All practice pages/Interatomic theory/Elements

10Ne20.18

Element 10, a noble gas

Neon

The gas that glows red-orange in a sign tube, and one of the least reactive substances there is.

At a glance

Symbol
Ne
Atomic number
10
Average atomic mass
20.18
Group
18
Period
2
Family
noble gas
Electron configuration
1s² 2s² 2p⁶, or [He] 2s² 2p⁶
Valence electrons
8
Electronegativity
none; it forms no compounds

On the table

123456789101112131415161718123456757-7189-103HHeLiBeBCNOFNeNaMgAlSiPSClArKCaScTiVCrMnFeCoNiCuZnGaGeAsSeBrKrRbSrYZrNbMoTcRuRhPdAgCdInSnSbTeIXeCsBaLaCePrNdPmSmEuGdTbDyHoErTmYbLuHfTaWReOsIrPtAuHgTlPbBiPoAtRnFrRaAcThPaUNpPuAmCmBkCfEsFmMdNoLrRfDbSgBhHsMtDsRgCnNhFlMcLvTsOg

Period 2, group 18. The other noble gases are tinted, and every cell opens its own article.

Electrons and bonding

Neon has 10 electrons, one for every proton, so the atom carries no charge. Below are the same 10 electrons written two ways.

Simple form: electrons per shell

Ne
shell 12shell 28
Counting outward from the nucleus: 2, 8. The outer shell is picked out.

Orbital form: electrons per subshell

1s² 2s² 2p⁶

Short form: [He] 2s² 2p⁶, where [He] stands for the 2 electrons helium already has.

2s²↑↓
2p⁶↑↓↑↓↑↓
The boxes hold the electrons beyond [He]. Each box is one orbital and takes two electrons at most, spinning opposite ways. They spread out singly before they pair up.

How to read the two

The simple form counts electrons shell by shell. The orbital form says which subshell each one sits in: s holds 2, p holds 6, d holds 10 and f holds 14. Shell 2 here is 2s² 2p⁶, and 2 + 6 is 8.

Neon sits in period 2 and has 2 shells. The period number counts the shells.

What that means for bonding

Ne

The outer shell holds 8 electrons. Those are the ones neon can lose, gain or share, so they are the ones that decide what it bonds with. For a main-group element the group number gives that count: group 18 means 8.

A full valence shell, so it has almost no tendency to gain, lose or share electrons, and it exists as single atoms.

Properties

State at 25 °C
gas
What it looks like
colorless, odorless gas
Melting point
−248.6 °C
Boiling point
−246.1 °C
Density
0.900 g/L at 0 °C and 1 atm

Where it is found

About 18 parts per million of air. It is the fifth most abundant element in the universe but rare on Earth, because as a light, unreactive gas it escaped into space while the planet formed. All of it is collected as a byproduct of separating liquid air into oxygen and nitrogen.

Discovery and name

William Ramsay and Morris Travers found it in 1898 by slowly boiling liquid air and examining each fraction; it glowed crimson in their spectrum tube. Ramsay's 13-year-old son suggested the Latin novum, new, and they chose the Greek neos instead.

What it is used for

Neon signs, though only the red-orange ones are pure neon; other colors come from argon, mercury vapor and colored glass or coatings. Neon also goes into the lasers that print patterns on computer chips, helium-neon lasers, high-voltage indicators and, as a liquid, cryogenic cooling.