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2006 BZ8

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2006 BZ8
Discovery[1]
Discovered byCSS
Discovery siteCatalina Stn.
Discovery date23 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 parameter 2
Observation arc1.71 yr (623 days)
Aphelion17.310 AU
Perihelion1.890 AU
9.600 AU
Eccentricity0.8031
29.75 yr (10,865 d)
181.859°
0° 1m 59.282s / day
Inclination165.302°
183.444°
82.014°
Earth MOID0.9708 AU
Jupiter MOID0.2159 AU
Saturn MOID1.6202 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]

See also

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Notes

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  1. ^ Linear fit of CSS V-band photometry using a phase slope of β = 0.054±0.008 mag per degree of phase angle.[5]
  2. ^ Two-parameter H-G modeling of V-band CSS photometry takes the opposition effect into account, yielding an absolute magnitude of H = 13.82±0.15 and a slope parameter of G = −0.12±0.10.[5]

References

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  1. ^ a b c d "2006 BZ8". Minor Planet Center. International Astronomical Union. Retrieved 8 August 2021.
  2. ^ a b "JPL Small-Body Database Browser: (2006 BZ8)" (2007-10-08 last obs.). Jet Propulsion Laboratory. Retrieved 8 August 2021.
  3. ^ Johnston, Wm. Robert (18 August 2020). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 8 August 2021.
  4. ^ "List Of Other Unusual Objects". Minor Planet Center. International Astronomical Union. 8 August 2021. Retrieved 8 August 2021.
  5. ^ a b c d e f Hergenrother, Carl W. (January 2018). "Photometry of Damocloid Asteroid 2006 BZ8". The Minor Planet Bulletin. 45 (1): 64–65. Bibcode:2018MPBu...45...64H. Retrieved 8 August 2021.
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