| Object type | Trojan (co-orbital) moon of Saturn[1] |
|---|---|
| Location | Trailing L5 Lagrange point of Dione[1] |
| Discovered | Images of 21 Oct. 2004, Cassini Imaging Science Team[1] |
| Named | 21 January 2005, after Polydeuces (Pollux)[1] |
| Diameter | ≈ 3 km[1] |
| Surface | Probably smooth, coated with icy particles from Enceladus[1] |
| Mean distance | ≈ 377,600 km from Saturn[3] |
| Orbital period | ≈ 2.74 days[3] |
| Eccentricity | ≈ 0.019[3] |
A trojan moon
Polydeuces shares Dione’s orbit, sitting around Dione’s trailing L5 Lagrange point. Helene occupies the leading point.[1][2]
The biggest wanderer
Perturbations from nearby moons make Polydeuces drift away from its Lagrange point periodically. Of Saturn’s four known trojan moons, it shows the largest displacement.[1]
Dusted with Enceladus ice
About 3 km across, Polydeuces is thought to have a smooth surface coated with fine icy particles from the cryovolcanic plumes of Enceladus.[1]
Spotted by blinking
The Cassini Imaging Science Team found it on 24 October 2004 in images taken on 21 October, using the blink comparison technique. Pre-discovery images went back to April 2004.[1]
Orbit
With Dione and Helene, Polydeuces orbits Saturn every 2.74 days at about 377,600 km, between Tethys and Rhea.[1][3]
The name
Polydeuces is another name for Pollux, twin brother of Castor and son of Zeus and Leda.[1]
Read more
Sources
- Polydeuces (moon) — Wikipedia
- Polydeuces — NASA Science
- Planetary Satellite Mean Elements — NASA JPL Solar System Dynamics
- Lagrange point — Wikipedia
- Dione (moon) — Wikipedia
Figures are rounded; where sources differ we note it. Spotted an error? Tell us.