astro.wikisort.org - StarGliese 251, also known as HIP 33226 or HD 265866, is a star located about 18 light years away from the Solar System. Located in the constellation of Gemini, it is the nearest star in this constellation.[10] It is located near the boundary with Auriga, 49 arcminutes away from the bright star Theta Geminorum; due to its apparent magnitude of +9.89 it cannot be observed with the naked eye.[2] The closest star to Gliese 251 is QY Aurigae, which is located 3.5 light years away.[11]
Star in the constellation Gemini
Gliese 251
Observation data Epoch J2000 Equinox J2000 |
Constellation |
Gemini |
Right ascension |
06h 54m 48.96009s[1] |
Declination |
+33° 16′ 05.4393″[1] |
Apparent magnitude (V) |
+10.11[2] |
Characteristics |
Spectral type |
M3.0Ve[3] |
U−B color index |
+1.20[4] |
B−V color index |
+1.60[4] |
Astrometry |
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Radial velocity (Rv) | 22.91[5] km/s |
Proper motion (μ) | RA: -723.99[1] mas/yr Dec.: -398.40[1] mas/yr |
Parallax (π) | 179.0629 ± 0.0280 mas[6] |
Distance | 18.215 ± 0.003 ly (5.5846 ± 0.0009 pc) |
Absolute magnitude (MV) | 11.23[7] |
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Details |
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|
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Mass | 0.360±0.015[8] M☉ |
Radius | 0.364±0.011[8] R☉ |
Surface gravity (log g) | 4.96±0.07[8] cgs |
Temperature | 3451±51[8] K |
Metallicity [Fe/H] | -0.03±0.16[8] dex |
Rotational velocity (v sin i) | ≤2[8] km/s |
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Other designations |
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Gliese 251, HD 265866, HIP 33226, LHS 1879, LTT 11941, Ross 578, Wolf 294, 2MASS J06544902+3316058 [9] |
Database references |
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SIMBAD | data |
ARICNS | data |
Location of Gliese 251 in the constellation Gemini |
Gliese 251 is a red dwarf with a spectral type of M3V[3] with an effective temperature of about 3300 K.[3] Its mass has been measured to be around 0.36 solar masses[8] and its radius is about 36% solar radii.[8] Its metallicity is likely slightly less than that of the Sun.[8] Observations at infrared wavelengths rule out the presence of a circumstellar disk around it.[12]
Planetary system
In 2019, two candidate planets were detected by the radial velocity method to orbit Gliese 251 at orbits of 1.74 and 607 days.[13] However, a new study in 2020 using CARMENES data refuted both candidates, as they found that both signals were caused by stellar activity. Based on the CARMENES data, the team announced that Gliese 251 is orbited by one single super-Earth (Gliese 251 b) at an orbit of 14.238 days.[8]
The Gliese 251 planetary system[8]
Companion (in order from star) |
Mass |
Semimajor axis (AU) |
Orbital period (days) |
Eccentricity |
Inclination |
Radius |
b |
≥4.0±0.4 M🜨 |
0.0818+0.0011 −0.0012 |
14.238±0.002 |
0.10+0.09 −0.07 |
— |
— |
References
- van Leeuwen, F.; et al. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.
- Høg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode:2000A&A...355L..27H.
- Lépine, Sébastien (2013). "A Spectroscopic Catalog of the Brightest (J < 9) M Dwarfs in the Northern Sky". The Astronomical Journal. 145 (4): 102. arXiv:1206.5991. Bibcode:2013AJ....145..102L. doi:10.1088/0004-6256/145/4/102. S2CID 117144290.
- Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode:1986EgUBV........0M.
- Nidever, David L.; et al. (2013). "Radial Velocities for 889 Late-Type Stars". The Astrophysical Journal Supplement Series. 141 (2): 503–522. arXiv:astro-ph/0112477. Bibcode:2002ApJS..141..503N. doi:10.1086/340570. S2CID 51814894.
- Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- "ARICNS 4C00526". ARICNS. Retrieved 8 February 2017.
- Stock, S.; et al. (2020), "The CARMENES search for exoplanets around M dwarfs Three temperate-to-warm super-Earths", Astronomy & Astrophysics, A112: 643, arXiv:2010.00474, Bibcode:2020A&A...643A.112S, doi:10.1051/0004-6361/202038820, S2CID 222090233
- "GJ 251". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 8 February 2017.
- "Closest Stars". Retrieved 8 February 2017.
- "Stars within 15 light-years of Wolf 294". The Internet Stellar Database. Retrieved 7 February 2017.
- Beichman, C. A.; et al. (2006). "New Debris Disks around Nearby Main-Sequence Stars: Impact on the Direct Detection of Planets". The Astrophysical Journal. 652 (2): 1674–1693. arXiv:astro-ph/0611682. Bibcode:2006ApJ...652.1674B. doi:10.1086/508449. S2CID 14207148.
- Barnes, J. R.; et al. (2019-06-11). "Frequency of planets orbiting M dwarfs in the Solar neighbourhood". arXiv:1906.04644 [astro-ph.EP].
Notes
← Celestial objects within 15–20 light-years |
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Primary member type | Celestial objects by systems. |
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Brown dwarfs | L-type |
- DEN 0255-4700 (15.877±0.014 ly)
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T-type | |
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Y-type | |
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Sub-brown dwarfs and rogue planets | |
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Constellation of Gemini |
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Stars | |
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 Category |
На других языках
- [en] Gliese 251
[es] Gliese 251
Gliese 251 (GJ 251)[1] es una estrella que se encuentra a 18,15 años luz de distancia del sistema solar. Situada en la constelación de Géminis, es la estrella más próxima en esta constelación.[2]
Se localiza cerca del límite con Auriga a 49 minutos de arco de la brillante θ Geminorum, aunque debido a su débil brillo —magnitud aparente +9,89—[1] no puede ser observada a simple vista.
La estrella conocida más cercana a Gliese 251 es QY Aurigae, distante 3,50 años luz.[3]
[ru] HD 265866
HD 265866 (Вольф 294) — одиночная звезда в созвездии Близнецов. Находится на расстоянии около 18,6 световых лет от Солнца. Это одна из ближайших к нам звёзд.
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