.png) A three-dimensional model of 819 Barnardiana based on its light curve | |
| Discovery | |
|---|---|
| Discovered by | Max Wolf |
| Discovery site | Heidelberg Observatory |
| Discovery date | 3 March 1916 |
| Designations | |
| (819) Barnardiana | |
| 1916 ZA | |
| Orbital characteristics[1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 111.49 yr (40722 d) |
| Aphelion | 2.5097 AU (375.45 Gm) |
| Perihelion | 1.8847 AU (281.95 Gm) |
| 2.1972 AU (328.70 Gm) | |
| Eccentricity | 0.14223 |
| 3.26yr (1189.6d) | |
| 183.04° | |
| 0° 18m 9.432s / day | |
| Inclination | 4.8983° |
| 333.162° | |
| 306.373° | |
| Physical characteristics | |
| 66.70 h (2.779 d) | |
| 12.0 | |
819 Barnardiana is aminor planet orbiting theSun, discovered on March 3, 1916, by the German astronomerMax Wolf inHeidelberg.
_mathilde.jpg) | This article about an asteroid native to theasteroid belt is astub. You can help Wikipedia byexpanding it. |
