2.2.5 · D2Fluid Mechanics

Visual walkthrough — Hydrostatics — pressure = ρgh, derivation

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Step 0 — What do the words even mean?

Before any physics, let's pin down the two ideas that carry the whole story: pressure and depth. A smart 12-year-old who has never seen these should be fine.

Look at the picture: the same hand pushes on a wide board and on a thin nail. Same force , but the nail's tiny area makes a huge pressure.

Figure — Hydrostatics — pressure = ρgh, derivation

WHY start here? Every later equation is really the sentence "force per area." If "pressure" stays fuzzy, the algebra is meaningless. Now it isn't.


Step 1 — Draw an imaginary column of water

We can't do force-balance on a whole ocean at once. So we cut out a shape we can reason about: a straight vertical cylinder of fluid.

WHAT: Imagine a tube-shaped chunk of the fluid — cross-section area , standing from the free surface (the top, open to air) straight down to depth .

WHY this shape: A vertical cylinder has only two flat faces that point up/down (top and bottom). Everything vertical happens on just those two faces. Its side wall is curved and vertical, so pushes on it are sideways — they will cancel and never bother us. Simple geometry = simple physics.

PICTURE: The red cylinder is our chosen "body." It is still made of ordinary water; we've only drawn an imaginary boundary around it.

Figure — Hydrostatics — pressure = ρgh, derivation

Step 2 — Weigh the column

Pressure comes from weight, and weight needs mass. Let's get the mass of our red cylinder.

WHAT: Its volume is height area, and mass is density volume:

WHY: Density answers "how many kilograms per cubic metre?" Multiply by how many cubic metres we have () and out pops the kilograms. (Density comes from Density and Specific Gravity.)

PICTURE: The column split into little unit cubes — count the cubes (), each cube weighs per unit volume, total mass stacks up as .

Figure — Hydrostatics — pressure = ρgh, derivation

Now turn mass into weight (the downward gravity force):

The symbol is doing one job: converting kilograms into newtons of downward pull.


Step 3 — Name every vertical force on the column

Now list all the up/down forces. There are exactly three, and each is a pressure area.

WHAT: three forces —

WHY these three, and no more: The top face feels the atmosphere pressing down ( is the pressure right at the surface). The bottom face feels the fluid underneath pressing up ( — this is the mystery we're solving for). Gravity pulls the whole mass down. Nothing else points vertically.

PICTURE: Three black arrows for the vertical forces, plus little grey sideways arrows on the wall — drawn only to show they cancel (each left push is matched by an equal right push at the same depth). This is why we never need them.

Figure — Hydrostatics — pressure = ρgh, derivation

Step 4 — Balance the forces (the physics happens here)

The column is at rest (that's what "hydrostatic" means). Newton's first law: at rest ⇒ net force up-forces equal down-forces.

WHAT:

Substitute each one from Step 3:

WHY: If the up-push were bigger, the column would shoot upward; if smaller, it would sink. It does neither — it just sits — so the two sides are exactly equal. This single equality carries all the answer.

PICTURE: A see-saw / balance beam. On the left pan sits (up); on the right pan sit and (down). The beam is level — perfectly balanced.

Figure — Hydrostatics — pressure = ρgh, derivation

Step 5 — Cancel the area, read off the law

Every term has an in it. The column's thickness shouldn't decide the pressure at a point, so let's remove it.

WHAT: Divide the whole equation by :

WHY dividing by is allowed and meaningful: was just the size of our imaginary tube — we invented it, so it must vanish from the physical answer. Its disappearance is a promise: pressure does not depend on how fat you drew the column. (That's the hydrostatic paradox, coming in Step 7.)

Term by term, the final law reads:

PICTURE: A vertical depth-axis with a ruler. At the pressure bar has height . As you go down, a red wedge is added on top — the bar grows in a perfectly straight line with depth.

Figure — Hydrostatics — pressure = ρgh, derivation

Step 6 — The edge cases (never leave a scenario undrawn)

A law you trust must survive its extremes. Let's check all of them on one figure.

  • At the surface, : . Correct — no fluid above you, only air. The red wedge has zero height.
  • Zero gravity, : everywhere. In free-fall or deep space, water has no weight, so depth stops mattering — pressure is uniform. The wedge collapses flat.
  • Very light fluid, (like thin gas): becomes tiny; pressure barely changes with depth. This is why we usually ignore the "depth" of the air in a room.
  • Going up instead of down ( negative): above the surface is negative — pressure drops. Same straight line, extended upward.

PICTURE: One graph of pressure vs depth showing four lines: the normal fluid (steep red line), the light gas (nearly flat), the case (vertical — no change), and the surface point where all meet at .

Figure — Hydrostatics — pressure = ρgh, derivation

Step 7 — Why the container's shape is invisible

The area cancelled in Step 5. Let's see what that promise means physically.

WHAT: Three containers — a thin straw, a fat barrel, a slanted funnel — all filled to the same depth . Bottom pressure is identical in all three, even though the barrel holds a thousand times more water.

WHY: Only the fluid directly above a point presses on it. In the fat barrel, the extra width of water off to the sides isn't stacked over that point — its weight is carried by the bottom and the walls, not by the point below the middle. So volume is irrelevant; only vertical depth counts.

PICTURE: Three differently shaped vessels side by side, water level dead-flat across all, a red dot at each bottom labelled with the same pressure .

Figure — Hydrostatics — pressure = ρgh, derivation

The one-picture summary

Here is the entire derivation compressed into a single frame: the red column, its three vertical forces, the balance, and the resulting straight pressure line — all at once.

Figure — Hydrostatics — pressure = ρgh, derivation
Recall Feynman retelling — the whole walkthrough in plain words

Picture a pool. I imagine drawing a skinny invisible tube of water, from the top surface straight down to my feet at depth . That tube of water isn't moving, so it must be perfectly balanced — whatever holds it up equals whatever pulls it down. Pulling down: the air pressing on its top () plus its own weight ( — density times how tall times gravity). Pushing up: the water underneath, pressing on its bottom face (). Set up equal to down: . The area was just the fatness of my imaginary tube — it can't be part of the real answer, so I divide it away and get . That's it. The piece is the extra squeeze from the water column; go twice as deep and it doubles. And because cancelled, it never mattered how wide or weirdly-shaped the container was — only how far down you go. At the surface () there's no water above you, so you feel just the air . In zero gravity the water is weightless and depth stops mattering at all. Everything checks out.


Connections

  • ← Parent: full derivation & examples
  • Pascal's Law — the cancelling- idea, pushed further
  • Atmospheric Pressure & Barometer — where comes from
  • Buoyancy & Archimedes' Principle — pressure difference between top and bottom faces
  • Manometers — reading as a height
  • Bernoulli's Equation — add motion; static limit returns this law
  • Density and Specific Gravity — supplies