Английская Википедия:51 Pegasi
Шаблон:Short description Шаблон:Starbox begin Шаблон:Starbox image Шаблон:Starbox observe Шаблон:Starbox character Шаблон:Starbox astrometry Шаблон:Starbox detail Шаблон:Starbox catalog Шаблон:Starbox reference Шаблон:Starbox end
51 Pegasi (abbreviated 51 Peg), formally named Helvetios Шаблон:IPAc-en,[1] is a Sun-like star located Шаблон:Convert from Earth in the constellation of Pegasus. It was the first main-sequence star found to have an exoplanet (designated 51 Pegasi b, officially named Dimidium) orbiting it.[2]
Properties
The star's apparent magnitude is 5.49, making it visible with the naked eye under suitable viewing conditions.
51 Pegasi was listed as a standard star for the spectral type G2IV in the 1989 The Perkins catalog of revised MK types for the cooler stars. Historically, it was generally given a stellar classification of G5V,[3] and even in more modern catalogues it is usually listed as a main-sequence star.[4] It is generally considered to still be generating energy through the thermonuclear fusion of hydrogen at its core, but to be in a more evolved state than the Sun.[5] The effective temperature of the chromosphere is about Шаблон:Convert, giving 51 Pegasi the characteristic yellow hue of a G-type star.[6] It is estimated to be about 6.1 billion years old, somewhat older than the Sun, with a radius 24% larger and 11% more massive. The star has a higher proportion of elements other than hydrogen/helium compared to the Sun; a quantity astronomers term a star's metallicity. Stars with higher metallicity such as this are more likely to host giant planets.[7] In 1996, astronomers Baliunas, Sokoloff, and Soon measured a rotational period of 37 days for 51 Pegasi.[8]
Although the star was suspected of being variable during a 1981 study,[9] subsequent observation showed there was almost no chromospheric activity between 1977 and 1989. Further examination between 1994 and 2007 showed a similar low or flat level of activity. This, along with its relatively low X-ray emission, suggests that the star may be in a Maunder minimum period[3] during which a star produces a reduced number of star spots.
The star rotates at an inclination of 79Шаблон:± degrees relative to Earth.[10]
Nomenclature
51 Pegasi is the Flamsteed designation. On its discovery, the star's planet — and actually the first exoplanet discovered around a main-sequence star — was designated 51 Pegasi b by its discoverers and unofficially dubbed Bellerophon, in keeping with the convention of naming planets after Greek and Roman mythological figures (Bellerophon was a figure from Greek mythology who rode the winged horse Pegasus).[11]
In July 2014, the International Astronomical Union launched NameExoWorlds, a process for giving proper names to certain exoplanets and their host stars.[12] The process involved public nomination and voting for the new names.[13] In December 2015, the IAU announced the names of Helvetios for this star and Dimidium for its planet.[14]
The names were those submitted by the Astronomische Gesellschaft Luzern, Switzerland. "Helvetios" is Latin for "the Helvetian" and refers to the Celtic tribe that lived in Switzerland during antiquity; 'Dimidium' is Latin for 'half', referring to the planet's mass of at least half the mass of Jupiter.[15]
In 2016, the IAU organized a Working Group on Star Names (WGSN)[16] to catalog and standardize proper names for stars. In its first bulletin of July 2016,[17] the WGSN explicitly recognized the names of exoplanets and their host stars approved by the Executive Committee Working Group Public Naming of Planets and Planetary Satellites, including the names of stars adopted during the 2015 NameExoWorlds campaign. This star is now so entered in the IAU Catalog of Star Names.[1]
Planetary system
On October 6, 1995, Swiss astronomers Michel Mayor and Didier Queloz announced the discovery of an exoplanet orbiting 51 Pegasi.[2] The discovery was made at Observatoire de Haute-Provence in France. On 8 October 2019, Mayor and Queloz shared the Nobel Prize in Physics for their discovery.[18]
51 Pegasi b (51 Peg b) was the first discovered planetary-mass companion of a main-sequence parent star. It orbits very close to the star, experiences estimated temperatures around Шаблон:Convert and has a mass at least half that of Jupiter. At the time of its discovery, this close distance was not compatible with theories of planet formation and resulted in discussions of planetary migration.[19] However, several hot Jupiters are now known to be oblique relative to the stellar axis.[20]
Шаблон:OrbitboxPlanet begin Шаблон:OrbitboxPlanet Шаблон:Orbitbox end
See also
Шаблон:Col-begin Шаблон:Col-break
- Star systems
- Other articles
- Portal
References
External links
- Шаблон:Cite web
- 51 Pegasi at SolStation.com.
- nStars database entry
- David Darling's encyclopedia
Шаблон:Stars of Pegasus Шаблон:Sky
- ↑ 1,0 1,1 Ошибка цитирования Неверный тег
<ref>
; для сносокIAU-CSN
не указан текст - ↑ 2,0 2,1 Ошибка цитирования Неверный тег
<ref>
; для сносокnature378_6555_355
не указан текст - ↑ 3,0 3,1 Ошибка цитирования Неверный тег
<ref>
; для сносокaaa508_3_1417
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокskiff
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокmittag
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокcsiro
не указан текст - ↑ Шаблон:Cite journal
- ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокapjl457_2_L99
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокcsvs
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокmnras408_3_1666
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокberkeley
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокiau1404
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокexoworlds
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокiau1514
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокnames
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокWGSN
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокWGSN1
не указан текст - ↑ Шаблон:Cite news
- ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокexoplaneteu
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокOjeda
не указан текст
- Английская Википедия
- Страницы с неработающими файловыми ссылками
- G-type main-sequence stars
- Solar analogs
- Maunder Minimum
- Planetary systems with one confirmed planet
- Pegasus (constellation)
- Durchmusterung objects
- Flamsteed objects
- Gliese and GJ objects
- Henry Draper Catalogue objects
- Hipparcos objects
- Bright Star Catalogue objects
- Страницы, где используется шаблон "Навигационная таблица/Телепорт"
- Страницы с телепортом
- Википедия
- Статья из Википедии
- Статья из Английской Википедии
- Страницы с ошибками в примечаниях