Discover · A route you could take
One current, two stories.
Which one is the moving one?
It starts with a magnet, a coil of wire and a needle that moves, all of it ordinary in 1904, and asks why the textbook needs two different explanations for one reading. Following that question through means giving up the idea that “at the same time” needs no definition.
A route you could take, not a transcript of Einstein’s private thoughts. Every step can be read without running anything.
The nagging fact
Push a magnet into a coil of wire, or move the coil over the magnet at the same relative speed, and the needle deflects by the same amount. The accepted theory of 1904 accounts for the two cases by two different mechanisms, and no measurement tells them apart.
The first honest question
If every measurement you can make comes out the same in both cases, what are you still entitled to say about which one is moving?
01 / Start where the paper starts
A magnet, a coil, and a needle that moves
Hold a coil of wire still and push a magnet into it: the needle deflects. Now hold the magnet still and move the coil over it instead, at the same relative speed: the needle deflects by the same amount. Every measurement you can make on the two arrangements agrees.
The accepted theory of 1904 does not describe them the same way. In the first case the moving magnet is said to produce an electric field in the space around it, and that field drives the current. In the second the field around the magnet is said to be unchanging, and the current arises instead because the wire is moving through it. Two mechanisms, two descriptions, one needle that cannot tell them apart.
02 / Decide whether that bothers you
An asymmetry in the telling, not in the measuring
This is not a crisis. Nothing is predicted wrongly. The two accounts agree on every number, and a physicist who shrugs and uses whichever is convenient will never be caught out by an experiment.
What is odd is that the theory distinguishes two situations that no measurement distinguishes. To tell the stories apart you have to say which object is really moving, and the only thing that could settle that is motion relative to the medium light travels in. Attempts to detect that motion had been made, with increasing care, and had found nothing.
How much the null results are worth here
Less than the usual telling suggests, and the route does not lean on them. They say that one route to distinguishing the two cases did not work, not that no route could. The paper refers to failed attempts to detect motion relative to the light medium in general terms, and nothing in it says which experiment mattered to its author; the shelf card says the same.
Three ways on
Every attempt to detect the Earth's motion through the light medium has failed. What do you do with the medium?
The branches vary which theoretical principle is taken as a starting postulate.
Keep an ether at rest, and speeds that add
Constrained by physical contradiction
- Hypothesis
- There is one frame at rest in the ether, and light travels at one speed relative to it. Speeds add in the ordinary way, and a moving transparent body drags light along only partly, by the fraction Fresnel proposed.
- Where it holds
- For every effect of the first order in the ratio of the Earth's speed to light's. That includes light in moving water, where Fizeau in 1851 found a displacement close to the value Fresnel's fraction gives, and the paper itself says that for quantities of the first order the laws are already known to be the same in every such frame.
Its steps (3)
- Send light out along an arm that moves through the ether at speed v, and back. Out, it gains on the far mirror at c − v; back, it meets the near one at c + v. The round trip takes longer than at rest, by the factor 1/(1 − v²/c²).
- Send it across the arm instead. It has to aim ahead of the moving mirror, and the round trip is longer by the smaller factor 1/√(1 − v²/c²). The two times differ in proportion to v²/c²: an effect of the second order.
- Michelson and Morley built an interferometer to see that difference. For their apparatus they expected a displacement of 0.4 of a fringe, and in 1887 they reported one certainly less than a twentieth of that.
It meets the first-order observations, Fizeau's moving water among them, and fails at the second order, where it predicts a displacement Michelson and Morley did not find. That is one prediction against one measurement, and it does not dispose of the ether itself, which the next branch keeps.
It fails against the measurement on the shelf.
Keep the ether, and let motion through it shorten bodies
Held by H. A. Lorentz, 1904
Empirically equivalent within stated scope
- Hypothesis
- Keep the ether at rest. Suppose that electrons, and bodies made of them, moving through it contract along their motion, and describe the moving system in a local time, a variable of the equations.
- Where it holds
- For every experiment on this shelf. Lorentz's paper of 1904 says the theory accounts for the negative results of Michelson, and of Rayleigh and Brace, and that it makes Trouton and Noble's clear at once.
Its steps (3)
- Shorten the arm that lies along the motion by the factor √(1 − v²/c²). Its round trip then takes exactly as long as the one across, and the second-order difference is gone.
- Give the electrons the same contraction and write the moving system's equations in local time. Every state of a system at rest then has a counterpart in motion, so no experiment of this kind can reveal the motion.
- Step 07 follows this account further. It reaches the same formulas as the paper.
Nothing on the shelf separates it from the paper's route, and this route does not call it refuted. Lorentz put it forward with all due reserve. What separates the two is what each takes as given and what each adds by hand, not a measurement either one fails.
