An experimental study of the photodegradation of polyoxymethylene at 122, 147 and 193 nm

Biology

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Polyoxymethylene, Uv Irradiation, Photodegradation, Experimental Design, Quantum Yields, Comets

Scientific paper

This paper presents results from a current experimental program whose aim is to determine quantitatively the photochemical evolution of organic molecules present or likely to be present in comets. Particularly, this includes the mechanisms involved in the degradation of high molecular weight compounds in cometary ices and dust, when they are submitted to photon bombardment in the surrounding area of the sun. Photodegradation of polyoxymethylene (-CH2-O-)n is studied at 122, 147 and 193 nm. Experimental setup and analytical methods are presented (FTIR, GC-MS). We have identified the main gaseous photodegradation products of polyoxymethylene : H2CO, CO, HCOOH, CO2, CH3OH, CH3OCHO, CH3OCH3OCH3 and C3H6O3 (trioxane). We have determined the production quantum yields for formaldehyde (phi122nm = 0.75 +/- 0.21, phi147nm = 0.96 +/- 0.19) and formic acid (phi122nm = 0.13 +/- 0.05, phi147nm = 0.26 +/- 0.10), and roughly estimated the yields for the other compounds. Such data, that were missing to interpret astronomical observations of comets, are now available for further theoretical studies. We also propose mechanisms involved in the production of these molecules from polyoxymethylene.

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