It was first observed on 31 March 2012 by Andrea Boattini, observing for the Mt. Lemmon Survey.[5][6]
Its orbit is characterized by low eccentricity (0.088), low inclination (4.97º) and a semi-major axis of 0.9895 AU.[6] It is an Atenasteroid but also an Earth crosser. As of 21 April 2012 its orbit is based on 35 observations spanning a data-arc of 21 days. This short observation arc results in an orbit uncertainty of 7. It has not been seen since and is unlikely to be seen again for several decades. It will remain both very dim (around apparent magnitude 27), and close in the sky to the Sun (solar elongation of less than 90 degrees), making it impossible to observe with current ground based telescopes till the 2060s. A number of times during the decade it will again be visible in the night sky and at times be brighter than apparent magnitude 21, as when it was first observed.[2]
Kozai resonator and future orbital evolution
2012 FC71 is locked in a Kozai resonance and as such it has a very slow orbital evolution and it will remain relatively unperturbed for hundreds of thousands of years.[4] It had a close encounter with the Earth on 18 April 2012 at 0.076 AU when it was discovered and another on 17 May 2013 at 0.0581 AU, which was not observed.
Origin
It may have been originated within the Venus-Earth-Mars region or in the main asteroid belt like other Near-Earth Objects, then transitioned to an Amor-class asteroid before entering Earth's co-orbital region.[4]
