THERMODYNAMICS OF SELECTED TRACE-ELEMENTS IN THE JOVIAN ATMOSPHERE

被引：21
作者：
FEGLEY, B
LEWIS, JS
机构：
[1] Department of Earth and Planetary Sciences, Massachusetts Institute of Technology, Cambridge
来源：
ICARUS | 1979年 / 38卷 / 02期
基金：
美国国家航空航天局;
关键词：
D O I：
10.1016/0019-1035(79)90176-3
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The thermochemistry of several hundred compounds of twelve selected trace elements (Ge, Se, Ga, As, Te, Pb, Sn, Cd, Sb, Tl, In, and Bi) has been investigated for solar composition material along a Jupiter adiabat. The results indicate that AsF3, InBr, TlI, and SbS, in addition to CO, PH3, GeH4, AsH3, H2Se, HCl, HF, and H3BO3 proposed by Barshay and Lewis (1978), may be potential chemical tracers of atmospheric dynamics. The reported observations of GeH4 is interpreted on the basis of new calculations as implying rapid vertical transport from levels where T ≥ 800°K. Upper limits are also set on the abundances of many gaseous compounds of the elements investigated. © 1979.
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页码：166 / 179
页数：14
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