NEON

(Ne), chemical element, inert gas of Group 0 (noble gases) of the periodic table, used in electric signs and fluorescent lamps. Colourless, odourless, tasteless, and lighter than air, neon gas occurs in minute quantities in the Earth's atmosphere and trapped within the rocks of the Earth's crust. Though neon is about 31/2 times as plentiful as helium in the atmosphere, dry air contains only 0.0018 percent neon by volume. This element is more abundant in the cosmos than on Earth. Neon liquefies at -246.048 C (-411 F) and freezes at a temperature only 21/2 lower. When under low pressure, it emits a bright orange-red light if an electrical current is passed through it. This property is utilized in neon signs (which first became familiar in the 1920s), in some fluorescent and gaseous conduction lamps, and in high-voltage testers. Neon was discovered (1898) by the British chemists Sir William Ramsay and Morris W. Travers as a component of the most volatile fraction of liquefied crude argon obtained from air. It was immediately recognized as a new element by its unique glow when electrically stimulated. The gas is produced industrially by the fractional distillation of liquid air; the most volatile fraction is composed of a mixture of helium, neon, and nitrogen. Nitrogen is removed by condensation under increased pressure and reduced temperature, followed by adsorption on highly cooled charcoal. Neon is separated from helium by selective adsorption on activated charcoal at low temperatures. Processing 88,000 pounds of liquid air will produce one pound of neon. No stable chemical compounds of neon have been observed. Molecules of the element consist of single atoms. Natural neon is a mixture of three stable isotopes: neon-20 (90.92 percent); neon-21 (0.26 percent); and neon-22 (8.82 percent). atomic number 10 atomic weight 20.183 melting point -248.67 C (-415.5 F) boiling point -246.048 C (-411 F) density (1 atm, 0 C) 0.89990 g/litre valence 0 electronic config. 2-8 or 1s22s22p6