Playground

A column of fluid with depth slider; pressure gradient shown as color intensity and a pressure gauge reading.

Variables

SymbolNameSIDimensionRange
PPPressure at Depthoutput
Total pressure at depth h
PaM·L⁻¹·T⁻²0 – 1000000
P0P_0Surface Pressure
Pressure at the surface
PaM·L⁻¹·T⁻²0 – 200000
ρρDensity
Fluid density
kg/m³M·L⁻³1 – 13600
ggGravity
Gravitational acceleration
m/s²L·T⁻²9.8 – 9.8
hhDepth
Depth below surface
mL0 – 1000

Deep dive

Derivation
Consider a thin horizontal slab of fluid at depth h, area A, thickness dh. Force balance: pressure on bottom × A = pressure on top × A + weight of slab. (P + dP)A = PA + ρgA·dh, giving dP/dh = ρg. Integrating from surface (P = P₀) to depth h yields P = P₀ + ρgh.
Experimental verification
Verified by Stevin's hydrostatic paradox demonstration with different-shaped vessels showing equal pressures at equal depths. Modern depth gauges and pressure transducers used in oceanography confirm to ppm precision.
Common misconceptions
  • The shape or width of the container does NOT affect the pressure — only depth matters
  • Pressure acts equally in all directions at a point, not just downward
  • Gauge pressure (ρgh) and absolute pressure (P₀ + ρgh) are different — be careful which one you need
Real-world applications
  • Submarine hull design and crush depth ratings
  • Dam wall thickness (thicker at the base where pressure is highest)
  • Scuba diving depth limits and decompression
  • IV drip bag height calculations in hospitals
  • Manometers for pressure measurement

Worked examples

Eardrum pressure at 3 m depth

Given:
ρ:
1000
g:
9.8
h:
3
Find: ΔP
Solution

ΔP = ρgh = 1000 × 9.8 × 3 = 29400 Pa ≈ 29.4 kPa

Pressure at the bottom of the Mariana Trench

Given:
ρ:
1025
g:
9.8
h:
11000
Find: ΔP
Solution

ΔP = 1025 × 9.8 × 11000 ≈ 1.10 × 10⁸ Pa ≈ 1090 atm

Scenarios

What if…
  • scenario:
    What if you use mercury instead of water?
    answer:
    Mercury is 13.6× denser, so the same depth gives 13.6× more pressure. This is why mercury barometers are short — only ~76 cm to balance one atmosphere.
  • scenario:
    What if the container is shaped like an hourglass or wide cone?
    answer:
    The pressure at any depth depends only on h, not shape. This is Stevin's hydrostatic paradox — a tall narrow tube exerts the same pressure on the base as a wide vat at the same depth.
  • scenario:
    What if gravity changed (e.g., on the Moon)?
    answer:
    Pressure scales with g. On the Moon (g ≈ 1.6 m/s²), the same depth of water would exert about 1/6 the pressure.
Limiting cases
  • condition:
    h = 0
    result:
    P = P_0
    explanation:
    At the surface, pressure equals atmospheric (or whatever sits on top).
  • condition:
    ρ → 0
    result:
    P → P_0
    explanation:
    A massless fluid carries no weight — no depth dependence.
  • condition:
    h = 10 m of water
    result:
    ΔP ≈ 1 atm
    explanation:
    Every 10 m of water adds roughly one atmosphere — handy diving rule of thumb.

Context

Simon Stevin · 1586

Stevin showed pressure depends only on depth, not container shape — the famous hydrostatic paradox illustrated with vessels of different shapes filled to the same height.

Hook

Why do your ears hurt at the bottom of a swimming pool?

Find the gauge pressure on your eardrum at 3 m below the surface of fresh water.

Dimensions: [ρgh] = (M·L⁻³)(L·T⁻²)(L) = M·L⁻¹·T⁻² = [P] ✓
Validity: Static, incompressible fluid in a uniform gravitational field. Fails for compressible atmospheres over large altitude ranges — use the barometric formula instead.

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