Abstract
The deep interiors of Jupiter, Saturn, Uranus, Neptune, and their satellites are discussed. The important issues relevant to the physics of condensed matter are identified. The discussion emphasizes H_2, H-He, H_2- H_2O, H_2-CH_4, NH_3, and CH_4·5.75H_2O. Present and future theory and experiment are of great benefit to planetary science.
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