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  2. Emission spectrum - Wikipedia

    en.wikipedia.org/wiki/Emission_spectrum

    The emission spectrum can be used to determine the composition of a material, since it is different for each element of the periodic table. One example is astronomical spectroscopy : identifying the composition of stars by analysing the received light.

  3. Krypton - Wikipedia

    en.wikipedia.org/wiki/Krypton

    Krypton is characterized by several sharp emission lines (spectral signatures) the strongest being green and yellow. [20] Krypton is one of the products of uranium fission . [ 21 ] Solid krypton is white and has a face-centered cubic crystal structure , which is a common property of all noble gases (except helium , which has a hexagonal close ...

  4. Strontium - Wikipedia

    en.wikipedia.org/wiki/Strontium

    The metal forms a dark oxide layer when it is exposed to air. Strontium has physical and chemical properties similar to those of its two vertical neighbors in the periodic table, calcium and barium. It occurs naturally mainly in the minerals celestine and strontianite, and is mostly mined from these.

  5. Hydrogen spectral series - Wikipedia

    en.wikipedia.org/wiki/Hydrogen_spectral_series

    There are emission lines from hydrogen that fall outside of these series, such as the 21 cm line. These emission lines correspond to much rarer atomic events such as hyperfine transitions. [1] The fine structure also results in single spectral lines appearing as two or more closely grouped thinner lines, due to relativistic corrections. [2]

  6. Holmium - Wikipedia

    en.wikipedia.org/wiki/Holmium

    Holmium (Holmia, Latin name for Stockholm) was discovered by the Swiss chemists Jacques-Louis Soret and Marc Delafontaine in 1878 who noticed the aberrant spectrographic emission spectrum of the then-unknown element (they called it "Element X"). [39] [40]

  7. Flame test - Wikipedia

    en.wikipedia.org/wiki/Flame_test

    The nature of the excited and ground states depends only on the element. Ordinarily, there are no bonds to be broken, and molecular orbital theory is not applicable. The emission spectrum observed in flame test is also the basis of flame emission spectroscopy, atomic emission spectroscopy, and flame photometry. [4] [13]

  8. Radon - Wikipedia

    en.wikipedia.org/wiki/Radon

    Emission spectrum of radon, photographed by Ernest Rutherford in 1908. Numbers at the side of the spectrum are wavelengths. Numbers at the side of the spectrum are wavelengths. The middle spectrum is of radium emanation (radon), while the outer two are of helium (added to calibrate the wavelengths).

  9. Neodymium - Wikipedia

    en.wikipedia.org/wiki/Neodymium

    The similar absorption of the yellow mercury emission line at 578 nm is the principal cause of the blue color observed for neodymium glass under traditional white-fluorescent lighting. Neodymium and didymium glass are used in color-enhancing filters in indoor photography, particularly in filtering out the yellow hues from incandescent lighting.