TY - JOUR
T1 - Comparative models of Uranus and Neptune
AU - Podolak, M.
AU - Weizman, A.
AU - Marley, M.
PY - 1995/12
Y1 - 1995/12
N2 - 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.
AB - 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.
UR - https://www.scopus.com/pages/publications/0039088566
U2 - 10.1016/0032-0633(95)00061-5
DO - 10.1016/0032-0633(95)00061-5
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AN - SCOPUS:0039088566
SN - 0032-0633
VL - 43
SP - 1517
EP - 1522
JO - Planetary and Space Science
JF - Planetary and Space Science
IS - 12
ER -