Where it gives the same numbers: Every observation on the 1904 shelf: the aberration of starlight, Fizeau's moving water, and the null results of Michelson and Morley, of Rayleigh and Brace, and of Trouton and Noble.
Raise the failure to a principle
The route taken in the 1905 paper
- Hypothesis
- The laws of physics are the same for every observer in uniform motion, so no experiment can reveal who is at rest. The ether is given nothing to do.
- Where it holds
- Wherever the principle holds. Poincaré had stated it in 1904 as a general principle of physics, an experimental result strongly generalized.
Its steps (3)
- Start where the paper starts: the unsuccessful attempts to detect a motion of the Earth relative to the light medium suggest that absolute rest corresponds to no property of the phenomena.
- Add the second statement of step 03, that light travels at one speed whatever its source does. Under the ordinary addition of speeds the two conflict.
- Step 04 finds what has to give: the assumption that observers in relative motion agree about which distant events happen at the same time.
This is the paper's route. It predicts the same null results as the branch before it, needs no medium at rest, and adds no contraction by hand: in § 4 the contraction comes out of the kinematics.
03 / Make a prediction
Can you keep both of these at once?
Here are two statements. First: the laws of physics look the same to anyone moving steadily, so there is no experiment that reveals who is really at rest. Second: light travels through empty space at a definite speed that does not depend on how fast its source was moving when it left.
Before reading on, decide whether they are compatible. If I am gliding past you at half the speed of light and we both watch the same flash, the ordinary way of adding speeds says we must get different answers for how fast it travels. Either one of the two statements is wrong, or something in the ordinary way of adding speeds is.
Why the third option is easy to miss
Adding speeds is not a law anybody tested. It follows from something more basic that has never needed defending: that you and I agree on what time it is, so we agree on how long the flash took, and we already agree on how far it went. That agreement is the assumption in the room, and it is invisible precisely because nothing has ever asked for it.
Two ways on
Does the speed of light depend on how fast its source is moving?
The branches vary which theoretical principle is taken as a starting postulate.
Light keeps its source's speed
Undecided on 1904 evidence
- Hypothesis
- Light leaves its source at one speed relative to the source, as a ball thrown from a moving hand does, and speeds add in the ordinary way. No medium and no frame at rest are needed, and the principle of relativity holds for light as it does in mechanics.
- Where it holds
- For Michelson and Morley's null result, at every order. Their lamp moved with the apparatus, so on this view the light went out and back at the same speed relative to both arms, whichever way the Earth was moving.
Its steps (3)
- In the interferometer the lamp rides with the mirrors. Relative to the arms the light travels at the same speed in every direction, so the view predicts no displacement of the fringes, which is what was found.
- Maxwell's equations fix one speed for a disturbance in the field and say nothing of its source. To keep this view you give up those equations as they stand, and nothing on the shelf supplies the ones that would replace them.
- To decide it you would compare light from sources moving at different speeds. No measurement on the shelf does that.
On the 1904 shelf this stays open, and the route does not call it refuted. In 1913 de Sitter argued from the observed motions of double stars that the velocity of light is independent of the motion of its source; that is later evidence, not on the shelf.
Why the 1904 shelf cannot decide: No measurement on the shelf compares light from sources moving at different speeds, so none of them tells this view from the next. What the shelf can weigh is the cost: this view gets the null result for nothing and gives up Maxwell's equations as they stand, while the paper's keeps the equations and gives up the ordinary addition of speeds.
The measurement that bears on it: de Sitter's argument from double stars (1913)
One speed, whatever the source does
The route taken in the 1905 paper
- Hypothesis
- Light travels in empty space at one definite speed, whatever the motion of the body that emits it, as a disturbance does in Maxwell's equations.
- Where it holds
- Wherever Maxwell's equations describe light in empty space. The paper keeps them for bodies at rest and builds on them.
Its steps (3)
- Keep Maxwell's equations as they stand: a disturbance in the field travels at the speed they fix, from whatever source.
- Set that beside the principle of relativity. Under the ordinary addition of speeds two observers in relative motion would have to measure different speeds for the same flash, which is the puzzle of step 03.
- The paper calls the two presuppositions only apparently incompatible, and step 04 shows why: they fit together once the time of a distant event is set by a stated procedure.
This is the paper's second presupposition, in its introduction: “that light is always propagated in empty space with a definite velocity V which is independent of the state of motion of the emitting body.”
04 / Find the assumption
What does it take to say two distant things happened at once?
Stop and ask what the claim even means. Two events at the same place happening together is something you can see. Two events far apart happening together is not: you have to compare two clocks, and to compare them you have to have set them, and to set them you have to send something between them that takes time to arrive.
So “at the same time” for distant events is not something you observe. It is something you establish, by a procedure you choose. Write the procedure down and the consequence follows at once: two observers moving relative to each other, each setting their clocks by the same rule, do not end up agreeing about which distant events are simultaneous. Neither has made a mistake.
