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Timeline of knowledge about the interstellar and intergalactic medium

  • 1848 – Lord Rosse studies M1 and names it the Crab Nebula
  • 1864 – William Huggins studies the spectrum of the Orion Nebula and
    shows that it is a cloud of gas
  • 1927 – Ira Bowen explains unidentified spectral lines from space as
    forbidden transition lines
  • 1930 – Robert Trumpler discovers absorption by interstellar dust by
    comparing the angular sizes and brightnesses of globular clusters
  • 1944 – Hendrik van de Hulst predicts the 21 cm hyperfine line of
    neutral interstellar hydrogen
  • 1951 – H.I. Ewen and Edward Purcell observe the 21 cm hyperfine line of
    neutral interstellar hydrogen
  • 1956 – Lyman Spitzer predicts coronal gas around the Milky Way
  • 1965 – James Gunn and Bruce Peterson use observations of the relatively
    low absorption of the blue component of the Lyman-alpha line from 3C9
    to strongly constrain the density and ionization state of the
    intergalactic medium
  • 1969 – Lewis Snyder, David Buhl, Ben Zuckerman, and Patrick Palmer find
    interstellar formaldehyde
  • 1970 – Arno Penzias and Robert Wilson find interstellar carbon monoxide
  • 1970 – George Carruthers observes molecular hydrogen in space
  • 1977 – Christopher McKee and Jeremiah Ostriker propose a three
    component theory of the interstellar medium
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