10NeNeon

Neon is a chemical element; it has symbol Ne and atomic number 10. It is the second noble gas in the periodic table. Neon is a colorless, odorless, inert monatomic gas under standard conditions, with approximately two-thirds the density of air.

Neon was discovered in 1898 alongside krypton and xenon, identified as one of the three remaining rare inert elements in dry air after the removal of nitrogen, oxygen, argon, and carbon dioxide. Its discovery was marked by the distinctive bright red emission spectrum it exhibited, leading to its immediate recognition as a new element. The name neon originates from the Greek word νέον, a neuter singular form of νέος (neos), meaning 'new'. Neon is a chemically inert gas; although neon compounds do exist, they are primarily ionic molecules or fragile molecules held together by van der Waals forces.

The synthesis of most neon in the cosmos resulted from the nuclear fusion within stars of oxygen and helium through the alpha-capture process. Despite its abundant presence in the universe and Solar System—ranking fifth in cosmic abundance following hydrogen, helium, oxygen, and carbon—neon is comparatively scarce on Earth. It constitutes about 18. 2 ppm of Earth's atmospheric volume and a lesser fraction in the Earth's crust. The high volatility of neon and its inability to form compounds that would anchor it to solids explain its limited presence on Earth and the inner terrestrial planets. Neon's high volatility facilitated its escape from planetesimals under the early Solar System's nascent Sun's warmth.

Neon's notable applications include its use in low-voltage neon glow lamps, high-voltage discharge tubes, and neon advertising signs, where it emits a distinct reddish-orange glow. This same red emission line is responsible for the characteristic red light of helium–neon lasers. Although neon has some applications in plasma tubes and as a refrigerant, its commercial uses are relatively limited. It is primarily obtained through the fractional distillation of liquid air, making it significantly more expensive than helium due to air being its sole source.

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Atomic properties

Standard atomic weight20.1797 ±6·10-4
Atomic mass20.1797 u

Atomic radii

Radius (calculated)38 pm
Covalent radius58 pm
Van der Waals radius154 pm

Atomic shell

Electron configurationHe 2s2 2p6
Ionization energy(1st) 21.56454 eV
(2nd) 40.96297 eV
(3rd) 63.4233 eV
(4th) 97.19 eV
(5th) 126.247 eV
Shell model
Electrons
k-shell:2
l-shell:8

Physical properties

Phasegaseous
Density9·10-4 g·cm−3 (273 K)
Molar volumesolid: 1.323·10-5 m3·mol−1
Speed of sound435 m·s−1

Temperatures

Melting point24.56 K
Boiling point27.1 K
Liquid range2.544 K
Triple point24.55 K @ 43.37 kPa
Critical point44.49 K @ 2.768 MPa

Enthalpies

Melting enthalpy0.34 kJ·mol-1
Enthalpy of vaporization1.75 kJ·mol-1
Binding energy0 kJ·mol-1

Heat and conductivity

Specific heat capacity1,030 J·kg−1·K−1
Thermal conductivity0.0491 W·m-1·K-1

Magnetism

Magnetismdiamagnetic
Magnetic susceptibility-6.74·10-6 cm3·mol−1 (298 K)

Optical properties

Refractive index1

Chemical properties

Basicity-
Oxidation state-

Electronegativity

Sanderson scale4.5
Allred-Rochow scale4.84
Mulliken scale3.98
Allen scale4.787
Ghosh-Gupta scale11.3 eV
Nagle scale4.89

Other properties

Natural occurrenceprimordial
Crystal structureFace-centered cubic
Goldschmidt Classificationatmophile
Superconductorwithout transition temperature
Price/kg240 USD

Natural abundances

satellite_alt
Universe
1.3·106 ppb ≈ 1.3·1016 M☉
sunny
Sun
1·106 ppb ≈ 1.98·1015 Mt
destruction
public
Earth’s crust
3 ppb ≈ 83.1 Mt
water_drop
Oceans
0.12 ppb ≈ 164 kt
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