A tentative identification of methanol as the progenitor of the 3.52-micron emission feature in several comets

Astronomy and Astrophysics – Astronomy

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Astronomical Spectroscopy, Austin Comet, Brorsen-Metcalf Comet, Infrared Radiation, Methyl Alcohol, Okazaki-Levy-Rudenko Comet, Comets, Emission Spectra, Halley'S Comet, Solar System

Scientific paper

Continuum emission has been detected during 3.44-3.64 micron spectral region observations of Comets P/Brorsen-Metcalf, Okazaki-Levy-Rudenko, and Levy. The spatial brightness profile of the 3.52-micron emission feature was measured and found to be consistent with uniform outflow from a central, unresolved source; the molecule generating the emission is either directly sublimated from the cometary surface or is a short-lived parent specie's dissociation product. The modeled IR spectrum of CH3OH implies the consistency of the observed spectra with a methanol origin for the 3.52 emission.

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