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Emission: Neon, LEDs, and Gas-Discharge Light

Most color in this library is reflected - light bounces off a surface and loses some wavelengths on the way. But some things make their own light: a neon tube, a sodium street lamp, a phone screen, the LED above your desk. Emissive sources don't subtract from a spectrum - they are the spectrum, and often a strange, spiky one. This is the interactive guide to light that glows, and why the source you light a room with decides what color everything in it appears.

Physics · 70 4 Live Demos ~33 min read Light sources
lines
Emission, not reflection
589 nm
Sodium's signature
blue+phosphor
How white LEDs work
CRI
How faithfully colors show
01

Light that makes itself

There are two ways for something to have color. Reflective color - an apple, a wall, a printed page - starts with a light source and subtracts: the surface absorbs some wavelengths and bounces the rest. Emissive color - a flame, a star, a neon tube, an LED - adds light into the world that wasn't there before. The color of an emitter is simply the shape of the spectrum it produces.

And those shapes vary wildly. The Sun and a hot filament give a smooth continuous spectrum across all visible wavelengths. A gas-discharge tube gives a handful of razor-thin lines. A fluorescent tube mixes lines with phosphor bands. A white LED is a blue spike with a broad phosphor hump. Each shape can look "white," or colored, and - crucially - each renders the objects it illuminates differently.

The one rule that explains everything below: a surface can only reflect wavelengths the light actually contains. Light with gaps in its spectrum simply cannot make those missing colors appear on anything. Emission shapes set the limits of every color you see under them.
02

Line spectra: the atomic fingerprint

Energize a thin gas - run a current through it - and its atoms jump to higher energy levels, then drop back, releasing the difference as photons. Because an atom's energy levels are quantized, only specific energy gaps exist, so only specific wavelengths come out: sharp, bright emission lines. The pattern is unique to each element - a barcode you can read to identify it across the galaxy. It is also why each gas tube has its own signature glow. Pick an element and see its lines and color.

Interactive 01 · Gas-discharge spectra

The emission lines of energized elements

Each bar is the visible spectrum; the bright vertical lines are the wavelengths that element actually emits, with height showing relative strength. The swatch is the color your eye builds by integrating those lines. Neon is a thicket of red-orange lines; sodium is essentially one yellow line; mercury is a few blues and a green. That is why their tubes glow as they do.

03

From lines to a color

How does a set of separate wavelengths become a single perceived color? Your three cone types each respond to the whole bundle at once and report just three numbers - so the brain can't tell a mixture of lines from a smooth spectrum that excites the cones the same way. Two narrow lines, a red and a green, land on the eye as yellow - a perfect metamer of a single yellow wavelength, even though no yellow light is present. Slide two lines and watch them fuse.

Interactive 02 · Two-line metamer

Two wavelengths, one perceived color

Place two emission lines anywhere in the spectrum. The swatch shows the single color your eye builds from the pair. A red line near 630 nm and a green near 530 nm combine into yellow that you cannot distinguish from a pure 580 nm beam - the heart of why three numbers (RGB) can stand in for a whole spectrum.

04

The white-LED trick

There is no such thing as a "white" LED chip. The white light in your home is a clever fake: a blue LED (a narrow spike near 450 nm) is coated with a phosphor that absorbs part of the blue and re-emits a broad band of yellow-green. The blue that leaks through plus the phosphor's yellow add up to white. More phosphor and the white goes warm; less and it goes cool and bluish. The tell-tale sign is the dip between the blue spike and the phosphor hump - the "cyan gap" that limits color rendering. Build one.

Interactive 03 · White-LED builder

Blue pump plus phosphor equals white

The curve is the LED's spectral power: a tall blue spike and a broad phosphor band. Add more phosphor to warm the white (lower color temperature); reduce it to let the blue dominate for a cool, harsh white. The swatch and the estimated correlated color temperature update as you balance the two - exactly the dial an LED maker tunes.

05

Why the source decides the color

Here is the payoff. Because a surface can only reflect what the light contains, the spectrum of your light source quietly rewrites the color of everything it touches. Under smooth daylight, all colors render faithfully. Under a low-pressure sodium lamp - one yellow line - reds, greens, and blues have nothing to reflect and collapse into yellows and grays; that orange motorway glow is monochrome. The Color Rendering Index (CRI) puts a number on this. Switch the light over a row of objects.

Interactive 04 · Color rendering

The same objects under different sources

The curve is the chosen source's spectrum; the swatches below are six fixed-reflectance objects rendered under it - computed by multiplying each object's reflectance by the source spectrum and integrating, exactly as your eye does. Daylight renders everything cleanly; incandescent warms and dulls blues; the LED is decent but uneven; sodium flattens the whole row to near-monochrome.

06

A tour of real sources

Every artificial light you meet is one of a few spectral shapes. Knowing the shape tells you the color it glows and how well it renders.

Incandescent / halogen
A hot filament: smooth, continuous, heavy in red. Warm and flattering, excellent rendering, but inefficient - mostly heat.
Fluorescent
A mercury discharge (UV + visible lines) exciting phosphors. Spiky; rendering ranges from poor to good depending on the phosphor blend.
Neon & noble gases
Pure line spectra. Neon glows red-orange; argon blue-violet; helium pale gold. The colors of classic signage are raw atomic lines.
Low-pressure sodium
Essentially one yellow line (589 nm). The most efficient lamp ever made and the worst at color - everything looks monochrome.
White LED (phosphor)
Blue chip plus yellow phosphor. Efficient and tunable, with a characteristic blue spike and cyan dip; good modern CRI.
RGB LED & OLED
Three (or more) narrow emitters combined. Great for vivid, tunable color and displays, but three lines render some object colors imperfectly.
07

Best practices and pitfalls

Read CRI and CCT
Color temperature tells you warm vs cool; CRI (or the stricter TM-30) tells you how faithfully colors render. You need both.
Beware spiky white
Two lights can share a CCT yet have very different spectra. A cheap LED and daylight both read "5000 K" but render reds differently.
Watch the cyan gap
The dip between an LED's blue spike and phosphor can mute cyans and skin. Higher-CRI LEDs add red phosphor to fill it.
Match light to task
Art, retail, and medical work need high CRI; a parking lot just needs lumens. Sodium's efficiency is fine where color doesn't matter.
Metamers can break
Two samples that match under one source can mismatch under another (metameric failure). Check critical matches under the real light.
Photograph under known light
Spiky sources fool auto white balance and can leave color casts. Shoot a gray reference and set white balance from it.
"A reflective color is a conversation between a surface and a light. Change the light and you change what the surface is allowed to say - which is why the same red shirt is crimson at noon, brown under sodium, and slightly off under a cheap bulb." Editorial summary · the source has the last word
The takeaway: emitters are their spectrum. Continuous spectra render everything; line spectra render only what their lines allow. White LEDs fake white with blue + phosphor, and the gaps in any source's spectrum are gaps in every color it can ever show.
08

Test your understanding

Six questions on emission, line spectra, white LEDs, and color rendering. Instant feedback, no scores recorded - a wrong answer comes with a short explanation.

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Continue your journey

Emission is one half of every color story; here is where it connects to spectra, measurement, and the light that fills a room.