Neon is a colorless, odorless, inert monoatomic gas at normal temperatures and pressures. It is the second lightest noble gas and glows reddish-orange in a vacuum discharge tube when subjected to high voltage electricity, which is how it’s commonly used for signs.
A team of chemists, led by Sir William Ramsay and Morris Travers, discovered neon in 1898 while working with argon. They evaporated liquid argon, which separated into krypton and neon gas, and ran the first sample through an atomic spectrometer—which allowed them to see each atom’s energy spectrum—and found it glowed a brilliant crimson. They named the new element neon, based on its Greek word meaning “new.”
As a noble gas, neon has an unpaired electron and a full octet of protons and neutrons. This means it’s very stable and doesn’t react with other elements. It is considered an electronegative element, which means it’s more attracted to negative electrons than positive ones. This allows it to form molecular ions and excimers, which are short-lived dimeric molecules.
While neon is relatively common in the universe and solar system (it’s fifth in cosmic abundance, after hydrogen, oxygen, helium, and carbon), it’s very rare on Earth. It only composes 0.0018 percent of our atmosphere, according to the Jefferson Laboratory. Most of the neon in our planet’s atmosphere was created inside stars during nuclear fusion. It is also produced in laboratories by distilling air from liquid helium. Liquid neon is sometimes used as a cryogenic refrigerant, since it has the narrowest temperature range in which it can be liquid.