05 / Build the map
What the definition forces
Now the work is mechanical, and this is the step that the story usually skips. Take the two statements from step 3 as given, take the clock-setting procedure from step 4, and ask what relation must hold between one observer’s coordinates and the other’s. Add that space and time are the same everywhere and in every direction, and the answer is forced: only one set of relations keeps both principles and reduces to the familiar one at everyday speeds.
Work it through rather than read it. The result is often presented as a formula handed down; here it is built from a measurement procedure you can carry out, and nothing enters it beyond the two principles, the clock-setting rule, and that sameness of space and time.
06 / Read off the consequences
Moving clocks, moving rods, and added speeds
A clock moving past you reads less elapsed time than yours between the same two events. A rod moving past you measures shorter along its direction of travel. And speeds no longer add the way they used to, which is the answer to the puzzle in step 3: the flash comes out at the same speed for both of us. Neither measurement is wrong; we disagree about the times and distances that go into it.
What the moving clock reading means
The claim is about what the clock itself reads when it arrives, compared with what your clocks read, both measured in the ordinary way. A camera is a separate question: what it records also involves how long the light took to reach it, and that contribution can be calculated on its own. Keeping the two apart is the whole of the distinction.
First the clock, as a formula.
Your clocks advance by t while a clock moving past you at speed v runs between two of its own ticks. What does the moving clock read? Write it using t, v and c, the speed of light.
Answers are compared for t from 1 to 100, v from 1 × 107 to 2.9 × 108 and c from 2.99 × 108 to 3 × 108.
Show a worked explanation
The moving clock reads less than yours by the factor √(1 − v²/c²), so it reads t·√(1 − v²/c²), which you can write t*sqrt(1-v^2/c^2) or t*sqrt(1-(v/c)^2). At v = 0.6c the factor is √0.64 = 0.8: the moving clock reads 8 seconds while yours read 10. The paper writes V for the speed of light, so its form is t·√(1 − (v/V)²). Dividing by the factor instead, t/√(1 − v²/c²), gives the time your clocks show while the moving clock reads t, which is the same fact seen from the other side.
Then the rod, on numbers.
Measured this way, a moving rod is shorter along its direction of travel by the factor √(1 − v²/c²), where v is its speed and c the speed of light, which the paper writes V. A rod 1 m long when it is at rest moves past you along its own length at 0.6 of the speed of light. You mark where its two ends are at the same moment, by your own clocks, and measure the distance between the marks. How long is it? Give it in metres or centimetres.
Show a worked explanation
With v/c = 0.6, v²/c² = 0.36, and √(1 − 0.36) = √0.64 = 0.8. The rod you measure is 0.8 × 1 m = 0.8 m, or 80 cm. Across its direction of travel nothing changes, and a ruler riding with the rod still reads 1 m: the 0.8 m belongs to your way of marking both ends at once.
An answer within 1 percent is the same answer, so 0.8 m and 80 cm agree.
07 / Meet the serious rival
Lorentz gets the same formulas, and is not refuted
Keep the light medium. Say that a body moving through it genuinely contracts, and that a clock moving through it genuinely runs slow, and that what a moving observer calls time is a bookkeeping device rather than the real thing. Work it through and you reach the same equations, and every experiment above comes out the same way.
This route does not tell you that account is wrong, and it would be dishonest to. Within the scope of these measurements the two are equivalent, and no experiment listed here separates them. What differs is the bookkeeping: one account posits a medium nobody can detect and then adds contraction and local time as properties of motion through it; the other takes the two principles of step 3 and gets the same relations with nothing else assumed.
What would it take to prefer one?
Economy, which is a reason and not a proof, and reach: the same kinematics applies to any law whatever, not only to electromagnetism, which is what makes the fourth paper of 1905 possible three months later. A reader who finds the ether account tidier is not making an error that this page can correct with a measurement.
08 / Check it against the world
What had already been measured
Light in moving water is dragged along, but only partly, by a fraction measured in 1851 and awkward for the theories of its day. The new way of adding speeds gives that fraction with nothing added. A star’s apparent position shifts through the year by an amount known since 1729, and the same transformation gives the shift and the accompanying change of frequency together, from one relation rather than two.
In the paperGo straight to the explanation: why two speeds do not simply add
InstrumentRecover the partial drag from velocity addition
InstrumentGet aberration and Doppler from one transformation
InstrumentWatch electric and magnetic fields change into each other
Those were measured before the paper, and the new kinematics gives them. Section 4 adds a consequence nobody had measured: a clock that moves runs slow, by a factor the paper writes down. The laboratory below computes it; the measurement came thirty-three years later.
