| Object type | Small inner moon of Saturn[1] |
|---|---|
| Discovered | June 1, 2004, Cassini Imaging Team[2] |
| First photographed | Possibly by Voyager 2 on 23 Aug. 1981[2] |
| Size | Mean radius ≈ 2.5 km[2] |
| Ring | Pallene Ring, ≈ 2,500 km wide[1] |
| Cassini flybys | 16 Oct. 2010 (36,000 km); 14 Sept. 2011 (44,000 km)[1] |
| Mean distance | ≈ 212,300 km from Saturn[3] |
| Orbital period | ≈ 1.16 days[3] |
A small inner moon
Pallene orbits between Mimas and Enceladus. Like Methone and Aegaeon, it is smooth and ellipsoidal, with a darker surface than expected.[1]
Seen in 1981?
After its 2004 discovery, Pallene was matched to a single Voyager 2 photo from 23 August 1981, once designated S/1981 S 14.[1]
A full dust ring
Cassini found a faint dust ring sharing Pallene’s orbit, about 2,500 km wide. Unlike Methone and Anthe, Pallene has a complete ring rather than an arc, because it is not in resonance.[1]
Near — but not in — resonance
Enceladus perturbs Pallene’s orbit. It was once thought to be in a 19:16 resonance with Enceladus, but is now known to be very close to, not in, resonance.[1]
Orbit
Pallene circles Saturn every 1.16 days at about 212,300 km.[3]
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Sources
- Pallene (moon) — Wikipedia
- Pallene — NASA Science
- Planetary Satellite Mean Elements — NASA JPL Solar System Dynamics
- Alcyonides — Wikipedia
Figures are rounded; where sources differ we note it. Spotted an error? Tell us.