Matter & Energy · Depth 2 · Introductory · 7 min read

Light & Waves

What waves are, how sound travels, the electromagnetic spectrum from radio waves to gamma rays, and how light reflects, bends and interferes.

On this page
  1. What this part of the map covers
  2. What a wave is
  3. Sound
  4. Light and the electromagnetic spectrum
  5. The speed of light
  6. Reflection, refraction and colour
  7. Diffraction and interference
  8. The math (optional)
  9. A short history
  10. Common misconceptions
  11. Going further
  12. Real-life examples
  13. Evidence & sources

What this part of the map covers

Mechanical waves and electromagnetic waves are two important ways that energy moves around the world.[5] Water waves and sound are mechanical waves; light is electromagnetic.[5] This page covers both kinds.

What a wave is

A mechanical wave forms when energy is passed through a medium, such as water or air.[18] In a transverse wave, the vibration is at right angles to the direction the wave travels, as on a vibrating string; in a longitudinal wave, it is along that direction.[23, 20]

The distance from one crest of a wave to the next is its wavelength.[5, 19] The number of crests passing a point each second is its frequency, measured in hertz (Hz): one hertz is one cycle per second.[5, 17] The longer the wavelength, the lower the frequency.[19, 16]

Sound

Sound waves are longitudinal: they travel by alternately squeezing (compression) and stretching (rarefaction) the air or water they pass through.[17, 18] Because sound needs a medium, it cannot travel through the vacuum of space.[5] The higher the pitch, the higher the frequency, and loudness goes with the wave’s amplitude, or intensity.[17, 18]

The speed of sound depends on the air or gas it travels through, not on what made the sound, and in air it rises with temperature.[16, 17] At sea level and 15 °C, sound travels at about 340 metres per second.[17] When a sound source moves, its waves bunch up in front of it and spread out behind it.[16] This Doppler shift happens with any kind of wave, light included.[15]

Light and the electromagnetic spectrum

The words light, electromagnetic waves and radiation all name the same thing: electromagnetic energy.[5] Unlike sound, electromagnetic waves need no medium, so they can cross the vacuum of space.[5, 19] Moving along the spectrum from long to short wavelengths, the energy increases.[5]

  • Radio waves have the longest wavelengths, from the length of a football to larger than our planet.[7]
  • Microwaves can get through haze, light rain, snow, clouds and smoke, which makes them useful for satellite communication.[8]
  • Infrared light is invisible to the eye, but we can feel it as heat.[9]
  • Visible light is typically the wavelengths from 380 to 700 nanometres (billionths of a metre).[10] The US Geological Survey (USGS) gives 0.4 to 0.7 micrometres.[19]
  • Ultraviolet light has shorter wavelengths than visible light; we can’t see it, but bumblebees can.[11]
  • X-rays have wavelengths between 0.03 and 3 nanometres.[12]
  • Gamma rays have the shortest wavelengths and the most energy.[13]

The speed of light

In a vacuum, light travels at 299,792,458 metres per second.[2, 1] That number is exact: since 1983 the metre has been defined as the distance light travels in a vacuum in 1/299,792,458 of a second.[3, 2] Light travels more slowly in air than in a vacuum, and more slowly still in water.[6, 27]

Reflection, refraction and colour

For any electromagnetic wave, the angle at which it strikes a surface equals the angle at which it bounces off: the law of reflection.[24] Refraction is the change of direction when light passes into a material with a different refractive index, a number comparing light’s speed in the material with its speed in a vacuum.[25, 6] It is why an object partly under water looks distorted, and it lets a lens focus light, as in eyeglasses and magnifying glasses.[25, 26]

The refractive index changes with wavelength, an effect called dispersion.[25] A prism separates white light into the colours of the rainbow because each colour is a different wavelength, from violet, the shortest, to red, the longest.[10, 19] An object’s colour is the wavelengths it reflects; the others are absorbed.[6, 24]

Diffraction and interference

Diffraction is the bending and spreading of waves around an obstacle, strongest when the obstacle is about as big as the wavelength.[6] Overlapping sound waves can reinforce or interfere with each other.[17] In the early 1800s Thomas Young shone light through two small, closely spaced openings and saw bright bands separated by dark regions.[22, 27] Only a wave could make such a pattern.[22]

Yet light is also made of packets of energy called photons, and all light has both wave-like and particle-like properties.[5, 22] The Modern Physics page picks up this story.

