| Discovery[1] | |
|---|---|
| Discovered by | CSS |
| Discovery site | Catalina Stn. |
| Discovery date | 23 January 2006 (first observed only) |
| Designations | |
| 2006 BZ8 | |
| centaur[2] · damocloid[3] unusual[4] · distant[1] | |
| Orbital characteristics[2] | |
| Epoch 1 July 2021 (JD 2459396.5) | |
| Uncertainty parameter2 | |
| Observation arc | 1.71 yr (623 days) |
| Aphelion | 17.310 AU |
| Perihelion | 1.890 AU |
| 9.600 AU | |
| Eccentricity | 0.8031 |
| 29.75 yr (10,865 d) | |
| 181.859° | |
| 0° 1m 59.282s / day | |
| Inclination | 165.302° |
| 183.444° | |
| 82.014° | |
| Earth MOID | 0.9708 AU |
| Jupiter MOID | 0.2159 AU |
| Saturn MOID | 1.6202 AU[1] |
| TJupiter | –1.024 |
| Physical characteristics | |
| 9.0–24.5 km[5] | |
| 5.960±0.003 h[5] | |
| 0.020+0.022 −0.010[5] | |
| 14.17±0.13 (linear)[a] 13.82±0.15 (H-G)[b] | |
2006 BZ8 is a dark centaur and damocloid on a retrograde and highly eccentric orbit from the outer region of the Solar System. It was first observed on 23 January 2006 by the Catalina Sky Survey at the Catalina Station near Tucson, Arizona, United States. It has not been observed since 2008.[1] This unusual object is estimated around 9–23.5 kilometers (5.6–15 miles) in diameter.[5]
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