is a trans-Neptunian object. Considered a detached object, it orbits the Sun in a highly eccentric orbit every 3,305 years at an average distance of 222 astronomical units (AU).
Description Mike Brown's website lists it with a diameter of based on an assumed albedo of 0.04. The albedo is expected to be low because the object has a blue (neutral) color. However, if the albedo is higher, the object could easily be half that size.
and Sedna differ from scattered-disc objects in that they are not within the gravitational influence of the planet Neptune even at their perihelion distances (closest approaches to the Sun). It is something of a mystery as to how these objects came to be in their current, far-flung orbits. Several hypotheses have been put forward: They were pulled from their original positions by a passing star. They were pulled from their original positions by a very distant, and as-yet-undiscovered (albeit unlikely), giant planet. They were pulled from their original positions by an undiscovered companion star orbiting the Sun such as Nemesis. They were captured from another planetary system during a close encounter early in the Sun's history. According to Kenyon and Bromley, there is a 15% probability that a star like the Sun had an early close encounter and a 1% probability that outer planetary exchanges would have happened. is estimated to be 2–3 times more likely to be a captured planetary object than Sedna.
is the first object discovered in the Solar System to have a semi-major axis exceeding 150 AU, a perihelion beyond Neptune, and an argument of perihelion of . It may be influenced by Planet Nine.
See also Planets beyond Neptune List of Solar System objects by greatest aphelion
References
External links Orbit Determination of Spacecraft escaping the Solar System (Heavens-Above) World Book: Worlds Beyond Pluto