Английская Википедия:HD 111031
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
HD 111031 (50 G. Corvi) is a double star in the southern constellation of Corvus. With an apparent visual magnitude of 6.87,[1] it is considered too faint to be readily visible to the naked eye. The distance to this star is 102 light years, but it is drifting closer to the Sun with a radial velocity of −20 km/s.[2] It has an absolute magnitude of 4.42.[1] The star has a relatively large proper motion, traversing the celestial sphere at an angular rate of Шаблон:Val.[3]
This object is a solar analog with a stellar classification of G5 V;[4] a G-type main-sequence star like the Sun that is generating energy through core hydrogen fusion. It is around five billion years old and is chromospherically inactive,[4] with a projected rotational velocity of 1.7 km/s. The star has 1.13 times the mass and 1.27 times the radius of the Sun. It is radiating 1.5 times the Sun's luminosity from its photosphere at an effective temperature of 5,836 K.[5]
In 2020, a stellar companion was identified using high-contrast imaging. The study authors deem this most likely a K-type main-sequence star with a class of K5V, an angular separation of Шаблон:Val along a position angle (PA) of 300° corresponding to a projected separation of Шаблон:Val, and around 11–15% of the mass of the Sun.[6] An independent study published in 2021 identified a companion through speckle imaging. They propose this is a faint red dwarf with a class of M6 or later and a visual magnitude difference of 7.9 or more compared to the primary. It is located at a separation of Шаблон:Val along a PA of 121°, as of 2021.[7]
A 2022 study claimed the presence of a brown dwarf companion to this star based on radial velocity and astrometry observations,[8] but according to a 2023 follow-up study this was in fact a detection of the previously known stellar companion, poorly characterized due to the baseline of observations being much shorter than the companion's orbital period.[9]
References
- ↑ 1,0 1,1 Ошибка цитирования Неверный тег
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; для сносокAnderson_Francis_2012
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; для сносокGaiaDR3
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; для сносокLuyten1995
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; для сносокGray_et_al_2003
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; для сносокSoto_Jenkins_2018
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; для сносокGonzales_et_al_2020
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; для сносокDalba_et_al_2021
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; для сносокFeng2022
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; для сносокPhilipot2023
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- Английская Википедия
- G-type main-sequence stars
- Double stars
- Corvus (constellation)
- Durchmusterung objects
- Gliese and GJ objects
- Gould objects
- Henry Draper Catalogue objects
- Hipparcos objects
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