.png) A three-dimensional model of 695 Bella based on its light curve | |
| Discovery | |
|---|---|
| Discovered by | Joel Hastings Metcalf |
| Discovery site | Taunton, Massachusetts |
| Discovery date | 7 November 1909 |
| Designations | |
| (695) Bella | |
| 1909 JB | |
| Orbital characteristics[1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 102.48 yr (37432 d) |
| Aphelion | 2.9457 AU (440.67 Gm) |
| Perihelion | 2.1375 AU (319.77 Gm) |
| 2.5416 AU (380.22 Gm) | |
| Eccentricity | 0.15900 |
| 4.05yr (1480.0d) | |
| 183.825° | |
| 0° 14m 35.7s / day | |
| Inclination | 13.838° |
| 275.632° | |
| 79.589° | |
| Physical characteristics | |
| 24.09±0.75km | |
| 14.222 h (0.5926 d) | |
| 0.1450±0.009 | |
| 9.30 | |
695 Bella is aminor planet orbiting theSun.
Although this asteroid has dynamic properties that make it a candidate for theMaria family, the spectral properties of the object indicate it is most likely an interloper. Instead, it may have been spalled off from6 Hebe or its parent body. 695 Bella and 6 Hebe orbit on opposite sides of the 3:1Kirkwood gap, and the two have similarorbital elements.[2]
_mathilde.jpg) | This article about an asteroid native to theasteroid belt is astub. You can help Wikipedia byexpanding it. |
