Английская Википедия:2015 KG163

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Шаблон:Short description Шаблон:Use dmy dates

Шаблон:Infobox planet

Шаблон:Mp, also known as Шаблон:Mp, is a trans-Neptunian object from the outermost region of the Solar System, approximately Шаблон:Convert in diameter. It was first observed on 24 May 2015, by astronomers of the Outer Solar System Origins Survey using the Canada–France–Hawaii Telescope at Mauna Kea Observatories, Hawaii, United States.[1] With an observation arc of 2 years, it passed perihelion around August 2022[2]Шаблон:Efn at a velocity of 6.5 km/s with respect to the Sun.

It is one a small number of detached objects with perihelion distances of 30 AU or more, and semi-major axes of 250 AU or more.[3] Such objects can not reach such orbits without some perturbing object, which lead to the speculation of Planet Nine. Its argument of perihelion is similar to that of Шаблон:Mpl, but its semi-major axis is larger, such that its orbit may cross that of Plant Nine.

Файл:Planet nine-etnos now-close-new.png
Closeup of current position near perihelion, passing downward from the upper left of this view

Notes

Шаблон:Notelist

References

Шаблон:Reflist

External links

Шаблон:Trans-Neptunian objects Шаблон:Small Solar System bodies Шаблон:Authority control

  1. Ошибка цитирования Неверный тег <ref>; для сносок MPC-object не указан текст
  2. Ошибка цитирования Неверный тег <ref>; для сносок perihelion не указан текст
  3. Ошибка цитирования Неверный тег <ref>; для сносок MPC-query не указан текст