2015 ER61 is a comet, centaur, inner Oort cloud object, Amor near-Earth asteroid, and possibly a damocloid. It has the fourth-largest aphelion of any known minor planet in the Solar System, after 2005 VX3, 2012 DR30, and 2013 BL76. It additionally has the most eccentric orbit of any known minor planet, with its distance from the Sun varying by about 99.9% during the course of its orbit, followed by 2005 VX3 with an eccentricity of 0.9973. On January 30, 2016, it was classified as a comet when it was 5.7 AU from the Sun.
It comes close to Jupiter, and a close approach in the past threw it on the distant orbit it is on now. It also has a small MOID to Mars of less 0.01 AU
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