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
Pressure is defined as force per unit area:
where is the force (in Newtons) applied perpendicular to a surface and is the area (in ) 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 . Other common units include atmospheres (), bars (), and millimeters of mercury ().

Hydrostatic Pressure Equation
The pressure at some depth below the surface of a fluid is given by:
Each variable means something specific:
- is the pressure at the surface. If the fluid is open to the atmosphere, this is atmospheric pressure, typically at sea level.
- is the density of the fluid in . Water has a density of about ; mercury is much denser at . The denser the fluid, the faster pressure builds with depth.
- is gravitational acceleration, approximately on Earth's surface.
- 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 () doubles.
Two factors control how quickly pressure grows: the fluid's density () and the local gravitational field strength (). Diving 10 meters in water adds about 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 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:
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Draw a diagram. Label the fluid, the surface of interest, the depth , and any known pressures.
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Identify knowns and unknowns. Write down what the problem gives you (density, depth, area, force) and what it asks for.
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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.
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Choose the right equation.
- For pressure at a depth:
- For force on a flat submerged surface:
- For hydraulic systems (Pascal's Principle):
- For buoyant force (Archimedes' Principle):
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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 tall, which is why .