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Wikipedia

Ethane

Ethane (US: /ˈɛθn/ ETH-ayn, UK: /ˈ-/ EE-) is a naturally occurring organic chemical compound with chemical formula C
2
H
6
. At standard temperature and pressure, ethane is a colorless, odorless gas. Like many hydrocarbons, ethane is isolated on an industrial scale from natural gas and as a petrochemical by-product of petroleum refining. Its chief use is as feedstock for ethylene production.

Ethane

Ball and stick model of ethane
Spacefill model of ethane
Names
Preferred IUPAC name
Ethane[1]
Systematic IUPAC name
Dicarbane (never recommended[2])
Identifiers
  • 74-84-0 Y
3D model (JSmol)
  • Interactive image
1730716
ChEBI
  • CHEBI:42266 Y
ChEMBL
  • ChEMBL135626 Y
ChemSpider
  • 6084 Y
ECHA InfoCard 100.000.741
EC Number
  • 200-814-8
212
MeSH Ethane
  • 6324
RTECS number
  • KH3800000
UNII
  • L99N5N533T Y
UN number 1035
  • DTXSID6026377
  • InChI=1S/C2H6/c1-2/h1-2H3 Y
    Key: OTMSDBZUPAUEDD-UHFFFAOYSA-N Y
  • CC
Properties
C2H6
Molar mass 30.070 g·mol−1
Appearance Colorless gas
Odor Odorless
Density
  • 1.3562 kg/m3 (gas at 0 °C)[3]

544.0 kg/m3 (liquid at -88,5 °C)
206 kg/m3 (at critical point 305.322 K)

Melting point −182.8 °C; −296.9 °F; 90.4 K
Boiling point −88.5 °C; −127.4 °F; 184.6 K
Critical point (T, P) 305.32 K (32.17 °C; 89.91 °F) 48.714 bars (4,871.4 kPa)
56.8 mg L−1[4]
Vapor pressure 3.8453 MPa (at 21.1 °C)
19 nmol Pa−1 kg−1
Acidity (pKa) 50
Basicity (pKb) −36
Conjugate acid Ethanium
-37.37·10−6 cm3/mol
Thermochemistry
52.49 J K−1 mol−1
−84 kJ mol−1
−1561.0–−1560.4 kJ mol−1
Hazards
GHS labelling:
Danger
H220, H280
P210, P410+P403
NFPA 704 (fire diamond)
Flash point −135 °C (−211 °F; 138 K)
472 °C (882 °F; 745 K)
Explosive limits 2.9–13%
Safety data sheet (SDS) inchem.org
Related compounds
Related alkanes
Related compounds
Supplementary data page
Ethane (data page)
Except where otherwise noted, data are given for materials in their standard state (at 25 °C [77 °F], 100 kPa).
Y verify (what is YN ?)

Related compounds may be formed by replacing a hydrogen atom with another functional group; the ethane moiety is called an ethyl group. For example, an ethyl group linked to a hydroxyl group yields ethanol, the alcohol in beverages.

History edit

Ethane was first synthesised in 1834 by Michael Faraday, applying electrolysis of a potassium acetate solution. He mistook the hydrocarbon product of this reaction for methane and did not investigate it further.[5] The process is now called Kolbe electrolysis:

CH3COO → CH3• + CO2 + e
CH3• + •CH3 → C2H6

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)[6] and ethyl iodide[7] with potassium metal, and, as did Faraday, by the electrolysis of aqueous acetates. They mistook the product of these reactions for the methyl radical (CH3), of which ethane (C2H6) is a dimer.

This error was corrected in 1864 by Carl Schorlemmer, who showed that the product of all these reactions was in fact ethane.[8] Ethane was discovered dissolved in Pennsylvanian light crude oil by Edmund Ronalds in 1864.[9][10]

Properties edit

At standard temperature and pressure, ethane is a colorless, odorless gas. It has a boiling point of −88.5 °C (−127.3 °F) and melting point of −182.8 °C (−297.0 °F). Solid ethane exists in several modifications.[11] On cooling under normal pressure, the first modification to appear is a plastic crystal, crystallizing in the cubic system. In this form, the positions of the hydrogen atoms are not fixed; the molecules may rotate freely around the long axis. Cooling this ethane below ca. 89.9 K (−183.2 °C; −297.8 °F) changes it to monoclinic metastable ethane II (space group P 21/n).[12] Ethane is only very sparingly soluble in water.

The bond parameters of ethane have been measured to high precision by microwave spectroscopy and electron diffraction: rC−C = 1.528(3) Å, rC−H = 1.088(5) Å, and ∠CCH = 111.6(5)° by microwave and rC−C = 1.524(3) Å, rC−H = 1.089(5) Å, and ∠CCH = 111.9(5)° by electron diffraction (the numbers in parentheses represents the uncertainties in the final digits).[13]

 
Ethane (shown in Newman projection) barrier to rotation about the carbon-carbon bond. The curve is potential energy as a function of rotational angle. Energy barrier is 12 kJ/mol or about 2.9 kcal/mol.[14]

Rotating a molecular substructure about a twistable bond usually requires energy. The minimum energy to produce a 360° bond rotation is called the rotational barrier.

