Despina (moon)
Despina as seen by Voyager 2 (smeared horizontally)
|
|
| Discovery | |
|---|---|
| Discovered by | Stephen P. Synnott and Voyager Imaging Team |
| Discovery date | July 1989 |
| Orbital characteristics | |
| Epoch 18 August 1989 | |
| 52 526 ± 1 km | |
| Eccentricity | 0.0002 ± 0.0002 |
| 0.33465551 ± 0.00000001 d | |
| Inclination |
|
| Satellite of | Neptune |
| Physical characteristics | |
| Dimensions | 180×148×128 km |
|
Mean radius
|
75 ± 3 km |
| Volume | ~1.8×106km³ |
| Mass | ~2.2×1018 kg (based on assumed density) |
|
Mean density
|
~1.2 g/cm³ (estimate) |
| ~0.026 m/s2 | |
| ~0.063 km/s | |
| synchronous | |
| zero | |
| Albedo | 0.09 |
| Temperature | ~51 K mean (estimate) |
| 22.0 | |
Despina (/dᵻˈspiːnə/ di-SPEE-nə or /dᵻˈspaɪnə/ di-SPY-nə; Latin: Despœna,; Greek: Δέσποινα), also known as Neptune V, is the third closest inner satellite of Neptune. It is named after Despoina, a nymph who was a daughter of Poseidon and Demeter.
Despina was discovered in late July 1989 from the images taken by the Voyager 2 probe. It was given the temporary designation S/1989 N 3. The discovery was announced (IAUC 4824) on August 2, 1989, but the text only talks of "10 frames taken over 5 days", giving a discovery date of sometime before July 28. The name was given on 16 September 1991.
Despina is irregularly shaped and shows no sign of any geological modification. It is likely that it is a rubble pile re-accreted from fragments of Neptune's original satellites, which were smashed up by perturbations from Triton soon after that moon's capture into a very eccentric initial orbit.
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