(523719) 2014 LM28, provisional designation 2014 LM28, is a trans-Neptunian object and centaur, approximately 46 kilometers (29 miles) in diameter. It was discovered on 16 May 2013, by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii, United States. The object's orbit is highly inclined and very eccentric, with a perihelion closer to the Sun than Uranus and at an aphelion 17 times farther from the Sun than Neptune.
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| - (523719) 2014 LM28 (en)
- (523719) 2014 LM28 (fr)
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| - (523719) 2014 LM28, provisional designation 2014 LM28, is a trans-Neptunian object and centaur, approximately 46 kilometers (29 miles) in diameter. It was discovered on 16 May 2013, by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii, United States. The object's orbit is highly inclined and very eccentric, with a perihelion closer to the Sun than Uranus and at an aphelion 17 times farther from the Sun than Neptune. (en)
- (523719) 2014 LM28 est un objet transneptunien ayant une orbite fortement inclinée et très excentrique l'emmenant, au périhélie, plus près du Soleil qu'Uranus et, à l'aphélie, 17 fois plus loin du Soleil que Neptune. (fr)
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| - (523719) 2014 LM28, provisional designation 2014 LM28, is a trans-Neptunian object and centaur, approximately 46 kilometers (29 miles) in diameter. It was discovered on 16 May 2013, by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii, United States. The object's orbit is highly inclined and very eccentric, with a perihelion closer to the Sun than Uranus and at an aphelion 17 times farther from the Sun than Neptune. (en)
- (523719) 2014 LM28 est un objet transneptunien ayant une orbite fortement inclinée et très excentrique l'emmenant, au périhélie, plus près du Soleil qu'Uranus et, à l'aphélie, 17 fois plus loin du Soleil que Neptune. (fr)
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| - 27 April 2019 (JD2458600.5)
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