Global color variations on Io

被引:97
作者
Geissler, PE [1 ]
McEwen, AS
Keszthelyi, L
Lopes-Gautier, R
Granahan, J
Simonelli, DP
机构
[1] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[3] SETS Technol Inc, Honolulu, HI 96813 USA
[4] Univ Hawaii, Sci & Technol Int, Honolulu, HI 96813 USA
[5] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA
关键词
Io; Galileo; spectroscopy; multispectral imaging;
D O I
10.1006/icar.1999.6128
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Visible and near-infrared images of Io from the Galileo spacecraft reveal a surface more colorful than previously thought. Red, yellow green, white, and black hues decorate the satellite, presumably caused by a varied composition of sulfur compounds and silicates. Almost a third of Io is covered by red and orange materials, particularly at polar latitudes above +/-30 degrees. These red regions were scarcely distinguishable in the shorter wavelength Voyager observations. Bright red pyroclastic deposits mark the locations of many hot spots, plumes, and visible surface changes, providing a prominent flag of recent volcanic activity. Io's equatorial regions are dominated by yellow materials, which occupy about 40% of the satellite's surface. White and gray materials cover about 27% of Io, primarily in equatorial areas and in localized deposits at high latitudes. These are identified with moderate-to-coarse-grained SO2 as mapped by the NIMS instrument on Galileo (R. W. Carlson et al, 1997, Geophys, Res. Lett. 24, 2479-2482). Greenish-yellow materials in small isolated spots on Io's anti-Jupiter hemisphere were recently discovered in 3 km/pixel color imaging from orbit 14. Unlike other ionian terrains, these regions have a negative near-infrared spectral slope, suggesting contamination by a nonsulfur component. Only about 1.4% of Io's surface is occupied by dark materials, which display a variety of visible colors ranging from black to red and green. Most dark spots have a shallow spectral absorption feature at 0.9 mu m, suggesting magnesium-rich silicates rather than black sulfur. Little large-scale alteration in the global color and albedo pattern has occurred between the Voyager and Galileo eras; 90% of the surface appears unchanged despite the vigorous volcanic activity which must have taken place in the intervening 17 years. This suggests that over a time scale of decades, the bulk of Io's resurfacing is restricted to a few small but persistently active areas. (C) 1999 Academic Press.
引用
收藏
页码:265 / 282
页数:18
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