Radio Doppler data from four encounters of the Galileo spacecraft with
the jovian moon Europa have been used to refine models of Europa's in
terior. Europa is most Likely differentiated into a metallic core surr
ounded by a rock mantle and a water ice-liquid outer shell, but the da
ta cannot eliminate the possibility of a uniform mixture of dense sili
cate and metal beneath the water ice-liquid shell. The size of a metal
lic core is uncertain because of its unknown composition, but it could
be as targe 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 abou
t 80 to 170 kilometers.