Photolysis of solid NH3 and NH3-H2O mixtures at 193 nm

被引:28
作者
Loeffler, M. J. [1 ,2 ]
Baragiola, R. A. [1 ]
机构
[1] Univ Virginia, Lab Atom & Surface Phys Engn Phys, Charlottesville, VA 22904 USA
[2] NASA, Goddard Space Flight Ctr, Astrochem Lab, Greenbelt, MD 20771 USA
关键词
MU-M BAND; ICY SATELLITES; WATER ICE; TRAILING HEMISPHERES; INFRARED-SPECTRUM; SOLAR-SYSTEM; AMMONIA; ENCELADUS; SPECTROSCOPY; ULTRAVIOLET;
D O I
10.1063/1.3506577
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
We have studied UV photolysis of solid ammonia and ammonia-dihydrate samples at 40 K, using infrared spectroscopy, mass spectrometry, and microgravimetry. We have shown that in the pure NH3 sample, the main species ejected are NH3, H-2, and N-2, where the hydrogen and nitrogen increase with laser fluence. This increase in N-2 ejection with laser fluence explains the increase in mass loss rate detected by a microbalance. In contrast, for the ammonia-water mixture, we see very weak signals of H-2 and N-2 in the mass spectrometer, consistent with the very small mass loss during the experiment and with a <5% decrease in the NH3 infrared absorption bands spectroscopy after a fluence of similar to 3 x 10(19) photons/cm(2). The results imply that ammonia-ice mixtures in the outer solar system are relatively stable under solar irradiation. (C) 2010 American Institute of Physics. [doi:10.1063/1.3506577]
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页数:7
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