Fig. 1

Radial distance of Jupiter’s H2O ice line (roughly horizontal lines) and centrifugal disk radius (curved solid line) during its final accretion phase. Inside about 4.5 AU from the Sun, Jupiter’s disk does not contain an H2O ice line in any of the CSD models (Hayashi 1981; Bitsch et al. 2015, see legend). Locations of the Galilean moons are indicated by symbols at 5.2 AU. Symbol sizes scale with the physical radii of the moons (orange: rocky, blue: icy composition).
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