Английская Википедия:15 Sagittae

Материал из Онлайн справочника
Версия от 11:21, 18 декабря 2023; EducationBot (обсуждение | вклад) (Новая страница: «{{Английская Википедия/Панель перехода}} {{Short description|G-type main sequence star in the constellation Sagitta}} {{Starbox begin}} {{Starbox observe | epoch = J2000.0 | constell = Sagitta | ra = {{RA|20|04|06.22091}}<ref name=GaiaDR2/> | dec = {{DEC|+17|04|12.6774}}<ref name=GaiaDR2/> | appmag_v = 5.80<ref name=Anderson2012/> }} {{Starbox character | type = main sequence | class = G0V + L4<ref name="Crepp...»)
(разн.) ← Предыдущая версия | Текущая версия (разн.) | Следующая версия → (разн.)
Перейти к навигацииПерейти к поиску

Шаблон:Short description Шаблон:Starbox begin Шаблон:Starbox observe Шаблон:Starbox character Шаблон:Starbox astrometry Шаблон:Starbox orbit Шаблон:Starbox detail Шаблон:Starbox catalog Шаблон:Starbox reference Шаблон:Starbox end

15 Sagittae (15 Sge) is a star in the northern constellation Sagitta, located around 58 light years away from the Sun. It is visible to the naked eye as a faint, yellow-hued star with an apparent visual magnitude of 5.80.[1] Considered a solar analog, it was the target of the first radial velocity survey from Lick Observatory, which found a drift due to a companion.[2] In 2002, the cause of this was found to be brown dwarf companion B via direct imaging.[3]

The companion is a high-mass substellar brown dwarf of spectral class L4 ± 1.5, only a few Jupiter masses below the limit for stars, in a long-period orbit around the primary star. Imaged by the Keck telescope, was the first brown dwarf candidate orbiting a sun-like star detected via imaging and is currently the only known companion brown dwarf which both has a significant radial velocity trend on the primary that has also been imaged.

The brown dwarf was originally thought to have a semi-major axis of 14 AU and a circular orbit viewed from pole-on,[4] but ten more years of observations found that the brown dwarf's orbit is viewed from nearly edge-on, is significantly eccentric and appeared to be moving in a circular orbit when first discovered, but is now approaching the primary as viewed from Earth.[5]

References

Шаблон:Reflist

External links

Шаблон:Stars of Sagitta

  1. Ошибка цитирования Неверный тег <ref>; для сносок Anderson2012 не указан текст
  2. Ошибка цитирования Неверный тег <ref>; для сносок Cumming1999 не указан текст
  3. Ошибка цитирования Неверный тег <ref>; для сносок Keck press release не указан текст
  4. Ошибка цитирования Неверный тег <ref>; для сносок Liu2002 не указан текст
  5. Ошибка цитирования Неверный тег <ref>; для сносок Crepp2012 не указан текст