Gliese 486 / Gar

Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Right ascension 12h 47m 56.62457s[1]
Declination +09° 45′ 05.0357″[1]
Apparent magnitude (V) 11.395
Characteristics
Evolutionary stage main sequence
Spectral type M3.5V[2]
Astrometry
Radial velocity (Rv)19.20±0.17[1] km/s
Proper motion (μ) RA: −1008.267 mas/yr[1]
Dec.: −460.034 mas/yr[1]
Parallax (π)123.7756 ± 0.0329 mas[1]
Distance26.351 ± 0.007 ly
(8.079 ± 0.002 pc)
Details[3]
Mass0.323±0.015 M☉
Radius0.328±0.011 R☉
Luminosity0.01210±0.00023 L☉
Temperature3340±54 K
Metallicity [Fe/H]−0.15±0.13[4] dex
Rotation49.9±5.5 d[4]
Rotational velocity (v sin i)<2[5] km/s
Age1-8[4] Gyr
Other designations
Gar, GJ 486, HIP 62452, Wolf 437, TOI-1827, TYC 882-1111-1, 2MASS J12475664+0945050[6]
Database references
SIMBADdata

Gliese 486, also known as Wolf 437 and formally named Gar, is a red dwarf star 26.4 light-years (8.1 parsecs) away in the constellation Virgo. It hosts one known exoplanet.[3]

Nomenclature

The designation Gliese 486 comes from the Gliese Catalogue of Nearby Stars. This was the 486th star listed in the first edition of the catalogue.

In August 2022, this planetary system was included among 20 systems to be named by the third NameExoWorlds project.[7] The approved names, proposed by a team from Spain, were announced in June 2023. Gliese 486 is named Gar and its planet is named Su, after the Basque words for "flame" and "fire".[8]

Properties

Gliese 486 has a surface temperature of 3340±54 K. Gliese 486 is similar to the Sun in its concentration of heavy elements, with a metallicity Fe/H index of 0.07±0.16. It was suspected to be a flare star,[9] although measurements available in 2019 did not reveal any flares.[10] The chemical makeup of the star is unremarkable and consistent with solar abundances or being slightly metal-poor.[4]

The star has an unremarkable magnetic field in the chromosphere of about 1.6 kilogauss.[5] It is rotating very slowly and is likely to be very old, belonging kinematically to the old thin disk of the Milky Way.[11]

Multiplicity surveys did not detect any stellar companions to Gliese 486 as of 2020.[12]

Planetary system

Artistic impression of the surface of the hot super-Earth Gliese 486b.

In 2021, one planet, named Gliese 486 b, was discovered on a tight, circular orbit.[3] It represents a rare class of rocky exoplanet suitable for spectroscopic characterization in the near future[13] by the James Webb Space Telescope.[14] As of 2022, no hydrogen or steam dominated atmosphere was detected, although a secondary planetary atmosphere with a higher molecular weight remains a possibility.[15] Observations by JWST announced in 2023 detected signs of water vapor, but it is unclear if this is from the planet's atmosphere or from its host star.[16][17]

The Gliese 486 planetary system[3]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b / Su 2.82+0.11
−0.12 M🜨		 0.01734+0.00026
−0.00027		 1.467119+0.000031
−0.000030		 <0.05 88.4+1.1
−1.4°		 1.305+0.063
−0.067 R🜨