Moving clocks
Static worked example
- Clock speed (fraction of c)
- 0.6
- Worldline
- a straight line at constant speed
- Coordinate duration
- 10 s
Worked example: a clock moving at 0.6c in a straight line: the platform clocks read 10 s while it reads 8 s.
| Proper time (τ) | 8 s |
|---|---|
| Coordinate time (t) | 10 s |
| τ / t | 0.8 |
| Exact loss per second | 0.2 |
|---|---|
| Printed second-order form (½β²) | 0.18 |
| This worldline never returns to the platform clock: there is no reunion event to compare. |
| Dilation factor (γ) | 1.25 |
|---|
| Proper tick (2L₀/c) | 2 s |
|---|---|
| Coordinate tick | 2.5 s |
A clock losing exactly one second per day moves at β ≈ 0.00481124.
A clock that travels away and comes back reads less time than an identical clock that stayed put. At 60 percent of the speed of light, a trip that takes 10 seconds on the clock at home takes only 8 seconds on the traveller.
Section 4 takes a clock at rest at the origin of the moving system k and asks how fast it runs, judged from the resting system K. Its position is x = vt, and the transformation gives its reading as τ = t√(1 − v2/c2), so each second it falls behind by 1 − √(1 − v2/c2) seconds, or ½(v/c)2 to within terms of fourth order. Einstein draws the consequence: a clock carried from A to B and set beside one that stayed there lags by ½t(v/c)2, and so does a clock taken round a closed path back to its start. The instrument computes that reunion for an out-and-back trip or a circle at constant speed. At 0.6c over 10 s of the resting clock, the traveller reads 8 s: the exact loss is 0.2 s per second, 2 s in all, where the printed approximation gives 0.18 s per second, 1.8 s. A light clock with an arm of 1 light-second ticks every 2 s in its own frame and every 2.5 s as judged from K, the same factor 1.25. The comparison is of clock readings at a shared event; it is not what a camera would see.
Take the resting system K and a clock moving along x at speed v = 0.6c, in seconds and light-seconds, so c = 1. The clock's position is x = vt. Section 3's transformation gives the moving system's time as τ = (t − vx/c2)/√(1 − v2/c2). Put x = vt into the top: t − v × vt/c2 = t(1 − v2/c2), and dividing by √(1 − v2/c2) leaves τ = t√(1 − v2/c2). At 0.6c, v2/c2 = 0.36, 1 − 0.36 = 0.64 and √0.64 = 0.8: the moving clock reads 0.8 s for every second of K, and loses 1 − 0.8 = 0.2 s each second. Einstein's approximation uses √(1 − ε) ≈ 1 − ε/2 for small ε, so the loss is about ½ × 0.36 = 0.18 s each second: very good at everyday speeds, 10 percent low at this one. For the trip, out for 5 s and back for 5 s of K's time at 0.6c both ways, the traveller reads 0.8 × 10 = 8 s against the home clock's 10 s, a lag of 2 s; the approximation says 1.8 s. The turn does not change this, because the rate depends only on the speed, so any path at 0.6c for 10 s gives 8 s. A light clock shows the same factor from geometry. In its own frame light crosses an arm of 1 light-second and returns, a tick of 2 s. Seen from K the arm moves at 0.6c while the light crosses, so each leg is the long side of a right triangle: if a leg takes a time T, then (cT)2 = 12 + (0.6cT)2, so 0.64T2 = 1 and T = 1.25 s, a tick of 2.5 s, and 2.5/2 = 1.25 = 1/0.8. At the equator the ground moves at 465 m/s, so (v/c)2/2 = 1.20 × 10−12, about 104 ns a day in special relativity alone. To lose a whole second a day a clock would need ½β2 = 1/86 400, so β = 0.0048, about 1440 km/s.
Modern qualifications
Einstein called the result a peculiar consequence. He proved it for a path made of straight pieces and assumed it for a curve, with a clock whose rate depends only on its speed, an assumption later named the clock hypothesis. His closing example, a balance-wheel clock at the equator running slower than one at a pole, holds in special relativity alone; on the real Earth the difference in gravitational potential cancels it, and clocks at sea level keep the same rate everywhere, which general relativity explains. The light clock is not in the paper: Lewis and Tolman used it in 1909. Hafele and Keating flew atomic clocks round the world in 1971 and found the lags predicted when both effects are included.
Show the code
The site’s own reference code for this law, in TypeScript. It computes the numbers above when the page runs it, and it is what the page uses wherever a FrankenSim result is not available.
dilationLossPerSecond · src/physics/reference/kinematics.ts · this site’s source, as built · sha256:16174608520a91b1901a27754605296b471556b17585818e16bd777a3027c413
This function computes the listed outputs when it runs.
