astro.wikisort.org - Planet
MOA-2007-BLG-192L is a low-mass red dwarf star or brown dwarf, approximately 3,000 light-years away in the constellation of Sagittarius. It is estimated to have a mass approximately 6% of the Sun's.[3] In 2008, an Earth-sized extrasolar planet was announced to be orbiting this object.[4]
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Sagittarius |
| Right ascension | 18h 08m 04s[1] |
| Declination | −27° 09′ 00″[1] |
| Astrometry | |
| Distance | 2300−400+700[2] ly (700−120+210[2][3] pc) |
| Details | |
| Mass | 0.060+0.028−0.021[3] M☉ |
| Database references | |
| SIMBAD | data |
Planetary system
The discovery of a planet, MOA-2007-BLG-192Lb, orbiting this object was announced on June 2, 2008.[4] This planet, with a mass of approximately 3.3 times that of Earth, is one of the smallest known extrasolar planets. It was found when it caused a gravitational microlensing event on the night of May 24, 2007, which was detected as part of the MOA-II gravitational microlensing survey at the Mount John University Observatory in New Zealand.[3]
| Companion | Mass | Observed separation (AU) |
| b | 3.3+4.9−1.6[3] M🜨 | 0.62+0.22−0.16[3] |
See also
References
- "Notes for star MOA-2007-BLG-192-L". The Extrasolar Planets Encyclopaedia. Archived from the original on 2008-09-26. Retrieved 2008-06-16.
- "Notes for Star MOA-2007-BLG-192L". Extrasolar Planets Encyclopaedia. Archived from the original on 26 September 2008. Retrieved 29 February 2012.
- Table 3, Bennett, D. P.; Bond, I. A.; Udalski, A.; Sumi, T.; Abe, F.; Fukui, A.; Furusawa, K.; Hearnshaw, J. B.; et al. (2008). "A Low‐Mass Planet with a Possible Sub‐Stellar‐Mass Host in Microlensing Event MOA‐2007‐BLG‐192". The Astrophysical Journal. 684 (1): 663–683. arXiv:0806.0025. Bibcode:2008ApJ...684..663B. doi:10.1086/589940. S2CID 14467194.
- MOA-2007-BLG-192Lb: A Low-Mass Planet with a Possible Sub-Stellar-Mass Host Archived 2008-06-06 at the Wayback Machine, David P. Bennett. Accessed on line July 3, 2008.
External links
- "MOA-2007-BLG-192Lb: A Low-Mass Planet with a Possible Sub-Stellar-Mass Host". Archived from the original on 2008-06-06. Retrieved 2008-06-28.
- "Notes for star MOA-2007-BLG-192-L". The Extrasolar Planets Encyclopaedia. Archived from the original on 2008-09-26. Retrieved 2008-07-02.
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На других языках
[de] MOA-2007-BLG-192L
MOA-2007-BLG-192L ist ein Roter Zwerg oder Brauner Zwerg mit geringer Masse. MOA-2007-BLG-192L ist annäherungsweise 3000 Lichtjahre entfernt, im Sternbild Schütze. Er hat wahrscheinlich in etwa 6 % der Sonnenmasse. 2008 wurde ein extrasolarer Planet entdeckt, welcher MOA-2007-BLG-192L umkreist.- [en] MOA-2007-BLG-192L
[ru] MOA-2007-BLG-192L
MOA-2007-BLG-192-L — звезда спектрального класса M, расположенная в созвездии Стрельца на расстоянии примерно 2300 световых лет от Солнечной системы. Она представляет собой чрезвычайно тусклый и холодный красный карлик с массой, составляющей 6 % от солнечной[2]. Вокруг звезды обращается, как минимум, одна планета.Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.
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