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(532037) 2013 FY 27 (provisional designation 2013 FY 27) is a trans-Neptunian object and binary system that belongs to the scattered disc (like Eris). [8] Its discovery was announced on 31 March 2014. [1] It has an absolute magnitude (H) of 3.2.
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2015 TH 367 is a trans-Neptunian object approximately 220 kilometers (140 miles) in diameter. As of 2021 it is approximately 90 AU (13 billion km) from the Sun. [8] At the time of its announcement in March 2018, it was the third most distant observed natural object in the Solar System, after Eris and 2014 UZ 224.
Mike Brown's website lists it as a possible dwarf planet with a diameter of 328 kilometres (204 mi) based on an assumed albedo of 0.04 . [5] The albedo is expected to be low because the object has a blue (neutral) color. [5]
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The most massive known dwarf planet, Eris, belongs to this category. Detached objects (extended scattered disk) with generally highly elliptical, very large orbits of up to a few hundred AU and a perihelion too far from Neptune 's orbit for any significant interaction to occur.
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