References

  1. 1 2 3 4 5 6 Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  2. ↑ Bozhinova, I.; Helling, Ch.; Scholz, A. (2014), "Planetary host stars: Evaluating uncertainties in cool model atmospheres", Monthly Notices of the Royal Astronomical Society, 450: 160–182, arXiv:1405.5416, Bibcode:2015MNRAS.450..160B, doi:10.1093/mnras/stv613
  3. 1 2 3 4 Trifonov, T.; et al. (2021), "A nearby transiting rocky exoplanet that is suitable for atmospheric investigation", Science, 371 (6533): 1038–1041, arXiv:2103.04950, Bibcode:2021Sci...371.1038T, doi:10.1126/science.abd7645, PMID 33674491, S2CID 232124642
  4. 1 2 3 4 Caballero, J. A.; et al. (2022), "A detailed analysis of the Gl 486 planetary system", Astronomy & Astrophysics, 665: A120, arXiv:2206.09990, Bibcode:2022A&A...665A.120C, doi:10.1051/0004-6361/202243548, S2CID 249889232
  5. 1 2 Moutou, Claire; Hébrard, Élodie M.; Morin, Julien; Malo, Lison; Fouqué, Pascal; Torres-Rivas, Andoni; Martioli, Eder; Delfosse, Xavier; Artigau, Étienne; Doyon, René (2017), "SPIRou input catalogue: Activity, rotation and magnetic field of cool dwarfs", Monthly Notices of the Royal Astronomical Society, 472 (4): 4563–4586, arXiv:1709.01650, Bibcode:2017MNRAS.472.4563M, doi:10.1093/mnras/stx2306
  6. ↑ "Wolf 437". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-03-10.
  7. ↑ "List of ExoWorlds 2022". nameexoworlds.iau.org. IAU. 8 August 2022. Retrieved 27 August 2022.
  8. ↑ "2022 Approved Names". nameexoworlds.iau.org. IAU. Retrieved 7 June 2023.
  9. ↑ O'Donoghue, D.; Koen, C.; Kilkenny, D.; Stobie, R. S.; Koester, D.; Bessell, M. S.; Hambly, N.; MacGillivray, H. (2003), "The DA+d Me eclipsing binary EC13471-1258: its cup runneth over ... Just", Monthly Notices of the Royal Astronomical Society, 345 (2): 506–528, arXiv:astro-ph/0307144, Bibcode:2003MNRAS.345..506O, doi:10.1046/j.1365-8711.2003.06973.x, S2CID 17408072
  10. ↑ Vida, Krisztián; Leitzinger, Martin; Kriskovics, Levente; Seli, Bálint; Odert, Petra; Kovács, Orsolya Eszter; Korhonen, Heidi; Van Driel-Gesztelyi, Lidia (2019), "The quest for stellar coronal mass ejections in late-type stars", Astronomy & Astrophysics, 623: A49, arXiv:1901.04229, doi:10.1051/0004-6361/201834264, S2CID 119095055
  11. ↑ Browning, Matthew K.; Basri, Gibor; Marcy, Geoffrey W.; West, Andrew A.; Zhang, Jiahao (2010), "Rotation and Magnetic Activity in a Sample of M-Dwarfs", The Astronomical Journal, 139 (2): 504, Bibcode:2010AJ....139..504B, doi:10.1088/0004-6256/139/2/504, S2CID 121835145
  12. ↑ Lamman, Claire; Baranec, Christoph; Berta-Thompson, Zachory K.; Law, Nicholas M.; Schonhut-Stasik, Jessica; Ziegler, Carl; Salama, Maïssa; Jensen-Clem, Rebecca; Duev, Dmitry A.; Riddle, Reed; Kulkarni, Shrinivas R.; Winters, Jennifer G.; Irwin, Jonathan M. (2020), "Robo-AO M-dwarf Multiplicity Survey: Catalog", The Astronomical Journal, 159 (4): 139, arXiv:2001.05988, Bibcode:2020AJ....159..139L, doi:10.3847/1538-3881/ab6ef1, S2CID 210718832
  13. ↑ Hot Super-Earth Discovered 26 Light-Years Away
  14. ↑ Newfound exoplanet could be 'Rosetta Stone' for studies of alien atmospheres
  15. ↑ Ridden-Harper, Andrew; Nugroho, Stevanus; Flagg, Laura; Jayawardhana, Ray; Turner, Jake D.; Ernst de Mooij; MacDonald, Ryan; Deibert, Emily; Tamura, Motohide; Kotani, Takayuki; Hirano, Teruyuki; Kuzuhara, Masayuki; Omiya, Masashi; Kusakabe, Nobuhiko (2023), "High-resolution Transmission Spectroscopy of the Terrestrial Exoplanet GJ 486b", The Astronomical Journal, 165 (4): 170, arXiv:2212.11816, Bibcode:2023AJ....165..170R, doi:10.3847/1538-3881/acbd39
  16. ↑ Moran, Sarah E.; Stevenson, Kevin B.; et al. (May 2023). "High Tide or Rip-Tide on the Cosmic Shoreline? A Water-Rich Atmosphere or Stellar Contamination for the Warm Super-Earth GJ 486b from JWST Observations". The Astrophysical Journal Letters. 948 (1): L11. arXiv:2305.00868. Bibcode:2023ApJ...948L..11M. doi:10.3847/2041-8213/accb9c.
  17. ↑ "Webb Finds Water Vapor, But From a Rocky Planet or Its Star?". webbtelescope.org. STScI. 1 May 2023. Retrieved 1 May 2023.
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