Visual walkthrough — Postulates of SR
We are going to answer one question:
If light always travels at the same speed for everyone, how long does one "tick" of a moving clock take?
Step 1 — What is a "light-clock"?
WHAT. Before we can time anything, we need a clock we fully understand. Forget gears. Our clock is two flat mirrors facing each other, a fixed distance apart, with a single flash of light bouncing straight up, hitting the top, and coming straight back down. One up-and-down trip = one tick.
WHY this clock. A normal clock has springs and gears we'd have to model. A light-clock has only one moving thing: a pulse of light. And light is the one thing the postulates make a promise about — its speed. So a clock built out of light is the cleanest possible way to test what the postulates do to time.
PICTURE. Two cyan mirrors, gap labelled ; the amber arrow is the light pulse going up then down.

Step 2 — Name the two events, then time one tick in the clock's own frame
WHAT. Everything in relativity is built from events — a point in space at a single instant, like a snap of the fingers. Our tick is bracketed by two of them:
- Event E₁ — emission: the light flash leaves the bottom mirror.
- Event E₂ — reception: the light flash returns to the bottom mirror.
The time between E₁ and E₂ is one tick. Now sit on the clock, riding along with it. From here the clock isn't going anywhere sideways — the light just goes straight up () and straight down (), a total path of — and, crucially, E₁ and E₂ happen at the very same spot (the bottom mirror hasn't moved in this frame).
WHY. We need a baseline: the time for one tick as measured by someone travelling with the clock. Because E₁ and E₂ occur at the same place in this frame, a single clock sitting there can be present at both — that is exactly what makes this time special, and it earns its own name and symbol.
The equation. Speed is distance divided by time, so time is distance divided by speed. Here the distance is and the speed is (defined in Step 1):
Reading it term by term:
- ::: (Greek "delta-tee-nought") the time between E₁ and E₂, measured by the observer riding the clock. The little marks it as the "home" time. Its proper name is proper time.
- ::: total distance the light covers — up , down .
- ::: the speed of light, defined in Step 1. This is the number the postulates freeze.
PICTURE. Straight vertical path, length , with E₁ and E₂ marked at the same bottom spot, timed at .

Step 3 — Now watch the same clock fly past you
WHAT. Stand on the ground. The clock drifts to the right at a steady speed . The same two events happen — E₁ emission at the bottom mirror, E₂ reception at the bottom mirror — but now the bottom mirror has slid forward between them, so E₁ and E₂ occur at different places in your frame. During the time the light is climbing, the top mirror slides forward too, so by the time the light reaches the top it is no longer directly above where the light started. The light had to travel along a slanted path to catch it.
WHY this changes everything. In your ground view the light is no longer going straight up — it goes up and across at the same time. A slanted path is longer than a straight-up path. Hold that thought: same light, longer road.
The symbols entering here.
- ::: the steady sideways speed of the whole clock, as seen from the ground. Because the clock never speeds up or slows down, this is an inertial frame (see Galilean Relativity).
- ::: (no little zero) the time between E₁ and E₂ as measured by you on the ground. This is the number we are hunting.
PICTURE. The clock shown at three moments as it slides right; the amber light traces a wide "V", with E₁ and E₂ marked at two different ground positions.

Step 4 — Draw the triangle hiding in the V
WHAT. Take just the first half of the tick — light going from the bottom mirror up to the top. Three lengths form a right triangle:
- vertical side — the mirror gap, still .
- horizontal side — how far the clock slid sideways in half a tick. Sideways speed over time gives distance .
- slanted side (hypotenuse) — the actual path the light took, at speed over time , giving length .
WHY the vertical side stays exactly (self-contained argument). The gap is across the direction of motion, not along it. Here is why a crossways length cannot change, argued on the page with no outside note:
That is why we may safely write (not some shrunken ) as the vertical side.
WHY a triangle, and why Pythagoras. The vertical and horizontal sides meet at a right angle (up is perpendicular to sideways). Whenever two sides meet at a right angle, the third side's length is locked by the Pythagorean theorem — hypotenuse² = side² + side². We use it because it is the one rule connecting a slanted length to a vertical and a horizontal length. No other tool answers "how long is the diagonal?"
The equation (Pythagoras on this triangle):
Term by term:
- ::: the slanted light-path, squared — light speed times half-tick time.
- ::: the vertical side squared — the mirror gap, shown above to be frame-independent.
- ::: the sideways slide, squared — clock speed times half-tick time.
PICTURE. The right triangle, every side labelled with its length.

