Astronomy:2007 BP102

From HandWiki
2007 BP102
Discovery[1][2]
Discovery siteMauna Kea Obs.
Discovery date24 January 2007
Designations
2007 BP102
Minor planet categorycentaur[3][4] · distant[1]
damocloid
Orbital characteristics[3]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 4
Observation arc9.30 yr (3,396 days)
|{{{apsis}}}|helion}}30.228 AU
|{{{apsis}}}|helion}}17.744 AU
23.986 AU
Eccentricity0.2603
Orbital period117.47 yr (42,907 days)
Mean anomaly23.523°
Mean motion0° 0m 30.24s / day
Inclination64.678°
Longitude of ascending node45.299°
125.63°
TJupiter1.990
Physical characteristics
Dimensions34 km (calculated)[4]
Geometric albedo0.09 (assumed)[4]
Absolute magnitude (H)10.6[3]


2007 BP102 is a high inclination centaur and damocloid from the outer regions of the Solar System, approximately 34 kilometers in diameter. It was first observed by astronomers at the Mauna Kea Observatories on 24 January 2007.[1][2][4]

With a Tisserand's parameter of 1.99, may be considered a member of the damocloids, a dynamical group of minor planets which have comet-like orbits without showing a cometary coma or tail. It orbits the Sun at a distance of 17.7–30.2 AU once every 117 years and 6 months (42,907 days). Its orbit has an eccentricity of 0.26 and an inclination of 65° with respect to the ecliptic.[3]

As of July 2017, it is one of 7 known objects with inclination (i) > 60° and perihelion (q) > 15 AU, along with the first discovered 2008 KV42.[5]

References

External links