Difference between revisions of "Neon" - New World Encyclopedia

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{{Elementbox_header | number=10 | symbol=Ne | name=neon | left=[[fluorine]] | right=[[sodium]] | above=[[helium|He]] | below=[[argon|Ar]] | color1=#c0ffff | color2=green }}
 
{{Elementbox_header | number=10 | symbol=Ne | name=neon | left=[[fluorine]] | right=[[sodium]] | above=[[helium|He]] | below=[[argon|Ar]] | color1=#c0ffff | color2=green }}
 
{{Elementbox_series | [[noble gas]]es }}
 
{{Elementbox_series | [[noble gas]]es }}
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{{Elementbox_footer | color1=#c0ffff | color2=green }}
 
{{Elementbox_footer | color1=#c0ffff | color2=green }}
  
'''Neon''' (chemical symbol '''Ne''', [[atomic number]] 10) is a [[chemical element]] that occurs in trace amounts in the air. It is a nearly inert gas and is classified as a [[noble gas]]. Under ordinary conditions, it is colorless, but in a vacuum discharge tube, it gives a reddish-orange glow.
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'''Neon''' (chemical symbol '''Ne''', [[atomic number]] 10) is the fourth most abundant [[chemical element]] in the universe, but it is just a trace element in the air. As a member of the [[noble gas]] series, it is nearly inert. Under ordinary conditions, it is colorless, but in a vacuum discharge tube, it gives a reddish-orange glow. Consequently, the main use of neon is to make flashy signs for advertising. In addition, a mixture of helium and neon gases is used to make a gas laser, and liquid neon is a low-temperature refrigerant.
 
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== Discovery and occurrence ==
 
== Discovery and occurrence ==
  
Neon (from the [[Greek language|Greek]] word ''νέος'', meaning "new") was discovered by Scottish chemist [[William Ramsay]]* and English chemist [[Morris Travers]]* in 1898, during their studies of liquefied air.
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Neon (from the [[Greek language|Greek]] word ''νέος'', meaning "new") was discovered by Scottish chemist [[William Ramsay]] and English chemist [[Morris Travers]] in 1898, during their studies of liquefied air.
  
 
Neon is the fourth most abundant element in the [[universe]].[http://education.jlab.org/itselemental/ele010.html] In the [[Earth's atmosphere]], however, it occurs in only trace amounts—at 1 part in 65,000. It is industrially produced by cryogenic fractional distillation of liquefied air.
 
Neon is the fourth most abundant element in the [[universe]].[http://education.jlab.org/itselemental/ele010.html] In the [[Earth's atmosphere]], however, it occurs in only trace amounts—at 1 part in 65,000. It is industrially produced by cryogenic fractional distillation of liquefied air.
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Neon is less dense than air and is the second-lightest noble gas, after helium. Its low density suggests that it may slowly leak out of the Earth's atmosphere and escape into space, thus providing an explanation for its scarcity on Earth. By contrast, [[argon]] (another noble gas) is denser than air and remains within the Earth's atmosphere.
 
Neon is less dense than air and is the second-lightest noble gas, after helium. Its low density suggests that it may slowly leak out of the Earth's atmosphere and escape into space, thus providing an explanation for its scarcity on Earth. By contrast, [[argon]] (another noble gas) is denser than air and remains within the Earth's atmosphere.
  
Neon has over 40 times the refrigerating capacity of liquid helium and three times that of liquid [[hydrogen]] (on a per unit volume basis). For most applications, it is a less expensive [[refrigerant]]* than helium.
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Neon has over 40 times the refrigerating capacity of liquid helium and three times that of liquid [[hydrogen]] (on a per unit volume basis). For most applications, it is a less expensive [[refrigerant]] than helium.
  
Of all the rare gases, neon has the most intense discharge at normal voltages and currents. As noted above, it glows reddish-orange in a [[vacuum discharge tube]]*.
+
Of all the rare gases, neon has the most intense discharge at normal voltages and currents. As noted above, it glows reddish-orange in a [[vacuum discharge tube]].
  
 
=== Isotopes ===
 
=== Isotopes ===
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*<sup>21</sup>Ne (0.27%), with 11 neutrons in the nucleus of each atom; and
 
*<sup>21</sup>Ne (0.27%), with 11 neutrons in the nucleus of each atom; and
 
*<sup>22</sup>Ne (9.25%), with 12 neutrons in the nucleus of each atom.
 
*<sup>22</sup>Ne (9.25%), with 12 neutrons in the nucleus of each atom.
 
