_R = \sqrt{F_H^2 + F_V^2}, \quad \theta_{force} = \arctan\left(\frac{F_V}{F_H}\right)


5. Archimedes' Principle & Floating Body Stability

Archimedes' Principle

Any body submerged in or floating on a fluid experiences an upward Buoyant Force ($F_B$) equal to the weight of the fluid displaced by the body: FB=ρfgVsubmerged=γfVsubmergedF_B = \rho_f g V_{submerged} = \gamma_f V_{submerged}

  • Submerged Body: $F_B$ acts vertically upward through the center of buoyancy ($B$), which is the centroid of the displaced fluid volume.
  • Floating Equilibrium: A body of weight $W = \gamma_{body} V_{body}$ floats in equilibrium when $W = F_B$, yielding the submerged volume ratio: VsubmergedVbody=ρbodyρfluid=SGbodySGfluid\frac{V_{submerged}}{V_{body}} = \frac{\rho_{body}}{\rho_{fluid}} = \frac{SG_{body}}{SG_{fluid}}

Stability of Floating Bodies

When a floating vessel heels through a small tilt angle $\theta$, the center of buoyancy shifts from $B$ to $B'$ due to the reconfigured displaced volume shape. Lines of action of original vertical buoyancy and tilted buoyancy intersect at the Metacenter ($M$).

  • Metacentric Height ($GM$): The distance between center of gravity ($G$) and metacenter ($M$): GM=MBGBGM = MB - GB where $GB$ is vertical distance between centroid of body ($G$) and initial center of buoyancy ($B$).

  • Metacentric Radius ($MB$): MB=IwaterlineVsubmergedMB = \frac{I_{waterline}}{V_{submerged}} where $I_{waterline}$ is minimum moment of inertia of the waterline cross-sectional area about the tilting axis.

  • Stability Criteria:

    1. Stable ($GM > 0$): $M$ is above $G$. A positive restoring moment $T_R = W \cdot GM \sin \theta$ rights the vessel.
    2. Neutral ($GM = 0$): $M$ coincides with $G$. No restoring or overturning moment is produced.
    3. Unstable ($GM < 0$): $M$ is below $G$. An overturning moment causes the vessel to capsize.

6. Worked Numerical Examples

Example 1: Hydrostatic Force on an Inclined Rectangular Gate

A rectangular gate $2.0\text{ m}$ wide and $3.0\text{ m}$ high is hinged along its top horizontal edge. The gate is submerged in water ($ \gamma = 9.81\text{ kN/m}^3$) inclined at an angle of $60^\circ$ to the horizontal. The top edge of the gate is located at a vertical depth of $4.0\text{ m}$ below the water surface. Calculate:

  1. The total hydrostatic force $F_R$ acting on the gate.
  2. The location of center of pressure $y_{cp}$ along the gate plane from the water surface.

Solution Step-by-Step:

  • Step 1: Calculate inclined distance to top edge ($y_1$) and centroid ($y_c$): y1=h1sin60=4.0sin60=4.619 my_1 = \frac{h_1}{\sin 60^\circ} = \frac{4.0}{\sin 60^\circ} = 4.619\text{ m} yc=y1+hgate2=4.619+3.02=6.119 my_c = y_1 + \frac{h_{gate}}{2} = 4.619 + \frac{3.0}{2} = 6.119\text{ m} hc=ycsin60=6.119×0.8660=5.300 mh_c = y_c \sin 60^\circ = 6.119 \times 0.8660 = 5.300\text{ m}

  • Step 2: Calculate gate area and hydrostatic force: A=b×h=2.0 m×3.0 m=6.0 m2A = b \times h = 2.0\text{ m} \times 3.0\text{ m} = 6.0\text{ m}^2 FR=γhcA=(9.81 kN/m3)(5.300 m)(6.0 m2)=311.94 kNF_R = \gamma h_c A = (9.81\text{ kN/m}^3)(5.300\text{ m})(6.0\text{ m}^2) = 311.94\text{ kN}

  • Step 3: Calculate center of pressure $y_{cp}$: Ixˉ=bh312=2.0×(3.0)312=4.50 m4I_{\bar{x}} = \frac{b h^3}{12} = \frac{2.0 \times (3.0)^3}{12} = 4.50\text{ m}^4 ycp=yc+IxˉycA=6.119+4.506.119×6.0=6.119+0.1226=6.2416 my_{cp} = y_c + \frac{I_{\bar{x}}}{y_c A} = 6.119 + \frac{4.50}{6.119 \times 6.0} = 6.119 + 0.1226 = 6.2416\text{ m}

  • Vertical depth to center of pressure $h_{cp} = y_{cp} \sin 60^\circ = 6.2416 \times 0.8660 = 5.405\text{ m}$.


Example 2: U-Tube Differential Manometer

A differential U-tube manometer containing mercury ($SG_m = 13.6$, $\gamma_m = 133.4\text{ kN/m}^3$) is connected between two pipelines A and B. Pipeline A contains water ($\gamma_w = 9.81\text{ kN/m}^3$) under pressure, while pipeline B contains oil ($SG_o = 0.85$, $\gamma_o = 8.34\text{ kN/m}^3$). Center of pipe A is $1.5\text{ m}$ higher than center of pipe B. The mercury level in the leg connected to pipe A is $0.40\text{ m}$ below pipe A centerline, and the mercury deflection $h_m$ is $0.25\text{ m}$. Determine pressure difference $P_A - P_B$.

