Английская Википедия:(119979) 2002 WC19

Материал из Онлайн справочника
Версия от 23:19, 17 декабря 2023; EducationBot (обсуждение | вклад) (Новая страница: «{{Английская Википедия/Панель перехода}} {{DISPLAYTITLE:{{mp|(119979) 2002 WC|19}}}} {{Infobox planet | minorplanet = yes | background = #C2E0FF | name = {{mp|(119979) 2002 WC|19}} | image = 2002 WC19.jpg | image_size = 250 | caption = {{mp|2002 WC|19}} and its satellite imaged by the Hubble Space Telescope in 2007 | discoverer = Palomar...»)
(разн.) ← Предыдущая версия | Текущая версия (разн.) | Следующая версия → (разн.)
Перейти к навигацииПерейти к поиску

Шаблон:Infobox planet

Шаблон:Mp is a twotino, that is, a planetoid in a 1:2 orbital resonance with Neptune. It was discovered on November 16, 2002 at the Palomar Observatory. If its derived diameter is correct it would have a higher density than Pluto, which is unusual as it appears to be much smaller than the expected size at which a Kuiper belt object usually becomes solid.

Knowing how many twotinos there are may reveal whether Neptune took roughly 1 million or 10 million years to migrate about 7 AU from its birth location.[1]

Satellite

A natural satellite was reported to be orbiting Шаблон:Mp (named S/2007 (119979) 1) on February 27, 2007. It is estimated to be Шаблон:Val from the primary, with an orbital period of Шаблон:Val days, an eccentricity of Шаблон:Val and an inclination of Шаблон:Val. Assuming similar albedos, it is a quarter the diameter of its primary, or around Шаблон:Convert in diameter.[2]

References

Шаблон:Reflist

External links

Шаблон:Minor planets navigator Шаблон:Small Solar System bodies Шаблон:Trans-Neptunian objects Шаблон:Dwarf planets Шаблон:Authority control

  1. Ошибка цитирования Неверный тег <ref>; для сносок on-the-fringe не указан текст
  2. Ошибка цитирования Неверный тег <ref>; для сносок johnston119979 не указан текст