2013 BL76

2013 BL76 is a trans-Neptunian object and centaur from the scattered disk and Inner Oort cloud approximately 30 kilometers in diameter. Using an epoch of February 2017, it is the minor planet with the 5th largest heliocentric semi-major axis in the Solar System (larger ones include 2014 FE72, 2012 DR30, and 2005 VX3). 2013 BL76 has a barycentric semi-major axis of ~964 AU, which is the third largest barycentric semi-major axis of any minor planet.

2013 BL76

2013 BL76 is a trans-Neptunian object and centaur from the scattered disk and Inner Oort cloud approximately 30 kilometers in diameter. Using an epoch of February 2017, it is the minor planet with the 5th largest heliocentric semi-major axis in the Solar System (larger ones include 2014 FE72, 2012 DR30, and 2005 VX3). 2013 BL76 has a barycentric semi-major axis of ~964 AU, which is the third largest barycentric semi-major axis of any minor planet.