Quasi-satellites orbit the Sun from the same distance as a planet, rather than the planet itself. Their orbits are unstable, and will fall into other resonances or be kicked into other orbits over thousands of years.[3] Quasi-satellites of Earth include 2010 SO16, (164207) 2004 GU9,[23] (277810) 2006 FV35,[24] 2002 AA29,[25] 2014 OL339, 2013 LX28, 2016 HO3 and 3753 Cruithne. Cruithne, discovered in 1986, orbits the Sun in an elliptical orbit but appears to have a horseshoe orbit when viewed from Earth.[3][26] Some went as far to nickname Cruithne "Earth's second moon".[26]