Cassini encounters Enceladus: Background and the discovery of a south polar hot spot

被引:422
作者
Spencer, JR
Pearl, JC
Segura, M
Flasar, FM
Mamoutkine, A
Romani, P
Buratti, BJ
Hendrix, AR
Spilker, LJ
Lopes, RMC
机构
[1] SW Res Inst, Dept Space Studies, Boulder, CO 80302 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
D O I
10.1126/science.1121661
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
The Cassini spacecraft completed three close flybys of Saturn's enigmatic moon Enceladus between February and July 2005. On the third and closest flyby, on 14 July 2005, multiple Cassini instruments detected evidence for ongoing endogenic activity in a region centered on Enceladus' south pole. The polar region is the source of a plume of gas and dust, which probably emanates from prominent warm troughs seen on the surface. Cassini's Composite Infrared Spectrometer (CIRS) detected 3 to 7 gigawatts of thermal emission from the south polar troughs at temperatures up to 145 kelvin or higher, making Enceladus only the third known solid planetary body-after Earth and lo-that is sufficiently geologically active for its internal heat to be detected by remote sensing. If the plume is generated by the sublimation of water ice and if the sublimation source is visible to CIRS, then sublimation temperatures of at least 180 kelvin are required.
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页码:1401 / 1405
页数:5
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