Anderson J D, Schubert G, Jacobson R A, Lau E L, Moore W B, Sjogren W L
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
Science. 1998 Sep 25;281(5385):2019-22. doi: 10.1126/science.281.5385.2019.
Radio Doppler data from four encounters of the Galileo spacecraft with the jovian moon Europa have been used to refine models of Europa's interior. Europa is most likely differentiated into a metallic core surrounded by a rock mantle and a water ice-liquid outer shell, but the data cannot eliminate the possibility of a uniform mixture of dense silicate and metal beneath the water ice-liquid shell. The size of a metallic core is uncertain because of its unknown composition, but it could be as large as about 50 percent of Europa's radius. The thickness of Europa's outer shell of water ice-liquid must lie in the range of about 80 to 170 kilometers.
伽利略号航天器四次飞越木星卫星木卫二时获取的无线电多普勒数据,已被用于完善木卫二内部结构模型。木卫二很可能分层为一个金属内核,其外环绕着岩石地幔以及一层水冰 - 液态外壳,但这些数据无法排除在水冰 - 液态壳之下存在致密硅酸盐与金属均匀混合物的可能性。由于金属内核成分未知,其大小尚不确定,但可能大至木卫二半径的约50%。木卫二水冰 - 液态外壳的厚度必定在约80至170千米的范围内。