SIMETRIUM .COM ΔN 0.37 → 0.01
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aether v ? 30 km/s → L 11 m · λ 589 nm ΔN < 0.01 aetheraetheraetheraetheraetheraether aether aether 00.10.20.30.4 expected 0.37 fringe shift ΔN SYMBOL PLATE c = 299 792 458 m/s Cleveland 1887 · Am. J. Sci. 34
Letter case
Lower-case Latin aether, in Greek αἰθήρ — «the upper air». There was no symbol and no unit: the aether was a medium, not a measure.
Do not confuse
The physicists’ luminiferous aether is not the chemist’s ether, diethyl ether (C₂H₅)₂O. Nor is it the «ether» of radio talk — that is just a word for broadcasting.
On the plate — the interferometer seen from above on its stone slab. A lamp shines onto a half-silvered mirror, the beam splits in two, the two beams travel to mirrors along and across, and meet again in the telescope. The lilac streaks are the aether wind that was supposed to blow against the Earth. The slab turns through a quarter of a revolution. In the eyepiece on the right the bright fringes barely move. Below, the marker first runs out to 0.37 — the shift that was expected — and comes back to zero, which is what was measured.
Quantity passport · obsolete · a medium for light

Luminiferous aether

Obsolete quantity with no unit · replaced by the constant speed of light

Cleveland, July 1887. Michelson and Morley lay a stone slab on a mercury float, set mirrors on it and turn it slowly. The Earth flies round the Sun at 30 km/s, and if light is a wave in a stationary aether, the oncoming aether wind should shift the fringes in the eyepiece by 0.4 of a fringe. They waited for the shift. It never came.

The aether was invented because a wave needs a medium. Sound travels through air, a wave through water — so light must travel through something that fills empty space. The aether had to be stiffer than steel to carry such fast waves, and yet not get in the way of the planets. The 1887 experiment showed that light moves the same way in every direction, however the Earth is flying. In 1905 Einstein made this a law, and the aether was no longer needed.

Notationaether · luminiferous aether · no symbol
How it was soughtvia the Earth’s speed through the aether — the shift of interference fringes
What was assumeda stationary medium · the speed of light depends on the observer’s motion
Introduced and withdrawnHuygens, 1690 · Fresnel, 1818 · Michelson and Morley, 1887 · Einstein, 1905
Today’s notationc = 299 792 458 m/s exactly, since 1983 — by the definition of the metre
Typical values0.37 fringe — expected in 1887 · under 0.01 — observed · 10⁻¹⁷ — precision today
To the conversion To the interferometer
01 · Definition

The medium light runs through

If light is a wave in the aether, it has a speed relative to the aether, c. An observer flying through the aether should see light faster when meeting it head-on and slower when chasing it. The Earth flies round the Sun at 30 km/s — one ten-thousandth of c. That was the difference people tried to catch.

Such a correction cannot be measured directly; it is too small. Michelson compared two paths of light: along the wind and across it. Like a swimmer going there and back along a river and then across it: the trip along the current takes longer. The difference is the square of a small ratio, (v/c)² = 10⁻⁸. Interference makes it visible: a shift of a fraction of a wavelength moves the bright fringes.

c — speed of light, m/s · v — speed relative to the aether · L — arm length, m · λ — wavelength, m · ΔN — fringe shift · β = v/c · γ = 1/√(1−β²)
Interactive · two swimmers on a river

Who gets back first

A river of width L flows from left to right; the lilac arrows are the current. Two swimmers swim at the same speed c: the golden one goes along the river and back, the blue one goes across to the far bank and back. The bars below are their travel times. The swimmer going across always gets back first. In the same way, a beam travelling across the aether wind should have beaten a beam travelling along it.

golden — along, blue — acrossbars — travel time, in units of 2L/c
Current v / c
Along
γ² = 1/(1−β²)
Across
γ = 1/√(1−β²)
Difference
≈ β²/2 for small β

