Jupiter, with its 67 known moons, can be viewed as a miniature solar system revolving around the Sun. Four of these moons are large enough to be visible with even a small telescope. These so-called Galilean satellites — Io, Europe, Ganymede, and Callisto — are of nearly planetary size.
But scientists haven’t been able to explain how these moons became so big. Now, scientists have conducted a study to suggest that Saturn might be to blame.
During the solar system’s earliest years, a huge rotating disk of gas and dust surrounded the Sun. The dust quickly glommed together into pebble-sized chunks, out of which the planets and most moons formed. As Jupiter came together, it acquired its own disk by sweeping clean a gap in the gaseous disk around the Sun. It’s likely that the Galilean moons began forming within Jupiter’s circumplanetary disk. But even as the giant collected gas from the circumsolar disk, it was carving the gap that would cut off its disk from material that would have helped build its moons.
René Heller (University of Göttingen, Germany), who was not involved in the new study, notes that astronomers have long been lacking a mechanism to deliver solid material to Jupiter’s circumplanetary disk. “This aspect has often been overlooked or simplified in previous models for the formation of the Galilean satellites; we assumed that the gas and dust was just there, out of nowhere,” he says.
One of the astronomers who investigated this impasse is Thomas Ronnet (Astrophysical Laboratory of Marseille,France). He realized that Jupiter’s massive neighbor Saturn might be involved. When the planets were forming, their orbits were still migrating — resulting in a solar system that looked very different from the one we see now, Saturn in particular is thought to have been in an orbit much closer to that of Jupiter. So Saturn could have dispersed pebbles that were stuck in the midplane of the circumsolar disk, allowing Jupiter to capture them.
