 Orbital diagram | |
| Discovery | |
|---|---|
| Discovered by | Auguste Charlois |
| Discovery date | 1 September 1891 |
| Designations | |
| (314) Rosalia | |
| Pronunciation | /roʊˈzeɪliə,-ɑːliə/[1] |
| Main belt | |
| Orbital characteristics[2] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 124.62 yr (45517 d) |
| Aphelion | 3.71009 AU (555.022 Gm) |
| Perihelion | 2.59640 AU (388.416 Gm) |
| 3.15325 AU (471.719 Gm) | |
| Eccentricity | 0.17659 |
| 5.60yr (2045.2d) | |
| 116.710° | |
| 0° 10m 33.679s / day | |
| Inclination | 12.5603° |
| 170.314° | |
| 190.369° | |
| Physical characteristics | |
| Dimensions | 59.65±2.2 km |
| 20.43 h (0.851 d) | |
| 0.0787±0.006 | |
| 10.0 | |
314 Rosalia is a largeMain beltasteroid. It was discovered byAuguste Charlois on 1 September 1891 inNice.[3]
Photometric observations of this asteroid collected during 2006 show arotation period of 20.43 ± 0.02 hours with a brightness variation of 0.21 ± 0.02magnitude.[4]
_mathilde.jpg) | This article about an asteroid native to theasteroid belt is astub. You can help Wikipedia byexpanding it. |
