2007 BP102

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]

2007 BP102
Discovery [1][2]
Discovery siteMauna Kea Obs.
Discovery date24 January 2007
Designations
2007 BP102
centaur [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)
Aphelion30.228 AU
Perihelion17.744 AU
23.986 AU
Eccentricity0.2603
117.47 yr (42,907 days)
23.523°
0° 0m 30.24s / day
Inclination64.678°
45.299°
125.63°
TJupiter1.990
Physical characteristics
Dimensions34 km (calculated)[4]
0.09 (assumed)[4]
10.6[3]

    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
    1. "2007 BP102". Minor Planet Center. Retrieved 14 October 2017.
    2. "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. Retrieved 14 October 2017.
    3. "JPL Small-Body Database Browser: (2007 BP102)" (2016-05-08 last obs.). Jet Propulsion Laboratory. Retrieved 14 October 2017.
    4. "List of known Trans-Neptunian Objects". Johnston's Archive. Retrieved 14 October 2017.
    5. http://minorplanetcenter.net/db_search/show_by_properties?perihelion_distance_min=15&inclination_min=60


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