User:Physchim62/Helium

From WikiChem
< User:Physchim62
Revision as of 07:07, 19 March 2010 by Physchim62 (talk | contribs) (History)
Jump to: navigation, search
hydrogenheliumlithium


He

Ne
Atomic properties
Atomic number 2
Standard atomic weight 4.002 602(2)
Electron configuration 1s2
Physical properties[1]
Melting point see text
Boiling point 4.22 K (−268.93 °C)
Thermodynamic properties[1]
Standard entropy 126.153(2) J K−1 mol−1
Miscellaneous
CAS number 7440-59-7
Where appropriate, and unless otherwise stated, data are given for 100 kPa (1 bar) and 298.15 K (25 °C).

Helium (symbol: He) is a chemical element, the lightest of the noble gases.

History

Helium is the only element to have been discovered extraterrestrially before being found on Earth, specifically in the Sun. A bright yellow spectral line (λ = 587.49 nm) was first observed by French astronomer Jules Janssen during the eclipse of 18 August 1868, which Janssen observed from Guntur in India, and independently by Norman Lockyer in London on 20 October 1868.[2][3][4] Lockyer, together with English chemist Edward Frankland, showed that the line could not be explained by any known element, and proposed the name helium, from the Greek ἥλιος (helios; the Sun).[5][6]

The first isolation of helium from a terrestrial source is usually credited to the British chemist William Ramsey, who isolated the helium that was occluded in the mineral cleveite (a uranium-containing mineral) and identified it by its spectrum.[7] The occluded gas had been noticed previously by American geochemist William Francis Hillebrand, but had been misidentified as nitrogen.[8] Helium had been identified (through its spectrum) on Earth as early as 1881 by Italian physicist Luigi Palmieri, but Palmieri could not isolate any of the element. Finally, helium was isolated independently in 1895 by Per Teodor Cleve and Abraham Langlet in Uppsala, Sweden, who collected enough of the gas to accurately determine its atomic weight.[9] Nevertheless, it was Ramsey who was awarded the Nobel Prize for Chemistry (in 1904), and who is usually credited with the discovery.

Occurrence and production

Country Production
106 m3
United States 122*
Algeria 24
Qatar 15
Russia 7
Poland 2.5
Estimates for 2009 from the
U.S. Geological Survey[10]
*U.S. figure includes 42 million
cubic metres withdrawn from the
federal government stockpile.

Helium is the second most common element in the Universe (after hydrogen), accounting for 23% of all atoms. However, the Earth's gravitational field is not strong enough to retain helium in the atmosphere for long periods, and all the Earth's primordial helium is believed to have escaped. The helium currently present on Earth has been formed from the alpha decay of radioactive nuclides: most of this helium escapes to the atmosphere and then into space, but some of it can be trapped underground by impermeable rock formations, often associated with natural gas deposits.

The commercial production of helium is based around its extraction from natural gas, which is economically viable when the helium fraction is greater than about 0.3%. The United States has historically been the predominant producer, although its de novo production is declining and Algeria and Qatar are gaining importance.

The U.S. Bureau of Land Management operates a stockpile of crude helium (~80%) at Cliffside Field, Potter County, Texas, and a crude-helium pipeline from Bushton, Kansas, passing through the Reichel Field (Kansas) and the Keyes Field (Oklahoma) to the Cliffside Field.[11]

Use

Total U.S. Consumpton (2009)
52.1 million cubic metres
Cryogenics 32%
Pressurizing and purging 18%
Controlled atmospheres 18%
Welding cover gas 13%
Leak detection 4%
Breathing mixtures 2%
Other uses 13%
Estimates for 2009 from the U.S. Geological Survey[10]

The main use of helium is in cryogenics, where helium is essential for temperatures below −256 °C (−429 °F),[10] the approximate boiling point of liquid hydrogen. Cooling with liquid helium allows an operating temperature of around −269 °C (−452 °F), just four kelvins. Such low temperatures are required for superconducting magnets to operate; these are used in a variety of applications, including NMR spectrometers and magnetic resonance imaging (MRI) scanners.

Uses for pressurizing and purging, in controlled atmosphere (e.g., glove boxes) and as a welding cover gas are only important in the United States, where helium is relatively cheap. In other countries, argon is used for these purposes.

References

  1. 1.0 1.1 Helium. In NIST Chemistry WebBook; National Institute for Standards and Technology, <http://webbook.nist.gov/cgi/inchi/InChI%3D1S/He>. (accessed 19 March 2010).
  2. Cortie, A. L. Sir Norman Lockyer, 1836–1920. Astrophys. J. 1921, 53 (4), 233–48, <http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1921ApJ....53..233C&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf>.
  3. Leggett, Hadley Aug. 18, 1868: Helium Discovered During Total Solar Eclipse; wired.com, August 18, 2009, <http://www.wired.com/thisdayintech/2009/08/dayintech_0818/>. (accessed 18 March 2010).
  4. C. R. Hebd. Acad. Sci. Paris 1868, 67, 836–41, <http://gallica.bnf.fr/ark:/12148/bpt6k3024c.image.r=comptes-rendus+hebdomadaires+Acad%C3%A9mie+des+Sciences.f836.langFR>.
  5. Helium. In Oxford English Dictionary; Oxford University Press, 2008, <http://dictionary.oed.com/cgi/entry/50104457?>. (accessed 20 July 2008).
  6. "Frankland and Lockyer find the yellow prominences to give a very decided bright line not far from D, but hitherto not identified with any terrestrial flame. It seems to indicate a new substance, which they propose to call Helium." Thomson, W. Rep. Brit. Assoc. 1872, 99.
  7. Ramsay, William On a Gas Showing the Spectrum of Helium, the Reputed Cause of D3, One of the Lines in the Coronal Spectrum. Preliminary Note. Proc. Roy. Soc. London 1895, 58, 65–67. DOI: 10.1098/rspl.1895.0006. Ramsay, William Helium, a Gaseous Constituent of Certain Minerals. Part I. Proc. Roy. Soc. London 1895, 58, 80–89. DOI: 10.1098/rspl.1895.0010. Ramsay, William Helium, a Gaseous Constituent of Certain Minerals. Part II. Proc. Roy. Soc. London 1895, 59, 325–30. DOI: 10.1098/rspl.1895.0097.
  8. Munday, Pat W. F. Hillebrand (1853–1925), geochemist and US Bureau of Standards administrator. In American National Biography; Garraty, John A.; Carnes, Mark C., Eds.; Oxford University Press, 1999; Vol. 10-11, pp 227–28, 808–9.
  9. Langlet, N. A. authorlink = Abraham Langlet Das Atomgewicht des Heliums. Z. Anorg. Chem. 1895, 10 (1), 289–92. DOI: 10.1002/zaac.18950100130.
  10. 10.0 10.1 10.2 Helium. In Mineral Commodities Summaries; U.S. Geological Survey, January 2010, <http://minerals.usgs.gov/minerals/pubs/commodity/helium/mcs-2010-heliu.pdf>.
  11. Helium. In 2008 Minerals Yearbook; U.S. Geological Survey, October 2009, <http://minerals.usgs.gov/minerals/pubs/commodity/helium/myb1-2008-heliu.pdf>.

External links