(60621) 2000 FE8 (provisional designation 2000 FE8) is a resonant and binary trans-Neptunian object, approximately 146 kilometers (91 miles) 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.

As a result, its position alternates between the Kuiper belt and the scattered disc.

[1] 2000 FE8 is part of a group of trans-Neptunian objects that orbit in a 2:5 resonance with Neptune.

The satellite was discovered by the Hubble Space Telescope seven years after 2000 FE8 itself was found.