2014 FC69
Orbit and classification. and based on an orbital uncertainty of 6–7 and an observation arc of only 682 days, " orbits the Sun at a distance of 40.1–104.2 AU once every 612 years and 10 months (223,847 days; semi-major axis of 72.15 AU). Its orbit has an eccentricity of 0.44 and an inclination of 30° with respect to the ecliptic. Based on the best-fit (albeit uncertain) orbital solution, ' is a scattered disc object, or "near-scattered" in the classification of the Deep Ecliptic Survey, that still interacts gravitationally with Neptune due to its relatively low perihelion  of 40.1 AU, contrary to the extended-scattered/detached objects and sednoids which never approach Neptune as close as ' does. Most distant objects from the Sun. " last came to perihelion around 1865, moving away from the Sun ever since and is currently about 85.6 AU from the Sun, which is further away than the dwarf planet . Other than long-period comets, it is the 10th-most-distant known larger body in the Solar System "(also see )". Physical characteristics. Based on a generic magnitude-to-diameter conversion from its magnitude of 4.6, is approximately in diameter, assuming an albedo of 0.9 . , no rotational lightcurve for this object has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown.