RI 2363 Helium

The story of helium is one of the romances of science . Probably nothing , except perhaps radium , compares with it in human interest . Helium is one of the best examples of a discovery in pure science that has wide commercial application . In 1868 , an eclipse of the sun was visible in India , several scientific men who were in India making observations of the eclipse turned a spectroscope for the first time on the solar chromosphere - that part of the atmosphere of the sun , about 10,000 miles deep , which merges into the corona . A bright yellow line was observed and was thought at first to be due to sodium . Janssen showed , however , that this line was not just the same as either the D or D₂ line of sodium, although it was extremely close to these lines , hence he suggested that the new line have the designation D₂ . Frankland and Lockyer decided that Dz was due to an element in the sun not previously discovered on the earth , and suggested for it the name "Helium" from the Greek work " Helios " the sun . For several years nothing more was done in connection with this element . In 1894 , Sir William Ransay , in conjunction with Lord Rayleigh , made his memorable discovery of argon in the atmosphere , which was announced at the British Association meeting in the same year . After this discovery , Ramsay looked for other sources of the element . Through Sir Henry Miers , he learned that Dr. W. F. Hillebrand , of the United States Geological Survey , had obtained an inert gas from certain uranium minerals , which gas he had decided was nitrogen . Ramsay believed that part of it might be argon ; he obtained from Hillebrand for experimentation , a sample of the mineral , cleveite , one of the uranium minerals , and after extracting gas from the mineral and purifying it , he ran it into a spectrum tube . The lines obtained ' were , however , different from those of argon; among them was the bright yellow line noted by Janssen . Thus was terrestrial heliun discovered .