Interactive · the Michelson–Morley interferometer, 1887

Turn the slab and watch the eyepiece

There is one main action — the «Turn the slab» button. The stone slab floats on mercury and slowly turns. In the centre it is seen from above: a golden lamp, blue beams running to the mirrors at the ends of the arms, with 16 reflections each, 11 m of path in all. The lilac strokes are the aether wind; its speed is set by the slider. On the right is the eyepiece: bright and dark fringes. If the aether exists, the fringes should sway while the slab turns. Under the eyepiece is a graph: the lilac curve is the shift predicted by aether theory, the golden dots are what is actually seen. The «World with aether / World of 1887» switch shows both answers.

left: observation log, fringe shift and slab angleright: eyepiece and fringe shift against rotation angle
Main action
Aether wind v30 km/s
30 km/s is the Earth’s orbital speed. The shift grows as the square of the speed: twice as fast — four times as much.
Arm length L11 m
In 1881 Michelson had 1.2 m, and the shift was lost in the noise. In 1887 mirrors bounced the light back and forth 16 times, giving 11 m.
Expected shift
—
—
Observed shift
—
—
Slab angle
—
—
Speed through the aether, at most
—
—

—

Graph · shift against angle, against speed, and a century of precision

02 · Conversion
Fraction of the speed of light β = v/c

The aether had no unit, so we convert the speed that was being sought. The fringe shift in the interferometer grows as β², the square of the fraction of the speed of light. The Earth’s orbital speed gives β = 10⁻⁴, β² = 10⁻⁸.

Today no speed is measured «relative to the aether». There is only motion relative to the cosmic microwave background: the Sun moves through it at 370 km/s, but that is an apparent motion, not the wind of a medium.

03 · Orders of magnitude
Deviation of the speed of light Δc/c — what the experiments were hunting, from 10⁻¹⁸ to 10⁻⁴

04 · Measuring instruments
interferometer
A beam splitter, two arms, two mirrors. The beams meet and form fringes, and a shift of a tenth of a fringe is visible to the eye. The same principle works in gravitational-wave detectors, only there the arms are 4 km long.
20.5″
stellar aberration
In 1727 Bradley saw that over a year the stars trace small ellipses of 20.5 arcseconds. The telescope has to be tilted in the direction of the Earth’s motion, like an umbrella in the rain. This was the first measurement of β = 10⁻⁴.
Fizeau’s water experiment
In 1851 Fizeau sent light with and against flowing water. The current dragged the light along only partly, with the factor 1 − 1/n². Fresnel explained this by partial aether drag. Relativity derives the same number from the addition of velocities.
10⁻¹⁷
optical cavity
Michelson’s experiment today: two crystal cavities at right angles on a rotating table, with lasers locked to their frequencies. The frequencies agree to within 10⁻¹⁷ — a hundred million times more precise than in 1887.
05 · Writing rules
Correct
c = 299 792 458 m/s — exact, no uncertainty
«luminiferous aether» — a historical term, in a nineteenth-century context
ΔN = 0.37 — the fringe shift Michelson and Morley expected
β = v/c, γ = 1/√(1−β²)
Incorrect
«speed relative to the aether» — in a modern text
c ≈ 3·10⁸ m/s ± … — c has had no uncertainty since 1983
«the experiment failed» — it gave a clear null result
confusing the luminiferous aether with the chemical ether
06 · Neighbouring units

Phlogiston vanished without a trace; caloric left the calorie behind. The aether left the most of all: Maxwell’s equations were written for an elastic aether, and they outlived it. And the constant speed of light that abolished the aether has itself become a foundation of measurement: the metre is defined through it.

07 · Historical section
1.5 m × 1.5 m · 0.3 mmercury float
stone slab
Metrological note

The 1887 experiment is a model of how to set up a measurement against noise. The sandstone slab floated on mercury so that it could be turned without jolts. Observations were made in a basement, at noon and in the evening, sixteen readings per revolution. They expected 0.4 of a fringe; the scatter of the readings was about 0.01.

The null result gave an upper bound: the Earth’s speed through the aether is less than about 5—8 km/s. A hundred years later the constancy of the speed of light became part of the definition of the metre. Since 1983 the metre has been the distance light travels in 1/299 792 458 of a second.

ΔN < 0.01
fringes in the eyepiece
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