A Listing of the Most Abundant
Interstellar Elements

Element
Symbol
Atomic Number
Relative Abundance
Hydrogen
1
10,000
Helium
2
1,000
Carbon
6
4
Nitrogen
7
1
Oxygen
8
9
Neon
10
1

Sources

  • Data from Anders and Grevesse, 1989
  • Flowers, David, Molecular Collisions, 1990


    A Partial Listing of Interstellar Molecules
    Found in Molecular Clouds

    Molecule
    Name
    H2
    Molecular Hydrogen
    CO
    Carbon Monoxide
    NO
    Nitric oxide
    C2
    Carbon Dimer
    OH
    Hydroxyl
    CH
    Methylidyne
    CN
    Cyanogen
    CS
    Carbon monosulfide
    SO
    Sulfurmonoxide
    SiO
    Silicon monoxide
    SiS
    Silicon sulfide
    PN
    Phosphorus nitride
    PO
    Phosphorus monoxide
    C2H
    Ethynyl
    HCN
    Hydrogen cyanide
    HNC
    Hydrogen isocyanide
    H2O
    Water
    HDO
    Deuterated water
    HCO+
    Formylion
    N2O
    Nitrous oxide
    SO2
    Sulfur dioxide
    C3N
    Cyanoethynyl
    C3O
    Tricarbon monoxide
    NH3
    Ammonia
    CH4
    Methane
    C3H
    Propynlidyne
    H2CO
    Formaldehyde
    H2C2O
    Ketene
    CH2NH
    Methylenimine
    C4H
    Butadiynyl
    C3H2
    Cyclopropenylidene
    CH3OH
    Methanol
    CH3C2H
    Methyl acetylene
    HCOOCH3
    Methylformate
    CH3CH2OH
    Ethanol
    NH2CH2COOH
    Glycine II

    Sources

    • All molecules with the exception of ammonia, water, and nitrous oxide
      • Irvene et al. (1987)
      • Hartquist, T. W., Molecular Astrophysics, 1990
    • Detection of Interstellar N2O: A New Molecule Containing an N - O Bond,
      L. M. Ziurys, A. J., Apponi, J. M. Hollis, and L. E. Snyder,
      Ap. J. (Letters), 436, L181 (1994).
    Note: This is only a partial listing of molecules detected in the cold confines of interstellar space. The majority of the compounds in the list have been detected using radio telescopes tuned to the faint glow of the rotational spectra of the molecule. The 12 meter radio telescope at the National Radio Astronomy Observatory Arizona Operations is currently being used to detect the mm wavelengths of interstellar molecules. A Millimeter Array will soon be constructed at the Arizona Site to facilitate in the discovery and identification of molecules in space.

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    Last modified: July 12, 2000
    by Jeff Mirick