About: 2006 BZ8     Goto   Sponge   NotDistinct   Permalink

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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. This unusual object is estimated around 9–23.5 kilometers (5.6–15 miles) in diameter.

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  • 2006 BZ8 (en)
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  • 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. This unusual object is estimated around 9–23.5 kilometers (5.6–15 miles) in diameter. (en)
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  • (en)
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aphelion
arg peri
asc node
background
  • #C7FF8F (en)
discovered
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eccentricity
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jupiter moid
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  • / day (en)
minorplanet
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  • centaurdamocloid (en)
  • unusualdistant (en)
observation arc
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saturn moid
semimajor
tisserand
  • –1.024 (en)
uncertainty
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  • 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. This unusual object is estimated around 9–23.5 kilometers (5.6–15 miles) in diameter. (en)
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apoapsis (km)
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page length (characters) of wiki page
apoapsis (μ)
discovery date
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  • 1 July 2021 (JD2459396.5)
orbital period (s)
periapsis (μ)
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