In words
The loss per coordinate second is 1 minus 1 over gamma. The function returns it as exact, computed as beta squared over (1 + the square root of 1 minus beta squared), and beside it printedSecondOrder, which is half of beta squared. The second is what the paper prints on page 904 when it says the moving clock falls behind by half of (v/V) squared per second, neglecting magnitudes of the fourth order and higher.
Implementation
/**
* Clock loss per coordinate second: 1 - 1/gamma = beta^2 / (1 + sqrt(1 - beta^2)).
* printedSecondOrder is (1/2) beta^2.
*/
export function dilationLossPerSecond(
beta: number,
): KinematicResult<Readonly<{ exact: number; printedSecondOrder: number }>> {
const bad = refuseBeta(beta);
if (bad) return bad;
if (isMode1904()) refuseModernSurface("gamma");
const root = Math.sqrt(1 - beta * beta);
return ok({
exact: (beta * beta) / (1 + root),
printedSecondOrder: 0.5 * beta * beta,
});
}The site’s own reference code for this law, in TypeScript. It computes the numbers above when the page runs it, and it is what the page uses wherever a FrankenSim result is not available.
reciprocalRates · src/experiments/sr05/worldline.ts · this site’s source, as built · sha256:268de30e365ff413ce4b418d22cee21a230f2cdee2730a1f9d744c75ad8b46b0
This function computes the listed outputs when it runs.
In words
There is no asymmetry to find here: the frame at rest reports the moving clock running slow by gamma, and the moving frame reports the resting clock slow by the same gamma. The function returns the single dilationFactor rather than a pair, because a pair would suggest the two numbers could differ.
Implementation
/** Each inertial frame reports the same dilation factor for the other clock's rate -- the
* symmetric statement this bead requires, without constructing a desynchronized separated-
* reading comparison (that needs events.ts's simultaneity apparatus, out of this bead's Scope
* to build). */
export function reciprocalRates(beta: number): KinematicResult<ReciprocalRatesSummary> {
const g = gamma(beta);
if (g.status !== "value") return g;
return ok({ dilationFactor: g.value });
}Model: an ideal clock whose rate depends only on its instantaneous speed. Not modeled: gravitational time dilation, real clock mechanisms under acceleration, rotating-frame synchronization, the geoid's actual shape, atomic-clock physics, and clock noise.
Check it against the world
A printed prediction
Section 4 of the paper draws a consequence that could be measured. A clock moving at speed v, judged from the resting system, reads t√(1 − v²/V²) when the resting clocks read t, V being the paper's letter for the speed of light, so it falls behind by 1 − √(1 − v²/V²) of a second in every second; the paper writes that to second order as ½(v/V)². Choose a worldline in the laboratory below and read what the relation gives.
Worked value
What § 4's relation gives at the laboratory's first setting
8 s on the moving clock for 10 s of the resting clocks, at 0.6 of the speed of light
From the laboratory above, as it now stands
A clock moving at 0.6 of the speed of light, in a straight line:
- The resting clocks read
- 10 s
- The moving clock reads
- 8 s
- It falls behind, in every second
- 0.2 s
An ideal clock whose rate depends only on its speed, computed here from the relation of § 4. Choose another worldline in the laboratory and these readings follow.
In 1938 Ives and Stilwell reported that the light given off by moving hydrogen atoms, each atom a clock, is lowered in frequency by the factor this relation gives. That is later evidence, not on the 1904 shelf, and this edition holds no table of their measurements, so the comparison is made in these words and no figure of theirs is set beside the readings above. They read the result within Lorentz’s theory, which predicts the same rate: it does not choose between that account and the paper’s.
Later evidence, not on the 1904 shelf
Published 1913De Sitter argues from spectroscopic double stars that if light from a source moving at speed u travelled at c + u, as in Ritz's theory, their observed motions would follow not Newton's law but a law depending on their distance from the Earth. Their observed velocities are represented by Keplerian orbits, in many cases confirmed by visual or eclipse observations, and he concludes that the velocity of light is independent of the motion of the source.
Later confirmation
De Sitter argues from spectroscopic double stars that if light from a source moving at speed u travelled at c + u, as in Ritz's theory, their observed motions would follow not Newton's law but a law depending on their distance from the Earth. Their observed velocities are represented by Keplerian orbits, in many cases confirmed by visual or eclipse observations, and he concludes that the velocity of light is independent of the motion of the source.
Historical context
Later empirical or theoretical confirmation developed after 1905.
Available by
Published 1913
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- A proof of the constancy of the velocity of light Proc. R. Acad. Amsterdam 15, 1297 (1913)
Published, 1938-07Ives and Stilwell study the light given off by moving hydrogen canal rays, and report that the experiment establishes the rate of a moving clock: its frequency in motion is its frequency at rest multiplied by √(1 − v²/c²), v being its speed. They present the result as evidence for the theory of Larmor and Lorentz, in which this change of rate is an essential element.