Ethane gives a classic, simple example of such a rotational barrier, sometimes called the "ethane barrier". Among the earliest experimental evidence of this barrier (see diagram at left) was obtained by modelling the entropy of ethane.[15] The three hydrogens at each end are free to pinwheel about the central carbon–carbon bond when provided with sufficient energy to overcome the barrier. The physical origin of the barrier is still not completely settled,[16] although the overlap (exchange) repulsion[17] between the hydrogen atoms on opposing ends of the molecule is perhaps the strongest candidate, with the stabilizing effect of hyperconjugation on the staggered conformation contributing to the phenomenon.[18] Theoretical methods that use an appropriate starting point (orthogonal orbitals) find that hyperconjugation is the most important factor in the origin of the ethane rotation barrier.[19][20]

As far back as 1890–1891, chemists suggested that ethane molecules preferred the staggered conformation with the two ends of the molecule askew from each other.[21][22][23][24]

Atmospheric and extraterrestrial edit

 
A photograph of Titan's northern latitudes. The dark features are hydrocarbon lakes containing ethane

Ethane occurs as a trace gas in the Earth's atmosphere, currently having a concentration at sea level of 0.5 ppb.[25] Global ethane quantities have varied over time, likely due to flaring at natural gas fields.[26] Global ethane emission rates declined from 1984 to 2010,[26] though increased shale gas production at the Bakken Formation in the U.S. has arrested the decline by half.[27] [28]

Although ethane is a greenhouse gas, it is much less abundant than methane, has a lifetime of only a few months compared to over a decade,[29] and is also less efficient at absorbing radiation relative to mass. In fact, ethane's global warming potential largely results from its conversion in the atmosphere to methane.[30] It has been detected as a trace component in the atmospheres of all four giant planets, and in the atmosphere of Saturn's moon Titan.[31]

Atmospheric ethane 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 → CH3• + •H
CH3• + •CH3 → C2H6

In Earth's atmosphere, hydroxyl radicals convert ethane to methanol vapor with a half-life of around three months.[29]

It is suspected that ethane produced in this fashion on Titan rains back onto the moon's surface, and over time has accumulated into hydrocarbon seas covering much of the moon's polar regions. In December 2007 the Cassini probe found at least one lake at Titan's south pole, now called Ontario Lacus because of the lake's similar area to Lake Ontario on Earth (approximately 20,000 km2). Further analysis of infrared spectroscopic data presented in July 2008[32] provided additional evidence for the presence of liquid ethane in Ontario Lacus. Several significantly larger hydrocarbon lakes, Ligeia Mare and Kraken Mare being the two largest, were discovered near Titan's north pole using radar data gathered by Cassini. These lakes are believed to be filled primarily by a mixture of liquid ethane and methane.

In 1996, ethane was detected in Comet Hyakutake,[33] 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.

In 2006, Dale Cruikshank of NASA/Ames Research Center (a New Horizons co-investigator) and his colleagues announced the spectroscopic discovery of ethane on Pluto's surface.[34]

Chemistry edit

The chemistry of ethane 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:

C2H5• + Cl2C2H5Cl + Cl•
Cl• + C2H6 → C2H5• + HCl

The combustion of ethane releases 1559.7 kJ/mol, or 51.9 kJ/g, of heat, and produces carbon dioxide and water according to the chemical equation:

2 C2H6 + 7 O2 → 4 CO2 + 6 H2O + 3120 kJ

Combustion may also occur without an excess of oxygen, yielding carbon monoxide, acetaldehyde, methane, methanol, and ethanol. At higher temperatures, especially in the range 600–900 °C (1,112–1,652 °F), ethylene is a significant product:

2 C2H6 + O2 → 2 C2H4 + H2O

Such oxidative dehydrogenation reactions are relevant to the production of ethylene.[35]

Production edit

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 more than 6% by volume. Prior to the 1960s, ethane and larger molecules were typically not separated from the methane component of natural gas, but simply burnt along with the methane as a fuel. Today, ethane is an important petrochemical feedstock and 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 produced 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 a turboexpander, and can recover more than 90% of the ethane in natural gas. In this process, chilled gas is expanded through a turbine, reducing the temperature to approximately −100 °C (−148 °F). 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.

Usage edit

The chief use of ethane is the production of ethylene (ethene) 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 alkenes (olefins), such as propene (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 producing this reaction have been patented, but poor selectivity for vinyl chloride and corrosive reaction conditions (specifically, a reaction mixture containing hydrochloric acid at temperatures greater than 500 °C) have discouraged the commercialization of most of them. Presently, INEOS operates a 1000 t/a (tonnes per annum) ethane-to-vinyl chloride pilot plant at Wilhelmshaven 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. The economic viability of this process may rely on the low cost of ethane near Saudi oil 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 cryo-electron microscopy. A thin film of water quickly immersed in liquid ethane at −150 °C or colder freezes too quickly for water to crystallize. Slower freezing methods can generate cubic ice crystals, which can disrupt soft structures by damaging the samples and reduce image quality by scattering the electron beam before it can reach the detector.