The math (optional)

For sound, speed equals wavelength times frequency.[17] For light, wavelength equals the speed of light divided by the frequency.[14]

sound: speed = wavelength × frequency

Our own example: a sound with a wavelength of 1 metre, travelling at 340 metres per second, has a frequency of 340 Hz.[17]

A short history

Ibn al-Haytham (Alhazen) gave the first correct explanation of vision, that light reflects from an object into the eye.[28] Willebrord Snell found the law of refraction in 1621 but never published it; Descartes published it first, in 1637.[27, 29]

In 1678 Christiaan Huygens argued for a wave theory of light.[30] Isaac Newton concluded that light is a stream of particles, and published Opticks in 1704.[33, 34] Young published his interference results in 1801, and the wave theory went on to win wide acceptance in the 19th century.[27, 34]

Around 1862 James Clerk Maxwell calculated that electromagnetic fields travel at about the speed of light, and proposed that light is electromagnetic.[31, 27] Heinrich Hertz proved radio waves exist in the late 1880s.[7] He did not expect much of them: “I do not think that the wireless waves I have discovered will have any practical application.”[32]

Common misconceptions

“The siren itself changes its note as it passes.” The change is in what a listener hears: for someone riding on the fire engine, the siren’s frequency stays the same.[15]

“Light must be either a wave or a particle.” It shows both kinds of behaviour.[5, 22]

Going further

Start with Energy & Work, then see Electricity & Magnetism, Heat & Thermodynamics and Space Telescopes. Lasers, the eye and quantum optics are left for deeper pages.

Real-life examples

  • How far away is the storm?

    The sound of thunder takes about 5 seconds to travel 1 mile, so you can estimate how far away lightning struck by counting the seconds between seeing the flash and hearing the thunder.[21]

  • A passing siren

    When an ambulance or fire engine passes with its siren on, the pitch you hear changes. This is the Doppler shift: waves from a source coming towards you arrive at a higher frequency, and from a source moving away at a lower one.[15, 16]

  • A microwave oven

    A microwave oven uses microwaves about 12 centimetres long to make water and fat molecules in food rotate. The interaction of these spinning molecules creates heat, and the food cooks.[8]

  • An X-ray picture

    Bones are dense and absorb more X-rays than skin does, so they leave shadows on X-ray film while the skin looks transparent.[12]

  • A blue sky

    Nitrogen and oxygen in the air scatter the shorter wavelengths of sunlight, blue and violet. Violet is scattered even more than blue, but the sky looks blue to us because our eyes are more sensitive to blue light.[6]

Connected across the map

Evidence & sources

Level 1 · Established

Supported by extensive evidence and broad scientific consensus.

Why this level? Waves, sound and the electromagnetic spectrum are long-established physics taught in every introductory course. The page is written from US government science agencies (NIST, NASA, USGS and NOAA), CERN's teaching material and Rutgers University, with history from MacTutor (University of St Andrews), the Stanford Encyclopedia of Philosophy and Cambridge's Whipple Museum, and optics notes from Molecular Expressions (Florida State University).

This is a Knowledge Atlas editorial classification of the sources we could find, not a certificate of truth. How we evaluate knowledge

Sources

Based on 34 sources from 10 institutions: NIST, NASA, USGS, NOAA, CERN and 5 more.

