néon - definizione. Che cos'è néon
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Cosa (chi) è néon - definizione

CHEMICAL ELEMENT WITH SYMBOL NE AND ATOMIC NUMBER 10; RARE GAS
Element 10; Solar neon; Liquid neon; Neon gas; Atomic number 10; Metargon; Ne (element); History of neon; Properties of neon
  • The first evidence for isotopes of a stable element was provided in 1913 by experiments on neon plasma. In the bottom right corner of [[J. J. Thomson]]'s photographic plate are the separate impact marks for the two isotopes neon-20 and neon-22.
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  • Neon [[gas-discharge lamp]]s forming the symbol for neon
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Neon         
Charles Duff. An object-oriented extension of FORTH, for the Mac. Inheritance, SANE floating-point, system classes and objects for Mac interfacing, overlays. Sold by Kriya Systems, 1985-1988. Modified, made PD and renamed Yerk.
neon         
1.
Neon lights or signs are made from glass tubes filled with neon gas which produce a bright electric light.
In the city squares the neon lights flashed in turn.
= fluorescent
ADJ: ADJ n
2.
Neon is a gas which occurs in very small amounts in the atmosphere.
...inert gases like neon and argon.
N-UNCOUNT
neon         
¦ noun
1. the chemical element of atomic number 10, an inert gaseous element of the noble gas group. (Symbol: Ne)
2. fluorescent lighting and signs using neon or another gas.
[as modifier] very bright or fluorescent in colour.
Origin
C19: from Gk, lit. 'something new', neut. of the adjective neos.

Wikipedia

Neon

Neon is a chemical element with the symbol Ne and atomic number 10. It is a noble gas. Neon is a colorless, odorless, inert monatomic gas under standard conditions, with about two-thirds the density of air. It was discovered (along with krypton and xenon) in 1898 as one of the three residual rare inert elements remaining in dry air, after nitrogen, oxygen, argon and carbon dioxide were removed. Neon was the second of these three rare gases to be discovered and was immediately recognized as a new element from its bright red emission spectrum. The name neon is derived from the Greek word, νέον, neuter singular form of νέος (neos), meaning 'new'. Neon is chemically inert, and no uncharged neon compounds are known. The compounds of neon currently known include ionic molecules, molecules held together by van der Waals forces and clathrates.

During cosmic nucleogenesis of the elements, large amounts of neon are built up from the alpha-capture fusion process in stars. Although neon is a very common element in the universe and solar system (it is fifth in cosmic abundance after hydrogen, helium, oxygen and carbon), it is rare on Earth. It composes about 18.2 ppm of air by volume (this is about the same as the molecular or mole fraction) and a smaller fraction in Earth's crust. The reason for neon's relative scarcity on Earth and the inner (terrestrial) planets is that neon is highly volatile and forms no compounds to fix it to solids. As a result, it escaped from the planetesimals under the warmth of the newly ignited Sun in the early Solar System. Even the outer atmosphere of Jupiter is somewhat depleted of neon, although for a different reason.

Neon gives a distinct reddish-orange glow when used in low-voltage neon glow lamps, high-voltage discharge tubes and neon advertising signs. The red emission line from neon also causes the well known red light of helium–neon lasers. Neon is used in some plasma tube and refrigerant applications but has few other commercial uses. It is commercially extracted by the fractional distillation of liquid air. Since air is the only source, it is considerably more expensive than helium.