MAN Energy Solutions currently manufactures two-stroke dual fuel engines (B&W ME-GIE) which can run on both Marine diesel oil and ethane.

Health and safety edit

At room temperature, ethane is an extremely 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. Until they warm to room temperature, the vapors from liquid ethane are heavier than air and can flow along the floor or ground, gathering in low places; if the vapors encounter an ignition source, the chemical reaction can flash back to the source of ethane from which they evaporated.

Ethane can displace oxygen and become an asphyxiation hazard. Ethane poses no known acute or chronic toxicological risk. It is not a carcinogen.[36]

See also edit

References edit

  1. ^ International Union of Pure and Applied Chemistry (2014). Nomenclature of Organic Chemistry: IUPAC Recommendations and Preferred Names 2013. The Royal Society of Chemistry. p. 133. doi:10.1039/9781849733069. ISBN 978-0-85404-182-4. The saturated unbranched acyclic hydrocarbons C2H6, C3H8, and C4H10 have the retained names ethane, propane, and butane, respectively.
  2. ^ IUPAC 2014, p. 4. "Similarly, the retained names 'ethane', 'propane', and 'butane' were never replaced by systematic names 'dicarbane', 'tricarbane', and 'tetracarbane' as recommended for analogues of silane, 'disilane'; phosphane, 'triphosphane'; and sulfane, 'tetrasulfane'."
  3. ^ "Ethane – Compound Summary". PubChem Compound. US: National Center for Biotechnology Information. 16 September 2004. Retrieved 7 December 2011.
  4. ^ Lide, D. R., ed. (2005). CRC Handbook of Chemistry and Physics (86th ed.). Boca Raton (FL): CRC Press. p. 8.88. ISBN 0-8493-0486-5.
  5. ^ Faraday, Michael (1834). "Experimental researches in electricity: Seventh series". Philosophical Transactions. 124: 77–122. Bibcode:1834RSPT..124...77F. doi:10.1098/rstl.1834.0008. S2CID 116224057.
  6. ^ Kolbe, Hermann; Frankland, Edward (1849). "On the products of the action of potassium on cyanide of ethyl". Journal of the Chemical Society. 1: 60–74. doi:10.1039/QJ8490100060.
  7. ^ Frankland, Edward (1850). "On the isolation of the organic radicals". Journal of the Chemical Society. 2 (3): 263–296. doi:10.1039/QJ8500200263.
  8. ^ Schorlemmer, Carl (1864). "Ueber die Identität des Aethylwasserstoffs und des Methyls". Annalen der Chemie und Pharmacie. 132 (2): 234–238. doi:10.1002/jlac.18641320217.
  9. ^ Roscoe, H.E.; Schorlemmer, C. (1881). Treatise on Chemistry. Vol. 3. Macmillan. pp. 144–145.
  10. ^ Watts, H. (1868). Dictionary of Chemistry. Vol. 4. p. 385.
  11. ^ Van Nes, G.J.H.; Vos, A. (1978). "Single-crystal structures and electron density distributions of ethane, ethylene and acetylene. I. Single-crystal X-ray structure determinations of two modifications of ethane" (PDF). Acta Crystallographica Section B. 34 (6): 1947. Bibcode:1978AcCrB..34.1947V. doi:10.1107/S0567740878007037. S2CID 55183235.
  12. ^ "Ethane as a solid". Retrieved 2019-12-10.
  13. ^ Harmony, Marlin D. (1990-11-15). "The equilibrium carbon–carbon single-bond length in ethane". The Journal of Chemical Physics. 93 (10): 7522–7523. Bibcode:1990JChPh..93.7522H. doi:10.1063/1.459380. ISSN 0021-9606.
  14. ^ J, McMurry (2012). Organic chemistry (8 ed.). Belmont, CA: Brooks. p. 95. ISBN 9780840054449.
  15. ^ Kemp, J. D.; Pitzer, Kenneth S. (1937). "The Entropy of Ethane and the Third Law of Thermodynamics. Hindered Rotation of Methyl Groups". Journal of the American Chemical Society. 59 (2): 276. doi:10.1021/ja01281a014.
  16. ^ Ercolani, G. (2005). "Determination of the Rotational Barrier in Ethane by Vibrational Spectroscopy and Statistical Thermodynamics". J. Chem. Educ. 82 (11): 1703–1708. Bibcode:2005JChEd..82.1703E. doi:10.1021/ed082p1703.
  17. ^ Pitzer, R.M. (1983). "The Barrier to Internal Rotation in Ethane". Acc. Chem. Res. 16 (6): 207–210. doi:10.1021/ar00090a004.
  18. ^ Mo, Y.; Wu, W.; Song, L.; Lin, M.; Zhang, Q.; Gao, J. (2004). "The Magnitude of Hyperconjugation in Ethane: A Perspective from Ab Initio Valence Bond Theory". Angew. Chem. Int. Ed. 43 (15): 1986–1990. doi:10.1002/anie.200352931. PMID 15065281.