<sup>21</sup>Ne and <sup>22</sup>Ne are [[nucleogenic]] and their variations are well understood. By contrast, <sup>20</sup>Ne is not known to be nucleogenic and the causes of its variation in the [[Earth]] have been hotly debated. The principal [[nuclear reaction]]s that generate neon [[isotope]]s are [[neutron emission]], [[alpha decay]] reactions on <sup>24</sup>Mg and <sup>25</sup>Mg, which produce <sup>21</sup>Ne and <sup>22</sup>Ne, respectively. The [[alpha particle]]s are derived from [[uranium]]-series [[decay chain]]s, while the [[neutron]]s are mostly produced by secondary reactions from alpha particles. The net result yields a trend towards lower <sup>20</sup>Ne/<sup>22</sup>Ne and higher <sup>21</sup>Ne/<sup>22</sup>Ne ratios observed in uranium-rich rocks such as [[granite]]s. Isotopic analysis of exposed terrestrial [[rock (geology)|rocks]] has demonstrated the [[cosmogenic]] production of <sup>21</sup>Ne. This isotope is generated by [[spallation]] reactions on [[magnesium]], [[sodium]], [[silicon]], and [[aluminium]]. By analyzing all three isotopes, the cosmogenic component can be resolved from [[magma]]tic neon and nucleogenic neon. This suggests that neon will be a useful tool in determining cosmic [[exposure age]]s of surficial rocks and [[meteorite]]s.[http://www.onafarawayday.com/Radiogenic/Ch11/Ch11-2.htm]
 
 
Similar to [[xenon]], neon content observed in samples of [[volcano|volcanic]] [[gas]]es are enriched in <sup>20</sup>Ne, as well as nucleogenic <sup>21</sup>Ne, relative to <sup>22</sup>Ne content. The neon isotopic content of these mantle-derived samples represent a non-atmospheric source of neon. The <sup>20</sup>Ne-enriched components are attributed to exotic primordial rare gas components in the Earth, possibly representing solar neon. Elevated <sup>20</sup>Ne abundances are also found in [[diamond]]s, further suggesting a solar neon reservoir in the Earth.[http://w=ww.mantleplumes.org/Ne.html]
 
 
8888888888
 
*nucleogenesis is the process that occurred a few minutes after the Big Bang when the atomic nuclei were created.
 
 
*Cosmogenic isotopes are rare radioactive isotopes created when cosmic radiation interacts with an atomic nucleus. These isotopes are produced on Earth, in Earth's atmosphere, and in extraterrestrial items such as meteorites.
 
 
*A radiogenic nuclide is one that is produced by a process of radioactive decay.
 
  
 
== Compounds ==
 
== Compounds ==
  
Given the extreme inertness of neon, its compounds are hard to find. It does, however, appear to form an unstable [[hydrate]]*. In addition, research involving specialized techniques (including ''mass spectrometry'') has shown that neon can form various ions, either by itself or in combination with other elements. These ions include Ne<sup>+</sup>, (Ne[[argon|Ar]])<sup>+</sup>, (Ne[[hydrogen|H]])<sup>+</sup>, and ([[helium|He]]Ne<sup>+</sup>).
+
Given the extreme inertness of neon, its compounds are hard to find. It does, however, appear to form an unstable [[hydrate]]. In addition, research involving specialized techniques (including ''mass spectrometry'') has shown that neon can form various ions, either by itself or in combination with other elements. These ions include Ne<sup>+</sup>, (Ne[[argon|Ar]])<sup>+</sup>, (Ne[[hydrogen|H]])<sup>+</sup>, and ([[helium|He]]Ne<sup>+</sup>).
  
 
== Applications ==
 
== Applications ==
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* wave meter tubes
 
* wave meter tubes
 
* [[television]] tubes
 
* [[television]] tubes
 
==References==
 
 
*[http://periodic.lanl.gov/elements/10.html Los Alamos National Laboratory &ndash; Neon]
 
*[http://wwwrcamnl.wr.usgs.gov/isoig/period/ne_iig.html USGS Periodic Table - Neon]
 
  
 
== External links ==
 
== External links ==
 
+
All links retrieved November 11, 2022.
 
* [http://www.webelements.com/webelements/elements/text/Ne/index.html WebElements.com &ndash; Neon]
 
* [http://www.webelements.com/webelements/elements/text/Ne/index.html WebElements.com &ndash; Neon]
 
* [http://education.jlab.org/itselemental/ele010.html It's Elemental &ndash; Neon]
 
* [http://education.jlab.org/itselemental/ele010.html It's Elemental &ndash; Neon]
* [http://www.compchemwiki.org/index.php?title=Neon Computational Chemistry Wiki]
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*[http://wwwrcamnl.wr.usgs.gov/isoig/period/ne_iig.html USGS Periodic Table - Neon]
  
 
[[Category:Physical sciences]]
 
[[Category:Physical sciences]]
 
[[Category:Chemistry]]
 
[[Category:Chemistry]]
 
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Latest revision as of 16:18, 11 November 2022