Show all 34 sourcesHide the list
  1. AuthoritativeNational Institute of Standards and Technology· Government agencyMeet the Constants (NIST SI redefinition)Opened and checked against this page on 30 Sept 2026
  2. AuthoritativeNational Institute of Standards and Technology· Government agencySI Units - Length (NIST)Opened and checked against this page on 29 Sept 2026
  3. AuthoritativeNational Institute of Standards and Technology· Government agencyMeter (NIST SI redefinition)Opened and checked against this page on 30 Sept 2026
  4. AuthoritativeNational Aeronautics and Space Administration· Government agencyIntroduction to the Electromagnetic Spectrum (NASA Science)Opened and checked against this page on 29 Sept 2026
  5. AuthoritativeNational Aeronautics and Space Administration· Government agencyAnatomy of an Electromagnetic Wave (NASA Science)Opened and checked against this page on 29 Sept 2026
  6. AuthoritativeNational Aeronautics and Space Administration· Government agencyWave Behaviors (NASA Science)Opened and checked against this page on 29 Sept 2026
  7. AuthoritativeNational Aeronautics and Space Administration· Government agencyRadio Waves (NASA Science)Opened and checked against this page on 29 Sept 2026
  8. AuthoritativeNational Aeronautics and Space Administration· Government agencyMicrowaves (NASA Science)Opened and checked against this page on 29 Sept 2026
  9. AuthoritativeNational Aeronautics and Space Administration· Government agencyInfrared Waves (NASA Science)Opened and checked against this page on 29 Sept 2026
  10. AuthoritativeNational Aeronautics and Space Administration· Government agencyVisible Light (NASA Science)Opened and checked against this page on 29 Sept 2026
  11. AuthoritativeNational Aeronautics and Space Administration· Government agencyUltraviolet Waves (NASA Science)Opened and checked against this page on 29 Sept 2026
  12. AuthoritativeNational Aeronautics and Space Administration· Government agencyX-Rays (NASA Science)Opened and checked against this page on 29 Sept 2026
  13. AuthoritativeNational Aeronautics and Space Administration· Government agencyGamma Rays (NASA Science)Opened and checked against this page on 29 Sept 2026
  14. AuthoritativeNational Aeronautics and Space Administration· Government agencyThe Electromagnetic Spectrum (Imagine the Universe)Opened and checked against this page on 30 Sept 2026
  15. AuthoritativeNational Aeronautics and Space Administration· Government agencyDoppler Shift (NASA Imagine the Universe)Opened and checked against this page on 29 Sept 2026
  16. AuthoritativeNational Aeronautics and Space Administration· Government agencyDoppler Effect (Glenn Research Center Beginner's Guide)Opened and checked against this page on 30 Sept 2026
  17. AuthoritativeNational Aeronautics and Space Administration· Government agencySpeed of Sound (educator guide, grades 9-12)Opened and checked against this page on 30 Sept 2026
  18. AuthoritativeNational Aeronautics and Space Administration· Government agencyThe Physics of Waves (Quesst: science of sound)Opened and checked against this page on 30 Sept 2026
  19. AuthoritativeU.S. Geological Survey· Government agencyLandsat Glossary (USGS)Opened and checked against this page on 30 Sept 2026
  20. AuthoritativeU.S. Geological Survey· Government agencyBody waves inside the Earth (USGS)Opened and checked against this page on 30 Sept 2026
  21. AuthoritativeNational Oceanic and Atmospheric Administration· Government agencyHow far away is lightning? (NOAA NESDIS)Opened and checked against this page on 30 Sept 2026
  22. AuthoritativeCERN· IntergovernmentalScience Centre to Go: the double slit experimentOpened and checked against this page on 30 Sept 2026
  23. ScholarlyRutgers University· UniversityStanding Waves on a String (Rutgers physics lab handout)Opened and checked against this page on 30 Sept 2026
  24. ReliableMolecular Expressions (National MagLab and Florida State University)· UniversityReflection of Light (Molecular Expressions)Opened and checked against this page on 30 Sept 2026 · License: All rights reserved, Florida State University Research Foundation (single copy for personal, non-commercial use); wording is never copied
  25. ReliableMolecular Expressions (National MagLab and Florida State University)· UniversityRefraction of Light (Molecular Expressions)Opened and checked against this page on 30 Sept 2026 · License: All rights reserved, Florida State University Research Foundation (single copy for personal, non-commercial use); wording is never copied
  26. ReliableMolecular Expressions (National MagLab and Florida State University)· UniversityLenses and Geometrical Optics (Molecular Expressions)Opened and checked against this page on 30 Sept 2026 · License: All rights reserved, Florida State University Research Foundation (single copy for personal, non-commercial use); wording is never copied
  27. ScholarlyMacTutor History of Mathematics (University of St Andrews)· UniversityLight through the ages: Ancient Greece to MaxwellOpened and checked against this page on 30 Sept 2026
  28. ScholarlyMacTutor History of Mathematics (University of St Andrews)· UniversityIbn al-Haytham - Biography (MacTutor)Opened and checked against this page on 29 Sept 2026
  29. ScholarlyMacTutor History of Mathematics (University of St Andrews)· UniversityWillebrord Snell - Biography (MacTutor)Opened and checked against this page on 29 Sept 2026
  30. ScholarlyMacTutor History of Mathematics (University of St Andrews)· UniversityChristiaan Huygens - Biography (MacTutor)Opened and checked against this page on 29 Sept 2026
  31. ScholarlyMacTutor History of Mathematics (University of St Andrews)· UniversityJames Clerk Maxwell - Biography (MacTutor)Opened and checked against this page on 29 Sept 2026
  32. ScholarlyMacTutor History of Mathematics (University of St Andrews)· UniversityHeinrich Hertz - Biography (MacTutor)Opened and checked against this page on 29 Sept 2026
  33. ScholarlyStanford Encyclopedia of Philosophy· Academic publisherNewton's Philosophy (Stanford Encyclopedia of Philosophy)Opened and checked against this page on 30 Sept 2026
  34. AuthoritativeUniversity of Cambridge· UniversitySir Isaac Newton's Opticks (Whipple Library)Opened and checked against this page on 30 Sept 2026