Helium

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Helium is a light gas, desirable for use in airships because as a non-reactive noble gas it is safer than hydrogen—but more difficult to produce or isolate.

Pierre Jules César Janssen first identified the unique spectrographic band for helium, known as D3, from observations of a solar eclipse in 1868. Norman Lockyer and Edward Frankland identified D3 as the sign of a new element and named it helium after Helios. William Ramsay and Lord Rayleigh in the 1890s made practical progress in the actual extraction of helium, in conjunction with their work on argon (a heavier noble gas following helium and neon).[1]

According to Richard B. Moore, Chief Chemist of the US Bureau of Mines, the serious pursuit of helium for use in dirigibles during World War I began in 1917, when the extraction of the element from natural gas in Kansas appeared possible and beneficial for the war effort. The Bureau of Mines set up several plants in Texas; meanwhile the British began similar operations in Ontario and Alberta. The first US plant began producing helium on 8 April 1918 and by September generated 4000–6000 cubic feet of 70% helium gas per day. Additional refinement was necessary to increase the percentage. By the time of armistice, the US plants had produced about 200,000 cubic feet of helium.[2]

References

  1. Moore, 1921, Helium, pp. 145–150.
  2. Moore, 1921, Helium, pp. 165–171.

Additional sources

Historical publications relevant to the discovery and exctraction of helium, but not necessarily its use in airships. Not yet indexed as publications on this site.

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Publications referring to Helium

Enclosing categories Gas
Subcategories
Keywords LTA
Start year 1868
End year