Английская Википедия:2010 EU65

Материал из Онлайн справочника
Версия от 15:05, 22 декабря 2023; EducationBot (обсуждение | вклад) (Новая страница: «{{Английская Википедия/Панель перехода}} {{DISPLAYTITLE:{{mp|2010 EU|65}}}} {{Use dmy dates|date=August 2021}} {{Infobox planet | minorplanet = yes | name = {{mp|2010 EU|65}} | background = #C7FF8F | image = | image_size = | caption = | discovery_ref = <ref name="MPC-object" /><ref name="MPC-List-Cen-and-SDO" /><ref name="MPEC" /> | discoverer = David L. Rabinowit...»)
(разн.) ← Предыдущая версия | Текущая версия (разн.) | Следующая версия → (разн.)
Перейти к навигацииПерейти к поиску

Шаблон:Use dmy dates Шаблон:Infobox planet

Шаблон:Mp is a centaur, approximately Шаблон:Convert in diameter, orbiting the Sun in the outer Solar System. The object is also a promising Uranus horseshoe librator candidate.[1] It was first observed on 13 March 2010, by American astronomers David Rabinowitz and Suzanne Tourtellotte, observing from Cerro Tololo and La Silla Observatory in Chile.[2][3][4] Шаблон:Asof, it has neither been numbered nor named.[2]

Orbit and classification

Шаблон:Mp is classified as a centaur, a group of non-resonant small Solar System bodies whose orbit around the Sun lie typically between the orbits of Jupiter and Neptune (5 to 30 AU). Centaurs are minor planets with characteristics of comets, and often classified as such. The dynamical group is formed due to Neptune's eroding effect on the Kuiper belt by means of gravitational scattering, sending objects inward to become centaurs, or outward to become scattered-disc objects, or removing them from the Solar System entirely. Centaurs themselves have unstable orbits with short lifetimes, transitioning from the inactive population of Kuiper belt objects to the active group of Jupiter-family comets within approximately one million years.

It orbits the Sun at a distance of 17.0–22.9 AU once every 89 years and 3 months (32,606 days; semi-major axis of 19.97 AU). Its orbit has an eccentricity of 0.15 and an inclination of 15° with respect to the ecliptic. It has a Tisserand's parameter with respect to Jupiter (TJ) of 2.94, near the threshold of 3, typically used to distinguish asteroids from Jupiter-family comets.[5] On 21 June 2021, the object came to perihelion at 17.0 AU and has since been moving away from the Sun.Шаблон:Efn Шаблон:Asof the object is at 17.009 AU, with a apparent magnitude of 21.71.[6] The body's observation arc begins with a precovery observation taken by the Mount Lemmon Survey in April 2009.[2]

Uranus horseshoe candidate

Based on its current heliocentric orbit, Шаблон:Mp follows a horseshoe orbit around Uranus' Шаблон:L3 point. Giving the fact that its orbit is, at present, poorly determined, the object is a promising Uranus horseshoe orbiter candidate.[1]

Physical properties

Шаблон:Mp has an absolute magnitude of 9.1. Based on a generic magnitude-to-diameter conversion, it measures approximately Шаблон:Convert in diameter assuming an albedo of 0.09.[7]

See also

Notes

Шаблон:Notelist

References

Шаблон:Reflist

External links

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

Партнерские ресурсы
Криптовалюты
Магазины
Хостинг
Разное

  1. ↑ 1,0 1,1 Ошибка цитирования Неверный тег <ref>; для сносок De-la-Fuente-Marcos-2013 не указан текст
  2. ↑ 2,0 2,1 2,2 Ошибка цитирования Неверный тег <ref>; для сносок MPC-object не указан текст
  3. ↑ Ошибка цитирования Неверный тег <ref>; для сносок MPC-List-Cen-and-SDO не указан текст
  4. ↑ Ошибка цитирования Неверный тег <ref>; для сносок MPEC не указан текст
  5. ↑ Ошибка цитирования Неверный тег <ref>; для сносок jpldata не указан текст
  6. ↑ Ошибка цитирования Неверный тег <ref>; для сносок AstDys-object не указан текст
  7. ↑ Ошибка цитирования Неверный тег <ref>; для сносок johnstonsarchive-TNO-list не указан текст
Источник — http://wikihandbk.com/ruwiki/index.php?title=Английская_Википедия:2010_EU65&oldid=12706614