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

被引:28
|
作者
Bernstein, MP [1 ]
Cruikshank, DP [1 ]
Sandford, SA [1 ]
机构
[1] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
关键词
ices; infrared observations; spectroscopy; surfaces; planets; satellites;
D O I
10.1016/j.icarus.2005.10.021
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:302 / 308
页数:7
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