Later confirmation
Ives and Stilwell study the light given off by moving hydrogen canal rays, and report that the experiment establishes the rate of a moving clock: its frequency in motion is its frequency at rest multiplied by √(1 − v²/c²), v being its speed. They present the result as evidence for the theory of Larmor and Lorentz, in which this change of rate is an essential element.
Historical context
Later empirical or theoretical confirmation developed after 1905.
Available by
Published, 1938-07
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- An Experimental Study of the Rate of a Moving Atomic Clock J. Opt. Soc. Am. 28, 215 (1938-07)
09 / Try it yourself
Four pieces of the argument to work by hand
The first three put the paper’s relations to work, in the modern c where the paper writes V. The checker evaluates what you write at many values and compares numbers, not text, so any correct way of writing an answer is accepted.
First, how two speeds combine, as section 5 finds.
Section 5 of the paper asks how speeds combine. A body moves at speed w relative to a system k, in the direction in which k itself moves at speed v relative to you. How fast does the body move relative to you? Write it using v, w and c, the speed of light, which the paper writes V.
Answers are compared for v from 1 × 106 to 2.9 × 108, w from 1 × 106 to 2.9 × 108 and c from 2.99 × 108 to 3 × 108.
Show a worked explanation
The ordinary rule would give v + w. Section 5 finds instead U = (v + w)/(1 + vw/V²), which you can write (v+w)/(1+v*w/c^2). At v = w = 0.6c the ordinary rule gives 1.2c, and this one gives 1.2c/1.36, about 0.882c, less than c. If either speed is c the result is c, whatever the other is: § 5 prints U = V for that case, since composing the speed of light with a smaller speed does not change it. At everyday speeds vw/c² is tiny, and the ordinary sum returns.
Next, a clock’s speed from what it reads and what the resting clocks read.
A clock moving past you in a straight line reads τ while your clocks read t. How fast is it moving? Write v using t, tau for τ, and c, the speed of light, which the paper writes V.
Answers are compared for t from 60 to 100, tau from 1 to 50 and c from 2.99 × 108 to 3 × 108.
Show a worked explanation
Section 4 gives the moving clock's reading as τ = t√(1 − v²/V²). Divide by t and square: τ²/t² = 1 − v²/c², so v²/c² = 1 − τ²/t², and v = c√(1 − τ²/t²), which you can write c*sqrt(1-tau^2/t^2). The check against the world at step 08 opens with 8 s on the moving clock for 10 s of the resting clocks, and this gives v = c√(1 − 0.64) = 0.6c. A reading equal to t gives v = 0, and a reading near zero a speed near c, never beyond it.
Then the light clock, a later picture of the same factor.
A light clock is two mirrors 1.5 m apart, and one tick is a trip of light from one mirror to the other and back. The clock moves at 0.6 of the speed of light, across the line between its mirrors. Judged from the resting system, how far does the light travel in one tick? Give it in metres or centimetres. The light clock is not in the paper, which writes V for the speed of light; it is a later way of seeing the factor of § 4.
Show a worked explanation
Seen from rest, the mirrors move while the light crosses, so each crossing is the long side of a right triangle: if it takes a time T, (cT)² = 1.5² + (0.6cT)², so cT = 1.5/√(1 − 0.36) = 1.875 m, and there and back is 3.75 m. In the clock's own frame the light travels 3 m. Both are covered at the speed c, so a tick judged from rest is longer by 3.75/3 = 1.25, the factor by which § 4's moving clock reads less than the resting ones.
An answer within 1 percent is the same answer, so 3.75 m and 375 cm agree.
One to put in your own words, from step 04.
Two observers in uniform motion relative to each other set their clocks by the same rule, and disagree about which distant events happen at the same time. In two or three sentences: why is neither of them wrong?
What you write stays in this box. Nothing on the page reads it, marks it or sends it anywhere, and it is gone when you leave.
Compare with a worked explanation
Only a person can judge an explanation, and here that person is you. Read yours against each of these in turn:
- For events far apart, “at the same time” is fixed by a procedure: clocks are set by light signals, taking the light’s travel time to be the same both ways.
- Each observer applies that procedure correctly in their own system, and light has the same speed in both.
- Applied in two systems in relative motion, the one procedure picks out two different sets of simultaneous events, so the disagreement follows from the rule and not from an error.
- No experiment can say which set is the real one; that is what the principle of relativity requires.
Neither observer saw two distant events happen at once; each established it, by setting clocks with light signals and taking the light’s time out to equal its time back. Both did so correctly, and light has the same speed for both. Because they move relative to each other, the same rule gives each a different answer about which distant events share a time. The principle of relativity allows no experiment to choose between them, so the disagreement is a fact about simultaneity, not a mistake by either.
