Neon is a colorless, odorless noble gas that glows reddish orange when subjected to an electric discharge. It is a minor component of Earth’s atmosphere and was discovered in 1898 by two British chemists. It is the fourth most abundant element in the universe but only makes up about 0.0018% of the Earth’s atmosphere.
Unlike other noble gases, neon does not form compounds with any other elements. However, it does share a chemical bond with fluorine which can give it the same glow that you see in classic neon signs.
This colorless, odorless noble gas is produced by fractional distillation of liquid air. It has a typical density of 0.9g/cm3 and is very inert under normal conditions. When subjected to an alternating current, however, it emits a glowing red/orange light that is used for a wide variety of purposes, including in neon advertising signs that are so popular around the world.
Georges Claude invented the first glass neon tubes in 1910, and his work was responsible for the brightly lit, iconic neon signage we all know and love. When a few thousand volts are applied to the neon, it separates its atoms into positive and negative electrodes and, when these atoms collide with each other, they create the visible light.
Neon is a relatively rare element on Earth but it is very common in stars and is created during nuclear fusion within large mass stars as they reach the high-energy stages of their lives. Neon is also found in planet-forming disks and helps astronomers study the process of how stars and their planets form. Neon gets its name from the Greek word neos meaning “new”.