  19. ^ Pophristic, V.; Goodman, L. (2001). "Hyperconjugation not steric repulsion leads to the staggered structure of ethane". Nature. 411 (6837): 565–8. Bibcode:2001Natur.411..565P. doi:10.1038/35079036. PMID 11385566. S2CID 205017635.
  20. ^ Schreiner, P. R. (2002). "Teaching the right reasons: Lessons from the mistaken origin of the rotational barrier in ethane". Angewandte Chemie International Edition. 41 (19): 3579–81, 3513. doi:10.1002/1521-3773(20021004)41:19<3579::AID-ANIE3579>3.0.CO;2-S. PMID 12370897.
  21. ^ Bischoff, CA (1890). "Ueber die Aufhebung der freien Drehbarkeit von einfach verbundenen Kohlenstoffatomen". Chem. Ber. 23: 623. doi:10.1002/cber.18900230197.
  22. ^ Bischoff, CA (1891). "Theoretische Ergebnisse der Studien in der Bernsteinsäuregruppe". Chem. Ber. 24: 1074–1085. doi:10.1002/cber.189102401195.
  23. ^ Bischoff, CA (1891). "Die dynamische Hypothese in ihrer Anwendung auf die Bernsteinsäuregruppe". Chem. Ber. 24: 1085–1095. doi:10.1002/cber.189102401196.
  24. ^ Bischoff, C.A.; Walden, P. (1893). "Die Anwendung der dynamischen Hypothese auf Ketonsäurederivate". Berichte der Deutschen Chemischen Gesellschaft. 26 (2): 1452. doi:10.1002/cber.18930260254.
  25. ^ . Atmosphere.mpg.de. Archived from the original on 2008-12-22. Retrieved 2011-12-08.
  26. ^ a b Simpson, Isobel J.; Sulbaek Andersen, Mads P.; Meinardi, Simone; Bruhwiler, Lori; Blake, Nicola J.; Helmig, Detlev; Rowland, F. Sherwood; Blake, Donald R. (2012). "Long-term decline of global atmospheric ethane concentrations and implications for methane". Nature. 488 (7412): 490–494. Bibcode:2012Natur.488..490S. doi:10.1038/nature11342. PMID 22914166. S2CID 4373714.
  27. ^ Kort, E. A.; Smith, M. L.; Murray, L. T.; Gvakharia, A.; Brandt, A. R.; Peischl, J.; Ryerson, T. B.; Sweeney, C.; Travis, K. (2016). "Fugitive emissions from the Bakken shale illustrate role of shale production in global ethane shift". Geophysical Research Letters. 43 (9): 4617–4623. Bibcode:2016GeoRL..43.4617K. doi:10.1002/2016GL068703. hdl:2027.42/142509.
  28. ^ "One oil field a key culprit in global ethane gas increase". University of Michigan. April 26, 2016.
  29. ^ a b Aydin, Kamil Murat; Williams, M.B.; Saltzman, E.S. (April 2007). "Feasibility of reconstructing paleoatmospheric records of selected alkanes, methyl halides, and sulfur gases from Greenland ice cores". Journal of Geophysical Research. 112 (D7). Bibcode:2007JGRD..112.7312A. doi:10.1029/2006JD008027.
  30. ^ Hodnebrog, Øivind; Dalsøren, Stig B.; Myrhe, Gunnar (2018). "Lifetimes, direct and indirect radiative forcing, and global warming potentials of ethane (C2H6), propane (C3H8), and butane (C4H10)". Atmospheric Science Letters. 19 (2). Bibcode:2018AtScL..19E.804H. doi:10.1002/asl.804.
  31. ^ Brown, Bob; et al. (2008). . NASA Jet Propulsion Laboratory. Archived from the original on 2011-06-05. Retrieved 2008-07-30.
  32. ^ Brown, R. H.; Soderblom, L. A.; Soderblom, J. M.; Clark, R. N.; Jaumann, R.; Barnes, J. W.; Sotin, C.; Buratti, B.; et al. (2008). "The identification of liquid ethane in Titan's Ontario Lacus". Nature. 454 (7204): 607–10. Bibcode:2008Natur.454..607B. doi:10.1038/nature07100. PMID 18668101. S2CID 4398324.
  33. ^ Mumma, Michael J.; 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 (5266): 1310–1314. Bibcode:1996Sci...272.1310M. doi:10.1126/science.272.5266.1310. PMID 8650540. S2CID 27362518.
  34. ^ Stern, A. (November 1, 2006). . The PI's Perspective. Johns Hopkins University Applied Physics Laboratory. Archived from the original on August 28, 2008. Retrieved 2007-02-12.
  35. ^ Najari, Sara; Saeidi, Samrand; Concepcion, Patricia; Dionysiou, Dionysios D.; Bhargava, Suresh K.; Lee, Adam F.; Wilson, Karen (2021). "Oxidative dehydrogenation of ethane: Catalytic and mechanistic aspects and future trends". Chemical Society Reviews. 50 (7): 4564–4605. doi:10.1039/D0CS01518K. PMID 33595011. S2CID 231946397.
  36. ^ Vallero, Daniel (June 7, 2010). "Cancer Slope Factors". Environmental Biotechnology: A Biosystems Approach. Academic Press. p. 641. doi:10.1016/B978-0-12-375089-1.10014-5. ISBN 9780123750891.

