Diffusion measurements of methane in amorphous solid water. (Poster OT-04)

XXV Reunión Nacional de Espectroscopia (XXV RNE) - IX Congreso Ibérico de Espectroscopia (IX CIE); Alicante, 20 – 22 de julio de 2016; http://web.csidiomas.ua.es/congresos/espectroscopia/index.htmlIcy mantles covering dust grains in dense clouds of the interstellar medium are known to be responsible of the large molecular complexity of our universe. Within those mantles atoms and molecules can meet and react with larger probablility than in the gas phase. The chemical reactivity of interstellar ice is limited by the diffusion of reacting atoms or molecules in water ice, its major component. For this reason the knowledge of diffusion coefficients of different molecules on water ice is of great astrophysical interest. In this work we have designed an experiment to determine the thermal diffusion of CH4 in amorphous water ice at 50 K. In a high vacum chamber methane ice layers covered by water ice layers were grown by vapor deposition at 30 K. Then, the two-layered system was warmed to 50 K and kept at that temperature while the diffusion of CH4 molecules was monitored by means of FTIR spectroscopy. The decay of intensity with time of the strong IR absorption asociated to the ¿3 mode of methane (see Figure1) is a measure of the number of methane molecules that have moved trough the hole water ice layer and left the sample. Diffusion coefficients were extracted from the isothermal experiments usign Flick¿s second law of diffusion [1,2]. [1] F. Mispelaer, P. Theulé, H. Aouididi, et al., A&A, 555 (in bold) , A13-11pp (2013). [2] L. J. Karssemeijer, S. Ioppolo, M. C. van Hemert, A. van der Avoird, et al., ApJ, 781, 16-15pp (2014).This research has been supported by the Spanish MINECO, Projects FIS2013-48087-C2-1-P and by the European Research Council, project ERC-2013-Syg-610256. G.M. acknowledges MINECO PhD grant BES-2014-069355Peer Reviewe