10 fluorineneonsodium
He

Ne

Ar
Ne-TableImage.png
periodic table
General
Name, Symbol, Number neon, Ne, 10
Chemical series noble gases
Group, Period, Block 18, 2, p
Appearance colorless
Ne,10.jpg
Atomic mass 20.1797(6) g/mol
Electron configuration 1s2 2s2 2p6
Electrons per shell 2, 8
Physical properties
Phase gas
Density (0 °C, 101.325 kPa)
0.9002 g/L
Melting point 24.56 K
(-248.59 °C, -415.46 °F)
Boiling point 27.07 K
(-246.08 °C, -410.94 °F)
Critical point 44.4 K, 2.76 MPa
Heat of fusion 0.335 kJ/mol
Heat of vaporization 1.71 kJ/mol
Heat capacity (25 °C) 20.786 J/(mol·K)
Vapor pressure
P/Pa 1 10 100 1 k 10 k 100 k
at T/K 12 13 15 18 21 27
Atomic properties
Crystal structure cubic face centered
Oxidation states no data
Ionization energies
(more)
1st: 2080.7 kJ/mol
2nd: 3952.3 kJ/mol
3rd: 6122 kJ/mol
Atomic radius (calc.) 38 pm
Covalent radius 69 pm
Van der Waals radius 154 pm
Miscellaneous
Magnetic ordering nonmagnetic
Thermal conductivity (300 K) 49.1 mW/(m·K)
Speed of sound (gas, 0 °C) 435 m/s
CAS registry number 7440-01-9
Notable isotopes
Main article: Isotopes of neon
iso NA half-life DM DE (MeV) DP
20Ne 90.48% Ne is stable with 10 neutrons
21Ne 0.27% Ne is stable with 11 neutrons
22Ne 9.25% Ne is stable with 12 neutrons

Neon (chemical symbol Ne, atomic number 10) is the fourth most abundant chemical element in the universe, but it is just a trace element in the air. As a member of the noble gas series, it is nearly inert. Under ordinary conditions, it is colorless, but in a vacuum discharge tube, it gives a reddish-orange glow. Consequently, the main use of neon is to make flashy signs for advertising. In addition, a mixture of helium and neon gases is used to make a gas laser, and liquid neon is a low-temperature refrigerant.

Discovery and occurrence

Neon (from the Greek word νέος, meaning "new") was discovered by Scottish chemist William Ramsay and English chemist Morris Travers in 1898, during their studies of liquefied air.

Neon is the fourth most abundant element in the universe.[1] In the Earth's atmosphere, however, it occurs in only trace amounts—at 1 part in 65,000. It is industrially produced by cryogenic fractional distillation of liquefied air.

Notable characteristics

Neon is part of the noble gas series in the periodic table. As such, it is an extremely unreactive element. It follows helium in group 18 (former group 8A) and is placed after fluorine in period 2. The gas is composed of single atoms and is therefore described as "monatomic."

Neon is less dense than air and is the second-lightest noble gas, after helium. Its low density suggests that it may slowly leak out of the Earth's atmosphere and escape into space, thus providing an explanation for its scarcity on Earth. By contrast, argon (another noble gas) is denser than air and remains within the Earth's atmosphere.

Neon has over 40 times the refrigerating capacity of liquid helium and three times that of liquid hydrogen (on a per unit volume basis). For most applications, it is a less expensive refrigerant than helium.

Of all the rare gases, neon has the most intense discharge at normal voltages and currents. As noted above, it glows reddish-orange in a vacuum discharge tube.

Isotopes

Neon has three stable isotopes:

  • 20Ne (90.48%), with 10 neutrons in the nucleus of each atom;
  • 21Ne (0.27%), with 11 neutrons in the nucleus of each atom; and
  • 22Ne (9.25%), with 12 neutrons in the nucleus of each atom.

Compounds

Given the extreme inertness of neon, its compounds are hard to find. It does, however, appear to form an unstable hydrate. In addition, research involving specialized techniques (including mass spectrometry) has shown that neon can form various ions, either by itself or in combination with other elements. These ions include Ne+, (NeAr)+, (NeH)+, and (HeNe+).

Applications

Neon is often used in signs

The reddish-orange color that neon emits in neon lamps is widely used for advertising signs. The word "neon" has become a generic term for these types of lights, although many other gases are used to produce different colors of light.

Neon and helium may be used together to make a type of gas laser called a helium-neon laser. In addition, liquefied neon is commercially used as a cryogenic refrigerant in applications not requiring the lower temperature range attainable with liquid helium, which is more expensive.

Neon is also used in the following devices:

  • vacuum tubes
  • high-voltage indicators
  • lightning arrestors
  • wave meter tubes
  • television tubes

External links

All links retrieved November 11, 2022.

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