External links edit

  • International Chemical Safety Card 0266
  • Market-Driven Evolution of Gas Processing Technologies for NGLs

ethane, this, article, about, chemical, compound, emergency, service, protocol, ethane, confused, with, ethene, ethyne, methane, naturally, occurring, organic, chemical, compound, with, chemical, formula, standard, temperature, pressure, ethane, colorless, odo. This article is about the chemical compound For the emergency service protocol see ETHANE Not to be confused with Ethene Ethyne or Methane Ethane US ˈ ɛ 8 eɪ n ETH ayn UK ˈ iː EE is a naturally occurring organic chemical compound with chemical formula C2 H6 At standard temperature and pressure ethane is a colorless odorless gas Like many hydrocarbons ethane is isolated on an industrial scale from natural gas and as a petrochemical by product of petroleum refining Its chief use is as feedstock for ethylene production Ethane Molecular geometry of ethane based on rotational spectroscopy Ball and stick model of ethane Spacefill model of ethane Names Preferred IUPAC name Ethane 1 Systematic IUPAC name Dicarbane never recommended 2 Identifiers CAS Number 74 84 0 Y 3D model JSmol Interactive image Beilstein Reference 1730716 ChEBI CHEBI 42266 Y ChEMBL ChEMBL135626 Y ChemSpider 6084 Y ECHA InfoCard 100 000 741 EC Number 200 814 8 Gmelin Reference 212 MeSH Ethane PubChem CID 6324 RTECS number KH3800000 UNII L99N5N533T Y UN number 1035 CompTox Dashboard EPA DTXSID6026377 InChI InChI 1S C2H6 c1 2 h1 2H3 YKey OTMSDBZUPAUEDD UHFFFAOYSA N Y SMILES CC Properties Chemical formula C 2H 6 Molar mass 30 070 g mol 1 Appearance Colorless gas Odor Odorless Density 1 3562 kg m3 gas at 0 C 3 544 0 kg m3 liquid at 88 5 C 206 kg m3 at critical point 305 322 K Melting point 182 8 C 296 9 F 90 4 K Boiling point 88 5 C 127 4 F 184 6 K Critical point T P 305 32 K 32 17 C 89 91 F 48 714 bars 4 871 4 kPa Solubility in water 56 8 mg L 1 4 Vapor pressure 3 8453 MPa at 21 1 C Henry s lawconstant kH 19 nmol Pa 1 kg 1 Acidity pKa 50 Basicity pKb 36 Conjugate acid Ethanium Magnetic susceptibility x 37 37 10 6 cm3 mol Thermochemistry Heat capacity C 52 49 J K 1 mol 1 Std enthalpy offormation DfH 298 84 kJ mol 1 Std enthalpy ofcombustion DcH 298 1561 0 1560 4 kJ mol 1 Hazards GHS labelling Pictograms Signal word Danger Hazard statements H220 H280 Precautionary statements P210 P410 P403 NFPA 704 fire diamond 140SA Flash point 135 C 211 F 138 K Autoignitiontemperature 472 C 882 F 745 K Explosive limits 2 9 13 Safety data sheet SDS inchem org Related compounds Related alkanes MethanePropaneButane Related compounds DisilaneDigermane Supplementary data page Ethane data page Except where otherwise noted data are given for materials in their standard state at 25 C 77 F 100 kPa Y verify what is Y N Infobox references Related compounds may be formed by replacing a hydrogen atom with another functional group the ethane moiety is called an ethyl group For example an ethyl group linked to a hydroxyl group yields ethanol the alcohol in beverages Contents 1 History 2 Properties 2 1 Atmospheric and extraterrestrial 3 Chemistry 4 Production 5 Usage 6 Health and safety 7 See also 8 References 9 External linksHistory editEthane was first synthesised in 1834 by Michael Faraday applying electrolysis of a potassium acetate solution He mistook the hydrocarbon product of this reaction for methane and did not investigate it further 5 The process is now called Kolbe electrolysis CH3COO CH3 CO2 e CH3 CH3 C2H6 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 6 and ethyl iodide 7 with potassium metal and as did Faraday by the electrolysis of aqueous acetates They mistook the product of these reactions for the methyl radical CH3 of which ethane C2H6 is a dimer This error was corrected in 1864 by Carl Schorlemmer who showed that the product of all these reactions was in fact ethane 8 Ethane was discovered dissolved in Pennsylvanian light crude oil by Edmund Ronalds in 1864 9 10 Properties editAt standard temperature and pressure ethane is a colorless odorless gas It has a boiling point of 88 5 C 127 3 F and melting point of 182 8 C 297 0 F Solid ethane exists in several modifications 11 On cooling under normal pressure the first modification to appear is a plastic crystal crystallizing in the cubic system In this form the positions of the hydrogen atoms are not fixed the molecules may rotate freely around the long axis Cooling this ethane below ca 89 9 K 183 2 C 297 8 F changes it to monoclinic metastable ethane II space group P 21 n 12 Ethane is only very sparingly soluble in water The bond parameters of ethane have been measured to high precision by microwave spectroscopy and electron diffraction rC C 1 528 3 A rC