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695 Bella
| Column 1 |
|---|
| A three-dimensional model of 695 Bella based on its light curve |
| Joel Hastings Metcalf |
| Taunton, Massachusetts |
| 7 November 1909 |
| (695) Bella |
| 1909 JB |
| Epoch 31 July 2016 (JD 2457600.5) |
| Uncertainty parameter 0 |
| 102.48 yr (37432 d) |
| 2.9457 AU (440.67 Gm) |
| 2.1375 AU (319.77 Gm) |
| 2.5416 AU (380.22 Gm) |
| 0.15900 |
| 4.05 yr (1480.0 d) |
| 183.825° |
| 0° 14m 35.7s / day |
| 13.838° |
| 275.632° |
| 79.589° |
| 24.09±0.75 km |
| 14.222 h (0.5926 d) |
| 0.1450±0.009 |
| 9.30 |
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695 Bella is a minor planet orbiting the Sun.
Although this asteroid has dynamic properties that make it a candidate for the Maria family, the spectral properties of the object indicate it is most likely an interloper. Instead, it may have been spalled off from 6 Hebe or its parent body. 695 Bella and 6 Hebe orbit on opposite sides of the 3:1 Kirkwood gap, and the two have similar orbital elements.
- 695 Bella at AstDyS-2, Asteroids—Dynamic Site
- Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
- 695 Bella at the JPL Small-Body Database
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