Discovery [1] | |
---|---|
Discovered by | Pan-STARRS 1 |
Discovery site | Haleakala Obs. |
Discovery date | 16 May 2013 |
Designations | |
(523719) 2014 LM28 | |
TNO
[2] ·
distant
[1] centaur [3] | |
Orbital characteristics [2] | |
Epoch 27 April 2019 ( JD 2458600.5) | |
Uncertainty parameter 1 | |
Observation arc | 4.04 yr (1,474 d) |
Aphelion | 538.89 AU |
Perihelion | 16.771 AU |
277.83 AU | |
Eccentricity | 0.9396 |
4631.05 yr (1,691,491 d) | |
0.1133 ° | |
0° 0m 0.72s / day | |
Inclination | 84.739° |
246.18° | |
38.364° | |
Physical characteristics | |
46 km [3] | |
9.9 [1] [2] | |
(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. [1] 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.
2014 LM28 orbits the Sun at a distance of 16.8–538.9 AU once every 4631 years and 1 month (1,691,491 days; semi-major axis of 277.83 AU). Its orbit has an eccentricity of 0.94 and an inclination of 85 ° with respect to the ecliptic. [2] The body's observation arc begins with its official discovery observation by Pan-STARRS at Haleakala Observatory in May 2013. [1]
This minor planet was numbered by the Minor Planet Center on 25 September 2018 ( M.P.C. 111779). [4] As of 2018, it has not been named. [1]
2014 LM28 has a highly inclined orbit typical of scattered objects and orbits nearly perpendicular to the ecliptic.
Discovery [1] | |
---|---|
Discovered by | Pan-STARRS 1 |
Discovery site | Haleakala Obs. |
Discovery date | 16 May 2013 |
Designations | |
(523719) 2014 LM28 | |
TNO
[2] ·
distant
[1] centaur [3] | |
Orbital characteristics [2] | |
Epoch 27 April 2019 ( JD 2458600.5) | |
Uncertainty parameter 1 | |
Observation arc | 4.04 yr (1,474 d) |
Aphelion | 538.89 AU |
Perihelion | 16.771 AU |
277.83 AU | |
Eccentricity | 0.9396 |
4631.05 yr (1,691,491 d) | |
0.1133 ° | |
0° 0m 0.72s / day | |
Inclination | 84.739° |
246.18° | |
38.364° | |
Physical characteristics | |
46 km [3] | |
9.9 [1] [2] | |
(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. [1] 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.
2014 LM28 orbits the Sun at a distance of 16.8–538.9 AU once every 4631 years and 1 month (1,691,491 days; semi-major axis of 277.83 AU). Its orbit has an eccentricity of 0.94 and an inclination of 85 ° with respect to the ecliptic. [2] The body's observation arc begins with its official discovery observation by Pan-STARRS at Haleakala Observatory in May 2013. [1]
This minor planet was numbered by the Minor Planet Center on 25 September 2018 ( M.P.C. 111779). [4] As of 2018, it has not been named. [1]
2014 LM28 has a highly inclined orbit typical of scattered objects and orbits nearly perpendicular to the ecliptic.