Ethane
| Ethane | | |
| General |
|---|
| Systematic name | Ethane |
| Other names | dimethyl, ethyl hydride methylmethane |
| Molecular formula | C2H6 |
| SMILES | CC |
| InChI | InChI=1/C2H6 /c1-2/h1-2H3 |
| Molar mass | 30.07 g/mol |
| Appearance | colorless gas |
| CAS number | [74-84-0] |
| Structure |
|---|
| Symmetry group | Staggered phase: D3d |
| Properties |
|---|
| Density and phase | 1.212 kg/m3, gas |
| Solubility in water | 4.7 g/100 ml (? °C) |
>| Melting point-182.76 °C (90.34 K) |
| Boiling point | -88.6 °C (184.5 K) |
| Acidity (pKa) | 50 |
| Hazards |
|---|
| MSDS | External MSDS |
| EU classification | Highly flammable (F+) |
| NFPA 704 | |
| R-phrases | |
| S-phrases | , , , |
| Flash point | -135 °C |
Autoignition temperature | 472 °C |
| Explosive limits | 3.0–12.5% |
| RTECS number | KH3800000 |
| Supplementary data page |
|---|
Structure & properties | n, εr, etc. |
Thermodynamic data | Phase behaviour Solid, liquid, gas |
| Spectral data | UV, IR, NMR, MS |
| Related compounds |
|---|
| Related alkanes | Methane Propane |
| Related compounds | Ethanol |
Except where noted otherwise, data are given for materials in their standard state (at 25°C, 100 kPa) Infobox disclaimer and references |
|
Ethane is a
chemical compound with
chemical formula C
2H
6. It is the only two-carbon
alkane, that is, an
aliphatic hydrocarbon. At
standard temperature and pressure, ethane is a colourless, odourless
gas.
Ethane is isolated on an industrial scale from
natural gas, and as a byproduct of
petroleum refining. Its chief use is as
petrochemical feedstock for
ethylene production.
Ethane was first prepared synthetically in 1834 by
Michael Faraday, by the
electrolysis of a
potassium acetate solution, but at the time, he mistook the hydrocarbon product of this reaction for
methane, and did not investigate it further. During the period 1847–1849, in an effort to vindicate the
radical theory of
organic chemistry,
Hermann Kolbe and
Edward Frankland produced ethane by the reductions of
propionitrile (ethyl cyanide) and
ethyl iodide with
potassium metal, and, as did Faraday, by the electrolysis of aqueous acetates. They, however, mistook the product of these reactions for
methyl radical, rather than the dimer of methyl, ethane. This error was corrected in 1864 by
Carl Schorlemmer, who showed that the product of all these reactions was in fact ethane.
Its name was made from the name of
ether, which at first meant
diethyl ether.
In the laboratory, ethane may be conveniently prepared by
Kolbe electrolysis. In this technique, an aqueous solution of an
acetate salt is
electrolysed. At the
anode, acetate is oxidized to produce
carbon dioxide and
methyl radicals, and the highly reactive methyl radicals combine to produce ethane:
CH3COOâˆ' â†' CH
3• +
CO2 +
eâˆ': CH
3• + •CH
3 â†' C
2H
6Another method, the oxidation of
acetic anhydride by
peroxides, is conceptually similar.
The chemistry of ethane also involves chiefly
free radical reactions. Ethane can react with the
halogens, especially
chlorine and
bromine, by
free radical halogenation. This reaction proceeds through the propagation of the
ethyl radical:
C
2H
5• +
Cl2 â†'
C2H5Cl + Cl•: Cl• + C
2H
6 â†' C
2H
5• +
HClBecause halogenated ethanes can undergo further free radical halogenation, this process results in a mixture of several halogenated products. In the chemical industry, more selective chemical reactions are used for the production of any particular two-carbon halocarbon.
Combustion
The complete
combustion of ethane releases 1561 kJ/mol, or 51.9 kJ/g, of heat, and produces
carbon dioxide and
water according to the
chemical equationC
2H
6 + 3½
O2 â†' 2
CO2 + 3
H2O + 1561 kJ/mol
Combustion occurs by a complex series of free-radical reactions.
Computer simulations of the
chemical kinetics of ethane combustion have included hundreds of reactions. An important series of reaction in ethane combustion is the combination of an ethyl radical with
oxygen, and the subsequent breakup of the resulting
peroxide into ethoxy and hydroxyl radicals.
C
2H
5• +
O2 â†' C
2H
5OO•: C
2H
5OO• + HR â†' C
2H
5OOH +
•R: C
2H
5OOH â†' C
2H
5O• + •OH
The principal carbon-containing products of incomplete ethane combustion are single-carbon compounds such as
carbon monoxide and
formaldehyde. One important route by which the carbon-carbon bond in ethane is broken to yield these single-carbon products is the decomposition of the ethoxy radical into a
methyl radical and formaldehyde, which can in turn undergo further oxidation.
C
2H
5O• â†' CH
3• +
CH2OSome minor products in the incomplete combustion of ethane include
acetaldehyde,
methane,
methanol, and
ethanol. At higher temperatures, especially in the range 600–900 °C,
ethylene is a significant product. It arises via reactions like
C
2H
5• +
O2 â†'
C2H4 + •OOH
Similar reactions (although with species other than oxygen as the hydrogen abstractor) are involved in the production of ethylene from ethane in
steam cracking.
