About: (523727) 2014 NW65     Goto   Sponge   NotDistinct   Permalink

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(523727) 2014 NW65, provisional designation: 2014 NW65, is a large centaur from the outer Solar System, approximately 220 kilometers (140 miles) in diameter. It was discovered on 14 July 2010 by astronomers with the Pan-STARRS-1 survey at Haleakala Observatory, Hawaii, in the United States. According to American astronomer Michael Brown, it is "possibly" a dwarf planet. The minor planet was numbered in 2018 and has not been named.

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  • (523727) 2014 NW65 (de)
  • (523727) 2014 NW65 (en)
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  • (523727) 2014 NW65, provisional designation: 2014 NW65, is a large centaur from the outer Solar System, approximately 220 kilometers (140 miles) in diameter. It was discovered on 14 July 2010 by astronomers with the Pan-STARRS-1 survey at Haleakala Observatory, Hawaii, in the United States. According to American astronomer Michael Brown, it is "possibly" a dwarf planet. The minor planet was numbered in 2018 and has not been named. (en)
  • (523727) 2014 NW65 ist ein Planetoid, der am 2. Juli 2014 am Pan-STARRS 1 entdeckt wurde und zur Gruppe der Zentauren gehört. Der Asteroid läuft auf einer mäßig exzentrischen Bahn in 111 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,52, wobei diese 20,46° gegen die Ekliptik geneigt ist. Wenn 2014 NW65 dasselbe Rückstrahlvermögen wie der mit Stand Oktober 2018 größte bestätigte Zentaur Chariklo hat, ist er sogar geringfügig größer als letzterer. (de)
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  • #C7FF8F (en)
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  • Pan-STARRS 1 (en)
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