Ices in the giant planets

被引:0
|
作者
Podolak, M [1 ]
Hubbard, WB [1 ]
机构
[1] Tel Aviv Univ, IL-69978 Tel Aviv, Israel
来源
SOLAR SYSTEM ICES | 1998年 / 227卷
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暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Interior models show that Jupiter and Saturn consist mostly of free hydrogen and helium, while Uranus and Neptune consist mostly of material with a zero-pressure density near 1 g cm(-3) The dominant material in Uranus and Neptune is almost certainly ice, while models imply that Jupiter and Saturn each contain roughly one Uranus or Neptune mass of non-hydrogen-helium material which is probably ice. Although the ice component of the giant planets is largely inaccessible to direct observation, a considerable body of indirect evidence suggests that these four planets contain the largest reservoirs of ice in the planetary system.
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页码:735 / 748
页数:14
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