H 1 088 5 A and CCH 111 6 5 by microwave and rC C 1 524 3 A rC H 1 089 5 A and CCH 111 9 5 by electron diffraction the numbers in parentheses represents the uncertainties in the final digits 13 nbsp Ethane shown in Newman projection barrier to rotation about the carbon carbon bond The curve is potential energy as a function of rotational angle Energy barrier is 12 kJ mol or about 2 9 kcal mol 14 Rotating a molecular substructure about a twistable bond usually requires energy The minimum energy to produce a 360 bond rotation is called the rotational barrier Ethane gives a classic simple example of such a rotational barrier sometimes called the ethane barrier Among the earliest experimental evidence of this barrier see diagram at left was obtained by modelling the entropy of ethane 15 The three hydrogens at each end are free to pinwheel about the central carbon carbon bond when provided with sufficient energy to overcome the barrier The physical origin of the barrier is still not completely settled 16 although the overlap exchange repulsion 17 between the hydrogen atoms on opposing ends of the molecule is perhaps the strongest candidate with the stabilizing effect of hyperconjugation on the staggered conformation contributing to the phenomenon 18 Theoretical methods that use an appropriate starting point orthogonal orbitals find that hyperconjugation is the most important factor in the origin of the ethane rotation barrier 19 20 As far back as 1890 1891 chemists suggested that ethane molecules preferred the staggered conformation with the two ends of the molecule askew from each other 21 22 23 24 Atmospheric and extraterrestrial edit nbsp A photograph of Titan s northern latitudes The dark features are hydrocarbon lakes containing ethane Ethane occurs as a trace gas in the Earth s atmosphere currently having a concentration at sea level of 0 5 ppb 25 Global ethane quantities have varied over time likely due to flaring at natural gas fields 26 Global ethane emission rates declined from 1984 to 2010 26 though increased shale gas production at the Bakken Formation in the U S has arrested the decline by half 27 28 Although ethane is a greenhouse gas it is much less abundant than methane has a lifetime of only a few months compared to over a decade 29 and is also less efficient at absorbing radiation relative to mass In fact ethane s global warming potential largely results from its conversion in the atmosphere to methane 30 It has been detected as a trace component in the atmospheres of all four giant planets and in the atmosphere of Saturn s moon Titan 31 Atmospheric ethane 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 CH3 H CH3 CH3 C2H6 In Earth s atmosphere hydroxyl radicals convert ethane to methanol vapor with a half life of around three months 29 It is suspected that ethane produced in this fashion on Titan rains back onto the moon s surface and over time has accumulated into hydrocarbon seas covering much of the moon s polar regions In December 2007 the Cassini probe found at least one lake at Titan s south pole now called Ontario Lacus because of the lake s similar area to Lake Ontario on Earth approximately 20 000 km2 Further analysis of infrared spectroscopic data presented in July 2008 32 provided additional evidence for the presence of liquid ethane in Ontario Lacus Several significantly larger hydrocarbon lakes Ligeia Mare and Kraken Mare being the two largest were discovered near Titan s north pole using radar data gathered by Cassini These lakes are believed to be filled primarily by a mixture of liquid ethane and methane In 1996 ethane was detected in Comet Hyakutake 33 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 In 2006 Dale Cruikshank of NASA Ames Research Center a New Horizons co investigator and his colleagues announced the spectroscopic discovery of ethane on Pluto s surface 34 Chemistry editThe chemistry of ethane 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 C2H5 Cl2 C2H5Cl Cl Cl C2H6 C2H5 HCl The combustion of ethane releases 1559 7 kJ mol or 51 9 kJ g of heat and produces carbon dioxide and water according to the chemical equation 2 C2H6 7 O2 4 CO2 6 H2O 3120 kJ Combustion may also occur without an excess of oxygen yielding carbon monoxide acetaldehyde methane methanol and ethanol At higher temperatures especially in the range 600 900 C 1 112 1 652 F ethylene is a significant product 2 C2H6 O2 2 C2H4 H2O Such oxidative dehydrogenation reactions are relevant to the production of ethylene 35 Production editAfter 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 more than 6 by volume Prior to the 1960s ethane and larger molecules were typically not separated from the methane component of natural