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🍏Principles of Physics I Unit 13 Review

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13.1 Fluid Statics and Pressure

13.1 Fluid Statics and Pressure

Written by the Fiveable Content Team • Last updated August 2025
Written by the Fiveable Content Team • Last updated August 2025
🍏Principles of Physics I
Unit & Topic Study Guides

Fluid Statics and Pressure

Fluid statics is the study of how liquids and gases behave when they're at rest. The central idea is pressure: how it builds with depth, how it acts on submerged objects, and how it transmits through enclosed fluids. These principles are the foundation for understanding hydraulics, buoyancy, and instruments like barometers and manometers.

The math here is straightforward. A few key equations let you calculate pressure at any depth and the force on any submerged surface.

Fluid Statics Fundamentals

Pressure in fluids, Pascal’s Principle and Hydraulics – University Physics Volume 1

Pressure in Fluids

Pressure is defined as force per unit area:

P=FAP = \frac{F}{A}

where FF is the force (in Newtons) applied perpendicular to a surface and AA is the area (in m2m^2) over which that force is distributed.

A few things to keep straight about fluid pressure:

  • It acts equally in all directions at a given point in a fluid, and always perpendicular to any surface it contacts. This is sometimes called Pascal's law of isotropy.
  • Force and pressure are directly proportional: double the force, double the pressure. Area and pressure are inversely proportional: spread the same force over a larger area and the pressure drops. That's why a thumbtack hurts your finger on the pointed end but not the flat end, even though the force is the same.
  • The SI unit is the Pascal (Pa), where 1 Pa=1 N/m21 \text{ Pa} = 1 \text{ N/m}^2. Other common units include atmospheres (1 atm=101,325 Pa1 \text{ atm} = 101{,}325 \text{ Pa}), bars (1 bar=100,000 Pa1 \text{ bar} = 100{,}000 \text{ Pa}), and millimeters of mercury (mmHg\text{mmHg}).
Pressure in fluids, Pressure & Pascal’s Principle – TikZ.net

Hydrostatic Pressure Equation

The pressure at some depth below the surface of a fluid is given by:

P=P0+ρghP = P_0 + \rho g h

Each variable means something specific:

  • P0P_0 is the pressure at the surface. If the fluid is open to the atmosphere, this is atmospheric pressure, typically 101.325 kPa101.325 \text{ kPa} at sea level.
  • ρ\rho is the density of the fluid in kg/m3\text{kg/m}^3. Water has a density of about 1000 kg/m31000 \text{ kg/m}^3; mercury is much denser at 13,546 kg/m313{,}546 \text{ kg/m}^3. The denser the fluid, the faster pressure builds with depth.
  • gg is gravitational acceleration, approximately 9.81 m/s29.81 \text{ m/s}^2 on Earth's surface.
  • hh is the vertical depth below the surface, measured in meters. Only vertical distance matters here, not the shape of the container.

Pressure Variation with Depth

Pressure increases linearly with depth in an incompressible fluid. If you go twice as deep, the pressure contribution from the fluid (ρgh\rho g h) doubles.

Two factors control how quickly pressure grows: the fluid's density (ρ\rho) and the local gravitational field strength (gg). Diving 10 meters in water adds about 98,100 Pa98{,}100 \text{ Pa} of pressure, roughly one full atmosphere. The same depth in mercury would add about 13.5 times more.

Pascal's Principle states that a pressure change applied to an enclosed, incompressible fluid is transmitted undiminished to every point in the fluid and to the walls of its container. This is the operating principle behind hydraulic systems: a small force applied to a small-area piston creates the same pressure increase at a large-area piston, producing a much larger output force.

One important distinction: liquids are nearly incompressible, so their density stays constant with depth and the equation P=P0+ρghP = P_0 + \rho g h works directly. Gases are highly compressible, so their density changes with pressure and the relationship becomes more complex. For this course, you'll mostly apply the hydrostatic equation to liquids.

Solving Fluid Statics Problems

Here's a reliable approach for pressure and force calculations:

  1. Draw a diagram. Label the fluid, the surface of interest, the depth hh, and any known pressures.

  2. Identify knowns and unknowns. Write down what the problem gives you (density, depth, area, force) and what it asks for.

  3. Check your units. Convert everything to SI (Pa, m, kg, N) before plugging into equations. A common mistake is mixing cm with m or atm with Pa.

  4. Choose the right equation.

    • For pressure at a depth: P=P0+ρghP = P_0 + \rho g h
    • For force on a flat submerged surface: F=PAF = PA
    • For hydraulic systems (Pascal's Principle): F1A1=F2A2\frac{F_1}{A_1} = \frac{F_2}{A_2}
    • For buoyant force (Archimedes' Principle): Fb=ρfluidgVdisplacedF_b = \rho_{\text{fluid}} \, g \, V_{\text{displaced}}
  5. Solve and check. Does the answer make physical sense? Pressure should increase with depth. A hydraulic lift should multiply force, not reduce it.

Common application: In a U-tube manometer, the pressure difference between two points is found by comparing the heights of fluid columns on each side. In a barometer, atmospheric pressure supports a column of mercury about 760 mm760 \text{ mm} tall, which is why 1 atm=760 mmHg1 \text{ atm} = 760 \text{ mmHg}.

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