Photolysis of H2O-H2O2 mixtures: The destruction of H2O2

被引:9
|
作者
Loeffler, M. J. [1 ,2 ]
Fama, M. [2 ]
Baragiola, R. A. [2 ]
Carlson, R. W. [3 ]
机构
[1] NASA, GSFC, Astrochem Lab, Greenbelt, MD 20771 USA
[2] Univ Virginia, Lab Atom & Surface Phys, Charlottesville, VA 22904 USA
[3] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
Europa; Ices; IR spectroscopy; Jupiter; satellites; Saturn; Photochemistry; HYDROGEN-PEROXIDE; WATER ICE; INFRARED-SPECTRA; QUANTUM YIELD; ION; ULTRAVIOLET; RADIATION; PHOTODISSOCIATION; ENCELADUS; MARS;
D O I
10.1016/j.icarus.2013.06.030
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present laboratory results on the loss of H2O2 in solid H2O + H2O2 mixtures at temperatures between 21 and 145 K initiated by UV photolysis (193 nm). Using infrared spectroscopy and microbalance gravimetry, we measured the decrease of the 3.5 mu m infrared absorption band during UV irradiation and obtained a photodestruction cross section that varies with temperature, being lowest at 70 K. We use our results, along with our previously measured H2O2 production rates via ionizing radiation and ion energy fluxes from the spacecraft to compare H2O2 creation and destruction at icy satellites by ions from their planetary magnetosphere and from solar UV photons. We conclude that, in many cases, H2O2 is not observed on icy satellite surfaces because the H2O2 photodestruction rate is much higher than the production rate via energetic particles, effectively keeping the H2O2 infrared signature at or below the noise level. Published by Elsevier Inc.
引用
收藏
页码:945 / 950
页数:6
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