gas but simply burnt along with the methane as a fuel Today ethane is an important petrochemical feedstock and 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 produced 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 a turboexpander and can recover more than 90 of the ethane in natural gas In this process chilled gas is expanded through a turbine reducing the temperature to approximately 100 C 148 F 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 Usage editThe chief use of ethane is the production of ethylene ethene 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 alkenes olefins such as propene 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 producing this reaction have been patented but poor selectivity for vinyl chloride and corrosive reaction conditions specifically a reaction mixture containing hydrochloric acid at temperatures greater than 500 C have discouraged the commercialization of most of them Presently INEOS operates a 1000 t a tonnes per annum ethane to vinyl chloride pilot plant at Wilhelmshaven 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 The economic viability of this process may rely on the low cost of ethane near Saudi oil 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 cryo electron microscopy A thin film of water quickly immersed in liquid ethane at 150 C or colder freezes too quickly for water to crystallize Slower freezing methods can generate cubic ice crystals which can disrupt soft structures by damaging the samples and reduce image quality by scattering the electron beam before it can reach the detector MAN Energy Solutions currently manufactures two stroke dual fuel engines B amp W ME GIE which can run on both Marine diesel oil and ethane Health and safety editAt room temperature ethane is an extremely 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 Until they warm to room temperature the vapors from liquid ethane are heavier than air and can flow along the floor or ground gathering in low places if the vapors encounter an ignition source the chemical reaction can flash back to the source of ethane from which they evaporated Ethane can displace oxygen and become an asphyxiation hazard Ethane poses no known acute or chronic toxicological risk It is not a carcinogen 36 See also editBiogas carbon neutral alternative to natural gas Biorefining Biodegradable plastic Drop in bioplasticReferences edit International Union of Pure and Applied Chemistry 2014 Nomenclature of Organic Chemistry IUPAC Recommendations and Preferred Names 2013 The Royal Society of Chemistry p 133 doi 10 1039 9781849733069 ISBN 978 0 85404 182 4 The saturated unbranched acyclic hydrocarbons C2H6 C3H8 and C4H10 have the retained names ethane propane and butane respectively IUPAC 2014 p 4 Similarly the retained names ethane propane and butane were never replaced by systematic names dicarbane tricarbane and tetracarbane as recommended for analogues of silane disilane phosphane triphosphane and sulfane tetrasulfane Ethane Compound Summary PubChem Compound US National Center for Biotechnology Information 16 September 2004 Retrieved 7 December 2011 Lide D R ed 2005 CRC Handbook of Chemistry and Physics 86th ed Boca Raton FL CRC Press p 8 88 ISBN 0 8493 0486 5 Faraday Michael 1834 Experimental researches in electricity Seventh series Philosophical Transactions 124 77 122 Bibcode 1834RSPT 124 77F doi 10 1098 rstl 1834 0008 S2CID 116224057 Kolbe Hermann Frankland Edward 1849 On the products of the action of potassium on cyanide of ethyl Journal of the Chemical Society 1 60 74 doi 10 1039 QJ8490100060 Frankland Edward 1850 On the isolation of the organic radicals Journal of the Chemical Society 2 3 263 296 doi 10 1039 QJ8500200263 Schorlemmer Carl 1864 Ueber die Identitat des Aethylwasserstoffs und des Methyls Annalen der Chemie und Pharmacie 132 2 234 238 doi 10 1002 jlac 18641320217 Roscoe H E Schorlemmer C 1881 Treatise on Chemistry Vol 3 Macmillan pp 144 145 Watts H 1868 Dictionary of Chemistry Vol 4 p 385 Van Nes G J H Vos A 1978 Single crystal structures and electron density distributions of ethane ethylene and acetylene I Single crystal X ray structure determinations of two modifications of ethane PDF Acta Crystallographica Section B 34 6 1947 Bibcode 1978AcCrB 34 1947V doi 10 1107 S0567740878007037 S2CID 55183235 Ethane as a solid Retrieved 2019 12 10 Harmony Marlin D 1990 11 15 The equilibrium carbon carbon single bond length in ethane The Journal of Chemical Physics 93 10 7522 7523 Bibcode 1990JChPh 93 7522H doi 10 1063 1 459380 ISSN 0021 9606 J McMurry 2012 Organic chemistry 8 ed Belmont CA Brooks p 95 ISBN 9780840054449 Kemp J D Pitzer Kenneth S 1937 The Entropy of Ethane and the Third Law of