After
methane, ethane is the second-largest component of
natural gas. Natural gas from different gas fields varies in ethane content from less than 1% to over 6% by volume. Prior to the 1960s, ethane was typically not separated from the methane component of natural gas, but simply burnt along with the methane as a fuel. Today, however, ethane is an important
petrochemical feedstock, and it is separated from the other components of natural gas in most well-developed gas fields. Ethane can also be separated from
petroleum gas, a mixture of gaseous hydrocarbons that arises as a byproduct of
petroleum refining.
Ethane is most efficiently separated from methane by liquefying it at cryogenic temperatures. Various refrigeration strategies exist: the most economical process presently in wide use employs turboexpansion, and can recover over 90% of the ethane in natural gas. In this process, chilled gas expands through a
turbine; as it expands, its temperature drops to about -100 °C. At this low temperature, gaseous methane can be separated from the liquefied ethane and heavier hydrocarbons by
distillation. Further distillation then separates ethane from the
propane and heavier hydrocarbons.
The chief use of ethane is in the chemical industry, in the production of
ethylene by
steam cracking. When diluted with steam and briefly heated to very high temperatures (900 °C or more), heavy hydrocarbons break down into lighter hydrocarbons, and
saturated hydrocarbons become
unsaturated. Ethane is favored for ethylene production because the steam cracking of ethane is fairly selective for ethylene, while the steam cracking of heavier hydrocarbons yields a product mixture poorer in ethylene, and richer in heavier
olefins such as
propylene and
butadiene, and in
aromatic hydrocarbons.
Experimentally, ethane is under investigation as a feedstock for other commodity chemicals. Oxidative chlorination of ethane has long appeared to be a potentially more economical route to
vinyl chloride than ethylene chlorination. Many processes for carrying out this reaction have been
patented, but poor selectivity for vinyl chloride and corrosive reaction conditions (specifically, a
hydrochloric acid-containing reaction mixture at temperatures greater than 500 °C) have discouraged the commercialization of most of them. Presently,
INEOS operates a 1000 t/a ethane-to-vinyl chloride pilot plant at
Wilhemshaven in
Germany.
Similarly, the
Saudi Arabian firm
SABIC has announced construction of a 30,000 t/a plant to produce
acetic acid by ethane oxidation at
Yanbu. This economic viability of this process may rely on the low cost of ethane near Saudi old fields, and it may not be competitive with
methanol carbonylation elsewhere in the world.
Ethane can be used as a refrigerant in cryogenic refrigeration systems. On a much smaller scale, in scientific research, liquid ethane is used to
vitrify water-rich samples for
electron microscopy. A thin film of water, quickly immersed in liquid ethane at -150 °C or colder, freezes too quickly for water to crystallize. This rapid freezing does not disrupt the structure of
soft objects present in the liquid state, as the formation of
ice crystals can do.
At room temperature, ethane is a flammable gas. When mixed with air at 3.0% – 12.5% by volume, it forms an
explosive mixture.
Some additional precautions are necessary where ethane is stored as a cryogenic liquid. Direct contact with liquid ethane can result in severe
frostbite. In addition, the vapors evaporating from liquid ethane are, until they warm to room temperature, heavier than air and can creep along the ground or gather in low places, and if they encounter an ignition source, can flash back to the body of ethane from which they evaporated.
Containers recently emptied of ethane may contain insufficient
oxygen to support life. Beyond this
asphyxiation hazard, ethane poses no known acute or chronic toxicological risk. It is not known or suspected to be a
carcinogen.
 |
A photograph of Titan's surface, taken from an altitude of 16 km by the Huygens probe. The dark features appear to be drainage channels, but the probe found no evidence for liquids presently on the surface of Titan. |
Ethane has been detected as a trace component in the atmospheres of all four
giant planets, and in the atmosphere of
Saturn's moon
Titan. Ethane in these atmospheres results from the Sun's
photochemical action on methane gas, also present in these atmospheres:
ultraviolet photons of shorter
wavelengths than 160
nm can photo-dissociate the methane molecule into a
methyl radical and a
hydrogen atom. When two methyl radicals recombine, the result is ethane:
CH4 â†' CH
3• + •H: CH
3• + •CH
3 â†' C
2H
6In the case of Titan, it was once widely hypothesized that ethane produced in this fashion rained back onto the moon's surface, and over time had accumulated into hydrocarbon seas or oceans covering much of the moon's surface. Infrared telescopic observations cast significant doubt on this hypothesis, and the
Huygens probe, which landed on Titan in 2005, failed to observe any surface liquids, although it did photograph features that could be presently dry drainage channels.
In 1996, ethane was detected in
Comet Hyakutake, and it has since been detected in some other
comets. The existence of ethane in these distant solar system bodies may implicate ethane as a primordial component of the
solar nebula from which the sun and planets are believed to have formed.
* Michael Faraday (1834). Experimental researches in electricity: Seventh series.
Philosophical Transactions, 124:77–122.
* Hermann Kolbe, Edward Frankland (1849). On the products of the action of potassium on cyanide of ethyl.
Journal of the Chemical Society, 1:60–74.
* Edward Frankland (1850). On the isolation of the organic radicals.
Journal of the Chemical Society, 2:263–296.
* Hermann Kolbe (1850). Researches on the electrolysis of organic compounds.
Journal of the Chemical Society, 2:157–184.
* Carl Schorlemmer (1864).
Annalen der Chimie, 132:234.
* Michael J. Mumma
et al. (1996). Detection of Abundant Ethane and Methane, Along with Carbon Monoxide and Water, in Comet C/1996 B2 Hyakutake: Evidence for Interstellar Origin.
Science, 272:1310–1314.
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