Abstract
Since the observation of the 3-µm band in interstellar infrared sources1–3, vapour-deposited amorphous ice, H2O(as), has been discussed as a major component of comets4–9, of satellites of the outer planets10,11 and of interstellar dust11–13. Some of the physical properties of H2O(as) important for these discussions appear to be contradictory: for example N2 adsorption isotherms at 77 K evaluated by the BET method24 gave surface areas of 241 m2 g−1 according to Ghormley14,15, but less than 12 m2 g−1 according to others16,17. We have reinvestigated adsorption of N2 on H2O(as) and find that it is a microporous solid. The differences between adsorption phenomena taking place in micropores and on the surface of intermediate pores or non-porous adsorbents should be of general importance for the various speculations of the role of H2O(as) in space. In particular, we discuss the influence of micro-pores on the H2 recombination rate on H2O(as) in interstellar dust and on adsorption of volatile gases in comets.
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Mayer, E., Pletzer, R. Astrophysical implications of amorphous ice—a microporous solid. Nature 319, 298–301 (1986). https://doi.org/10.1038/319298a0
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DOI: https://doi.org/10.1038/319298a0
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