Step 5 — Solve the triangle for the time
WHAT. We now do pure algebra: rearrange the Pythagoras line until sits alone. Follow the manipulations line by line — the figure below shows the same three stages as boxes, but here is the full spoken walk-through.
WHY. The equation contains the answer but has tangled on both sides. Isolating it turns "a relationship" into "a formula you can plug numbers into."
Line 1 — multiply out the squares. Squaring gives , and squaring gives :
Line 2 — clear the fractions. Multiply every term on both sides by ; the 's in the denominators cancel:
Line 3 — gather the unknown. Both sides have a term; subtract from each side so every sits on the left, then factor it out:
Line 4 — undo the square. Divide both sides by to leave alone:
Now take the square root. Squaring loses a sign, so mathematically could be or . But is an elapsed time — a duration measured on a stopwatch — and a duration can never be negative. So we keep the positive root and discard the negative one:
Reading it:
- ::: the round-trip distance, same as Step 2.
- ::: a mathematical factor in the denominator — not a real velocity of anything. It is smaller than (because we subtracted ), and a smaller denominator makes larger. That is the seed of the stretching we are about to reveal.
PICTURE. The algebra as a flow of three boxes, ending at .

Step 6 — Connect the two times: the punchline
WHAT. We have two expressions for the same physical tick:
- ground time:
- home time: , so .
Substitute into the ground formula:
WHY factor out . We want the messy square root to become something clean. Pull a out of the root: . The two 's cancel:
Term by term:
- ::: what the ground observer times for one tick — always the bigger number.
- ::: what the riding observer times — the proper time.
- ::: the Lorentz factor, the "stretch factor." Because , the fraction is less than 1, the square root is less than 1, and dividing by something-less-than-1 makes bigger than .
PICTURE. The two clocks side by side; the moving one's tick visibly stretched by .

This is Time Dilation, and the same drives Length Contraction and the full Lorentz Transformations.
Step 7 — The edge cases (what happens at the extremes)
WHAT. A formula is only trustworthy if it behaves sanely at its limits. We check three:
- Clock at rest, . Then , so , giving . Both observers agree — exactly what should happen when nobody is moving. This is Galilean Relativity reappearing.
- Everyday speeds, . Then is a tiny number (for a car, ), , and the stretch is invisible. This is why Newton worked for 200 years.
- Approaching light speed, . Then , the square root , and . The tick stretches without limit: a clock at light speed would appear frozen. And you may not set — then is negative, its square root is not a real number, and time itself has no meaning. The maths itself forbids exceeding .
WHY these matter. The reader must never meet a case we skipped. Rest, slow, and near-light cover every allowed from up to (but never reaching) .
PICTURE. A graph of against : flat near 1 for small speeds, shooting to infinity as .

The one-picture summary
Everything above, on a single diagram: the moving clock, the slanted light-V, the hidden right triangle with sides , , , and the boxed result .

Recall Feynman: the whole walkthrough in plain words
Build a clock out of nothing but a light beam ping-ponging between two mirrors — one bounce is one tick, bracketed by two events: the flash leaving the bottom (E₁) and returning to the bottom (E₂). If you ride along with it, both events happen at the same spot and the light just goes straight up and down, giving the "home" tick time. Now let the clock fly past me. From where I stand, the two events happen at different places, and while the light climbs, the mirror scoots sideways, so the light has to travel a slanted, longer path to catch it. Here's the stubborn rule of the universe: light won't speed up to cover that extra distance — it always moves at the same speed. Longer path, same speed... the only thing left that can stretch is the time. So I see the flying clock tick slower than my own, by exactly the factor . When the clock barely moves, is basically 1 and nobody notices. When it races toward light speed, blows up and the clock nearly freezes. Nature would rather bend time than let light change its speed.
Connections
- Postulates of SR — the parent: the two rules this whole picture rests on.
- Time Dilation — the result we just built.
- Length Contraction — the same , applied to distance.
- Lorentz Transformations — the full machinery belongs to.
- Michelson-Morley Experiment — the evidence that light's speed really is fixed.
- Galilean Relativity — the low-speed limit we recover when .