(provisional designation ) is a resonant and binary trans-Neptunian object, approximately in diameter, located in the outermost region of the Solar System. It was discovered on 27 March 2000, by astronomers John Kavelaars, Brett Gladman, Jean-Marc Petit and Matthew Holman at Mauna Kea Observatory on Hawaii. This distant object resides in an eccentric orbit and is locked in a 2:5 orbital resonance with Neptune. It is known to have a 111-kilometer sized companion, which was discovered in January 2007.
has an extremely eccentric orbit which crosses the paths of many other trans-Neptunian objects, including almost all of the dwarf planets and dwarf planet candidates. As a result, its position alternates between the Kuiper belt and the scattered disc.
is part of a group of trans-Neptunian objects that orbit in a 2:5 resonance with Neptune. That means that for every five orbits that Neptune completes, makes only two. Several other objects are in the same orbital resonance, the largest of which is .
Like many objects of the Kuiper belt and scattered disc, has a satellite. The satellite was discovered by the Hubble Space Telescope seven years after itself was found. The moon orbits at 1180 kilometres away from , completing one orbit in approximately 7 days. It is thought to be 115 km in diameter, just 75.7% the diameter of 2000 FE<sub>8</sub> itself.
This minor planet was numbered by the Minor Planet Center on 14 June 2003. , it has not been named.