机构:
Tel Aviv Univ, IL-69978 Tel Aviv, IsraelTel Aviv Univ, IL-69978 Tel Aviv, Israel
Podolak, M
[1
]
Hubbard, WB
论文数: 0引用数: 0
h-index: 0
机构:
Tel Aviv Univ, IL-69978 Tel Aviv, IsraelTel Aviv Univ, IL-69978 Tel Aviv, Israel
Hubbard, WB
[1
]
机构:
[1] Tel Aviv Univ, IL-69978 Tel Aviv, Israel
来源:
SOLAR SYSTEM ICES
|
1998年
/
227卷
关键词:
D O I:
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.