Last, a prediction to make before you change anything, in the laboratory at step 08.
Predict, change one thing, then explain
Predict
Predict first. One clock goes out and back at 0.6 of the speed of light while the resting clocks advance 10 s; another circles at the same speed for the same 10 s. When each returns to the clock that stayed, which reads less, or do they read the same?
Change one thing
In the laboratory at step 08, press “Out and back at 0.6c” and read the moving clock; then press “Constant-speed circle at 0.6c” and read it again. Last, press “Low speed, β = 10⁻⁴” and set the exact loss per second beside the printed second-order form.
Explain
Explain why the two paths give the same reading, and say what the laboratory computes rather than measures.
Explain what you saw: why the clock that went out and back and the clock that circled read the same when they returned, and what the printed second-order form is.
What you write stays in this box. Nothing on the page reads it, marks it or sends it anywhere, and it is gone when you leave.
Compare with a worked explanation
Only a person can judge an explanation, and here that person is you. Read yours against each of these in turn:
- In § 4 a moving clock's rate depends only on its speed, so any path at 0.6 of the speed of light for 10 s of the resting clocks gives the same reading, 8 s.
- The paper proves this for a path made of straight pieces and assumes it for a curved one: that a clock’s rate depends only on its speed is an assumption about the clock.
- The printed ½(v/V)² is the loss to second order: close to the exact loss at low speed, and at 0.6c it gives 0.18 s a second against the exact 0.2.
- The laboratory computes what the relation implies for an ideal clock; it is not a measurement of any clock.
Section 4's clock loses 1 − √(1 − v²/V²) of a second in every second, which depends on its speed and not its direction, so a turn does not change its rate. Out and back or round a circle, at 0.6 of the speed of light for 10 s of the resting clocks, the traveller reads 8 s. The paper proves the result for a path made of straight pieces and assumes it for a curve. At one ten-thousandth of the speed of light the exact loss and the printed ½(v/V)² agree to many figures; at 0.6c the printed form gives 0.18 s a second against the exact 0.2. The laboratory computes all of this from the relation; the measurement that tested a moving clock's rate is Ives and Stilwell's of 1938, later evidence.
The 1904 shelf
Nothing here is imported from later. The most interesting card is Lorentz’s, which is on the shelf as a live alternative rather than as a foil.
This list is a reconstruction aid assembled for learning, not a documentary history of what Einstein read.
Published 1687Absolute, true and mathematical time flows equably of itself, without relation to anything external; hours, days, months and years are its relative, apparent measures.
Available by the end of 1904
Absolute, true and mathematical time flows equably of itself, without relation to anything external; hours, days, months and years are its relative, apparent measures.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published 1687
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- Philosophiae Naturalis Principia Mathematica Scholium to the Definitions (1687)
Published, 1728–1729A star's apparent position shifts through the year by an amount set by the Earth's speed and the speed of light.
Available by the end of 1904
A star's apparent position shifts through the year by an amount set by the Earth's speed and the speed of light.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published, 1728–1729
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- A Letter from the Reverend Mr. James Bradley Savilian Professor of Astronomy at Oxford, and F.R.S. to Dr. Edmond Halley Astronom. Reg. &c. giving an Account of a new discovered Motion of the Fix'd Stars Phil. Trans. R. Soc. 35, no. 406, 637 (1728-1729)
Published 1851Light travelling through moving water is carried along by it, but only partly, by a measured fraction rather than fully.
Available by the end of 1904
Light travelling through moving water is carried along by it, but only partly, by a measured fraction rather than fully.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published 1851
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- Sur les hypothèses relatives à l'éther lumineux Comptes Rendus 33, 349 (1851)
Published 1873The equations of the electromagnetic field fix the speed at which an electromagnetic disturbance travels, and Maxwell argues that light is such a disturbance, because that speed and the measured speed of light agree as far as the measurements go.
Available by the end of 1904
The equations of the electromagnetic field fix the speed at which an electromagnetic disturbance travels, and Maxwell argues that light is such a disturbance, because that speed and the measured speed of light agree as far as the measurements go.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published 1873
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- A Treatise on Electricity and Magnetism Oxford: Clarendon Press, vol. II, ch. XX, §§ 781-787 (1873)
Published 1887A careful attempt to detect the Earth's motion through the light medium found no effect of the size expected.
Available by the end of 1904
A careful attempt to detect the Earth's motion through the light medium found no effect of the size expected.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published 1887
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- On the Relative Motion of the Earth and the Luminiferous Ether Am. J. Sci. (3) 34, 333 (1887)
Published 1904Keep the ether at rest, suppose that moving electrons and bodies contract along their motion, and describe the moving system in a local time: then every state of a system at rest has a counterpart when it moves, which accounts for the negative results of Michelson, of Rayleigh and Brace, and of Trouton and Noble.
