Across the planet

How light carries your call through glass

Optical fibre carries your call as flashes of light through a strand of glass thinner than a hair: light for a one, dark for a zero. A laser sends the flashes in, the glass keeps them inside for tens of kilometres, and a receiver turns them back into data at the far end. Fibre optic internet, phone calls and the links between cities and countries all travel this way. Today one fibre carries many colours of light at once, each with its own stream of ones and zeros. In American English it is spelled fiber.

0 km80 km160 km0 km40 km80 kmEXCHANGEYOUR CITYYOUR CALL0110 1001AMPLIFIERREGENERATOREXCHANGE160 KM AWAY80 KM AWAYYOUR FRIEND
Try it
Purple: your callKey
  • Purple: your call
  • Other colours: other calls and data
  • Hut by the road: the amplifier
  • Hut by the road: the regenerator

100% of the light left in the glassof the light left in the glass

160 km of fibre · seven colours ready to send

Press a button, or click the cable or the hut to look inside.Press a button, or tap the cable or the hut to look inside.

Switch to 1988, the year the first fibre crossed the Atlantic: one colour of light, and a regenerator every 40 km or so that turned it into electricity and back.

Anatomy of an optical fibre link: one call between two exchanges 160 km apart, as it works today and as it worked in 1988. The rooms are drawn big and the field between them small. The colours stand for wavelengths of infrared light, which no eye can see.

  1. Follow one call

    Press Play to watch the call, or scroll down and the drawing follows you one step at a time. Try it, under the drawing, makes your own call.Press Play to watch the call, or Next to go one step at a time. Try it, under the drawing, makes your own call.

  2. Step 1 of 6

    Your voice becomes ones and zeros

    You call a friend in a city 160 km away. Your phone system measures your voice 8,000 times a second and sends each measurement as a number, written in ones and zeros. At the exchange in your city, a rack gathers your call with other calls and data going the same way.

    How many ones and zeros make up a call?

    An ordinary phone call needs 64,000 a second in each direction. That is 8,000 measurements a second, each written with 8 bits, and a bit is a one or a zero.

    By the time your call reaches the fibre, it is only numbers.

    Sources: ITU-T G.711: pulse code modulation of voice frequencies (1988)

  3. Step 2 of 6

    A laser flashes them out as light

    On the bench, a laser takes your ones and zeros and turns them into light: a flash for a one, dark for a zero. It switches far too fast for any eye to follow. The laser itself is a chip about the size of a grain of sand, inside the small box you see.

    Can you see the light?

    No. It is infrared light with a wavelength of about 1.55 micrometres, longer than the red light eyes can see. Glass loses the least light at that wavelength, so long links use it.

    The drawing paints each wavelength in its own colour, so you can tell them apart. Your call's light is purple.

    In 1988, the lasers on TAT-8, the first fibre cable across the Atlantic, sent 280 million ones and zeros a second, at a wavelength of 1.3 micrometres.

    Sources: Nobel Prize: popular information, the physics prize (2009); Nobel Prize: scientific background, the physics prize (2009); IEEE: Milestone, TAT-8, the first fibre-optic cable across an ocean (2016)

  4. Step 3 of 6

    Many colours share one fibre

    Six more lasers stand beside yours, each tuned to its own wavelength, its own colour, and each carrying other calls and data. Short yellow cords take their light to a combiner, which sends all seven colours down one fibre. They travel together without mixing, the way radio stations share the air. Engineers call this wavelength division multiplexing, or WDM.

    How many colours fit in one fibre?

    The ITU, the United Nations agency for telecoms, sets the colours on a grid around 193.1 terahertz, a wavelength of about 1,552.5 nanometres. With the colours 50 gigahertz apart, the band where glass loses least, from 1,530 to 1,565 nanometres, holds about 80 of them. The drawing shows seven.

    In 1988 a fibre carried one colour. All the calls on it took turns, a few ones and zeros at a time.

    Sources: ITU-T G.694.1: spectral grids for WDM applications (2020); ITU-T G.652: single-mode optical fibre and cable (2024)

  5. Step 4 of 6

    The glass keeps the light inside

    The cable runs under the field in a duct. Inside it, the fibre is a strand of glass 0.125 mm across. At its centre sits the core, about 0.009 mm across, made of glass that bends light slightly more than the cladding around it. So whenever the light strays towards the edge, it reflects back into the core. Physicists call this total internal reflection, and it keeps the light in the glass for kilometre after kilometre.

