The Formation of Acetic Acid (CH3COOH) in Interstellar Ice Analogs

Details The Formation of Acetic Acid (CH3COOH) in Interstellar Ice Analogs The Formation of Acetic Acid (CH3COOH) in Interstellar Ice Analogs

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007apj...660.1289b&link_type=abstract

The Astrophysical Journal, Volume 660, Issue 2, pp. 1289-1295.

Astronomy and Astrophysics

Astronomy

10

Ism: Cosmic Rays, Ism: Molecules, Methods: Laboratory, Molecular Processes, Planets And Satellites: General

Scientific paper

Binary ice mixtures of methane (CH4) and carbon dioxide (CO 2) ices were irradiated at 12 K with energetic electrons to mimic the energy transfer processes that occur in the track of the trajectories of MeV cosmic-ray particles. The formation of trans-acetic acid (CH3COOH) was established through the appearance of new bands in the infrared spectrum at 1780, 1195, 1160, 1051, and 957 cm-1 two dimeric forms of acetic acid were assigned via absorptions at 1757 and 1723 cm-1 . During warm-up of the ice sample, the mass spectrometer recorded peaks of m/z values of 60 and 45 associated with the C2H 4O2+ and COOH+ molecular ion and fragment, respectively. The kinetic fits of the column densities of the acetic acid molecule suggest that the initial step of the formation process appears to be the cleavage of a carbon-hydrogen bond from methane to generate the methyl radical plus atomic hydrogen. The hydrogen atom holds excess kinetic energy allowing it to overcome entrance barriers required to add to a carbon dioxide molecule, generating the carboxyl radical (HOCO). This radical can recombine with the methyl radical to form acetic acid molecule. Similar processes are expected to form acetic acid in the interstellar medium, thus providing alternatives to gas-phase processes for the generation of complex chemical species whose fractional abundances compared to molecular hydrogen of typically a few×10-9 cannot be accounted for by solely gas-phase chemistry.

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