Available by the end of 1904
Keep the ether at rest, suppose that moving electrons and bodies contract along their motion, and describe the moving system in a local time: then every state of a system at rest has a counterpart when it moves, which accounts for the negative results of Michelson, of Rayleigh and Brace, and of Trouton and Noble.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published 1904
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- Electromagnetic phenomena in a system moving with any velocity smaller than that of light Proc. R. Acad. Amsterdam 6, 809 (1904)
Presented 1904The laws of physical phenomena must be the same for an observer at rest and for one carried along in uniform translation, so that there is no means of telling whether one is so carried: one of the general principles of mathematical physics, which Poincaré calls results of experiment strongly generalized.
Available by the end of 1904
The laws of physical phenomena must be the same for an observer at rest and for one carried along in uniform translation, so that there is no means of telling whether one is so carried: one of the general principles of mathematical physics, which Poincaré calls results of experiment strongly generalized.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Presented 1904
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- L'état actuel et l'avenir de la physique mathématique Address at St Louis, 24 September 1904; Bull. sci. math. (2) 28, 302 (1904)
Where this enters the paper
The paper is thirty-one pages in two parts. The magnet and the coil are its opening paragraph, the clock-setting procedure is section 1, simultaneity is section 2, the construction is section 3, clocks and rods are section 4, velocity addition is section 5, and the electrodynamic half from section 6 onwards carries the field transformations, Doppler and aberration, and the dynamics of the electron. Its German text and an English translation are on this site.
In the 1905 paper
The paper opens on the same apparatus this route opens on, and calls the two accounts of it an asymmetry that does not attach to the phenomena. The same paragraph states the two principles it will keep.
In the 1905 paper
The move. Section 1 lays down, by definition, that light takes the same time out and back between two clocks, and so fixes what it means for clocks at different places to agree.
In the 1905 paper
Measuring a moving rod means marking where its ends are at one time, and section 1 has just made that phrase depend on the frame the marks are made in. The paper draws the consequence before it has any transformation to point at.
In the 1905 paper
With the clock rule granted, the paper asks what relation between one observer's coordinates and another's keeps light at the same speed in both directions, and finds the relations forced up to a scale it then fixes.
In the 1905 paper
The two results a reader has worked by hand here, taken from the map rather than assumed: what a moving clock reads, and what a moving rod measures, each stated with the procedure that measures it.
In the 1905 paper
Adding speeds keeps the denominator the ordinary rule leaves out, so two speeds below the speed of light compose to a speed below it, which is the exercise in this route's last step.
Two doors lead to the same place, the map of section 3: the paper’s own construction from the clock-setting rule, and the map built one requirement at a time in a laboratory, a programmer’s way in. Both arrive at the same equation.
Ways in
Multiple routes, one arrival point
All doors arrive at the same result: the map of § 3: x′ = γ(x − vt) and t′ = γ(t − vx/c²), with γ = 1/√(1 − v²/c²), which the paper writes ξ = β(x − vt) and τ = β(t − vx/V²)
The drawing gives every route the same box and the same line on purpose. Neither door is the real one and neither is a detour: the paper's own construction and the routes beside it reach the result named above, and the journey says so. What it does not show is what each route costs a reader to walk, which is the only respect in which they genuinely differ and is written in the cards below rather than in the picture.
The paper's route
The paper's construction from the clock-setting rule, § 3
Set the moving system's clocks by the rule of § 1, ask what time τ an event must have for light to take equal times out and back, and solve. An unknown factor φ(v) is left, and the paper fixes it at 1 with a third system moving back at −v, and a rod set across the motion whose measured length cannot depend on the direction of travel.
Arrives at: the map of § 3: x′ = γ(x − vt) and t′ = γ(t − vx/c²), with γ = 1/√(1 − v²/c²), which the paper writes ξ = β(x − vt) and τ = β(t − vx/V²)
Another route
The map from its requirements, for programmers
Start from a candidate map x′ = a(x − vt), t′ = bt + dx with unknown coefficients, and add requirements one at a time: light at c in both directions, a map back of the same kind, no preferred direction in space, and nothing changed at v = 0. One map survives. Writing it as a table of coefficients is a later way of seeing it; the paper solves equations.
Arrives at: the map of § 3: x′ = γ(x − vt) and t′ = γ(t − vx/c²), with γ = 1/√(1 − v²/c²), which the paper writes ξ = β(x − vt) and τ = β(t − vx/V²)
Rebuilding this paper is a different exercise from reading it, and long enough to be worth doing on its own. The capstone carries both halves, the kinematics and the electrodynamic sections that follow it, and marks the two steps the paper chooses rather than derives: Rebuild the electrodynamics of moving bodies. It is optional, and nothing above depends on it.