471325 Taowu
Trans-Neptunian object on a retrograde polar orbit
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471325 Taowu (provisional designation 2011 KT19, formerly nicknamed Niku (/ËniËkuË/)) is a trans-Neptunian object whose orbit is tilted 110° with respect to the ecliptic. Thus, it has a nearly polar retrograde orbit around the Sun from the reference point of Earth's orbital plane.[5]
Taowu imaged by the CanadaâFranceâHawaii Telescope on 22 May 2014 | |
| Discovery[1] | |
|---|---|
| Discovered by | Mount Lemmon Survey |
| Discovery site | Mount Lemmon Obs. |
| Discovery date | 31 May 2011 |
| Designations | |
| (471325) Taowu | |
| Pronunciation | /ËtaÊËwuË/ |
Named after | Taowu |
| |
| TNO[2] · centaur[3][4] distant[1] | |
| Orbital characteristics | |
| Epoch 17 October 2024 (JD 2460600.5) | |
| Uncertainty parameter 2 | |
| Observation arc | 14.05 yr (5,131 d) |
| Earliest precovery date | 10 May 2010 |
| Aphelion | 47.588 AU |
| Perihelion | 23.839 AU |
| 35.713 AU | |
| Eccentricity | 0.3325 |
| 213.43 yr (77,955 d) | |
| 42.884° | |
| 0° 0m 16.625s / day | |
| Inclination | 110.311° |
| 243.903° | |
| â 15 May 1999 ±0.13 days[2] | |
| 322.913° | |
| Physical characteristics | |
| 177 km (assumed albedo 0.058)[4] | |
| 22[1] | |
| 7.45[2][1] | |
Discovery
Taowu was discovered on 31 May 2011 by the Mount Lemmon Survey in Arizona. It was announced by the Minor Planet Center on 2 June 2011, after other telescopes confirmed the object with additional observations.[6] The object was given the minor planet provisional designation 2011 KT19, which reflects its discovery date.[6] Initial calculations of Taowu's orbit using these few observations suggested it was a centaur on a prograde elliptical orbit (semi-major axis 28 AU, eccentricity 0.41, inclination 38°).[6][5]:â2â However, Taowu was only observed for up to 8 days before being lost, due to large uncertainties in its orbit.[5]:â2â
In 2016, a team of astronomers led by Ying-Tung Chen performed a search for outer Solar System objects in observations by the Pan-STARRS 1 survey.[7][8][5]:â1â They rediscovered Taowu in Pan-STARRS observations from 2013â2016 and recognized it had an unusual retrograde polar orbit. Chen's team made follow-up observations at Lulin Observatory in Taiwan and found additional observations of the object in archival images from the Dark Energy Survey and CanadaâFranceâHawaii Telescope.[8][5]:â2â After Chen's team submitted their observations of Taowu to the Minor Planet Center, it was recognized that Taowu had been previously observed by the Mount Lemmon Survey in 2011.[5]:â2â Taowu received its permanent minor planet catalog number 471325 on 18 August 2016 and the Minor Planet Center declared Mount Lemmon Survey as the object's official discoverer.[9]:â512â
Name
The object is named after Taowu (檮æ; Táowù), one of the Four Perils in Chinese mythology. The name follows the International Astronomical Union's naming conventions for centaurs on Neptune-crossing orbits (perihelion <30 AU), which are named after mythological chimeras.[10]:â8â The name was announced by the International Astronomical Union on 3 February 2025.[11]
The object had previously been nicknamed Niku (é骨; nìgÇ) by Ying-Tung Chen, who was involved with rediscovering the object and studying its orbit in 2016. The nickname is a Mandarin adjective meaning "rebellious", in reference to the object's unusual retrograde orbit.[8][7]
Orbit
Taowu is in a 7:9 resonance with Neptune. Currently it is the only object with a nearly polar orbit that is in resonance with a planet.[12] Notably, it is part of a group of objects that orbit the Sun in a highly inclined orbit; the reasons for this unusual orbit are unknown as of August 2016.[5] Taowu's orbital characteristics have been compared to those of 2008 KV42 (nicknamed "Drac"). The orbits of Taowu, 2008 KV42, 2002 XU93, 2010 WG9, 2007 BP102, and 2011 MM4 appear to occupy a common plane, with three in prograde and three in retrograde orbits. The probability of this alignment occurring by chance is 0.016%. These orbits should leave a common plane in a few million years because the precession of prograde and retrograde orbits are in opposite directions. Simulations including the hypothetical Planet Nine did not maintain a common orbital plane and the plane does not coincide with the plane of the predicted high-inclination large semi-major axis objects of that model. Other simulations with a few Earth-mass dwarf planet on a high-inclination orbit also failed to reproduce the alignment.[5]
| The orbit of Taowu (white) in relation to Pluto and the planets of the Solar System |
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| The orbit of Taowu (purple), is shown with another steep retrograde TNO, 2008 KV42 (yellow), and the other planets. Pluto's orbit is in red. |
Physical characteristics
The diameter of Taowu has not been measured, but it can be estimated from its brightness (absolute magnitude) using a range of plausible values for its surface reflectivity (geometric albedo). If Taowu reflects between 5% and 25% of visible light, then its diameter is between 100 and 200 km (62 and 124 mi).[13] A 2023 study has attempted to check if Taowu exhibits brightness variability due to its rotation, but results have not yet been published.[14]
