Abstract
Models of Uranus and Neptune are computed based on the assumption that these planets consist of three layers: a rock core, an ice shell, and an atmosphere. Uranus models require that the ice shell have a density some 10% lower than the canonical density for an ice mixture. Two Neptune models are found, one with the canonical density in the ice shell, and one with a density 20% lower. The implications of these models are discussed.
Original language | English (US) |
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Pages (from-to) | 1517-1522 |
Number of pages | 6 |
Journal | Planetary and Space Science |
Volume | 43 |
Issue number | 12 |
DOIs | |
State | Published - Dec 1995 |
Externally published | Yes |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science