Saturn possesses more than 60 known moons. (A table summarizing data for Saturn's moons appears in Appendix B, "Moons of Saturn.") Of the first 18 discovered, all but the much more distant moon Phoebe orbit within about 3.6 million km (2.2 million miles) of Saturn. Nine are more than 100 km (60 miles) in radius and were discovered telescopi-cally before the 20th century; the others were found in an analysis of Voyager images in the early 1980s. Several additional inner moons—tiny bodies with radii of 3-4 km (1.9-2.5 miles)—were discovered in Cassini spacecraft images beginning in 2004. All of the inner moons are regular, having prograde, low-inclination, and low-eccentricity orbits with respect to the planet. The eight largest are thought to have formed along Saturn's equatorial plane from a protoplanetary disk of material, in much the same way as the planets formed around the Sun from the primordial solar nebula.

A second, outer group of moons lies beyond about 11 million km (6.8 million miles). They are irregular in that all of their orbits have large eccentricities and inclinations; about two-thirds revolve around Saturn in a retrograde fashion— they move opposite to the planet's rotation. Except for Phoebe, they are less than about 20 km (12 miles) in radius. Some were discovered from Earth beginning in 2000 as the result of efforts to apply new electronic detection methods to the search for fainter—and hence smaller—objects in the solar system; others were found by Cassini. These outer bodies appear to be not primordial moons but rather captured objects or their fragments.

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