541132 Leleākūhonua
Discovery[1][2] | |
---|---|
Discovered by | D. J. Tholen C. Trujillo S. S. Sheppard |
Discovery site | Mauna Kea Obs. |
Discovery date | 13 October 2015 |
Designations | |
(541132) Leleākūhonua | |
Pronunciation | English: /ˌlɛleɪɑːˌkuːhoʊˈnuːə/ Hawaiian: [lelejaːkuːhoˈnuwə] |
Perihelion | 65.16±0.21 AU |
1085±111 AU | |
Eccentricity | 0.93997±0.00636 |
35760±5510 yr | |
359.418° | |
0° 0m 0.099s / day | |
Inclination | 11.654° |
300.780° | |
≈ 11 June 2078[9] ±4.5 months | |
117.778° | |
Physical characteristics | |
Mean radius | 110+14 −10 km[10] |
0.21+0.03 −0.05[10] | |
24.5[11] | |
5.50±0.13[1][6] | |
541132 Leleākūhonua (/ˌlɛleɪɑːˌkuːhoʊˈnuːə/) (provisional designation 2015 TG387) is an extreme trans-Neptunian object and sednoid in the outermost part of the Solar System. It was first observed on 13 October 2015, by astronomers at the Mauna Kea Observatories, Hawaii. Based on its discovery date near Halloween and the letters in its provisional designation 2015 TG387, the object was informally nicknamed "The Goblin" by its discoverers[3] and later named Leleākūhonua, comparing its orbit to the flight of the Pacific golden plover. It was the third sednoid discovered, after Sedna and 2012 VP113, and measures around 220 kilometers (140 miles) in diameter.[10]
Discovery
Leleākūhonua was first observed on 13 October 2015 at the
Orbit and classification
Leleākūhonua orbits the Sun at a distance varying from 65 to about 2000 AU once roughly every 32,000 years (
Implications of orbit
Along with the similar orbits of other distant trans-Neptunian objects, the orbit of Leleākūhonua suggests, but does not prove, the existence of a hypothetical Planet Nine in the outer Solar System.[7][13]
As of 2019[update], the object is inbound 78 AU from the Sun;[11] about two-and-a-half times farther out than Pluto's current location.[4] It will come to perihelion (closest approach to the Sun) in 2078.[6] As with Sedna, it would not have been found had it not been on the inner leg of its long orbit. This suggests that there may be many similar objects, most too distant to be detected by contemporary technological methods. Following the discovery of Leleākūhonua, Sheppard et al. concluded that it implies a population of about 2 million inner Oort cloud objects larger than 40 km (25 mi), with a combined total mass of 1×1022 kg, about the mass of Pluto (a fraction the mass of Earth's moon but several times the mass of the asteroid belt).[7]
Numbering and naming
This
Physical characteristics
The size of Leleākūhonua depends on the assumed
Visualizations
-
Simulated view of Solar System as seen from Leleākūhonua, showing the orbits of major planets and positions of other extremeTrans-Neptunian objects.
-
View of Leleākūhonua from Earth, showing retrograde loops every year, with current position near γ Pegasi
See also
- List of Solar System objects most distant from the Sun
- List of Solar System objects by greatest aphelion
- V774104
References
- ^ a b c d e "(541132) Leleakuhonua = 2015 TG387". Minor Planet Center. Retrieved 21 October 2019.
- ^ Minor Planet Electronic Circular. 1 October 2018. Retrieved 13 December 2018.
- ^ a b Guarino, Ben (2 October 2018). "New dwarf planet spotted at the very fringe of our solar system". The Washington Post. Retrieved 3 October 2018.
- ^ a b Chang, Kenneth (2 October 2018). "A Goblin World That Points Toward Hidden Planet Nine in the Solar System". The New York Times. Retrieved 2 October 2018.
- ^ Trujillo, C.; Sheppard, S.S.; Tholen, D.J.; Kaib, N. (24 October 2018). A New Inner Oort Cloud Object. 50th annual meeting of the AAS Division of Planetary Sciences. abstract 311.09. Retrieved 19 October 2018.
- ^ a b c d e f "JPL Small-Body Database Browser: (2015 TG387)" (2018-10-17 last obs.). Jet Propulsion Laboratory. Retrieved 13 December 2018.
- ^ S2CID 119071596.
- ^ Johnston, Wm. Robert (13 July 2019). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 21 October 2019.
- 3-sigma.)
- ^ S2CID 219039999. 230.
- ^ a b c "2015 TG387 – Ephemerides". AstDyS-2, Asteroids – Dynamic Site, Department of Mathematics, University of Pisa, Italy. Retrieved 12 December 2018.
- ^ Mortillaro, Nicole (2 October 2018). "Discovery of new object supports theory of 'super-Earth' at edge of solar system". CBC News. Retrieved 2 October 2018.
- S2CID 125361517. Retrieved 2 October 2018.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 21 October 2019.
- ^ "M.P.C. 123453" (PDF). Minor Planet Center. International Astronomical Union. 3 June 2020. Retrieved 3 June 2020.
- creation chant, the Kumulipo. However, the name/phrase does not actually occur there. Like other recently coined Hawaiian names for astronomical objects, it is a descriptive phrase created by students in a Hawaiian language-revival class.
- ^ Meghan Bartels, 'The Goblin' dwarf planet and an ancient quasar receive Hawaiian names Space.com, July 01, 2020
- ^ "Hawaiian name given to dwarf planet orbiting Sun". UH News. University of Hawaiʻi Hilo. 16 November 2020. Retrieved 28 November 2020.
- ^ a b Drake, Nadia (2 October 2018). "New object beyond Pluto hints at mysterious 'Planet X'". National Geographic. Archived from the original on 3 October 2018. Retrieved 11 October 2018.
External links
- List Of Centaurs and Scattered-Disk Objects, Minor Planet Center
- 541132 Leleākūhonua at AstDyS-2, Asteroids—Dynamic Site
- 541132 Leleākūhonua at the JPL Small-Body Database