<blockquote><font class="small">In reply to:</font><hr /><p>I have no prejudice against the capture theory. But if you speak of comparisons, well there are only two gas giants, Jupiter and Saturn. <br />Uranus and Neptune are ice giants.<p><hr /></p></p></blockquote><br /><br />I don't think that distinction is particularly relevant in this case. I think we can generalise to a position that natural satellites which form in situ do so as some part of the planetary formation process (e.g. from accretion disks or perhaps Prentice's neo-Laplacian hypothesis) and we should expect some regularities from natural satellite families. Looking at unusually large single moons, we only have our own Moon, which apparently had an unusual genesis (result of massive protoplanet collision, so didn't form in "the usual way") and Triton, which seems to be a captured ice dwarf, i.e it didn't form in orbit around Neptune either.<br /><br />The final form of the "mother planets" doesn't matter too much I think. I'm just looking at a very generalised picture of bodies of reasonably large size forming with a reasonably regular satellite family in situ.<br /><br /><blockquote><font class="small">In reply to:</font><hr /><p>upiter has precisely two moons in the same class as Ttian (Ganymede and Callisto). So I don't see why Titan is so odd on the global picture.<p><hr /></p></p></blockquote><br /><br />My previous (perhaps unwise heh) jokey presentation aside, my observation such as it is is that Titan doesn't in general look like the rest of the Saturnian satellite family. It's very much larger, it has large quantities of gaseous volatiles which e.g. Ganymede and Callisto lack. I think there's reason to suspect that it formed elsewhere from the Saturn system. So perhaps Mimas, Enceladus, Tethys, Dione, Rhea and Iapetus are Saturn's orginal satellite family, analogous to the Galileans and the Uranian family, and Titan is an interloper in the system.<br /><br />It's not so much about absolute size. Trying to predict what sizes