13 Egeria
| Discovery | |
|---|---|
| Discovered by | Annibale de Gasparis |
| Discovery site | Naples Obs. |
| Discovery date | 2 November 1850 |
| Designations | |
| (13) Egeria | |
| Pronunciation | /ɪˈdʒɪəriə/ |
Named after | Egeria |
| Main belt | |
| Adjectives | Egerian |
| Symbol | (historical) |
| Orbital characteristics | |
| Epoch 17.0 October 2024 (JD 2460600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 63566 days (174.03 yr) |
| Aphelion | 2.79788 AU (418.557 Gm) |
| Perihelion | 2.35759 AU (352.690 Gm) |
| 2.57774 AU (385.624 Gm) | |
| Eccentricity | 0.085403 |
| 4.14 yr (1511.7 d) | |
Average orbital speed | 18.56 km/s |
| 305.547° | |
| 0° 14m 17.34s / day | |
| Inclination | 16.532° |
| 43.208° | |
| 79.222° | |
| Earth MOID | 1.43636 AU (214.876 Gm) |
| Jupiter MOID | 2.35842 AU (352.815 Gm) |
| TJupiter | 3.363 |
| Physical characteristics | |
| Dimensions | 214.8 km × 192 km 238 km × 199 km × 182 km (± 12 km × 11 km × 10 km) |
| 202±3 km 207.6 ± 8.3 km (IRAS) | |
| Flattening | 0.24 |
| Mass | (9.2±2.1)×1018 kg (15.9±4.4)×1018 kg |
Mean density | 2.13±0.49 g/cm3 3.4±1.0 g/cm3 |
Equatorial surface gravity | ≈0.0580 m/s2 |
Equatorial escape velocity | ≈0.1098 km/s |
| 0.2935 d (7.044 h) 7.045 h 7.046664±0.000003 h | |
| 59° | |
Pole ecliptic latitude | 31°±5° |
Pole ecliptic longitude | 38°±5° |
| 0.087 0.049 ± 0.028 0.085 ± 0.007 | |
| Temperature | ~174 K |
| G-type asteroid | |
| 9.71 to 12.46 | |
| 6.91 6.74 | |
13 Egeria is a large main-belt G-type asteroid. It was discovered by Annibale de Gasparis on November 2, 1850. Egeria was named by Urbain Le Verrier, whose computations led to the discovery of Neptune, after the mythological nymph Egeria of Aricia, Italy, the wife of Numa Pompilius, second king of Rome.
The historical symbol for Egeria was a buckler. It is in the pipeline for Unicode 17.0 as U+1CEC6 ().
Egeria occulted a star on January 8, 1992. Its disc was determined to be quite circular (217×196 km). On January 22, 2008, it occulted another star, and this occultation was timed by several observers in New Mexico and Arizona, coordinated by the IOTA Asteroid Occultation Program. The result showed that Egeria presented an approximately circular profile to Earth of 214.8×192 km, well in agreement with the 1992 occultation. It has also been studied by radar.
In 1988 a search for satellites or dust orbiting this asteroid was performed using the UH88 telescope at the Mauna Kea Observatories, but the effort came up empty. Spectral analysis of Egeria shows it to be unusually high in water content, 10.5–11.5% water by mass. This makes Egeria a prominent candidate for future water-mining ventures.