2013 BL76

2013 BL76 is a minor planet (centaur) from the scattered disk/Inner Oort cloud. Using an epoch of December 2014, it is the minor planet with the third-largest heliocentric semi-major axis in the Solar system (after 2005 VX3 and 2012 DR30). 2013 BL76 has a barycentric semi-major axis of ~964 AU, which is also the third largest barycentric semi-major axis of any minor planet. It will not be 50 AU from the Sun until 2045. After leaving the planetary region of the Solar System, 2013 BL76 will have a barycentric aphelion of 1920 AU with an orbital period of 29900 years.

2013 BL76

2013 BL76 is a minor planet (centaur) from the scattered disk/Inner Oort cloud. Using an epoch of December 2014, it is the minor planet with the third-largest heliocentric semi-major axis in the Solar system (after 2005 VX3 and 2012 DR30). 2013 BL76 has a barycentric semi-major axis of ~964 AU, which is also the third largest barycentric semi-major axis of any minor planet. It will not be 50 AU from the Sun until 2045. After leaving the planetary region of the Solar System, 2013 BL76 will have a barycentric aphelion of 1920 AU with an orbital period of 29900 years.