| Object type | Irregular, retrograde moon of Jupiter[1] |
|---|---|
| Group | Pasiphae group[1] |
| Discovered | Dec. 9, 2001, Mauna Kea, Hawaii[2] |
| Discoverers | S. S. Sheppard, D. C. Jewitt, J. T. Kleyna[2] |
| Named | August 2003[1] |
| Diameter | ≈ 3 km[1] |
| Mean distance | ≈ 22.9 million km from Jupiter[3] |
| Orbital period | ≈ 708 days[3] |
| Inclination | ≈ 149° (retrograde)[3] |
| Eccentricity | ≈ 0.29[3] |
Found with a sibling
Eurydome was discovered together with Hermippe by Sheppard’s team in 2001, and designated S/2001 J 4.[1] It is about 3 km across.[1]
The Pasiphae group
Eurydome belongs to the Pasiphae group, retrograde moons at 22.8–24.1 million km with inclinations of 144.5°–158.3°.[1] Most or all of them are thought to come from one captured asteroid broken by a collision.[2]
The parent body
The group’s original body is calculated to have been about 60 km across, about the size of Pasiphae itself.[4]
The name
Named in August 2003, Eurydome is sometimes described in Greek myth as the mother of the Graces by Zeus.[1]
Orbit
Eurydome orbits backwards between about 16.3 and 29.5 million km, once every 708 days.[3]
Hands-on science
Orbits, gravity and collisions are fun to explore at home. Our science kit picker suggests kits by age and interest.
Read more
Orbital elements explained, with Eurydome
Semi-major axis, eccentricity, inclination and period in plain language.
Read →Eurydome and Hermippe: discovered together
Two moons found in the same December 2001 search.
Read →The 60-kilometre parent of the Pasiphae group
What one broken asteroid left behind.
Read →Sources
- Eurydome (moon) — Wikipedia
- Eurydome — NASA Science
- Planetary Satellite Mean Elements — NASA JPL Solar System Dynamics
- Pasiphae group — Wikipedia
Figures are rounded; where sources differ we note it. Spotted an error? Tell us.