| Object type | Small inner moon of Saturn[1] |
|---|---|
| Discovered | June 1, 2004, Cassini Imaging Team[2] |
| Shape | Egg-shaped triaxial ellipsoid[1] |
| Size | Mean radius ≈ 1.6 km[2] |
| Density | ≈ 0.31 g/cm³ — among the lowest known[1] |
| Resonance | 14:15 with Mimas[1] |
| Closest Cassini flyby | May 20, 2012, ≈ 1,900 km[1] |
| Mean distance | ≈ 194,700 km from Saturn[3] |
| Orbital period | ≈ 24 hours[2] |
An egg in orbit
Cassini’s close-up images in May 2012 revealed a remarkably smooth, non-spherical moonlet.[1] NASA says it’s hard not to think of an egg.[2]
Icy fluff
Methone’s smoothness suggests an equipotential surface of mobile icy fluff, which might explain its lack of craters.[1]
Lighter than water
Assuming its shape balances Saturn’s tides and its own gravity, Methone’s density is about 0.31 g/cm³ — among the lowest values for any Solar System body.[1]
Rocked by Mimas
A 14:15 resonance with Mimas makes Methone’s semi-major axis vary by about 20 km over about 450 days.[1]
Orbit
Methone orbits about 194,700 km from Saturn in about 24 hours.[3][2]
Methone ring arc
Material blasted off Methone is believed to feed a faint partial ring discovered in September 2006.[1]
Read more
Sources
- Methone (moon) — Wikipedia
- Methone — NASA Science
- Planetary Satellite Mean Elements — NASA JPL Solar System Dynamics
- Alcyonides — Wikipedia
- Hydrostatic equilibrium — Wikipedia
Figures are rounded; where sources differ we note it. Spotted an error? Tell us.