A model of Jupiter's early circumplanetary disk shows that self-shadowing creates a ~100 K cold trap around 10 Jupiter radii that can condense volatile ices and may shape Galilean moon compositions.
E., Mousis, O., & Ronnet, T
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Impact of Jupiter's heating and self-shadowing on the Jovian circumplanetary disk structure
A model of Jupiter's early circumplanetary disk shows that self-shadowing creates a ~100 K cold trap around 10 Jupiter radii that can condense volatile ices and may shape Galilean moon compositions.