Difference between revisions of "User:Physchim62/Helium"

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{{Infobox element
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|name = helium
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|symbol = He
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|left = [[hydrogen]]
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|right = [[lithium]]
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|above = –
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|below = [[Neon|Ne]]
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|atomic-number = 2
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}}
 
'''Helium''' (symbol: '''He''') is a [[chemical element]], the lightest of the [[noble gas]]es.
 
'''Helium''' (symbol: '''He''') is a [[chemical element]], the lightest of the [[noble gas]]es.
  
 
==History==
 
==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''&nbsp;= 587.49&nbsp;nm) was first observed by French astronomer [[Jules Janssen]] during the eclipse of 18&nbsp;August 1868, which Janssen observed from Guntur in India, and independently by [[Norman Lockyer]] in London on 20&nbsp;October 1868.<ref>{{citation | title = Sir Norman Lockyer, 1836–1920 | url = http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1921ApJ....53..233C&amp;data_type=PDF_HIGH&amp;whole_paper=YES&amp;type=PRINTER&amp;filetype=.pdf | last = Cortie | first = A. L. | journal = Astrophys. J. | year = 1921 | volume = 53 | issue = 4 | pages = 233–48}}.</ref><ref>{{citation | url = http://www.wired.com/thisdayintech/2009/08/dayintech_0818/  | publisher = wired.com | accessdate = 2010-03-18 | title = Aug. 18, 1868: Helium Discovered During Total Solar Eclipse | date = August 18, 2009 | first = Hadley | last = Leggett}}.</ref><ref>{{citation | journal = C. R. Hebd. Acad. Sci. Paris | volume = 67 | year = 1868 | pages = 836–41 | url = http://gallica.bnf.fr/ark:/12148/bpt6k3024c.image.r=comptes-rendus+hebdomadaires+Acad%C3%A9mie+des+Sciences.f836.langFR}}.</ref> 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 {{Polytonic|ἥλιος}} (''helios'', the Sun).
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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''&nbsp;= 587.49&nbsp;nm) was first observed by French astronomer [[Jules Janssen]] during the eclipse of 18&nbsp;August 1868, which Janssen observed from Guntur in India, and independently by [[Norman Lockyer]] in London on 20&nbsp;October 1868.<ref>{{citation | title = Sir Norman Lockyer, 1836–1920 | url = http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1921ApJ....53..233C&amp;data_type=PDF_HIGH&amp;whole_paper=YES&amp;type=PRINTER&amp;filetype=.pdf | last = Cortie | first = A. L. | journal = Astrophys. J. | year = 1921 | volume = 53 | issue = 4 | pages = 233–48}}.</ref><ref>{{citation | url = http://www.wired.com/thisdayintech/2009/08/dayintech_0818/  | publisher = wired.com | accessdate = 2010-03-18 | title = Aug. 18, 1868: Helium Discovered During Total Solar Eclipse | date = August 18, 2009 | first = Hadley | last = Leggett}}.</ref><ref>{{citation | journal = C. R. Hebd. Acad. Sci. Paris | volume = 67 | year = 1868 | pages = 836–41 | url = http://gallica.bnf.fr/ark:/12148/bpt6k3024c.image.r=comptes-rendus+hebdomadaires+Acad%C3%A9mie+des+Sciences.f836.langFR}}.</ref> 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 {{Polytonic|ἥλιος}} (''helios''; the Sun).
  
 
==Occurrence and production==
 
==Occurrence and production==

Revision as of 13:03, 18 March 2010

hydrogenheliumlithium


He

Ne
Atomic properties
Atomic number 2
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.[1][2][3] 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).

Occurrence and production

Country Production
km3
United States 122*
Algeria 24
Qatar 15
Russia 7
Poland 2.5
Estimates for 2009 from the
U.S. Geological Survey[4]
*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.[5]

References