Galileo search for SO2-frost condensation on Io's nightside

被引:9
|
作者
Simonelli, DP
Veverka, J
Senske, DA
Fanale, FP
Schubert, G
Belton, MJS
机构
[1] Cornell Univ, Ctr Radiophys & Space Res, Ithaca, NY 14853 USA
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[3] Univ Hawaii, Inst Geophys, Honolulu, HI 96822 USA
[4] Univ Calif Los Angeles, Dept Earth & Space Sci, Los Angeles, CA 90095 USA
[5] Natl Opt Astron Observ, Tucson, AZ 85719 USA
关键词
atmospheres; dynamics; Galileo spacecraft; Io; surfaces; satellite;
D O I
10.1006/icar.1998.5974
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
New, high-quality Galileo images of Io's dayside and Jupiterlit nightside, examined for diurnal changes in violet albedo patterns and diurnal changes in hemispheric color, do not provide any evidence for significant nighttime condensation of the satellite's thin SO2 atmosphere. In particular, the Galileo images do not show the major change in Io's average hemispheric color between day and night that was reported by Buratti et al. (1995, Icarus 118, 418-422) in a study of Voyager data. The lack of detectable nighttime frost deposition in the Galileo images is not surprising, given the tenuous, "patchy" nature of Io's SO2 atmosphere and the associated difficulty in producing optically thick nighttime frost layers. (C) 1998 Academic Press.
引用
收藏
页码:166 / 174
页数:9
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