Matches in DBpedia 2016-04 for { ?s ?p "(55637) 2002 UX25 is a possible dwarf planet that orbits the Sun in the Kuiper belt beyond Neptune. Its orbit takes roughly 280 years, and it has one known moon. This moon makes it much easier to calculate mass, and when the size is known, also a density. The low density of about 0.82 g/cm3 surprised astronomers.It is a trans-Neptunian object with an absolute magnitude of 4.0, making it highly likely to be a dwarf planet. The Spitzer Space Telescope results estimate it to be about 681 km in diameter. It was discovered on 30 October 2002, by the Spacewatch program. It is a mid-sized cubewano similar in size to 20000 Varuna."@en }
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- (55637)_2002_UX25 abstract "(55637) 2002 UX25 is a possible dwarf planet that orbits the Sun in the Kuiper belt beyond Neptune. Its orbit takes roughly 280 years, and it has one known moon. This moon makes it much easier to calculate mass, and when the size is known, also a density. The low density of about 0.82 g/cm3 surprised astronomers.It is a trans-Neptunian object with an absolute magnitude of 4.0, making it highly likely to be a dwarf planet. The Spitzer Space Telescope results estimate it to be about 681 km in diameter. It was discovered on 30 October 2002, by the Spacewatch program. It is a mid-sized cubewano similar in size to 20000 Varuna.".
- Q155539 abstract "(55637) 2002 UX25 is a possible dwarf planet that orbits the Sun in the Kuiper belt beyond Neptune. Its orbit takes roughly 280 years, and it has one known moon. This moon makes it much easier to calculate mass, and when the size is known, also a density. The low density of about 0.82 g/cm3 surprised astronomers.It is a trans-Neptunian object with an absolute magnitude of 4.0, making it highly likely to be a dwarf planet. The Spitzer Space Telescope results estimate it to be about 681 km in diameter. It was discovered on 30 October 2002, by the Spacewatch program. It is a mid-sized cubewano similar in size to 20000 Varuna.".