.png) A three-dimensional model of 382 Dodona based on its light curve | |
| Discovery | |
|---|---|
| Discovered by | Auguste Charlois |
| Discovery date | 29 January 1894 |
| Designations | |
| (382) Dodona | |
| Pronunciation | /dəˈdoʊnə/[1] |
Named after | Dodona |
| 1894 AT | |
| Main belt | |
| Orbital characteristics[2] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 122.21 yr (44636 d) |
| Aphelion | 3.6577 AU (547.18 Gm) |
| Perihelion | 2.58301 AU (386.413 Gm) |
| 3.1204 AU (466.81 Gm) | |
| Eccentricity | 0.17221 |
| 5.51yr (2013.3d) | |
| 6.32892° | |
| 0° 10m 43.716s / day | |
| Inclination | 7.3928° |
| 313.511° | |
| 270.036° | |
| Physical characteristics | |
| Dimensions | 58.37±2.8 km[2] 58.37 km[3] |
| 4.113 h (0.1714 d) | |
| 0.1610±0.017[2] 0.161[3] | |
| M | |
| 8.77[2][3] | |
382 Dodona is a largeMain beltasteroid that was discovered by the French astronomerAuguste Charlois on 29 January 1894 inNice. It is classified as anM-type asteroid.
Measurements of thethermal inertia of 115 Thyra give an estimated range of 15–150 J m−2 K−1 s−1/2, compared to 50 forlunar regolith and 400 for coarse sand in an atmosphere.[3]
_mathilde.jpg) | This article about an asteroid native to theasteroid belt is astub. You can help Wikipedia byexpanding it. |
