| Object type | Irregular, retrograde moon of Neptune[1] |
|---|---|
| Discovered | 14 Aug. 2002, Cerro Tololo, Chile[1] |
| Named | 3 Feb. 2007, after one of the Nereids[1] |
| Diameter | ≈ 42–62 km[1] |
| Colour | Grey, similar to Nereid[1] |
| Brightness | Apparent magnitude ≈ 24[1] |
| Mean distance | ≈ 16.6 million km from Neptune[3] |
| Orbital period | ≈ 1,879 days (5.1 years)[3] |
| Inclination | ≈ 120° (retrograde)[3] |
| Eccentricity | ≈ 0.52 (varies 0.19–0.90)[1] |
Neptune’s second retrograde moon
Halimede is the second-innermost known retrograde moon of Neptune, after Triton. It takes about 5.1 years to orbit.[1]
A wandering orbit
The Sun’s gravity changes Halimede’s orbit substantially over thousands of years: its eccentricity ranges from 0.19 to 0.90 and its inclination from 111° to 145°.[1]
On a collision course?
A 2004 study estimated a 41% chance that Halimede hits Nereid within 4.5 billion years.[1] Its colour is similar to Nereid’s, so it might even be a fragment of Nereid.[1]
Found from the ground
Matthew Holman’s team found Halimede on 14 August 2002 with the 4-m Blanco Telescope, using shift-and-add imaging. It was among the first Neptunian moons found from the ground since Nereid in 1949.[1][2]
Orbit
JPL’s mean elements give an average distance of about 16.6 million km, ranging from about 7.9 to 25.2 million km.[3]
The name
Halimede is named after one of the fifty Nereids, daughters of Nereus and Doris. The “e” ending marks its retrograde orbit.[1]
Read more
Sources
- Halimede (moon) — Wikipedia
- Halimede — NASA Science
- Planetary Satellite Mean Elements — NASA JPL Solar System Dynamics
- Nereid (moon) — Wikipedia
- Neptune — Wikipedia
Figures are rounded; where sources differ we note it. Spotted an error? Tell us.