Structure of the atmosphere of Jupiter: Galileo probe measurements

被引:93
|
作者
Seiff, A
Kirk, DB
Knight, TCD
Mihalov, JD
Blanchard, RC
Young, RE
Schubert, G
vonZahn, U
Lehmacher, G
Milos, FS
Wang, J
机构
[1] NASA,AMES RES CTR,MOFFETT FIELD,CA 94035
[2] NASA,LANGLEY RES CTR,HAMPTON,VA 23681
[3] UNIV CALIF LOS ANGELES,DEPT EARTH & SPACE SCI,LOS ANGELES,CA 90024
[4] UNIV ROSTOCK,INST ATMOSPHARENPHYS,KUHLUNGSBORN,GERMANY
[5] NASA,GODDARD SPACE FLIGHT CTR,GREENBELT,MD 20771
关键词
D O I
10.1126/science.272.5263.844
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
Temperatures and pressures measured by the Galileo probe during parachute descent into Jupiter's atmosphere essentially followed the dry adiabat between 0.41 and 24 bars, consistent with the absence of a deep water cloud and with the low water content found by the mass spectrometer. From 5 to 15 bars, lapse rates were slightly stable relative to the adiabat calculated for the observed H-2/He ratio, which suggests that upward heat transport in that range is not attributable to simple radial convection, In the upper atmosphere, temperatures of >1000 kelvin at the 0.01-microbar level confirmed the hot exosphere that had been inferred from Voyager occultations. The thermal gradient increased sharply to 5 kelvin per kilometer at a reconstructed altitude of 350 kilometers, as was recently predicted, Densities at 1000 kilometers were 100 times those in the preencounter engineering model.
引用
收藏
页码:844 / 845
页数:2
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