Solution Step-by-Step:

  • Step 1: Express elevation levels and specific weights: γA=9.81 kN/m3\gamma_A = 9.81\text{ kN/m}^3 γm=13.6×9.81=133.416 kN/m3\gamma_m = 13.6 \times 9.81 = 133.416\text{ kN/m}^3 γB=0.85×9.81=8.3385 kN/m3\gamma_B = 0.85 \times 9.81 = 8.3385\text{ kN/m}^3

  • Step 2: Apply hydrostatic manometer equation starting at $P_A$: PA+γAhAγmhmγBhB=PBP_A + \gamma_A h_A - \gamma_m h_m - \gamma_B h_B = P_B where: $h_A = 0.40\text{ m}$ (water column down to mercury interface in left leg) $h_m = 0.25\text{ m}$ (mercury column deflection) $h_B = 0.40 + 1.50 - 0.25 = 1.65\text{ m}$ (oil column up to pipe B centerline)

  • Step 3: Solve for $P_A - P_B$: PA+(9.81×0.40)(133.416×0.25)(8.3385×1.65)=PBP_A + (9.81 \times 0.40) - (133.416 \times 0.25) - (8.3385 \times 1.65) = P_B PA+3.92433.35413.759=PBP_A + 3.924 - 33.354 - 13.759 = P_B PA43.189 kPa=PB    PAPB=+43.19 kPaP_A - 43.189\text{ kPa} = P_B \implies P_A - P_B = +43.19\text{ kPa}


Example 3: Metacentric Height of a Rectangular Pontoon

A rectangular pontoon is $10.0\text{ m}$ long, $6.0\text{ m}$ wide, and $3.0\text{ m}$ deep. It has a total mass of $90,000\text{ kg}$ and floats in seawater ($\rho_{sw} = 1025\text{ kg/m}^3$). Its center of gravity $G$ is located $1.80\text{ m}$ above the flat bottom base. Calculate:

  1. The draft $d$ of the pontoon.
  2. The metacentric height $GM$.
  3. The restoring moment for a heel tilt angle of $\theta = 5^\circ$.

Solution Step-by-Step:

  • Step 1: Determine submerged draft ($d$): W=mg=(90,000 kg)(9.81 m/s2)=882.9 kNW = m \cdot g = (90,000\text{ kg})(9.81\text{ m/s}^2) = 882.9\text{ kN} FB=ρswgVsub=(1025)(9.81)(L×B×d)=WF_B = \rho_{sw} g V_{sub} = (1025)(9.81)(L \times B \times d) = W 1025×10.0×6.0×d=90,000    d=90,00061,500=1.4634 m1025 \times 10.0 \times 6.0 \times d = 90,000 \implies d = \frac{90,000}{61,500} = 1.4634\text{ m}

  • Step 2: Find centers of buoyancy ($B$) and gravity ($G$): KB=d2=1.46342=0.7317 m from bottomKB = \frac{d}{2} = \frac{1.4634}{2} = 0.7317\text{ m from bottom} KG=1.8000 m from bottomKG = 1.8000\text{ m from bottom} GB=KGKB=1.80000.7317=1.0683 mGB = KG - KB = 1.8000 - 0.7317 = 1.0683\text{ m}

  • Step 3: Calculate metacentric radius ($MB$) and metacentric height ($GM$): Iwaterline=LB312=10.0×(6.0)312=180.0 m4I_{waterline} = \frac{L \cdot B^3}{12} = \frac{10.0 \times (6.0)^3}{12} = 180.0\text{ m}^4 Vsub=L×B×d=10.0×6.0×1.4634=87.804 m3V_{sub} = L \times B \times d = 10.0 \times 6.0 \times 1.4634 = 87.804\text{ m}^3 MB=IwaterlineVsub=180.087.804=2.0500 mMB = \frac{I_{waterline}}{V_{sub}} = \frac{180.0}{87.804} = 2.0500\text{ m} GM=MBGB=2.0500 m1.0683 m=+0.9817 mGM = MB - GB = 2.0500\text{ m} - 1.0683\text{ m} = +0.9817\text{ m} Since $GM = +0.982\text{ m} > 0$, the pontoon is floating stably!

  • Step 4: Calculate restoring moment at $\theta = 5^\circ$: TR=WGMsinθ=(882.9 kN)(0.9817 m)sin(5)T_R = W \cdot GM \sin\theta = (882.9\text{ kN})(0.9817\text{ m}) \sin(5^\circ) TR=866.74×0.087156=75.54 kNmT_R = 866.74 \times 0.087156 = 75.54\text{ kN}\cdot\text{m}

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Submerged Inclined Surface Hydrostatic Pressure & Center of Pressure
Test Your Knowledge

A vertical rectangular gate 3.0 m wide and 4.0 m high is submerged in water (γ = 9.81 kN/m³) such that its top horizontal edge is flush with the water surface. What is the total hydrostatic force acting on the gate, and how far below the surface is the center of pressure?

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Test Your Knowledge

A U-tube differential manometer measures the pressure drop across an orifice in a water pipe (γ_w = 9.81 kN/m³). The manometer fluid is mercury (SG = 13.6). If the differential deflection of mercury in the U-tube is h_m = 0.15 m, what is the pressure differential P1 - P2 across the pipe points?

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Test Your Knowledge

A flat-bottom barge with beam width B = 8.0 m and draft d = 3.0 m floats in fresh water. The center of gravity G is located 2.5 m above the bottom. What is the metacentric height GM of the barge?

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