4.5 Article

Near-infrared spectra of laboratory H2O-CH4 ice mixtures S.2005.10.021

Journal

ICARUS
Volume 181, Issue 1, Pages 302-308

Publisher

ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.icarus.2005.10.021

Keywords

ices; infrared observations; spectroscopy; surfaces; planets; surfaces; satellites

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We present 1.25-19 mu m infrared spectra of pure solid CH4 and H2O/CH4 = 87, 20, and 3 solid mixtures at temperatures from 15 to 150 K. We compare and contrast the absorptions of CH4 in solid H2O with those of pure CH4. Changes in selected peak positions, profiles, and relative strength with temperature are presented, and absolute strengths for absorptions of CH4 in solid H2O are estimated. Using the two largest (v(3) + v(4)) and (v(1) + v(4)) near-IR absorptions of CH4 at 2.324 and 2.377 mu m (4303 and 4207 cm(-1)), respectively, as examples, we show that peaks of CH4 in solid H2O are at slightly shorter wavelength (higher frequency) and broader than those of pure solid CH4. With increasing temperature, these peaks shift to higher frequency and become increasingly broad, but this trend is reversible on re-cooling, even though the phase transitions of H2O are irreversible. It is to be hoped that these observations of changes in the positions, profiles, and relative intensities of CH4 absorptions with concentration and temperature will be of use in understanding spectra of icy outer Solar System bodies. (c) 2005 Elsevier Inc. All rights reserved.

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