2015 TH367

) on the far left, alongside the twin Keck telescopes and NASA's Infrared Telescope Facility was first observed by Scott Sheppard, Chad Trujillo, and David Tholen on 13 October 2015 using the Subaru Telescope, a large reflecting telescope at the Mauna Kea Observatories on the summit of Mauna Kea with a primary mirror in diameter. In 2015 it was only observed for 26 days, which is a very short observation arc for a trans-Neptunian object as objects far from the Sun move very slowly across the sky. It is calculated that it will remain in the constellation of Aries from 1994 until 2077. It was announced on 13 March 2018 alongside several other trans-Neptunian objects with a current heliocentric distance greater than 50 AU. The trans-Neptunian objects 541132 Leleākūhonua and were also discovered by this team on 13 October 2015. == Orbit ==

The orbit of is poorly constrained, as it has only been observed 10 times over 2 years due to how dim it is. At a visual apparent magnitude of 26.2, it is about 75 million times fainter than what can be seen with the naked eye, and it is one of the dimmest trans-Neptunian objects ever observed, only being able to be seen by the largest modern telescopes. The JPL Small-Body Database estimates that it came to perihelion (closest approach to the Sun) in the year 1888 and will reach aphelion (farthest distance from the Sun) at 128 AU in 2238. Project Pluto estimates perihelion was in 1886. == Distance from the Sun ==

The precise distance of still remains unknown due to its poorly understood orbit and the fact it has not been observed since 2016. It is currently outbound roughly from the Sun, and will require further observations to better refine the orbit. At magnitude 26, it is only observable with a small number of telescopes that are capable of following it up and refining its orbit. It is expected to come to opposition in the constellation of Aries around 3 November 2021 when it should have a solar elongation of roughly 175°. , there are only five known minor planets further from the Sun than under its nominal orbit: Eris (95.9 AU), (97.2 AU), (99.0 AU), (123.5 AU), and (~132 AU). Observed Solar System objects that periodically become more distant than 89 AU from the Sun include (which is much larger in size), , , , and . There are 804 known objects that have aphelia more than 89 AU from the Sun as of March 2018. This distance is about double the outer limit of the torus-shaped Kuiper belt that lies outside Neptune's orbit. Far beyond this region is the vast spherical Oort cloud enshrouding the Solar System, whose presence was deduced from the orbits of long-period comets. Study of the population of Solar System objects that are significantly more distant than will likely require new instruments. The proposed Whipple spacecraft mission is designed to determine the outer limit of the Kuiper belt and directly detect Oort cloud objects out to 10,000 AU. Such objects are too small to detect with current telescopes except during stellar occultations. The proposal involves use of a wide field of view and rapid recording cadence to allow detection of many such events. ==Confusion with 541132 Leleākūhonua ==

In November 2015, a reporter for Nature attended a meeting of the American Astronomical Society’s Division for Planetary Sciences where the Trujillo team announced the discovery of the previous month. Nature then issued a press release on the discovery of V774104, the internal designation of , as the most distant Solar System object ever observed, at around 103 AU. This press release received considerable media attention, but contained two errors, and because the Trujillo team had not themselves issued a press release or even submitted the discovery to the Minor Planet Center, there was no other public information. First, the object was not but another discovery from the same night's observation, the sednoid , now known as 541132 Leleākūhonua, that had also been announced at the meeting. Their internal designations had been conflated in the reporting. Second, the distance was significantly closer than 103 AU (and Leleākūhonua closer still), though it is not clear if this was misreporting or an inaccurate first estimate based on an extremely short observation arc. == Notes ==