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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
Best practices and pitfalls
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.
Quick check
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.
Spectral Power Distributions and Why RGB Is Not Enough
The SPD curves every emission source produces.
Physics · 3The Physics of Light, Wavelength, and Spectrum
Photons and energy levels - why atoms emit specific lines.
Physics · 48Fluorescence, Phosphorescence, and Optical Brighteners
The phosphor that converts blue LED light into white.
Colorimetry · 8CIE XYZ Explained
How a spectrum becomes the three numbers of a color.
Colorimetry · 11Metamerism Explained
Why two different spectra can look like the same color.
Physics · 28Color Temperature and White Balance
What "warm" and "cool" white actually mean.