Matches in DBpedia 2014 for { ?s ?p 2013 FY27, also written 2013 FY27, is a trans-Neptunian object that belongs to the scattered disc (like Eris). Its discovery was announced on 31 March 2014. It has an absolute magnitude (H) of 3.0, which makes it very likely to be a dwarf planet. Assuming an albedo of 0.15, it would be approximately 850 km in diameter. It is the ninth-intrinsically-brightest known trans-Neptunian object.2013 FY27 will come to perihelion around 2198, at a distance of about 36 AU. It is currently near aphelion, 80 AU from the Sun, and as a result has an apparent magnitude of 22. Its orbit has a significant inclination of 33°.First observed on 17 March 2013, it has an observation arc of about 1 year. It came to opposition in early March 2014. 2012 VP113 was announced before 2013 FY27, and 2013 FZ27 afterwards.. }
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- 2013_FY27 abstract "2013 FY27, also written 2013 FY27, is a trans-Neptunian object that belongs to the scattered disc (like Eris). Its discovery was announced on 31 March 2014. It has an absolute magnitude (H) of 3.0, which makes it very likely to be a dwarf planet. Assuming an albedo of 0.15, it would be approximately 850 km in diameter. It is the ninth-intrinsically-brightest known trans-Neptunian object.2013 FY27 will come to perihelion around 2198, at a distance of about 36 AU. It is currently near aphelion, 80 AU from the Sun, and as a result has an apparent magnitude of 22. Its orbit has a significant inclination of 33°.First observed on 17 March 2013, it has an observation arc of about 1 year. It came to opposition in early March 2014. 2012 VP113 was announced before 2013 FY27, and 2013 FZ27 afterwards.".