Thermodynamics Hindered Rotation of Methyl Groups Journal of the American Chemical Society 59 2 276 doi 10 1021 ja01281a014 Ercolani G 2005 Determination of the Rotational Barrier in Ethane by Vibrational Spectroscopy and Statistical Thermodynamics J Chem Educ 82 11 1703 1708 Bibcode 2005JChEd 82 1703E doi 10 1021 ed082p1703 Pitzer R M 1983 The Barrier to Internal Rotation in Ethane Acc Chem Res 16 6 207 210 doi 10 1021 ar00090a004 Mo Y Wu W Song L Lin M Zhang Q Gao J 2004 The Magnitude of Hyperconjugation in Ethane A Perspective from Ab Initio Valence Bond Theory Angew Chem Int Ed 43 15 1986 1990 doi 10 1002 anie 200352931 PMID 15065281 Pophristic V Goodman L 2001 Hyperconjugation not steric repulsion leads to the staggered structure of ethane Nature 411 6837 565 8 Bibcode 2001Natur 411 565P doi 10 1038 35079036 PMID 11385566 S2CID 205017635 Schreiner P R 2002 Teaching the right reasons Lessons from the mistaken origin of the rotational barrier in ethane Angewandte Chemie International Edition 41 19 3579 81 3513 doi 10 1002 1521 3773 20021004 41 19 lt 3579 AID ANIE3579 gt 3 0 CO 2 S PMID 12370897 Bischoff CA 1890 Ueber die Aufhebung der freien Drehbarkeit von einfach verbundenen Kohlenstoffatomen Chem Ber 23 623 doi 10 1002 cber 18900230197 Bischoff CA 1891 Theoretische Ergebnisse der Studien in der Bernsteinsauregruppe Chem Ber 24 1074 1085 doi 10 1002 cber 189102401195 Bischoff CA 1891 Die dynamische Hypothese in ihrer Anwendung auf die Bernsteinsauregruppe Chem Ber 24 1085 1095 doi 10 1002 cber 189102401196 Bischoff C A Walden P 1893 Die Anwendung der dynamischen Hypothese auf Ketonsaurederivate Berichte der Deutschen Chemischen Gesellschaft 26 2 1452 doi 10 1002 cber 18930260254 Trace gases archived Atmosphere mpg de Archived from the original on 2008 12 22 Retrieved 2011 12 08 a b Simpson Isobel J Sulbaek Andersen Mads P Meinardi Simone Bruhwiler Lori Blake Nicola J Helmig Detlev Rowland F Sherwood Blake Donald R 2012 Long term decline of global atmospheric ethane concentrations and implications for methane Nature 488 7412 490 494 Bibcode 2012Natur 488 490S doi 10 1038 nature11342 PMID 22914166 S2CID 4373714 Kort E A Smith M L Murray L T Gvakharia A Brandt A R Peischl J Ryerson T B Sweeney C Travis K 2016 Fugitive emissions from the Bakken shale illustrate role of shale production in global ethane shift Geophysical Research Letters 43 9 4617 4623 Bibcode 2016GeoRL 43 4617K doi 10 1002 2016GL068703 hdl 2027 42 142509 One oil field a key culprit in global ethane gas increase University of Michigan April 26 2016 a b Aydin Kamil Murat Williams M B Saltzman E S April 2007 Feasibility of reconstructing paleoatmospheric records of selected alkanes methyl halides and sulfur gases from Greenland ice cores Journal of Geophysical Research 112 D7 Bibcode 2007JGRD 112 7312A doi 10 1029 2006JD008027 Hodnebrog Oivind Dalsoren Stig B Myrhe Gunnar 2018 Lifetimes direct and indirect radiative forcing and global warming potentials of ethane C2H6 propane C3H8 and butane C4H10 Atmospheric Science Letters 19 2 Bibcode 2018AtScL 19E 804H doi 10 1002 asl 804 Brown Bob et al 2008 NASA Confirms Liquid Lake on Saturn Moon NASA Jet Propulsion Laboratory Archived from the original on 2011 06 05 Retrieved 2008 07 30 Brown R H Soderblom L A Soderblom J M Clark R N Jaumann R Barnes J W Sotin C Buratti B et al 2008 The identification of liquid ethane in Titan s Ontario Lacus Nature 454 7204 607 10 Bibcode 2008Natur 454 607B doi 10 1038 nature07100 PMID 18668101 S2CID 4398324 Mumma Michael J 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 5266 1310 1314 Bibcode 1996Sci 272 1310M doi 10 1126 science 272 5266 1310 PMID 8650540 S2CID 27362518 Stern A November 1 2006 Making Old Horizons New The PI s Perspective Johns Hopkins University Applied Physics Laboratory Archived from the original on August 28 2008 Retrieved 2007 02 12 Najari Sara Saeidi Samrand Concepcion Patricia Dionysiou Dionysios D Bhargava Suresh K Lee Adam F Wilson Karen 2021 Oxidative dehydrogenation of ethane Catalytic and mechanistic aspects and future trends Chemical Society Reviews 50 7 4564 4605 doi 10 1039 D0CS01518K PMID 33595011 S2CID 231946397 Vallero Daniel June 7 2010 Cancer Slope Factors Environmental Biotechnology A Biosystems Approach Academic Press p 641 doi 10 1016 B978 0 12 375089 1 10014 5 ISBN 9780123750891 External links edit nbsp Wikimedia Commons has media related to Ethane International Chemical Safety Card 0266 Market Driven Evolution of Gas Processing Technologies for NGLs Staggered and eclipsed ethane Retrieved from https en wikipedia org w index php title Ethane amp oldid 1215927357, wikipedia, wiki, book, books, library,

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