Gliese 282

Gliese 282 is a star system composed of four stars in the equatorial constellation of Monoceros. At a distance of 36 light years, this star has an apparent magnitude of 7.26 when viewed from Earth. It is not visible to the naked eye.

Gliese 282
Observation data
Epoch J2000      Equinox 2000
Constellation Monoceros
Right ascension 07h 39m 59.33s[1]
Declination −03° 35′ 51.0″
Apparent magnitude (V) (7.30 + 9.01)[2]
Characteristics
Spectral type K2V[3] + K7V[4] + M1.5Ve[5]
Apparent magnitude (U) 12.9
Apparent magnitude (B) 11.844
Apparent magnitude (V) 10.385
Apparent magnitude (R) 9.365
Apparent magnitude (I) 8.065
Apparent magnitude (J) 6.795
Apparent magnitude (H) 6.306
Apparent magnitude (K) 6.032
Variable type A: BY Dra[6]
Astrometry
Radial velocity (Rv)−18.15[7] km/s
Proper motion (μ) RA: 69.90[1] mas/yr
Dec.: -278.33[1] mas/yr
Parallax (π)91.65 ± 3.50 mas[1]
Distance36 ± 1 ly
(10.9 ± 0.4 pc)
Details
Gl 282 A
Surface gravity (log g)4.40[8] cgs
Temperature4,956[8] K
Metallicity [Fe/H]−0.12[8] dex
Rotational velocity (v sin i)1.77[6] km/s
Age300−350[5] Myr
Gl 282 B
Metallicity [Fe/H]−0.25[9] dex
Age680−720[5] Myr
Other designations
Gl 282, HD 61606, HIP 37349, WDS J07400-0336, 2MASS J07395932-0335506, V869 Mon[10]
Gl 282 A: BD−03° 2001, SAO 134954
Gl 282 B: BD−03° 2002, SAO 134958
Gl 282 C: G 112-29, NLTT 18149
Database references
SIMBADAB
A
B
C
ARICNSA
B
C

The Gl 282AB star system is composed of two K- type main-sequence stars. The primary component, Gliese 282A, is a BY Draconis type variable star with a stellar classification of K2V. It has an effective temperature of 4,956 K. The companion, Gliese 282B, is a smaller, class K5V star. As of 2003, the pair had an angular separation of 58.30 arc seconds along a position angle of 113°.[2] This is equivalent to a projected physical separation of 824 AU.[5]

There is a distant common proper motion companion (G 112-29) at an angular separation of 1.09°. At the estimated distance of Gl 282AB, this corresponds to a projected separation of 55,733 AU, making it one of the widest known physical companions. Initially believed to be a red dwarf star with a stellar classification of M1.5Ve,[5] it turned out to be a pair of red dwarfs (Ca and Cb) with masses 0.55M☉ and 0.19M☉, orbiting each other on 6591+136
−177 days orbit.[11]

References
  1. van Leeuwen, F. (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.
  2. Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466–3471, Bibcode:2001AJ....122.3466M, doi:10.1086/323920, retrieved 2015-07-22.
  3. Montes, D.; et al. (2001), "Late-type members of young stellar kinematic groups - I. Single stars" (PDF), Monthly Notices of the Royal Astronomical Society, 328 (1): 45–63, arXiv:astro-ph/0106537, Bibcode:2001MNRAS.328...45M, doi:10.1046/j.1365-8711.2001.04781.x, S2CID 55727428.
  4. Gray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal, 132 (1): 161–170, arXiv:astro-ph/0603770, Bibcode:2006AJ....132..161G, doi:10.1086/504637, S2CID 119476992.
  5. Poveda, A.; et al. (November 2009), "G 112-29 (=NLTT 18149): A Very Wide Companion to GJ 282 AB with a Common Proper Motion, Common Parallax, Common Radial Velocity, and Common Age", The Astrophysical Journal, 706 (1): 343–347, arXiv:0910.2956, Bibcode:2009ApJ...706..343P, doi:10.1088/0004-637X/706/1/343, S2CID 116938161.
  6. Mishenina, T. V.; et al. (November 2012), "Activity and the Li abundances in the FGK dwarfs", Astronomy & Astrophysics, 547: 8, arXiv:1210.6843, Bibcode:2012A&A...547A.106M, doi:10.1051/0004-6361/201118412, S2CID 119287319, A106.
  7. Nidever, David L; et al. (August 2002), "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.
  8. Mishenina, T. V.; et al. (April 2013), "Abundances of neutron-capture elements in stars of the Galactic disk substructures", Astronomy & Astrophysics, 552: 12, arXiv:1303.1730, Bibcode:2013A&A...552A.128M, doi:10.1051/0004-6361/201220687, S2CID 119268097, A128.
  9. Newton, Elisabeth R.; et al. (January 2014), "Near-infrared Metallicities, Radial Velocities, and Spectral Types for 447 Nearby M Dwarfs", The Astronomical Journal, 147 (1): 24, arXiv:1310.1087, Bibcode:2014AJ....147...20N, doi:10.1088/0004-6256/147/1/20, S2CID 26818462, 20.
  10. "HD 61606". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2016-01-05.{{cite web}}: CS1 maint: postscript (link)
  11. Baroch, D.; et al. (2021), The CARMENES search for exoplanets around M dwarfs Spectroscopic orbits of nine M-dwarf multiple systems, including two triples, two brown dwarf candidates, and one close M-dwarf–white dwarf binary, arXiv:2105.14770
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