    Look inside The fibre

    1. 1Coating
    2. 2Cladding
    3. 3Core
    4. 4Light

    About 80 colours can share one fibre, each with its own stream of flashes. The drawing shows seven.

    1. 1Coating
    2. 2Cladding
    3. 3Core
    4. 4Light

    1 colour of light on each fibre, at 1.3 micrometres, on TAT-8 in 1988. The glass was the same kind as today.

    Why doesn't the light leak out?

    It is the same effect you see from under water. Light going from water into air at a shallow angle does not get out at all. It reflects back into the water. Light in the core meets the cladding at just such a shallow angle, so the edge of the core works like a perfect mirror.

    The light is fast even in glass. It needs about 5 millionths of a second for each kilometre, so it covers about 200,000 km a second, two thirds of its speed in empty space. Over the 160 km in the drawing that adds up to 0.8 thousandths of a second. The drawing runs it 6,000 times slower.

    Sources: Nobel Prize: popular information, the physics prize (2009); Nobel Prize: scientific background, the physics prize (2009); ITU-T G.652: single-mode optical fibre and cable (2024); ITU-T G.114: one-way transmission time (2003); ITU-T G.694.1: spectral grids for WDM applications (2020)

  6. Step 5 of 6

    An amplifier tops the light up

    Even this clear glass loses a little light on every kilometre. After 80 km, less than 1% of it is left. So every 80 km or so the cable comes up into a hut by the road. Inside, an amplifier makes the light strong again. It is a coil of fibre with the metal erbium in it, fed with energy by a pump laser. It boosts every colour at once, and the light never leaves the glass.

    Look inside The amplifier

    1. 1Fibre in
    2. 2Pump laser
    3. 3Erbium fibre
    4. 4Fibre out

    630 times stronger light from 3 m of erbium fibre, in the first such amplifier, at Southampton in 1987

    1. 1Photodiode
    2. 2Circuit board
    3. 3Laser
    4. 4Fibre in and out

    280 million ones and zeros a second through each regenerator on TAT-8, the first fibre cable across the Atlantic

    What was in the hut in 1988?

    A regenerator. A photodiode turned the weak light into electricity, a circuit board read the ones and zeros and cleaned them up, and a new laser sent them on as fresh light. It worked on one colour, at 1.3 micrometres, where glass loses more light, so the huts stood about 40 km apart.

    The erbium amplifier came out of a lab at the University of Southampton in 1987. There, 3 m of fibre with erbium in it made the light up to 630 times stronger. Amplifiers like it have since replaced most of the regenerators.

    Sources: ITU-T G.652: single-mode optical fibre and cable (2024); ITU-T G.692: optical interfaces for systems with optical amplifiers (1998); ITU-T G.977: optically amplified submarine cable systems (2015); ITU-T G.957: optical interfaces for SDH equipment and systems (2006); AT&T Technical Journal: lasers and photodetectors for submarine lightwave cables (1985); Electronics Letters: a low-noise erbium-doped fibre amplifier (1987); Nobel Prize: scientific background, the physics prize (2009)

  7. Step 6 of 6

    The colours split, and light turns back into data

    At the far exchange, a splitter sends each colour down its own cord to its own receiver. There a photodiode turns light into a tiny electric current: current for a one, none for a zero. The rack turns your numbers back into sound and sends your call on to your friend. Your voice has spent 0.8 thousandths of a second in the glass.

    Why glass and not copper?

    Light carries far more. It can carry tens of thousands of times more information than radio waves.

    Glass also shrugs off the weather. Unlike copper, it is not affected by lightning, and unlike radio, it is not affected by bad weather.

    The same light, in the same kind of glass, carries calls under the oceans too, with amplifiers in pods on the seabed.

    Sources: Nobel Prize: popular information, the physics prize (2009); AT&T Technical Journal: lasers and photodetectors for submarine lightwave cables (1985)

Look inside: 1988 and today

The glass hardly changed. The light in it did: dozens of colours instead of one, and amplifiers that boost them all without turning them into electricity.

The same glass, and the box in the hut, 38 years apart. Point at a part, or tap it, to see what it does.

1988

Today

The fibre

  1. 1Coating
  2. 2Cladding
  3. 3Core
  4. 4Light

1 colour of light on each fibre, at 1.3 micrometres, on TAT-8 in 1988. The glass was the same kind as today.

The fibre

  1. 1Coating
  2. 2Cladding
  3. 3Core
  4. 4Light

About 80 colours can share one fibre, each with its own stream of flashes. The drawing shows seven.

