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2010 FX86
Classical Kuiper belt object From Wikipedia, the free encyclopedia
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2010 FX86 is a relatively bright trans-Neptunian object[2] with an absolute magnitude of about 4.65.[2][3][6]
It was first discovered on 17 March 2010, at Las Campanas Observatory in Chile, by S. S. Sheppard, A. Udalski and I. Soszynski. No earlier precovery images for it have been found. It is estimated to be about 520 kilometres (320 mi) in diameter,[6] with a rotation period of approximately 15.80 hours,[2] but as of yet no detailed photometry has been taken to properly determine colour or albedo, or to better confirm its rotational lightcurve.
2010 FX86 has not yet been imaged by high-resolution telescopes, so it has no known moons. The Hubble Space Telescope is planned to image it in 2026, which should determine if it has significantly sized moons.[7]
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