Quote:
Originally Posted by Kraydak
2) Formation mechanism (direct gravitational collapse, like a star, or core-accretion building up a rocky core, like a planet). While more conceptually useful than definition (1), it doesn't make any observational predictions…
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Direct gravitational collapse alone would result in an object with a solar nebula abundance. Core-accretion would result in an object with greater amounts of metals, rocky material, and possibly ices. It is
possible that such a difference could be measurable or at least rule out certain formation models for certain objects.
To bring this back on topic: it seems based on everything I'm hearing that you can safely ignore the heat given off by a gas giant for it's moons, unless your system is still in the process of forming.