Colours of light on one fibreIEEE; ITU-T G.694.1; ITU-T G.652

1

At 1.3 micrometres

About 80

50 gigahertz apart, near 1.55 micrometres

What tops up the lightAT&T Technical Journal; Nobel Prize

Regenerator

Light into electricity, and back into new light

Amplifier

Erbium fibre boosts every colour, as light

Distance between hutsITU-T G.957; ITU-T G.692

About 40 km

About 80 km

Ones and zeros a second, one pair of fibres across the AtlanticIEEE; Google

280 million

TAT-8

About 20 million million

Dunant, 250 terabits a second on 12 pairs

The glass itselfITU-T G.652

Single-mode

The ITU's standard fibre, first set out in 1984

Single-mode

The same standard, revised in 2024

The amplifier

  1. 1Photodiode
  2. 2Circuit board
  3. 3Laser
  4. 4Fibre in and out

280 million ones and zeros a second through each regenerator on TAT-8, the first fibre cable across the Atlantic

The amplifier

  1. 1Fibre in
  2. 2Pump laser
  3. 3Erbium fibre
  4. 4Fibre out

630 times stronger light from 3 m of erbium fibre, in the first such amplifier, at Southampton in 1987

How clear the glass became

Light fades as it travels through glass, and engineers measure the loss in decibels per kilometre. Losing 20 decibels means 99 parts in 100 of the light are gone. So a fibre's loss per kilometre tells you how far its light gets before only 1% is left.

How far light gets before 99% of it is lost

  • Glass fibres before 1966About 1,000 decibels per km

    20 m
  • Charles Kao's target, 196620 decibels per km

    1 km
  • Corning's first fibre, 197017 decibels per km

    1.2 km
  • Corning, a few years later4 decibels per km, at 850 nanometres

    5 km
  • Fibre today, at 1.55 micrometresUnder 0.2 decibels per km

    Over 100 km

Worked out from each glass's loss per kilometre. The first fibres lost 99% of their light in 20 m. Kao showed in 1966 that most of the loss came from impurities in the glass, not from the glass itself.

Nobel Prize; IEEE

Light left after 1 km

95 in 100

Today, 95 in every 100 parts of the light are still there after a full kilometre of fibre. Kao's 1966 goal was 1 in 100.

Nobel Prize

How it came to be

  1. 1880

    Speech on a beam of light

    Alexander Graham Bell and his assistant Charles Sumner Tainter send speech 1,300 feet, about 400 m, on a beam of light with the photophone. Bell later called it his greatest invention, greater than the telephone.

    IEEE History Center: the unknown Bell

  2. 1966

    The glass is the problem

    In London, Charles Kao shows that glass fibres lose their light because of impurities in the glass. Purify it, he says, and light could carry calls for kilometres. He set a target of 1% of the light left after 1 km.

    Nobel Prize: popular information, the physics prize (2009)

  3. 1970

    Clear enough to use

    At Corning Glass Works in New York State, Robert Maurer, Donald Keck and Peter Schultz make a fibre that loses 17 decibels per kilometre, better than Kao's target.

    IEEE: Milestone, the first low-loss optical fibre (2012)

  4. 1975

    The first working links

    The first optical fibre links in everyday service open in the United Kingdom, and soon after in the United States and Japan.

    Nobel Prize: scientific background, the physics prize (2009)

  5. 1987

    Light that boosts light

    At the University of Southampton, a team shows that 3 m of fibre with erbium in it can make light up to 630 times stronger. Erbium amplifiers go on to replace most regenerators.

    Electronics Letters: a low-noise erbium-doped fibre amplifier (1987)

  6. 1988

    Fibre crosses the ocean

    TAT-8, the first fibre-optic cable across an ocean, enters service on 14 December between North America and Europe. It uses one colour of light, at 1.3 micrometres, and carries 40,000 calls at once.

    IEEE: Milestone, TAT-8, the first fibre-optic cable across an ocean (2016)

  7. 2009

    A Nobel Prize for the glass

    Charles Kao shares the Nobel Prize in Physics for his work on carrying light in fibres for communication, which by then carried almost all the world's calls and data.

    Nobel Prize: popular information, the physics prize (2009)

Where Voxbi fits

Voxbi, a cloud phone system hosted in the European Union, sends your calls over the internet as data, so between cities and countries they travel as light in fibre like this.

See it in Voxbi

Keep exploring